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Joe Rogan Experience #2506 - Michelle Thaller

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Joe Rogan Experience #2506 - Michelle Thaller

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4606 segments

0:01

Joe Rogan podcast. Check it out.

0:03

>> The Joe Rogan Experience.

0:06

>> TRAIN BY DAY. JOE ROGAN PODCAST BY

0:08

NIGHT. All day.

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>> I like that.

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>> Absolutely.

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>> It's also there's some things that are

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so awesome. It's like that's

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awesome.

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>> I I was I was trying to talk about black

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holes to some high school students just

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seriously earlier this week and I was I

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kept saying, you know, what the f

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Yeah. So, I I got nothing to pitch, but

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I I uh um I the Shorewood Men's Club, I

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was giving a talk there. The Shorewood,

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Wisconsin is where I live. The men's

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club invited me to give a talk about

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astronomy last week, and when I

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mentioned I was coming to the show, they

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just freaked out. And so, the only thing

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I have is my Shorewood Men's Club uh uh

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uh water.

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>> Well, shout out to the Shorewood Men's

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Club. That's awesome. That's so cool

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that you give those speeches. I love

0:52

your YouTube talks. They are fantastic.

0:55

>> Oh, thank you. Wow. I have watched

0:59

probably every one you've ever done.

1:01

I've I've watched at least I mean how

1:02

many have you done? I've done I've

1:04

watched at least like 10 of them.

1:06

>> Yeah. I mean, so I mean pretty much what

1:08

I did at at NASA I did a lot of sort of

1:10

the science spokesperson stuff and so so

1:13

most of that was you know I I'm more on

1:15

the NASA videos. I hosted like launch

1:17

events. I haven't done much privately on

1:20

YouTube. I'm I'm I'm thinking about

1:22

starting some stuff. Oh,

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>> you should. I I'll Yeah, I'll work on

1:25

that. Okay.

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>> 100%.

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>> Thank you.

1:27

>> 100%. You said so many things that made

1:29

me just go, "What?"

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>> Ah,

1:32

>> like here's a big one that you said. You

1:33

were talking about if the size of Earth,

1:37

if the Earth was the dot of an eye in a

1:39

book in regular print.

1:41

>> Yes.

1:42

>> That the Milky Way galaxy would be as

1:45

large as the Earth itself.

1:47

>> Actually, a little bigger. Yeah. So, I

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mean, the thing is this is an

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interesting thing about science

1:51

communication.

1:53

You say that if if the if the sun were

1:55

the size of a dot of an eye and you got

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to remember you can fit a million earths

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inside the sun, right? This is a huge

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thing. So if that's the size of a dot of

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an eye on text, then the galaxy would be

2:05

the size of the earth. That's when

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people's eyes get big and people respond

2:08

to it.

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>> So it's not just the earth, it's the the

2:10

sun. So if the sun was the dot of an

2:11

eye.

2:12

>> Yes, that's right. So let's let's make

2:13

this clear. So the sun were the size of

2:15

the dot of an eye on a page of text. So

2:17

you could fit a million earths inside

2:19

that dot of an eye, then the Milky Way

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galaxy would be bigger than the Earth.

2:24

>> Yeah. I think

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>> So if the Earth was the dot of an eye,

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then how big is the Milky Way galaxy?

2:30

Cuz the sun is how many millions Earths

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>> volume wise, you could fit over a

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million Earths inside the sun. Yeah.

2:36

Yeah. The the sun is about 800,000 miles

2:38

across. You could fit about 110 Earths

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across it. The diameter. We do those

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things where you show the the

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differences between our sun and

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different stars and immense stars and

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you go bigger and bigger and bigger and

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you you get to the point where you're

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like I can't my this is not working. I

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can't get I can't process this. It's too

2:57

kooky.

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>> There there's nobody that can process

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it. I mean I mean one one of the the the

3:01

really kind of you know the thing about

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sort of demystifying scientists is the

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idea that our brains somehow work any

3:06

differently and like we can visualize

3:09

what a lightyear is, right? you know, a

3:10

lightyear is about six trillion miles.

3:13

That, you know, the distance light

3:14

travels in a year. No, we're human

3:15

beings. We we get used to using the

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terms. We get used to, you know, using

3:20

the numbers, but but we've got the same

3:22

brain as everybody else. Nobody can

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visualize what a galaxy really is. And

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you can take pictures of them. You can

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say the word galaxy, but people have no

3:32

idea what what monsters these are. and

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and and then with like with the James

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Webb Space Telescope, you know, all of a

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sudden you're taking pictures of

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billions of them and you know, they're

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right in front of your eyes. This is not

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something that you can argue about. It's

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an image and and you see these these

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foggy hazes of of of stars, you know,

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basically so many stars you can't see

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them individually. And that's real. And

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and I mean, it still gives me

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goosebumps.

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>> That's awesome.

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It gives me goosebumps, too. But it's so

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cool that it gives it to you and you

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actually study it your whole life.

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>> Oh, that's that's that's the whole

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point. I I mean, you know, working for

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NASA was a huge huge honor. And I mean,

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all of us there are doing this. I mean,

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we were all science fiction fans. We all

4:17

love imagination. Um, you know, we

4:22

that was the best thing about working at

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NASA was was the joy and and and the the

4:26

teamwork and the camaraderie and the

4:28

people that you're working with that uh

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you know, they they think this is the

4:30

best thing in the world to do. Well, I

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mean, there's a a real problem that we

4:35

have where I think that cities and light

4:38

pollution have really for, you know,

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it's great that we have cities. It's

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wonderful. It's wonderful that we have

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all this electricity and that we can see

4:46

things at night time, but boy, we have

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done ourselves a massive disservice by

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not being able to see the stars all the

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time. And I think people have kind of

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lost the wonder of it when you're only

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looking at it as images on your phone or

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when, you know, the only time you get it

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is on vacation. Occasionally, you look

5:00

up in the sky. Wow, look at all the

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stars here. It's different here. This is

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something that everyone should be

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absolutely blown away by. At night, you

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have a vision of the most spectacular

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thing any human being has ever seen

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ever. Just the Milky Way galaxy alone.

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It's nuts. It's crazy to think that

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those are all stars and that you can't

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count them. It's insane. There's so many

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of them and it's above you every day.

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And we're just blas blas. We're just

5:29

like so used to it. We're so dismissive

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of it. So it doesn't mean anything. It

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It's exciting when someone's excited by

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it because I'm like more people need to

5:38

get the away from the cities and

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just go see how crazy this is that we

5:42

are flying through space.

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>> Yeah,

5:46

it is profound. And to be that close, I

5:48

mean just looking up, you don't even

5:50

need a telescope or a pair of

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binoculars. The presence of something so

5:54

much larger than you. But I mean, if

5:56

you've if you've listened to some of my

5:57

my podcasts, and I think you you know

5:59

that the big deal for me is that you are

6:02

such a part of this. You are such an

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intimate, intrinsic part of this. It's

6:07

not we're separate from space. You know,

6:09

we look up and there's something

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separate from us. You know, that's the

6:12

story of us up there. you know, the the

6:14

only way the universe makes atoms, the

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only way that makes, you know, the

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chemicals all around us, you know, the

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the aluminum, the iron, the oxygen, the

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carbon, you know, the phosphorus,

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everything that makes me up, you know,

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the only thing in the universe that

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makes atoms is the interior of a star.

6:29

It's the only place where nuclear fusion

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puts atoms together. So, so everything

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that you are, the the story is up there.

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And, you know, so you're you're not

6:38

looking at something separate and

6:40

distant, you know. I mean astrophysics

6:42

is the story of you know the end of your

6:44

nose literally I mean I mean we are part

6:47

of this beautiful bigger thing

6:49

>> that's a weird concept the I mean that's

6:52

from that old song you know we are

6:53

stardust

6:54

>> yeah we're golden to get ourselves back

6:58

yeah um that that's real that's what we

7:00

are and that's what all life is and that

7:02

that's just a very strange thing for

7:04

people to wrap their heads around as

7:06

we're sort of slowly getting a greater

7:09

and greater understanding of the

7:11

complexity of the universe itself which

7:13

is relatively recent in terms of h human

7:16

history. I mean we really didn't know

7:19

all all what we just we know now because

7:22

the James Webb telescope is so crazy

7:25

where they're seeing these new these

7:26

galaxies they're confusing like why are

7:28

they formed so early.

7:29

>> Oh yeah. Oh I I I gave a talk about

7:31

those just a few weeks ago. The the red

7:33

dots. Yes. And they never let

7:34

astronomers name anything. Right. You're

7:36

seeing something so dramatic and they

7:37

call it the little red dots, right? you

7:39

know, or you know, there's a storm on

7:40

Jupiter that's three times the size of

7:42

the Earth with 400 mph winds, and they

7:44

call it, you know, the red spot.

7:45

>> How come no one's allowed to name them?

7:47

>> Well, naming conventions, uh, well,

7:49

they're they're complex. So, so if you

7:51

if you discover a comet, you get to know

7:53

if you discover an asteroid, you get to

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name it. If you discover a comet, the

7:57

comet is named after you. But anything

7:59

else has to be done by international

8:00

committee. And so, you know, they they

8:03

because of that, things don't end up

8:04

with very interesting names. They all

8:05

end up with, you know, catalog numbers,

8:07

you you know, basically phone numbers.

8:09

>> What do they call that weird hexagon on

8:11

Jupiter? Is it a hexagon?

8:12

>> Saturn. Hexagon. I think they call that,

8:15

you know, the hexagon on Saturn. They

8:17

don't even they don't really the

8:18

hexagonal storm. It's fantastic. Uh you

8:21

could fit about two Earths across that.

8:23

And it it it's a it's a hex it's a

8:25

hexagon jetream basically. You've got

8:28

super fast moving winds around the pole

8:30

of Saturn. and and Saturn is so cold,

8:33

the gas is so cold that there's almost

8:35

no friction in the gas. So unlike here,

8:38

you know, the jetream here, there's kind

8:40

of this joke. Oh, there's a picture.

8:42

Hey, that's fantastic. Um,

8:44

>> that's wild.

8:45

>> One of my favorite pictures NASA ever

8:47

took. If you look at the little dot in

8:49

the middle of that, the sort of little

8:50

eye of the storm. We actually have a

8:52

picture from Cassini where you can see

8:54

the sun glinting off of hundreds of mile

8:58

high. There you go. It's down in the

8:59

bottom there. It's in the bottom in the

9:00

middle. Yeah, that picture. One more

9:03

over. Yeah, that that that's a picture

9:04

uh from the Cassini space mission.

9:06

That's a real image.

9:07

>> Wow.

9:07

>> And that's the eye of that storm. And

9:10

and those are, like I said, hundreds of

9:12

miles high banks of clouds catching the

9:14

sunlight and the poles of Saturn. And

9:16

you know, we did that. We we went there.

9:19

We flew over that storm.

9:20

>> That's crazy. And uh uh and and yeah, I

9:22

mean as amazing as the storm is, it's um

9:25

it's at least fairly well understood as

9:28

a very low temperature jetream. You

9:29

know, I mean, you may be familiar here.

9:31

People kind of joke about like, you

9:32

know, the weather's the same. A week

9:33

from now, the weather will be about the

9:34

same as it is now. There patterns that

9:36

get set up in in the jetream of the

9:37

Earth and you you take away all the heat

9:39

and all the friction and it forms this

9:41

this beautiful storm.

9:43

>> What why what is the theories why it

9:45

forms a hexagon?

9:46

>> It's it's something called a standing

9:48

wave. the the the the the jetream

9:50

basically sets up a wave inside this

9:52

circulation and and I'm I I will admit

9:54

I'm not an atmospheric specialist, but

9:56

that that's what I know. And and and

9:58

that wave kind of kind of makes this

9:59

hexagonal shape and and then you cool

10:02

everything down without friction and

10:03

that's how the whole thing works. They

10:05

they have done computer simulations of

10:08

very fastm moving jet streams under the

10:10

conditions of Saturn and you can get

10:11

this sort of shape to set up.

10:13

>> Wow.

10:14

>> God, it's so fascinating. And it's so

10:16

fascinating that we think of that as

10:18

being so far away.

10:19

>> That's just right in our neighborhood.

10:20

>> It's just right there. It's super hard

10:23

to get to. Takes a long time, but it's

10:26

just right there.

10:26

>> Well, we're hoping to launch, when I say

10:28

we, NASA's hoping to launch a new

10:30

mission to one of the moons of Saturn.

10:32

Uh hopefully in in like 2028. It'll take

10:34

it something like, you know, six, seven

10:36

years to get out to Saturn. But there's

10:37

a there's that giant moon of Saturn,

10:39

Titan, which has a thick atmosphere.

10:41

It's the only place where the air

10:42

pressure the air pressure is actually

10:44

even a little bit greater than the room

10:45

here. And uh um it's it's very cold. You

10:49

know, it's it's you know almost close to

10:50

300 degrees below zero, but it's got

10:52

this thick atmosphere and tons of

10:53

organic molecules and evidence of liquid

10:55

water below the surface. It's one of the

10:57

places that that might be friendly for

10:59

life. And so they're they're designing,

11:00

have you heard about this? It's called

11:01

Dragonfly. It's a it's an octacopter.

11:03

It's a big drone. There you go. Perfect.

11:06

And so so so Dragonfly is going to be

11:09

this big opticopter that we're going to

11:11

land on this moon Titan. We've already

11:12

landed on this moon once with the

11:14

Cassini mission. And it's got this this

11:16

really kick-ass uh chemical uh

11:19

laboratory inside to look for the

11:21

conditions for life, you know, anything,

11:23

you know, that we might be able to find

11:24

and and obviously sample more than one

11:26

site. You actually fly around and and go

11:28

to different places. There's rain, there

11:30

are oceans, there are rivers. The only

11:31

place we know there are open, you know,

11:33

great lakesized lakes on Titan.

11:35

>> Wow. Wow.

11:35

>> But it's so cold that it's not uh liquid

11:38

water. It's actually liquid natural gas.

11:39

Liquid methane and ethane. Yeah. Yeah.

11:42

And again, you know, the the

11:45

we we've already landed there. We

11:47

actually sent a probe there as part of

11:48

the Cassini mission to land on Titan. I

11:50

mean, it's just badass that you know

11:53

that that we humans have been there.

11:55

That that's a that's an artist

11:56

conception, but that's what it would

11:57

look like. You know, we we sent a probe

11:59

there. You know, it took a bunch of

12:00

readings and then and eventually froze

12:02

to death. But uh but but some of the

12:04

readings that it took were intriguing

12:07

about the possibility of life on Titan.

12:09

>> Didn't the Russians land something on

12:11

Venus?

12:12

>> Yeah. Well, more than once. Yeah.

12:13

They're the the Soviet Union is the only

12:15

nation you former Soviet Union now that

12:17

ever landed on Venus. And landing on

12:20

Venus is way hard.

12:22

>> They got crazy pictures, too.

12:23

>> The surface temperature is about a

12:24

thousand degrees and the air pressure is

12:27

similar to being about a mile below the

12:29

ocean.

12:30

>> That's a photo.

12:30

>> Yeah, it's a photo. Yep. That's real.

12:32

And it's a photo taken in a thousand

12:34

degree temperature.

12:35

>> Yes. Didn't last long. But uh um

12:39

everything is crushed flat. I mean the

12:41

the landscape is just crushed flat by

12:43

that you know huge pressure. Uh you know

12:46

this incredible dense atmosphere. The

12:48

clouds are sulfuric acid. That's why it

12:50

looks yellow. That's real. Uh you know

12:52

sulfuric acid clouds. I mean it is like

12:54

you know classic vision of hell. It it's

12:57

it's it's heavy and deep and uh and

12:59

dense and sulfuric acid. What's so

13:02

interesting too that our understanding

13:04

of planets in terms of like just what's

13:06

in our solar system, they're all

13:08

different. They vary so much and this is

13:10

just all we know about the known

13:12

universe in terms of planets. Is it

13:14

possible that there could be some

13:15

planets out there that are set up

13:17

completely different than the planets in

13:19

our solar system?

13:20

>> Oh, absolutely. Um, one of my favorite

13:22

websites, just for fun, I mean, so the

13:24

um, it changes every day how many

13:26

planets around other stars we know

13:27

about, we call them exoplanets, exterior

13:29

planets. Um, I think we're up to about

13:33

5,000 that we know of.

13:34

>> When did we start noticing them?

13:36

>> Um, so this was at least detecting them.

13:38

>> Yeah. Yeah. This is something I was been

13:40

involved with ever since I was in

13:41

college. When when I was in college, my

13:44

uh my research adviser was a man named

13:45

David Leam and he was trying to to find

13:48

the first evidence. I mean, we we

13:49

figured other stars have planets. I

13:51

mean, it can't be just us, but but

13:53

they're hard to see. They're tiny.

13:55

They're dark. I mean, compared to a

13:57

star, right? Right? I mean, planets

13:58

don't glow themselves, right? So, they

14:00

just reflect starlight. I mean, we we

14:02

literally said it was like trying to see

14:04

a firefly around a search light from 200

14:06

miles away, right? How would you do it?

14:08

And uh I mean, now we're actually

14:10

getting so good at it, we find more

14:12

every every week, almost every day. I

14:14

mean, pretty soon it's going to be I I

14:16

think thousands of new planets every

14:17

single year. And um and

14:20

>> do you have actual images? So, for the

14:22

most part, we don't have images, but

14:24

that doesn't mean we don't have really

14:25

cool uh uh observations, including the

14:28

chemistry of their atmospheres. This is

14:30

really amazing to me. So, they're so

14:32

tiny, it's hard to actually get a pixel.

14:34

They're smaller than a pixel. But when

14:36

these things pass in front of their

14:37

star, right? So, there's a star and they

14:39

they they pass in front of it. So,

14:41

you're looking at this thing pass in

14:43

front of the star, it makes a tiny

14:44

little solar eclipse. It goes by, it

14:45

blocks a little bit of the star light.

14:47

And we find them that way. We find the

14:49

stars twinkling as little planets go

14:51

around them again and again. They have

14:53

to come back three times for us to say

14:54

it's a planet. Otherwise, it could be a

14:56

spot on the star or something else. And

14:59

um the the amazing thing is that the

15:02

starlight will shine through the

15:03

atmosphere of that planet and we can

15:05

actually we can actually probe the

15:07

chemistry of the atmosphere. So we find

15:09

planets that have you know they're the

15:11

size of the earth about the temperature

15:12

of the earth. They have evidence of

15:14

water vapor, carbon dioxide, oxygen. And

15:17

then uh last year there was this

15:19

fantastic controversial discovery. I

15:21

mean it's it's very real. We need to

15:23

follow it up. Um we think we're starting

15:25

to see the evidence of organic

15:26

molecules. It's it's it's it's not, you

15:28

know, a very strong signal yet. And this

15:31

this this was this was a press release

15:32

from the James Webb Space Telescope. And

15:35

there were some scientists that wondered

15:37

if these could be organic molecules that

15:40

that that might someday be traceable

15:41

even to the presence of life. they they

15:43

they resembled something that plankton

15:45

might might give off on an ocean world.

15:48

And then of course I the rest of the

15:49

scientists said the data is not good

15:51

enough yet. We need much better

15:53

observations before you can say that.

15:55

You know, we could maybe believe it's an

15:56

organic carbon-based molecule, but we

15:58

don't know which one it is yet. So, you

16:00

know, I mean, stay tuned. I mean, I

16:02

would never have thought the first

16:04

evidence of life outside the Earth, like

16:07

a really hard chemical scientific

16:09

evidence, would be on a planet around

16:10

another star. I thought we maybe find on

16:12

Mars or on some of the moons of Jupiter

16:14

and Saturn. But now with the James Webb

16:16

Space Telescope and the telescopes that

16:17

will come afterwards, we might be able

16:20

to actually, you know, get get enough of

16:22

a sense of the atmosphere of these

16:23

planets to start looking for life

16:25

science. Yeah.

16:26

>> So the sun, the star is passing light

16:30

through this little tiny thing that's

16:32

smaller than a pixel and through the

16:34

atmosphere where the light passes

16:36

through. What are we using to detect

16:38

that? It's a technique called

16:39

spectroscopy and it's a really really

16:42

powerful thing. I This is what most

16:43

scientists do. As as beautiful as images

16:46

are of a gorgeous galaxy or a star.

16:51

That's not really what we do. We look at

16:52

these little squiggly lines. We get very

16:54

excited. We we let the light from the

16:57

star pass through um a grading that that

16:59

actually draws it into a rainbow. You

17:01

take takes that white light. You've seen

17:02

pictures of like prism, you know, dark

17:04

side of the moon, Pink Floyd. You know,

17:06

white light goes in, rainbow comes out.

17:08

If you measure really really carefully

17:10

how much light is coming in every color,

17:13

you can tell astounding things. You you

17:15

can tell how hot the star is, how fast

17:17

it's rotating, uh in some cases, how far

17:20

away a galaxy is. That's how we measure

17:22

how far away they are from us in space.

17:24

And you can measure the chemistry

17:26

molecule by molecule. You can tell

17:28

exactly what atoms and molecules are in

17:30

that object. Here we go. Look at that.

17:33

So what you're amazing person by the way

17:36

that that's incredible. Thank you so

17:38

much. Um

17:40

>> every every every element carbon,

17:42

nitrogen, oxygen has a fingerprint in

17:45

the rainbow and it's like you know it's

17:47

that there's nothing else like it. You

17:49

know that you see carbon and nitrogen if

17:51

you see these colors of the rainbow

17:52

shining at that particular light. And

17:55

it's not just simple things like carbon,

17:57

nitrogen, oxygen, but it's it's water

17:58

vapor, carbon dioxide, um organic

18:01

molecules. Everybody has their

18:02

fingerprint in the rainbow. And so when

18:05

when the starlight shines through the

18:07

atmosphere, there you go. That's how we

18:09

tell what these things are made of. You

18:10

know, this is a dying star. This is

18:12

actually in the Karina Nebula. And uh

18:14

the most the one of the most luminous

18:16

stars there is. And we we pass the light

18:18

through a rainbow. And then looking

18:20

really really carefully at how much

18:22

light comes at every color, you can pick

18:23

apart exactly what it's made of.

18:26

>> Wow.

18:26

>> Yeah. Did Did you know that you know

18:28

helium you know the element helium,

18:29

right? You you may be familiar that the

18:31

the Greek the Greek sun god's name is

18:33

helios. Helium is an element we

18:35

discovered on the sun before we ever

18:37

knew it was here in in in the the turn

18:39

of the last century in the late 1800s

18:41

when they were passing sunlight through

18:42

a prism and they were looking at all

18:44

these patterns of light. There was one

18:46

chemical that we'd never seen before

18:47

here. And so they named it after the

18:49

sun, helium. It was on the sun but not

18:51

here. We we never knew the helium was

18:53

here. That was found later. It was later

18:55

we found it, you know, in like, you

18:56

know, a natural gas, you know,

18:58

radioactive decay. Helium is such a

19:00

light gas. It just leaves the Earth. It

19:01

just doesn't stick around. And so, you

19:03

know, helium, we saw this this pattern

19:05

of colors in the sun's light. We were

19:07

like, what what the hell is that? And it

19:09

turned out to be a new element we'd

19:10

never found before.

19:11

>> What year was that?

19:12

>> We should look this up. I don't know

19:14

exactly, but if we Google what year was

19:16

helium found, um, I'm sure we can find

19:18

it. Well, I mean, I've been thinking

19:20

about helium balloons and people who,

19:22

you know, suck helium, make their voice

19:24

go really high.

19:25

>> We didn't even know about helium until

19:27

>> 1868. There we go.

19:29

>> That's nuts. So, they figured out that

19:32

there was helium in the sun in 1868.

19:36

>> Long before we ever identified it on

19:37

this planet.

19:39

>> That is so nuts.

19:41

>> Yeah. Just think what's out there. We

19:43

didn't even know about helium. It's not

19:45

just that it's what's out there, but

19:46

that there's people out there that can

19:48

figure out how to do that. In 1868,

19:51

shout out to Pierre Jeansen,

19:54

uh, a French astronomer who figured it

19:57

out.

19:58

>> When you when you think about, you know,

20:00

I know that one thing you you you love

20:01

is the idea of uh, you know, Einstein

20:03

and time being different and all that.

20:06

>> You know, they figured all of this out

20:08

around like like 1908. It was more than

20:10

a hundred years ago. And you know, we

20:12

don't really even have a better thing

20:14

yet. You know, I mean, they they they

20:16

figured out that time isn't the way that

20:18

we experience it just by really simple,

20:22

brilliant thought processes,

20:24

observations and some years ago, 100 a

20:26

little more than 120 years ago. Yeah.

20:28

Incredible.

20:30

>> The idea that the faster you go, the

20:32

slower time is is so hard to wrap one's

20:36

head around. And one of the things that

20:38

I heard you talking about, you were

20:39

talking about GPS satellites

20:41

>> and you were saying that GPS satellites

20:43

because they're going about what are

20:44

they going like 20,000 miles an hour or

20:46

something like that. So actually if we

20:48

want to break this down a little bit

20:49

there there are a couple different

20:50

effects about time and and one of the

20:53

things that that you know NASA does is

20:55

we you know calibrates the GPS

20:57

satellites and the signal coming and and

20:58

you wouldn't I mean I think I heard that

21:00

I mean within within a day if we didn't

21:03

take into account the time difference

21:05

these things are in that we we'd be

21:07

about six miles off I mean in a in a

21:09

single day.

21:09

>> That's crazy.

21:10

>> Oh yeah it's it's a big deal.

21:11

>> That's so crazy.

21:13

>> Yeah.

21:14

>> That's so crazy. And that's just above

21:17

us.

21:18

>> Time really is something. I mean, this

21:20

this is not a theory. Time time is is is

21:23

variable depending on how fast you're

21:24

going and also how far off the Earth's

21:26

surface you are or how I should say how

21:27

far away from a big gravity body you

21:29

are. In the case of the GPS satellites,

21:31

there's there's there's two things going

21:33

on. And it's it's it's kind of fun

21:35

because it's actually the reverse for

21:36

the astronauts. So, let's want to break

21:38

this down. This is really fun. Okay.

21:42

We have clocks that are so accurate that

21:44

if you move about two feet above where

21:47

you if we had a clock on this desk and

21:49

then if we moved it up about two feet,

21:51

we could actually detect time flowing

21:53

differently because you're just that far

21:55

away from the Earth's gravity. Just two

21:57

feet. Your head and the and your feet,

22:01

we spend most of our lives say standing

22:03

up are actually going through time at

22:05

slightly different rates. If the farther

22:07

away you are from a gravitational

22:09

source, I mean you you probably like

22:10

movies like Interstellar, right? With

22:12

with you know Matthew McConna,

22:13

>> remember the big black hole? And the

22:15

closer they get to the big black hole,

22:17

the slower time goes.

22:18

>> That's not a theory. That's something we

22:20

can actually measure with clocks. And a

22:22

black hole has so much gravity it does

22:24

it a lot more dramatically. But it's

22:26

happening right in this room. Seriously,

22:28

your head is in a different time frame

22:30

than your feet right now.

22:31

>> That's nuts.

22:32

>> Yeah. And you and I mean it's

22:33

measurable. you you you need extremely

22:36

accurate clocks. But in the case of the

22:39

GPS satellites, the GPS satellites are

22:41

in what we call a medium orbit. They're

22:42

not as far away as the geostationary

22:44

satellites, but they're they're not

22:46

actually going that fast. They're only

22:48

going about 9,000 m an hour around the

22:50

Earth. The the astronauts in the space

22:52

station, by the way, are going much

22:53

faster. They're they're going more like

22:55

let's say approximately 20,000 mph. So,

22:57

the GPS satellites are going a little

22:59

slower and and Yeah. Okay. 8,000 m an

23:01

hour is is a lot. And that does slow

23:03

your time down, but the bigger effect

23:05

for GPS satellites is how far away from

23:07

the Earth they are.

23:09

>> Wow.

23:09

>> We're actually going slower in time than

23:11

they are because we're closer to the

23:13

Earth's gravity. And they're so far

23:15

away, they're actually going a little

23:16

faster than we are in time. Now, they're

23:19

also slowed down by their fast velocity.

23:22

The the faster you go, the slower your

23:24

time goes. But people don't realize

23:26

there's another factor and that's how

23:28

far away you are from gravity. For the

23:30

astronauts, the astronauts are closer to

23:32

the Earth, right? So they're actually

23:33

not so far away as the satellites and

23:35

they're going much faster. So for the

23:37

astronauts, it's the it's the motion.

23:38

It's the time dilation from the motion

23:40

that's a bigger effect. Uh if you are on

23:42

the space station for a year, you come

23:44

back about 1/100th of a second younger

23:46

than you should be. And uh you know,

23:48

obviously that's not a big deal, but

23:50

it's easily measurable.

23:51

>> Wow.

23:52

>> And in the case of the satellites, you

23:54

wouldn't get the right location. The

23:55

data wouldn't be right unless we take

23:56

into account two things. How fast

23:58

they're going. The closer to the speed

24:00

of light you go, the slower time goes.

24:02

But also how far away from the

24:04

gravitational pull of the Earth they

24:05

are. The the closer you are into

24:07

gravity, the slower time goes.

24:09

>> I think the weirdest thing that I've

24:10

ever heard anybody say is that all time

24:12

exists currently.

24:15

>> That's Einstein. I mean, that goes back

24:17

that goes back 120 years.

24:19

>> That's such a bizarre thought. We don't

24:22

know if it's true but but it's I mean

24:24

Einstein really thought there wasn't

24:26

much of a way around it because he said

24:28

okay well if everything is going at

24:30

different velocities compared to

24:31

everything else right I mean it's a

24:33

great question a kid can ask how fast am

24:35

I going through space you know and the

24:38

earth you if you're on the equator of

24:40

the earth that goes around at about uh u

24:42

you know about about 1 th000 miles an

24:44

hour you know and then you know we go we

24:46

go around the sun at about 67,000 miles

24:48

an hour in our orbit the sun's going

24:50

around a galaxy about half a million

24:52

miles an hour around the galaxy. The

24:55

galaxy is going towards a galactic

24:56

cluster at more than a million miles an

24:58

hour.

25:00

But you know how fast are we going

25:02

really? And the the only thing you can

25:05

measure is how fast are you going

25:06

relative to something else? There's no

25:08

answer.

25:10

You know, how fast am I going? Well, I

25:12

mean, am I still or am I actually

25:13

traveling close to the speed of light

25:14

right now? I don't know. So, so Einstein

25:17

said the only way he could really think

25:18

about how that would work is if the

25:20

universe was just one big thing. You

25:23

know, all of time and space exists in a

25:25

big whole thing. There's only one now.

25:29

Einstein famously said, "The past,

25:31

present, and future are, you know,

25:33

persistently annoying illusions."

25:36

Now, again, do we know this to be true?

25:40

At the moment, we don't have any better

25:41

physics. And and I doubt the physics

25:43

will get any less weird than that.

25:46

But yeah, I mean I mean that's sort of

25:49

the way modern physics thinks the

25:50

universe may be is is a big whole thing

25:54

that started from beginning to end and

25:56

is all nowish.

25:58

>> But if that's the case, so subjectively

26:01

we can measure

26:04

things. We can measure time but but what

26:08

are we measuring

26:10

if it's I mean are are we making

26:12

artificial time constraints? Are we are

26:15

we doing it oursel? When we're when we

26:17

create a clock, we create a watch

26:19

>> and the watch is, you know, 24 hours a

26:21

day it's running. What is it what is it

26:24

measuring?

26:25

>> Yeah.

26:26

>> Right.

26:27

>> That is exactly the question Albert

26:29

Einstein asked. That that is that is a

26:31

deep excellent question.

26:34

And and so that was the problem. I mean

26:36

in a famous thought experiment, Einstein

26:38

made a clock by setting up two mirrors

26:40

and having light bounce between the two

26:41

mirrors. And that was the tick of the

26:43

clock. Tick tick tick tick tick. And and

26:46

the problem was that, you know, that's

26:47

how he started thinking about the speed

26:49

of light is that if you had this thing

26:50

in a spaceship that was going a huge

26:51

fraction of the speed of light, then a

26:53

person standing watching it go by would

26:55

actually watch the light kind of trace

26:57

out a pattern like this because you it's

26:59

it's it's actually ticking between the

27:00

mirrors, but the mirrors are moving

27:01

along. And so you see the light make

27:03

this sort of bouncy movement. And that

27:05

means it's actually traveled farther

27:08

than the person on the ground who thinks

27:09

that the mirrors are just sort of the

27:11

the light is making just a straight up

27:12

and down line from mirror to mirror.

27:14

That that question that you asked is

27:16

what completely

27:18

I mean it completely revolutionized

27:20

physics. Everything fell apart when

27:22

people said, "How do you even measure

27:24

time? What does it mean to make a clock?

27:27

What are we measuring?"

27:29

>> I still don't understand what we're

27:30

measuring.

27:31

>> Oh lord. Yeah.

27:32

>> I I get it. I mean we I don't know if I

27:35

have an answer for you. I don't think

27:36

anybody does. But but but here's the

27:38

deal. So the the clock in Einstein's

27:42

experiment, so the the clock has, you

27:45

know, two mirrors and there's light

27:46

bouncing between it and then that's the

27:48

distance that it travels in one tick,

27:49

>> right?

27:51

But now you put this mirror, you put

27:52

that clock on a spaceship and the

27:54

spaceship's going really fast. And as it

27:56

goes by, you see that that that clock as

27:58

as it streams by you really fast, you

28:00

see the light make this motion.

28:02

And and this line is actually longer

28:05

than that line. This this line if you

28:07

measure it, that's actually a longer

28:09

line that I drew than the the original

28:11

one between just the two mirrors because

28:12

now it's at an angle.

28:14

And this is what made Einstein say time

28:17

has to change. If anything moves, the

28:20

tick of a clock changes. What? However

28:22

you measure time, whatever time is,

28:24

whether you measure it with a bouncing

28:26

clock or whether you measure it with a

28:27

vibrating atom like we do in the Bureau

28:29

of Standards, or whether you measure

28:31

with a spring that's slowly unwinding in

28:33

a wristwatch.

28:36

Anything you can do to measure one

28:38

moment to the next changes when motion

28:40

is involved. There's no way to get

28:42

around it. It's not just the

28:44

measurement. It's time itself is

28:47

changing. any way we have to measure

28:49

this thing we call time. And I have to

28:52

tell you, Joe, I I don't think we have

28:54

an answer to what time is. What are we

28:57

measuring?

29:00

I think I think right there, I think

29:02

you're asking for the next revolution in

29:04

physics that we don't have yet. I really

29:06

mean that. So when we're measuring time

29:08

currently, like when I w look down on my

29:10

watch, I'm measuring time in this

29:14

particular space, like where I am, what

29:17

altitude I'm at, how fast I'm moving,

29:21

>> and the watch just does a reasonable job

29:23

of calculating all that.

29:25

>> And that's and that's you. I mean,

29:26

that's what you see here, sitting still

29:28

with your watch looking at it.

29:29

>> If someone's flying by at close to the

29:31

speed of light,

29:32

>> they won't see you measure time the same

29:34

way. Yeah. But you said something else

29:36

too that freaked me out that

29:39

that if you traveled at the speed of

29:41

light, the the problem would be you

29:43

would have infinite mass.

29:46

>> Well, anything with mass. Yeah. Yeah.

29:48

That's the thing.

29:48

>> So, if a person was in a spaceship and

29:51

it traveled the speed of light, that

29:52

spaceship would have infinite mass.

29:55

>> It's basically it's what makes

29:57

accelerating up to the speed of light

29:58

impossible. That anything with mass

30:01

can't travel at the speed of light. I

30:03

mean the the equations blow up. But what

30:04

does infinite mass mean? Do you have

30:06

more mass than the whole universe? What

30:07

the hell is that? As you approach the

30:10

speed of light, if you have mass, it

30:12

takes more and more energy to accelerate

30:14

you even just a little bit more. So you

30:15

never get to the speed of light. You

30:17

know, you're speed you're going 99.9%

30:19

the speed of light. Okay, I want to go a

30:21

little faster. It it takes more and more

30:23

energy each little tiny step you make.

30:25

So it's it basically you never get to

30:27

the speed of light. It it takes an

30:28

infinite amount of energy.

30:30

So, you know, when it comes to things

30:32

like interstellar travel, I I I don't

30:35

think we're ever going to take a

30:36

spaceship and accelerate it to the speed

30:38

of light, I I I mean, I we might get

30:41

very close. There are particles in space

30:43

that do have mass, like nutrinos, tiny

30:45

little bits of mass. They travel very

30:46

close to the speed of light, but they

30:47

don't travel at the speed of light.

30:50

But to me, you know, I I think that the

30:53

the the idea of traveling interstellar

30:56

distances or even intergalactic

30:57

distances, you know, the thing that

30:59

starts to really get me is the question

31:00

of this this what is space and what is

31:02

time at all? Quantum entanglement,

31:04

>> right? Glad you brought that up.

31:05

>> Oh, yeah.

31:07

Uh I I I'm going to say I I hope your

31:10

listeners I I I I don't want to get I

31:12

don't want to I I want people to come

31:13

along with us.

31:14

>> Oh, they're coming along.

31:16

>> Yeah. I I don't want to say things that

31:17

sound so stupid. They're like, you know,

31:18

why are they saying this? So, please

31:20

stop me if we need some more background.

31:21

>> This does not sound stupid in any way,

31:23

shape, or form,

31:24

>> but the idea of quantum entanglement, we

31:26

should explain that to people.

31:28

>> Yeah.

31:28

>> And what it essentially means is that

31:31

things are entangled, they're connected

31:33

at regardless of the distance.

31:35

>> Yes.

31:35

>> And it could be an immeasurable amount

31:38

of distance like

31:39

>> any distance

31:39

>> like

31:40

>> Yeah. Literally the beginning of the

31:43

universe distance like 13.8 8 billion

31:46

life years away distance.

31:48

>> You're entangled with that.

31:50

>> It's amazing because once again, let's

31:52

go back to the idea that this this is a

31:54

real experimental fact, right? I mean, a

31:57

lot of times this this crazy stuff that,

31:59

you know, scientists will will say this

32:01

stuff and and people hear it, you know,

32:03

for the first time and they say, "Well,

32:04

that that sounds like idiotic. That

32:05

sounds stupid. Why where did they get

32:07

that from?" And the the idea that time

32:12

changes is now it's one of the most

32:15

commonly proven facts every day. Like I

32:17

said, we needed to calibrate the GPS

32:18

satellites. It's easy to measure.

32:21

Quantum entanglement was something that

32:23

that even Albert Einstein 100 years ago

32:26

um he understood that quantum mechanics

32:28

was pointing that way, but he really

32:29

didn't like it. He called it he called

32:31

it spooky action at a distance. He hated

32:33

it because he realized that quantum

32:35

mechan mechanics had this implication

32:37

that that if things could somehow be

32:39

connected quantum mechanically, you

32:41

could take them any distance away from

32:43

each other and they would somehow be

32:44

able to respond to each other

32:46

instantaneously with with no time

32:48

difference.

32:49

And you know, he didn't think that would

32:51

ever actually happen. And then back in

32:52

the in the in the mid 1990s, we started

32:54

to do experiments with atoms and we

32:57

found out that it was real. That uh uh

33:00

it it can start off pretty simply. you

33:02

you have two atoms that are in an orbit

33:04

around you know so an atom has a nucleus

33:07

of protons and electrons in the middle

33:09

sorry an atom has a nucleus of protons

33:12

and neutrons the electrons are flying

33:14

around in orbits around the uh the atom

33:17

um two electrons can be in the same

33:19

orbit only if they are spinning in

33:21

different directions they they have an

33:22

an angular momentum it's called spin and

33:25

the only way these two electrons can fit

33:26

in that orbit together is if they're

33:28

spinning one is spinning in an upward

33:29

direction one's say spinning in in a

33:31

downward ction. Hate the broken finger.

33:34

Um, so if if you take these electrons

33:36

out of the atom and you can do that, you

33:39

know that they're in different spins

33:41

because they had to be to be in that

33:42

that orbit together. So now you separate

33:44

them. You can separate them by any

33:46

distance you want. You can separate them

33:47

by centimeters in a laboratory. The

33:50

Chinese have done this up to the space

33:51

station that they run in back. You you

33:53

could conceivably do it to another

33:55

galaxy. If you take those electrons and

33:57

you separate them, you know that they

33:59

were spinning in opposite directions. So

34:01

if you take an electric field and you

34:02

change the spin of one, the other one

34:05

immediately changes in response

34:07

>> regardless of the distance.

34:08

>> Regardless of the distance and we know

34:10

this to be true. We've done this. And

34:14

the amazing thing is the universe is

34:16

saying these two things are the same

34:19

quantum mechanical system. They're

34:21

basically the same object. They're

34:22

connected to each other. They're

34:23

entangled together. And it doesn't

34:26

matter. Space and time don't matter. You

34:29

can you separate them in space any

34:32

distance you want. How does that work?

34:35

The universe says the space and time

34:36

between them doesn't matter. They're the

34:38

same system.

34:41

To me, that's the real intriguing thing

34:43

about you. Could a civilization learn

34:45

how to harness that, you know, you're

34:48

not really even having to worry about

34:49

traveling from one part to another. Have

34:51

did you watch the um uh the threebody

34:53

problem show? Yeah. So, so you have

34:55

these things called sons, right? and

34:57

sofans are entangled to this alien

34:59

civilization and they can respond

35:02

instantaneously because they're

35:03

entangled. Yes. I mean I mean that's

35:06

fantastic science and as far as I can

35:07

tell that that could be theoretically

35:10

possible. Yeah.

35:11

>> Well, that's what's bonkers is that we

35:14

are made out of all this stuff that's

35:16

entangled.

35:17

>> What's it entangled to? Is it entangled

35:18

to stuff inside a black hole right now?

35:20

Is it entangled to stuff that is on the

35:22

other side of the universe from us? If

35:24

the big bang had all of this stuff in a

35:26

small volume at once, are we entangled

35:28

to everything in some way?

35:33

>> Seriously.

35:34

>> Seriously.

35:34

>> I mean I mean are is a part of me

35:36

quantum mechanically right now in the

35:38

Andromeda galaxy? Yeah, actually that

35:41

would be the implication.

35:43

I mean talk about

35:46

I don't think we understand yet what

35:47

reality is. I really don't. What does it

35:51

mean? Are we all somehow the same

35:53

particle entangled to each other? You

35:56

know, are we connected to everything

35:59

all at once?

36:01

I mean, that could be where physics is

36:04

taking us now.

36:05

>> That's bananas. It's very difficult to

36:08

think about when you you think you're a

36:11

person in Austin. My feet are on the

36:13

ground. Yeah.

36:13

>> Here I am touching this desk. I'm going

36:15

to get in my car later and go get

36:17

something to eat.

36:17

>> No kidding. You got to feed the cat,

36:19

right?

36:19

>> Yeah. But that's not really what's going

36:20

on.

36:22

It's way more complex, way bigger. And

36:24

you were speculating that that could be

36:27

how some advanced, super advanced

36:30

intelligent life form travels.

36:33

>> It's always been more compelling to me

36:35

than the idea of taking a spaceship and

36:37

traveling somewhere.

36:38

>> That seems super crude.

36:39

>> Yeah.

36:40

>> That seems like the idea of making a

36:42

horse fly.

36:43

>> Yeah. Yeah. I I you know we we we talked

36:46

about that movie Interstellar because

36:48

there were a lot of good teaching

36:49

moments in that movie for for a

36:51

physicist. You know the idea that time

36:52

really does slow down close to a black

36:54

hole. And again we we observe this when

36:56

we observe things orbiting close to a

36:58

black hole. You can tell that that

36:59

happens and the idea that this advanced

37:02

civilization that we never actually see

37:04

in the movie somehow communicates

37:05

through basically space and time itself

37:08

through gravity. Um, you know, that's

37:10

how Matthew McConna is able to even like

37:12

go back, you know, in time and space to

37:14

help his daughter solve, you know,

37:16

gravity and all that. You know, I was

37:18

like I was like, I wonder I wonder if

37:20

that's really more what it be like, you

37:22

know, advanced civilizations.

37:24

I mean, you got to think, right? I mean,

37:26

you look around the earth and there are,

37:28

you know, things like grasshoppers and

37:29

hamsters that are fantastic, incredibly

37:32

complex beings, but I mean, you try to

37:34

teach them quantum mechanics or ask them

37:35

to, you know, crochet a blanket or

37:37

whatever. They they don't have the

37:38

capacity. And you you've got to think

37:40

that there's the similar jump where I

37:43

mean, we don't even know the right

37:44

questions to ask that sort of a

37:46

civilization,

37:47

>> you know? I mean, can they see the

37:49

universe as a whole thing? Do they know

37:51

that they're connected to everything?

37:53

And can they somehow use that to travel?

37:56

You know, maybe.

37:57

>> Maybe. And if you just extrapolate, if

37:59

you just think about where we've gone

38:02

from primitive man to what we're

38:04

currently experiencing, and you take

38:06

that thousands of years, millions of

38:09

years, whatever it is,

38:10

>> yeah,

38:10

>> you you keep going. And as long as

38:13

civilization

38:15

gets rid of war and figures out a way to

38:17

not die of disease and natural disaster,

38:19

you could potentially continue this

38:22

process of technological innovation for

38:25

millions of years. And you would imagine

38:26

that it would go exponentially

38:29

greater and greater in its ability to do

38:31

things.

38:32

>> Yeah. and its ability to

38:34

not just

38:37

not even things that we can imagine like

38:41

we have a crude understanding amazing

38:44

understanding of the universe but crude

38:47

in comparison

38:48

to what's potentially out there. Well,

38:51

we could pot we could potentially be

38:54

observing

38:55

in a physical way every planet on every

38:58

star one day.

39:01

But we're not we can't even think of

39:03

that as being a possibility now. But but

39:06

what we're doing right now is insane to

39:09

people that lived in the 1400s.

39:10

>> Yeah.

39:12

If

39:12

>> you showed someone from the 1400s a

39:14

nuclear power plant, they'd be like,

39:16

"What the are you guys doing?"

39:18

Like, "What is this?" See, if you showed

39:19

them a nuclear detonate, if you showed

39:21

them FaceTime on a phone, they'd be

39:23

like, "This is insanity."

39:25

>> I just got on a little metal tube and

39:26

came here from Milwaukee and I'll fly

39:27

back tonight. Yeah. Yeah. Absolutely.

39:30

>> And we're just accustomed to it. It it

39:32

it becomes normal. And it would become

39:33

normal as technology increased further

39:36

and further and further. And this idea

39:38

that the entire universe would be

39:41

accessible is just bananas. Have you

39:44

ever wondered if maybe the real followon

39:47

to humanity someday will be some form of

39:49

AI?

39:50

>> I think so.

39:51

>> I mean, yeah. I I mean, I do wonder if

39:53

the human brain is just kind of limited.

39:55

I mean, if you if you say there are

39:56

multiple dimensions and time is

39:58

something that changes. I mean, I just

40:00

said that, you know, I mean, scientists

40:02

are no better than anybody else at

40:04

comprehending a big number or a big

40:05

amount of space. We just kind of get

40:07

used to it, you You know, I mean, I

40:08

mean, will we have a creature someday

40:10

that we've created, an AI that then all

40:13

of a sudden can comprehend these things,

40:16

you know, is is is that really the real

40:18

evolutionary path of humanity?

40:20

>> Yeah, I think so. I think it's just a

40:23

completely different kind of life and

40:24

that we're thinking of it as artificial.

40:27

I don't think it's artificial at all. I

40:29

think it's a life. It's a just a

40:31

different kind of life that we're

40:32

>> It's an earthling. I mean, I mean,

40:33

seriously, it's our children. We we

40:35

created this.

40:36

>> Yeah. I always describe ourselves as

40:38

like we're an electronic caterpillar and

40:41

we're making a cocoon. We don't even

40:43

know why we're doing it because it's

40:44

just what we do. I mean, the thing about

40:46

human beings is we've always been

40:48

completely fascinated with innovation.

40:51

I've always said that if you looked at

40:52

us objectively for some like what does

40:54

this species do? Oh, they make better

40:56

things. They keep making better things.

40:58

They're never satisfied with the things.

41:00

Bees made the beehive and like I think

41:01

we got it, boys. This is it.

41:04

we're not satisfied at all. And so if

41:07

you just kept going with that, like

41:08

where does it go? Well, it has to go to

41:10

life. It has to go to some sort of a

41:13

human created new kind of life form that

41:16

exists out of the components of the

41:18

earth, but instead of being born out of

41:21

evolution and out of, you know, natural

41:23

mutation and natural selection, it's

41:25

random mutation. It's made out of us. We

41:28

made it and it'll probably make better

41:31

versions of it. And that would be the

41:33

new life. And that's how you get over

41:35

all the biological hurdles that we have.

41:37

You think about like the things that

41:38

trouble us, war and crime and violence

41:41

and all these different things that are

41:43

a real problem with the human race.

41:44

Well, that all goes away when you stop

41:46

being human.

41:48

And if we really are entangled with

41:51

everything, we that will be us.

41:54

It'll just be us in a completely

41:56

different realm.

41:57

>> Yeah. I I I mean I I do like this idea

41:59

that what we call AIs now isn't

42:02

something separate. I mean they are our

42:03

children. It is an Earthling. It is

42:05

something we've created.

42:07

The the question I've often wondered is,

42:09

you know, sometimes I think sometimes we

42:12

lack imagination about what might be

42:14

possible. I've always enjoyed science

42:15

fiction where the AI also learn about

42:20

about love or about the arts or about

42:22

creativity. I mean whether you want to

42:24

go with like the new battlest star

42:25

galactica or whether you want to go with

42:27

um uh a pretty profound experience I had

42:30

with a friend of mine who's an author

42:31

who has colear implants and you know he

42:34

realizes that he doesn't hear like a

42:36

human you he mean the colear implants

42:39

don't replicate perfectly what it means

42:41

to hear the way our ears do they bypass

42:44

our ears they they wire directly into

42:46

his brain and stimulate the experience

42:48

of sound

42:50

and so he's hearing in his words like a

42:52

cyborg

42:53

This is Michael Chorus, a wonderful man

42:55

that did some essays about this. And and

42:58

he he talked about how much um emotional

43:00

response he has to music now, something

43:02

he could never experience. How being a a

43:05

cyborg, quote unquote, you know, and

43:07

experiencing something in a non-human

43:09

way has added joy and depth and and

43:13

passion,

43:15

you know? Are are we so sure that

43:18

technology makes us more and more, you

43:20

know, kind of 1950s robot-like, or could

43:23

it take us into new experiences of being

43:24

connected with each other, you know, new

43:26

ways of loving each other, new ways of

43:28

understanding things? I mean, I mean,

43:30

does it have to be all bad? This

43:32

>> Well, all of our differences fall apart

43:34

if we realize we're all one thing.

43:36

>> Yeah.

43:36

>> If we realize we're all one thing, then

43:39

all of our

43:41

monopoly of resources, all that, all

43:43

that stuff goes away. If we realize

43:45

we're all one thing. I mean, part of the

43:46

problem with human beings is we're very

43:48

selfish.

43:49

>> And the reason why we're very selfish is

43:51

because that's how you had to survive.

43:52

If you wanted your genes to if you

43:54

wanted to to survive and you wanted your

43:56

genes to be passed on to the next

43:58

generation, you had to be selfish

43:59

because other people were being selfish

44:01

too. And that's the game the humans were

44:02

playing. If we get to a point of

44:04

universal telepathy,

44:07

like universal telepathy with a

44:08

universal language where all human

44:10

beings are sharing thoughts, there are

44:12

no secrets. We are all one thing.

44:14

Everyone's terrified of that. People

44:16

love secrets. Love I don't want people

44:18

listening to my phone. I don't want

44:19

people Well, I don't I don't either

44:21

because it would be people doing that

44:23

and those people have their own ulterior

44:24

motives and it's gross that they would

44:26

have control. They'd know your emails.

44:29

But what if there's no secrets? It's not

44:32

possible because our understanding of

44:34

each other is now complete.

44:36

>> Mhm.

44:37

>> It's like we read each other's minds in

44:40

a sense, but it's much more complex than

44:42

that. and much more much more in depth

44:45

like you feel what that person feels.

44:48

You are that person and we're all one

44:50

thing that that could be possible

44:54

through technology. And this is this is

44:56

where I have hope where a lot of people

44:59

are like very fatalist with AI and you

45:01

know they look at it in this dystopian

45:03

sense of these oligarchs these technical

45:05

oligarch technology oligarchs going to

45:07

be controlling off through AI and

45:09

they're going to have access to it and

45:10

power. I don't know if anybody's gonna

45:13

control it. And I have a feeling it's

45:15

going to be kind of like the internet in

45:17

a way where I don't think they really

45:18

thought what the internet was going to

45:19

be. I think they had this understanding

45:21

of being able to exchange information

45:23

through universities and I think it got

45:26

to a point where I if they knew what the

45:29

internet would be today and how little

45:31

control they would have over the

45:32

population and narratives and I think

45:34

they probably would have shut it down a

45:35

long time ago. I have a feeling that's

45:37

going to be the same way with AI and

45:40

especially AI as it integrates with us,

45:44

which I think is the only way that the

45:46

human species really truly survives.

45:49

Otherwise, we're just this archaic

45:51

biological entity living in this new

45:55

world of this ultra superior life form.

45:58

But if we integrate with that thing

46:01

through wearables, implants,

46:05

engineering, if we figure out a way, and

46:08

this is going to sound terrible to

46:10

anybody who loves being a person, but

46:12

all the flaws of being a primate,

46:15

there's a lot of these biological reward

46:17

systems that are built into us that are

46:19

really problematic for progress. I mean,

46:21

the reason why are we at war right now?

46:23

Well, because there's people with

46:25

certain ideologies and there's resources

46:27

and there's people that are making money

46:29

from their military contractors and

46:32

there's politicians that are beholden to

46:33

certain interests and then what are we

46:35

doing? We're doing the same stupid

46:36

that we've been doing for thousands and

46:37

thousands of years. Well, how do we get

46:38

past that? We get past that by stop

46:40

being people.

46:42

>> I think you may be right. I mean, again,

46:44

that that future is is it is frightening

46:47

in some ways, but I I'm I'm I'm more

46:49

interested in the imagination. I mean,

46:51

instead of just the dystopia, what could

46:53

this mean,

46:53

>> right?

46:54

>> You know, I mean, I mean, how much more,

46:56

like we said, I mean, when we were

46:57

little tribal groups, you know, the

46:59

little wars we had, the skirmishes

47:01

didn't really hurt the planet as a

47:02

whole. I mean, now we're getting there

47:04

so many people and we're still having

47:06

these little tribal skirmishes and and

47:07

now we're in danger of of, you know,

47:09

massive destruction. I mean, we can't

47:12

just keep going this way. I mean, it's

47:14

it's it's not it's not survivable.

47:15

>> It's not. So I mean you know could AI

47:18

help us you know tap into some kind of

47:19

group consciousness. I mean when we we

47:22

were talking about Einstein's idea that

47:24

the universe may all be this one big

47:25

thing you and this is pure metaphysics

47:28

pure conjecture but you know even when I

47:30

was a little kid and I heard that I

47:31

wondered well you know if all time and

47:33

space happens at once is there need for

47:35

more than one consciousness even are we

47:37

all are we all just looking out of you

47:39

know one consciousness looking out of

47:40

out of everybody's eyes simultaneously

47:43

and not just humans but everything in

47:45

the universe you know it's it's a

47:47

spectacular idea that you know If there

47:50

is a moment, if the universe is just one

47:52

big thing, you know, we are part now,

47:56

even now, of

47:58

beings we have no names for, you know,

48:01

super advanced beings that have figured

48:03

all of this out and can span the

48:05

universe with their consciousness, you

48:07

know, that's part of the eyes, too.

48:09

That's another part of this

48:10

consciousness that we're part of right

48:11

now. If if if there's one instant,

48:15

you know, it it reminds me of some of

48:16

the tenants of, you know, of Buddhism.

48:19

There there might be these perfectly

48:20

enlightened beings, bodhisattvas, and we

48:22

are past lives of them. We're all

48:23

existing at once.

48:26

You know, it's a it's a fantastically

48:27

beautiful idea.

48:28

>> It is a beautiful idea. And our survival

48:31

instincts are attuned to maintaining

48:35

what we are. There there's this thing,

48:37

well, I don't want to lose being a

48:38

person. But I guarantee you if you went

48:40

to an australythecus

48:42

and you could somehow communicate to

48:44

them, listen, you're going to change and

48:46

you're going to be this thing that gets

48:48

sick seven times a year and maybe you're

48:50

obese and maybe you have a problem with

48:52

cigarettes and you know, maybe you drink

48:54

too much and you like to gamble and

48:55

you're going to your life up here

48:57

and there, but you're going to have a

48:58

cell phone and you're going to live in a

49:01

city and you're going to be breathing

49:02

break dust every day and you, you know,

49:04

your doctor's going to give you a bunch

49:05

of stuff you don't really need because

49:06

he's trying to make money.

49:08

The Australians are probably like, "Fuck

49:10

that.

49:12

I know what I'm doing here. Sounds much

49:14

better."

49:15

>> Yeah. I I know where the food is. Like,

49:17

get out of here. I don't want any part

49:19

of that. And I think that's just part of

49:22

survival instincts. Survival instincts

49:24

don't want you to radically change into

49:26

something completely different with its

49:27

own new set of problems.

49:29

>> You you want to stay. You want to

49:31

maintain. You know, country boy can't

49:33

survive. Keep me in the woods. You know

49:34

what I mean?

49:36

people have this like natural

49:37

inclination to keep things simple cuz

49:39

they understand them.

49:40

>> But I think that's not possible anymore.

49:43

And I think we're going to just have to

49:45

let it go. Just let that idea go and

49:48

relax and uh accept whatever this new

49:51

thing is. And I think we're very very

49:54

fortunate to be born at this time while

49:56

we're experiencing it as regardless of

49:59

the outcome. This is a very unique time.

50:02

like one of the weirdest times I think

50:05

objectively in human history

50:07

>> and we're very fortunate to be

50:08

experiencing it.

50:09

>> I mean you and I are are roughly the

50:11

same age and you know I I I think that I

50:13

mean for for me having this what they

50:14

now kind of you know call the fearal

50:16

childhood right where I was unplugged

50:18

and and there were you know there were

50:19

there were vast stretches of time even

50:21

as a small child where I was on my own

50:23

you know in the neighborhood stuff and

50:24

and I loved it. I mean, I remember going

50:26

to, you know, a YMCA camp when I was 11

50:28

years old and, you know, everybody had

50:30

to show up at breakfast and then there

50:31

was an activity time and everybody had

50:33

to show up at lunch. But what you did

50:34

between that time, you were on your own.

50:36

I mean, as an 11-year-old kid, you know,

50:38

in the woods, there were activities, you

50:39

could do some archery, there was a

50:41

rifle, there was craft shop, there was

50:42

swimming, and you had to check in at

50:44

certain times. But sometimes I just went

50:46

and sat in the woods, you know, 11 years

50:48

old. I mean, can you imagine?

50:49

>> I had this similar experience in the Boy

50:51

Scouts.

50:51

>> Yeah. Yeah. And you know the thing was

50:53

you know so so you and I had this

50:55

experience of living unplugged and and

50:58

sort of the the idea of of of a quiet

51:01

mind and imagination

51:04

and but we also saw this tremendous

51:06

change and this connectivity which I

51:08

love. I mean I also love having the

51:10

internet and this my cell phones and all

51:11

of that but but but this is a real

51:14

change in human civilization that we

51:16

went through personally

51:18

and I agree with you. I I feel a

51:20

tremendous sense of gratitude for for

51:22

both ends of my life.

51:23

>> Right. We could have been born in the

51:24

1500s were the 1500s to the 1600s.

51:28

>> Not that much changed. I mean

51:30

>> for a lot of people. Yeah.

51:31

>> Sure. I mean politically things changed,

51:33

leaders got overthrown, but as far as

51:35

like the way you interfaced with the the

51:37

world

51:38

>> pretty much the same way. You wrote

51:40

stuff down with feathers.

51:43

>> Yeah.

51:44

you know, and and gratitude and like you

51:46

said, I mean, maybe instead of all the

51:48

dystopia and all the worry and all the

51:50

panic right now, you know, going forward

51:51

with gratitude.

51:53

>> Yeah. Well, I think the unknown gives

51:55

people a tremendous amount of anxiety.

51:57

>> Sure.

51:57

>> For a good reason, you know, I mean, the

51:59

unknown could potentially be dangerous

52:01

and scary and terrifying or awesome and

52:03

you really don't know and so you're

52:05

like, what is it going to be? And

52:07

there's all these college kids that are

52:08

really freaking out because they're

52:11

they're went into debt. They're getting

52:13

these co college degrees. They're

52:15

leaving with this burden, this financial

52:17

burden that they can never get rid of.

52:19

And on top of that, they have a degree

52:21

that might not be worth anything because

52:23

AI might completely eradicate their

52:25

field. That's a real concern. And so

52:28

they they I think kids today that are

52:30

graduating from college and graduating

52:32

from high school, they probably have the

52:34

most amount of anxiety about the future.

52:36

That and then there's people that, you

52:38

know, they haven't saved any money up.

52:40

They don't even know if money is going

52:41

to be valuable in the future. Like what

52:43

does it even mean? Are are we gonna

52:45

abandon all money? Like what what is

52:47

what is it going to mean when AI

52:49

completely controls all of the

52:50

resources, all of the government, all of

52:52

everything, all transportation, and you

52:55

don't have to do your job anymore? You

52:56

just get some funds from the government

52:59

where you can buy food. Like this is

53:01

what people are talking about. Like this

53:02

is a potential, you know, 100 years from

53:05

now future.

53:06

>> Very seriously so. Yes. Absolutely.

53:08

which is terrifying to people that are

53:10

thinking, hey, you know, I want to do

53:12

what my dad did and what my mom did and

53:15

I want to go out there in the world and

53:17

I want to find something that I'm

53:19

passionate about and make it a career

53:21

and like maybe that's not possible. That

53:24

to kids right now, I think is really

53:27

freaking them out because the adults,

53:29

the people like us that are supposed to

53:31

be the ones that say, "Well, let me tell

53:32

you how it all works. You're going to be

53:34

fine. This is what you have to do." And

53:35

if you do that and just cross your eyes

53:37

and dot your tees, you're going to be

53:39

okay, Bob. But maybe you're not going to

53:40

be okay. Like maybe we don't know

53:43

because that's the reality. The reality

53:44

is you and I, the adults, have no idea

53:47

what this world's going to look like in

53:48

50 years. And these poor kids are they

53:51

have no one to turn to. There's no one

53:53

that can explain what this and so

53:55

they're entering out into the world

53:57

having to take care of themselves for

53:58

the very first time with this real

54:00

possibility that there might not be any

54:02

jobs.

54:05

On the on the flip side of that, are you

54:07

in fact describing the Star Trek

54:09

universe, right? You know, a time where

54:11

people do not work for everybody has,

54:13

you know, anything they need as far as,

54:15

you know, apparently survivability, you

54:17

know, food, whatever. You know, and now

54:19

you have a chance to say, am I going to

54:20

be a writer or an explorer or an artist

54:22

or a captain or a musician?

54:24

>> Yes.

54:24

>> You know, I mean, does it does it I mean

54:26

I mean I mean is there something in that

54:28

that might be hugely liberating?

54:30

>> 100%. And I've talked about this as well

54:32

that this idea that you have to toil and

54:35

you have to be a hunter gatherer or you

54:37

know some that you have to do this in

54:39

order to find meaning in life is kind of

54:40

crazy because we could find meaning a

54:42

lot of ways. There's very wealthy people

54:45

that never have to work that have

54:46

tremendous meaning in their life because

54:48

they're doing things all the time

54:49

without thinking about work at all.

54:51

They're not thinking about it as work.

54:52

whatever hobbies they're pursuing or

54:54

interests or education they're pursuing,

54:57

they're doing it just out of pure

54:58

interest and fascination and love and

55:00

passion. And that could be all of us.

55:04

But there's going to be a tremendous

55:06

transition period where people are going

55:08

to have to rethink what it means to be a

55:11

human being in society. And that's

55:14

what's weird because our entire society

55:16

is structured out of getting up in the

55:18

morning, putting in the work, working

55:20

towards a future. You got a 401k, you

55:23

got investments, you got this, you got

55:24

that, you got a mortgage. And this is

55:26

how we've structured our entire

55:29

existence and what we what meaning we

55:32

gather from life. It's based on that.

55:35

We're going to have to figure out a way

55:37

to realize and to rethink this. And it's

55:40

going to be very difficult for people

55:41

that are like 40 and 50 that are just

55:44

completely set in their ways and now

55:47

their ways change. And I don't know how

55:49

many of them are going to be able to

55:50

make that switch and what could be done

55:53

to assist them in that what can be done.

55:56

And maybe that that comes with whatever

55:58

this technological interface is. Maybe

56:00

that comes with when we become what's

56:03

essentially a cyborg that you get a a

56:06

much greater understanding of what it

56:08

means to exist. And that this idea that

56:10

you exist only because the insurance

56:12

company you work for is kind of

56:14

ridiculous. And we abandon that. I mean

56:17

the in the way that now when you open up

56:19

your phone and you use perplexity, you

56:22

have access to uh

56:25

something that's as smart as every human

56:27

being on earth in every field. You can

56:30

ask it about anything and it'll give you

56:33

the state-of-the-art and whatever the

56:35

science is, whatever the the

56:37

understanding of history, whatever

56:39

mathematics,

56:40

tax law, whatever it is, it can give it

56:43

to you on your phone instantaneously.

56:46

And we've just sort of accepted that.

56:48

This is our new thing. And I think this

56:50

is like a baby step into what it's going

56:52

to what this technology could

56:55

potentially if you're looking at things

56:56

with a glass half full. It could

56:59

potentially change the way we look at

57:01

everything, the way we look at

57:03

ourselves, the way we look at what it

57:04

means to be a person and what we find

57:06

meaning out of. And this because that's

57:09

the problem. The problem is meaning and

57:10

the the the feeling like you matter,

57:12

feeling like you're important. And I

57:14

think part of that is because we're all

57:15

so isolated from each other. But that

57:17

might go away entirely if the boundaries

57:21

between all thought and consciousness.

57:23

If we realize like, oh, consciousness is

57:25

just a thing that we're all enveloped in

57:28

and what our brain is is just a antenna.

57:31

It's like tuning into consciousness. And

57:33

the depending on how good your antenna

57:35

is, you're going to be a little bit

57:36

better about how you interface with the

57:39

world and whatever thing you desire and

57:41

whatever thing you decide to put your

57:43

energy and attention to, you maybe

57:45

you'll be better at it than another

57:46

person because you have a better

57:47

antenna. But we might understand that

57:49

like we are really truly all one thing.

57:52

So all our fears about

57:56

you know finding your place in the world

57:58

that might be nonsense.

58:00

>> I really like that idea. I like the idea

58:02

of search for meaning and I agree with

58:04

you. I think that as as like you said as

58:06

you know Australopythecus as people that

58:07

used to exist in these little tribal

58:09

groups and families

58:11

um the the the modern isolated life. I

58:14

mean it's something that I struggle with

58:16

a lot. You know I I I'm always wondering

58:18

you know where is my family? Where are

58:20

my friends?

58:20

>> Right?

58:21

>> You know I I've had to to do a lot of

58:23

sort of interior work about you know I'm

58:25

just going to bring along my own

58:27

>> family inside somehow. you know, I I had

58:30

to provide this all for myself. The idea

58:32

of being of being less alone, being less

58:35

isolated.

58:36

That's one thing that I wanted from the

58:38

internet. You know, it started out on

58:40

Facebook. I could I could keep up with

58:41

my friends, you know, I I saw what they

58:43

were doing. They were posting pictures

58:44

of their life. It was it was less

58:45

isolating. And then now it's evolved to

58:48

I can't even find them on Facebook

58:49

anymore. It's all, you know, all all the

58:51

ads and everything like that. But but

58:53

but but I mean, for me, I mean, you you

58:55

talk about meaning and you talk about

58:57

solving isolation.

59:00

Tell me tell me more about that. I I

59:02

mean the the the how has your sense of

59:04

meaning in your life evolved? How has it

59:06

changed over your life? How how do you

59:08

find meaning?

59:10

>> I find meaning in what? Well, there's a

59:12

bunch of things, right? First of all,

59:14

it's the people that are in your life.

59:16

This is a a giant factor because without

59:19

people that you love and people that you

59:21

enjoy spending time with, life loses all

59:24

of its value. If you're an insanely

59:26

wealthy, insanely successful person who

59:29

has no friends, who lives alone, you're

59:31

living in hell. And if you are a poor

59:33

person that has amazing friends and

59:35

you're just getting by, you are a

59:36

happier person. But I guarantee that

59:39

poor person would switch places with

59:40

that rich person in a heartbeat because

59:43

we're programmed to think that success

59:45

is numbers. That success is what you can

59:49

what you can accumulate as far as like

59:51

objects and desired material

59:53

possessions.

59:55

But it's not. It's like true success is

59:57

happiness and the the amount of joy that

60:01

you get out of life and the amount of

60:02

satisfaction you get in what you do. So

60:04

I think for everybody that answer is a

60:07

different answer because for some people

60:08

it's going to be music. For some people

60:10

it's going to be lit. They're going to

60:11

write they're going to there's going to

60:12

be a thing that you enjoy putting

60:14

yourself into that you feel satisfaction

60:17

and you feel meaning on top of friends

60:20

and family. So friends and family I

60:22

think is foremost, but then they can get

60:26

in the way too if they don't have their

60:27

together. So like they have to have

60:29

a thing that they're enjoying as well.

60:32

They have to have a thing that's helping

60:33

them grow as an individual. And there's

60:36

a thing from martial arts. My instructor

60:38

told me that when I was very young that

60:39

I never forgot that was martial arts is

60:41

a vehicle for developing your human

60:43

potential. And that if you find things

60:46

that test you and you find things that

60:48

are complex and these puzzles that you

60:50

have to solve, the more you do that, the

60:52

more you get of an understanding of who

60:53

you are and what you can do and what you

60:55

can do out there in the world. And the

60:56

more you do it, the more you can do

60:58

other things. And I think that's where I

61:01

find meaning. I find meaning in doing

61:03

things and enjoying time with my family,

61:06

enjoying time with my friends, having

61:08

joy and fun and laughter and then also

61:13

difficult pursuits. I like things that

61:16

are complex, the things that are hard to

61:18

solve. I like things that are hard to do

61:20

where I I really have to force myself to

61:23

do it and then I feel satisfaction

61:25

afterwards and I understand my ability

61:26

to force myself to do things and in

61:30

doing that I find meaning and uh I'm a

61:33

relatively happy person. I think I'm

61:36

very happy in terms of like the average

61:38

person. I think that's why. But if

61:42

someone just took that all away, if all

61:44

that's gone, would you still have

61:46

happiness? Like what is happiness,

61:48

right? What is meaning? And what is it

61:52

entirely connected to your job? That

61:55

seems kind of crazy because a job is

61:57

just a constructed thing that it would,

62:00

you know, 500 years ago didn't even

62:01

exist. So what do what it do? We have to

62:05

have mean are we these complex

62:08

problem-solving biological organisms

62:11

that have this thirst for innovation and

62:13

to constantly make things better?

62:17

Are we tricking ourselves with jobs to

62:21

to be happy? Are we filling the need of

62:24

whatever? Like when a cat chases a ball,

62:26

what is it doing? What thinks it's

62:28

killing something? That's its design.

62:30

This is its biological need. You throw a

62:32

ball past a cat, it goes after it

62:34

because it's got this biological need to

62:37

chase things that are running away from

62:38

it so it could kill it and eat. And I

62:40

think we're kind of doing a similar

62:42

thing with our hunter gatherer tribal

62:45

organism that we're still trapped in

62:48

that we're we're tricking it. We're

62:50

tricking it with complex problems and

62:52

we're tricking it with community. We're

62:54

tricking it with all these different

62:55

things that that keep it happy.

62:57

>> I agree with you. Yeah, I I think that's

62:59

that's a wonderful answer. I mean, there

63:01

there's something about the, you know,

63:02

the the happy poor person, isolated rich

63:04

person thing that I I I I agree with.

63:06

But at the same time, you know, seeing

63:08

what grinding poverty does to people's

63:10

minds and breaking them down with

63:12

exhaustion and and demoralization, you

63:14

know, there there's obviously some kind

63:15

of a a sweet spot for there. You know, I

63:17

mean, I I've had to work quite hard in

63:19

different parts of my life.

63:21

>> And I I was just very aware of of the of

63:24

the of the soul grinding, you know, not

63:26

having enough, not wondering where your

63:28

next meal is coming from. and and and I

63:30

have it nowhere near as bad as some.

63:32

But, you know, the the thing that was

63:34

absolutely for me um unbelievable about

63:38

working for NASA was the idea of solving

63:39

complex problems with people you trusted

63:42

and people that you thought really had

63:43

your back and and no organization is

63:45

perfect. But, you know, the idea that

63:47

there is it's not a zero- sum game,

63:50

right? I I mean, you want the whole team

63:51

to succeed. I mean, even if there are

63:53

missions you think should have been

63:54

lower priority or maybe we should spend

63:56

more money on this and less money on

63:57

that, at the end of the day, you you

64:00

want whatever is going on to be

64:02

fantastic and you want it to succeed and

64:03

you want all the people around you to

64:05

succeed. And the idea that again, I

64:08

mean, this isn't hunter gathering, you

64:10

know? I mean, we're we're we're solving

64:11

problems. We're saying, you know, can

64:14

you take a picture of the black part of

64:16

a black hole? You know, can you actually

64:18

see the light area, the event horizon

64:20

getting sucked in? I'm talking about the

64:22

event horizon telescope, not a NASA

64:23

mission. But, you know, there were times

64:26

in my life like when I first saw that

64:27

picture come together and I didn't think

64:31

they'd be able to do that. I don't think

64:33

people really understand what happened

64:34

there. They they they were doing

64:36

something right on the on the on the

64:39

fuzzy edge of physics being possible.

64:42

You need to catch the same front of a

64:45

wavelength of light, right? So, light's

64:46

coming by. It's a wave. It travels at

64:48

the speed of light. the wavelength of

64:50

light is tiny. Let's say for a minute,

64:52

you know, that they they were they were

64:54

dealing with with microwaves. So, let's

64:56

say like a millionth of a meter. So,

64:58

something that's a a me a meter divided

65:00

by a million is traveling past you at

65:02

the speed of light.

65:05

And the Earth is is round and the Earth

65:07

is moving. And they had they had these

65:09

eight observatories all around the

65:11

planet. And they had to catch that same

65:13

wavefront, the same one. If it was if it

65:16

was one wavefront later, one one

65:19

millionth of a meter later traveling at

65:20

the speed of light, they wouldn't have

65:21

gotten the image. They needed to catch

65:23

the same wave wavelength, the same

65:25

photon, the same wave of light had to be

65:28

caught in all of those telescopes at

65:29

once. One was at the South Pole, some

65:31

were in the in the United States, some

65:33

were in Chile. They were all over the

65:36

planet. And if you caught the same

65:39

freaking wave of light,

65:41

>> here it is.

65:41

>> There you go.

65:42

>> Wow.

65:44

>> They they managed to make a telescope

65:45

that's actually as big as the Earth. And

65:47

they were able to take a picture of the

65:49

dark parts of a black hole. Now, now

65:51

that's that's something called the

65:52

shadow of the event horizon. It's

65:54

basically the event horizon where time

65:56

and space stop. We don't even know if

65:58

there really is an interior to a black

66:00

hole. All the equations blow up. Time

66:01

and space don't exist in there. and and

66:04

light. Nothing can escape that darkness.

66:07

The uh the black spot you're seeing

66:09

there is a little bigger than the event

66:10

horizon itself. It's called the shadow

66:12

of the event horizon because um time and

66:14

space are bent around the black hole.

66:17

And so some of the light that actually

66:19

gets sucked in is light that would have

66:21

gone around the black hole. It gets

66:22

sucked into the back end of the black

66:24

hole. Literally space and time curve

66:26

around the black hole. And so that that

66:28

dark part is actually a little bigger

66:30

than the event horizon. It's called the

66:31

shadow of the event horizon. And um they

66:34

said they were going to go take a

66:35

picture of it. And I was like, you have

66:39

to catch the same wavefront of light

66:43

in all of these telescopes. I mean,

66:44

that's going to depend on the height of

66:45

the mountain, how fast that part of the

66:47

Earth is moving. They did it. They

66:49

did it. And they they they

66:51

didn't do it just once, right? And you

66:54

know, and and and now we can take a

66:55

picture of an area right in front of

66:57

your eyes where space and time doesn't

66:59

exist. I mean to a to a lesser extent,

67:03

one of the NASA missions that I thought

67:04

was just spectacular was a small

67:06

inexpensive mission called NICER. Uh

67:09

you're like, who's the nicer person?

67:10

Nicer NICE R. It's the Neutron Star

67:13

Interior Composition Explorer. And a

67:15

neutron star. You probably know about

67:17

these, but but you know, if when a star

67:19

dies and the nuclear reactions inside a

67:21

star cease, all of that gravity of this

67:24

massive object comes crushing in and

67:27

it'll create an object sometimes called

67:29

a neutron star. They're about 20 miles

67:31

across, but they have about twice the

67:33

mass of the sun. And we study many of

67:35

these at NASA. They're they're they're

67:37

all over the place. They're real.

67:39

They're something you can take a an

67:40

image of, you can take a picture of. And

67:42

you know, these neutron stars have

67:44

physics that we don't understand. You

67:46

you take you take two times the mass of

67:47

the sun, you crush it into 20 miles. We

67:50

know that we can't describe the interior

67:52

of that thing yet. You know, we don't

67:54

have the physics that matches that type

67:55

of density. And um this this this this

68:00

crazy little little contraption, I mean,

68:02

it's about the size of a washing

68:03

machine. It was built in a lab just on

68:05

the floor that I used to work at at

68:06

NASA. It's cheap, easy to make. I

68:09

shouldn't say easy, uh, but I mean it

68:11

it's actually able to create maps of

68:13

what the surface of these objects are

68:15

like. They're 20 miles across. They're

68:17

thousands of light years away.

68:20

And you can actually create a map of

68:21

what the temperature is like. And one of

68:23

the things we see on these maps is the

68:26

distortion where space and time curves

68:28

around these objects. You know, they'll

68:30

they they rotate very fast and there are

68:32

hot spots we see coming in and off the

68:34

the neutron star. But then as the

68:36

hotspot goes behind the star, the light

68:38

bends up and over and we can actually

68:40

still see the hotspot because space and

68:42

time are bending around these objects.

68:44

You can see that that that's not a

68:47

mathematical simulation. That's not a

68:49

theory. You can see space and time

68:52

bending around these objects. You can

68:54

see space and time bending into that

68:56

event horizon. You know, I mean, it's

68:58

absolutely crazy what we've been able to

69:01

do. And whether it's a you know a huge

69:03

project like the event horizon telescope

69:05

where I I I would have bet that they

69:07

would not have been able to make that

69:08

measurement and they did you know there

69:11

there were so many hard drives of data

69:14

uh one of the uh one of the telescopes

69:15

was at the south pole and uh you wanted

69:17

you wanted the telescopes to be as far

69:19

apart on the earth as possible because

69:20

then you could basically make a giant

69:22

telescope the size of the separation of

69:24

these telescopes and uh um there wasn't

69:27

I mean there's there's pretty good email

69:28

links down to the South Pole but but the

69:31

email link wasn't fast enough for all of

69:32

this data. They they sent back literally

69:34

there was a ton a ton of hard drives to

69:38

actually they had to play them all at

69:39

the same time and make sure they caught

69:40

the same photon. If they had caught

69:43

seriously one photon following behind

69:45

the other, the image wouldn't have

69:47

worked. They had to catch that same

69:48

photon. You know, humans are incredible.

69:52

>> Some of us

69:54

>> Oh, hey,

69:55

>> some of them, I should say.

69:56

>> Maybe maybe pretty much all of us in

69:58

different ways. Yeah, I mean, you know,

69:59

I

70:00

>> unrealized potential.

70:01

>> No, I I got to go back to this. I mean,

70:02

I mean, one of my good I I have three

70:04

friends now have won the Nobel Prize,

70:06

which is always like, you know, what the

70:07

hell am I doing?

70:07

>> That's awesome.

70:08

>> Um, but group Yeah,

70:10

>> but you have good group chats.

70:11

>> Well, see, the funny thing is we we

70:13

certainly don't all get together and

70:14

talk theoretical physics. I mean, that's

70:15

not really what we do. But I was seated

70:17

next to one of them at a meal one time

70:18

and somebody came by and said, "Oh, look

70:20

at all the brain power here." And I I

70:22

actually in this I try to be kind of

70:24

nice about it, but I said, you know,

70:26

there's a single mother working three

70:27

jobs part-time, you know, who's waiting

70:29

tables over there. And I mean, the the

70:31

mental capacity and the strength of that

70:34

person is something that,

70:36

>> you know, I mean, don't look at us. Go

70:38

go go go go praise that person.

70:39

>> Well, that's brain power, too. It's just

70:41

a different thing.

70:42

>> It's survival. I mean, it's trying to

70:43

keep your life and and soul together.

70:45

the the the privilege of being able to

70:47

work at NASA and and to be able to work

70:50

with a team like that and do things you

70:52

think are impossible,

70:54

you know, that that was kind of a part

70:56

of my life you could stick a pen in and

70:58

say that meant something. You know, that

70:59

that that gave me some meaning. That

71:01

that gave me joy.

71:03

And as you said, it's not so much being

71:06

a hunter gatherer. It it's it's it's,

71:08

you know, can we ask a question that we

71:10

think is impossible and can we just go

71:11

and do it? Yeah.

71:13

>> Yeah. the ultimate expression of human

71:15

curiosity when you say that we don't

71:17

have the physics when when you're trying

71:20

to understand what's happening in a

71:22

neutron star. What do you mean?

71:23

>> So you can measure how big these things

71:25

are and you can measure how massive they

71:27

are and so then you can do a calculation

71:29

as to what the density inside would be.

71:32

And you know it I mean to put it I mean

71:34

probably the interior core is denser

71:36

than the outer regions but if you had a

71:38

teaspoon of this material it would have

71:40

about as much mass as Mount Everest.

71:43

And um the reason they're called neutron

71:45

stars is that the gravity is so intense

71:48

on these things. I mean this I mean I I

71:51

hate I hate sort of a simple view of

71:53

atoms as little balls going around each

71:54

other because they're not they're

71:55

they're waves of energy, but the gravity

71:58

actually crushes the electrons into the

72:00

nucleus. They combine with protons to

72:01

become neutrons. So they're they're

72:03

mainly little balls of neutrons. But we

72:06

we do There you go. Uh you see the big

72:08

question mark there at the core. So So

72:11

here's the problem. you you you you you

72:13

run our our basic laws of physics, our

72:15

understanding of how particles work and

72:17

you get to the density of a neutron core

72:19

and and the equations don't work.

72:21

They're not making the right

72:22

predictions. We can tell that there is

72:25

um there's actually a really great NASA

72:27

video I I would I would I would suggest

72:29

you watch it. It's called um the the

72:31

interior of a neutron star. uh well I

72:34

can help you find it but it it basically

72:36

says that that the

72:37

>> the models we have about how matter

72:40

works at that sort of density none of

72:42

them give the right predictions for the

72:43

the size of the neutron star.

72:45

>> Why is that?

72:46

>> We don't have the right physics for it

72:48

yet.

72:48

>> So so you know we run our physics and we

72:50

say if you have this much volume and

72:52

this much mass what should that interior

72:54

be like? And and none of our current

72:57

models of how matter works gives us the

72:59

right observations gives us the right

73:00

size.

73:01

>> So what are we missing? Well, um, for

73:04

one thing, you know, what you're

73:06

probably looking at inside a neutron

73:08

star is some type of interaction of

73:10

quarks, the actual the actual sort of

73:11

building blocks of neutrons and protons,

73:13

the particles that make up protons and

73:15

neutrons.

73:16

>> Oo, that's cool.

73:16

>> Yeah. There. Oh, you got it. You got it.

73:18

You're amazing. I I I have to say I'm

73:20

seriously impressed by this person's uh

73:22

ability. Yeah. So, I mean, this is a

73:25

video that it was done by uh by NASA,

73:27

Testing Matters Limits. It's a 4-minute

73:29

video and and while I don't think it's

73:31

an absolutely perfect video, I'm I think

73:33

it's fantastic. And so you see the uh

73:36

this is supposed to represent the

73:37

electrons being pulled into the the

73:39

nucleus and making neutrons. And then at

73:42

the very heart of these things, we're in

73:44

a state of matter that we have no

73:46

description for yet. We we we can't tell

73:48

you how it behaves. We we've never

73:50

created it in a lab. We we you we don't

73:53

know how this type of matter acts. It's

73:55

a new state of matter. We we don't know

73:57

what it's like.

73:58

>> Wow.

73:58

>> And uh you know it's it's made when when

74:01

one of these giant stars explodes you

74:03

know the the core of the star becomes

74:05

compressed. And then this this will take

74:07

you through us trying to figure out what

74:09

you know whether you know you have

74:10

particles as discrete particles as

74:12

neutrons and protons or whether there's

74:14

some type of quark soup inside. But but

74:17

pretty much every model so far doesn't

74:20

match what we actually measure from

74:23

these things. We we we cannot describe

74:25

them yet. We we need better physics.

74:27

>> Are there any other structures that are

74:29

similar in our lack of understanding of

74:31

them in the universe?

74:32

>> Well, we got you got two big ones right

74:33

in front of you. Neutron stars and black

74:35

holes, right? So, so I mean these the

74:37

black holes as well. You know, what is

74:39

inside a black hole? Is there an inside

74:42

if space and time don't really exist? Um

74:45

you know, and then and then much more

74:47

easy to see are these neutron stars. The

74:50

the people who study neutron stars at

74:51

NASA, they had this wonderful

74:52

expression. They're like, "With a black

74:54

hole, you can't see anything. it

74:55

collapses into an event horizon.

74:56

Nothing's coming out. With a neutron

74:58

star, you got the freaking thing right

74:59

there in front of you. You can actually

75:00

observe something. And so, you know,

75:03

they they figured that neutron stars are

75:04

much more exciting than black holes

75:05

because you can actually like do

75:07

experiments, take a picture, build a

75:08

telescope. And uh but but this

75:11

experiment was an inexpensive small

75:14

observatory that that's up on the

75:15

International Space Station. And I mean

75:17

I mean it's they're they're doing

75:19

incredible work about the the nature of

75:22

physics and and and testing where our

75:24

limits are. It's it's unbelievable what

75:25

you can do with even a a relatively

75:27

inexpensive mission.

75:29

>> When you look at the size of some black

75:32

holes, we were talking the other day

75:34

about the largest black hole where the

75:36

event horizon goes past Pluto.

75:38

>> Yeah.

75:39

>> If it was the the size of our solar

75:40

system.

75:41

>> Absolutely. that that's almost

75:43

impossible to even think about that

75:46

there's a black hole that's bigger than

75:48

our solar system. And how did it get

75:51

that big?

75:52

>> How much time does it take for it to

75:55

gather up that much matter to get that

75:58

big?

75:58

>> Well, you were talking about these

75:59

little red dots that the web telescope

76:01

is seeing. So, I mean, what you've just

76:02

done is put your finger on, I think, one

76:05

of the most fascinating unanswered

76:06

questions in astronomy right now. that

76:09

every major galaxy has a has a big black

76:12

hole in the center. You know, the the

76:13

one in the middle of our galaxy is about

76:15

4 million times the mass of the sun and

76:18

and physically it's not that big. It's

76:20

it's about let's say around about the

76:22

orbit of say the inner solar system

76:23

Mercury kind of around there. But then

76:26

the bigger ones we know in other

76:28

galaxies can get up to hundreds you know

76:30

I mean let's say you know tens of

76:32

billions of times the mass of the sun

76:34

and and those the event horizons about

76:36

the size of the orbit of Pluto.

76:39

The the question is how do you gather 10

76:42

billion times the mass of a star

76:44

together in the beginning? You know we

76:47

black holes the only thing we know that

76:49

forms big black holes like that. So a

76:51

star collapses a star dies and this you

76:54

know this tremendous crush of gravity as

76:56

the star collapses creates this

76:58

bottomless pit of gravity called a black

77:00

hole. So how do you get that many stars

77:03

to die? How do you I mean in the early

77:05

universe, how many stars what how many

77:06

generations of stars had had to burn

77:09

through to actually get that to happen?

77:11

And there was nothing that we could

77:13

figure out. I mean I mean how do you

77:14

make that big of a black hole? So these

77:16

these little red dots that we're seeing

77:18

with with with web and and when we don't

77:21

know exactly what these are, but but but

77:24

right now the observations are pushing

77:25

us in a very interesting direction.

77:28

They're they're about a million times

77:30

the mass of the sun. And at first we

77:34

thought, okay, well, are these whole

77:35

galaxies? And and that was the the

77:36

controversy you alluded to that that how

77:38

how could there be galaxies that far

77:40

back in time? We're we're looking back

77:42

to a time about 400 million years after

77:45

the Big Bang. We're looking so far away.

77:47

The light took that long to travel to

77:48

us.

77:50

So we we we saw these these these sort

77:52

of bright objects. At first we thought

77:54

they were galaxies, and that was like,

77:55

whoa, how'd they get there so fast? But

77:58

then we took a better look at them and

77:59

they don't actually shine in the same

78:01

light a galaxy would. They and they

78:03

appear to have the signature of

78:05

something inside. Some of them rotating

78:07

very fast. Very fast.

78:10

And what we're wondering is if the first

78:13

generation of stars, the very first

78:15

stars that existed were nothing at all

78:18

like the stars we have today. The

78:20

universe was denser. There was probably

78:22

more of this stuff called dark matter

78:24

that had gravity pulling everything

78:26

together. So maybe at at that time the

78:29

universe had just there were cores of

78:31

huge amounts of gas that collapsed

78:32

together. Instead of forming a star, the

78:36

core basically collapsed into a black

78:37

hole immediately and it started pulling

78:40

in material and all this sort of hot

78:41

stuff formed what they call a pseudo

78:44

star. There's all this this this

78:46

atmosphere of hot gas being heated up by

78:48

by the black hole in the middle. As as

78:50

as the gas spirals in towards the black

78:51

hole, it gets hotter and hotter. So

78:53

instead of a nuclear fusion core of a

78:55

star, you have a black hole heating

78:57

everything up on the inside,

78:59

accumulating all this mass. And are we

79:02

looking at for the first time the seeds

79:05

of these giant black holes

79:07

that instead of there being you know the

79:10

first thing was stars the way we think

79:12

of stars was the first thing huge

79:15

amounts of gas and dust collapsing into

79:17

black holes and heating up sort of a you

79:20

know a pseudo star around it millions of

79:22

times the mass of the sun and then in a

79:25

dense area like the heart of a galaxy

79:27

these things then start to combine over

79:29

time gravity pulls them together and you

79:31

build bigger and bigger black holes.

79:34

So once again, we don't know yet that

79:37

these are what what's that's what go

79:39

that these objects are. But at the

79:40

moment, it's one of the best

79:41

explanations we have and it fits the

79:44

data quite well. So you know, we will

79:47

keep observing these things. We will

79:48

keep finding new ones. Uh one of the big

79:51

questions has been why don't they give

79:52

off more X-rays? Because if there's

79:54

matter streaming down a black hole, it

79:56

should give off very high radiation like

79:58

X-rays. And then just in the last couple

80:00

of months, there are some uh some

80:01

observations coming out where we're

80:03

finding some of these are indeed X-ray

80:04

sources.

80:06

So, we may have found the answer to

80:09

where you get these big black holes.

80:11

>> And and that was one of the the big

80:14

hopes for the James Webb Space Telescope

80:16

that it would help us answer the

80:18

question of where do you get these giant

80:20

black holes in the cores of galaxies?

80:22

Where do they come from? There shouldn't

80:24

have been enough time for that many

80:25

stars to make them.

80:28

I watched a documentary around black

80:30

holes once where they were talking about

80:31

that in the center of every galaxy

80:33

there's a super massive black hole

80:34

that's 1/ half of 1% of the mass of the

80:37

entire galaxy.

80:38

>> It seems to be correlated. Yeah. The

80:39

bigger the galaxy, the bigger the black

80:40

hole. Yeah.

80:40

>> Which is nuts. And the what they were

80:43

theorizing was that if you went through

80:48

that black hole, you could potentially

80:50

be in a completely different universe

80:52

filled with galaxies all that have black

80:54

holes inside of them. through that

80:56

another universe that you would have an

80:59

infinite number of universes that exist

81:02

and all there's these like black holes

81:04

and if you can go through them all of

81:06

them and it broke my brain cuz I'm just

81:09

sitting there I'm thinking like wait a

81:10

minute how many billions of galaxies are

81:12

there?

81:13

>> Yeah.

81:13

>> Like what and each one of them has a

81:15

black hole in the center of it?

81:16

>> Yeah. Well, and and I mean we don't know

81:19

yet how many uh I mean there there are

81:22

these giant black holes in the middle of

81:23

galaxies and then there are smaller

81:24

black holes caused when massive stars

81:26

dies and you our galaxy probably has

81:28

millions of those. But the uh the ones

81:31

in the in the in the center of the

81:32

galaxies are fascinating. The um the one

81:34

in our galaxy so we're about about

81:37

25,000 lighty years away from the sky so

81:39

we're safe. But um

81:42

we actually observed stars that are

81:44

trapped around the black hole that are

81:46

orbiting the black hole. This was the

81:47

first way we found the location of the

81:49

black hole. Stars were orbiting kind of

81:51

like this angry swarm of bees almost in

81:53

every direction. And they were orbiting

81:55

around something you didn't see. And the

81:57

mass needed to make all these stars

81:59

orbit was about four million times the

82:00

mass of the sun. There was a star called

82:03

S2 we observed orbiting close to the

82:05

black hole, kind of like a comet. It

82:07

would come in and whip around the black

82:08

hole, then go back out again. and an S2

82:10

at closest approach when it whips around

82:12

the black hole. This is a star goes

82:15

nearly 20 million miles an hour as it

82:18

whips around the black hole. And then

82:20

just recently we found another star that

82:22

actually gets up to over 50 million

82:24

miles an hour as the black hole whips it

82:27

around. And this is how we test the idea

82:29

that time is different around a black

82:30

hole. We actually see these stars

82:32

whipping so close to a black hole. We

82:34

can tell that there are changes in their

82:36

orbit, that they're actually going

82:37

through different time.

82:39

And uh um and so we see these stars

82:41

whipping around the black hole at the

82:43

middle of our galaxy. They will probably

82:44

eventually go down that black hole. I

82:46

mean, maybe everything in our galaxy

82:48

will eventually kind of spiral down into

82:50

that black hole. But you know, we we

82:53

this is this is not conjectural. These

82:56

are observations from telescopes. You

82:59

know, look up S2. Look up I don't know

83:01

what the name of the one that it goes

83:02

faster. It's a telephone telephone

83:04

number, but that's real.

83:08

Now, the question about what happens if

83:10

you could survive going into a black

83:12

hole, and this is another place where we

83:14

need better physics. Quite honestly, our

83:15

physics gives up.

83:18

There are all kinds of wonderful,

83:21

fascinating possibilities. I mean,

83:23

people have pointed out this is not

83:25

observation. Now, we're going from

83:27

observation, we see these things,

83:28

they're real to conjecture. People have

83:32

said that if you take the entire

83:33

universe, the the the entire mass of the

83:36

universe and the radius that the

83:38

diameter of the observable universe

83:40

almost exactly matches a black hole. You

83:43

know, you could it be that, you know,

83:45

inside a black hole, a new universe

83:47

forms when a black hole forms. Is that

83:49

what the big bang was? Was the big bang

83:51

a black hole forming in another universe

83:53

and popping off our own universe? Are

83:56

black holes somehow connected to other

83:57

universes? These are all incredible

84:00

questions. We we don't yet have the

84:02

physics to answer them. But you know,

84:05

people have said, you know, why is it

84:07

the universe has about the same density

84:09

of a black hole, the same size and mass?

84:12

Is that just a coincidence or are we

84:14

looking at something deeper?

84:15

>> Or is it fractal? Is it the entire

84:17

universe exists inside of a black hole?

84:19

>> Yes, exactly.

84:20

>> That's bananas.

84:21

>> Yeah. There there we have the the very

84:24

large array that was at the uh that was

84:26

in Chile. That's a wonderful

84:27

observatory. There we have a a great uh

84:30

depiction. Oh, he he you found Okay.

84:32

Yeah, I've never seen a depiction like

84:35

that's the stars moving around a black

84:36

hole.

84:36

>> Yeah, the stars moving around a black

84:37

hole.

84:38

>> What's coming? What would this ejection

84:40

be?

84:40

>> Um so that Okay. What what that is is

84:42

that that's a consequence of the black

84:44

holes. Um that doesn't come from inside

84:46

the black hole. All of that swirling gas

84:48

gets really fast. We actually observe

84:50

some of the swirling gas going close to

84:52

the speed of light. Black holes, you

84:54

know, they're they're going down the

84:55

drain. They're going faster and faster

84:56

as you get closer to the black hole. And

84:58

um all of that very very hot gas

85:00

generates a very strong magnetic field.

85:03

And so what you're looking at with those

85:04

jets is that that's just the magnetic

85:06

field of the hot gas going around the

85:08

black hole. Some of that hot gas gets

85:10

directed into jets by the magnetic

85:12

field. There's nothing coming out of the

85:13

black hole. Nothing that we know of

85:15

comes out of a black hole. But black

85:17

holes are incredibly This is This is

85:19

wonderfully ironic. They're incredibly

85:21

bright because if there's gas trying to

85:23

get around a spinning around a black

85:24

hole, the gravity accelerates that gas

85:27

so fast it spins it up to in some cases

85:29

millions or billions of degrees. You can

85:31

see them clear across the observable

85:33

universe. They're the brightest objects

85:34

in the sky. And this this is not light

85:37

coming from inside the black hole. It's

85:38

light coming from stuff trapped around

85:40

the black hole as it spirals in. And

85:43

these huge jets, we we see some of these

85:45

jets going, you know, in some cases more

85:47

than 100,000 lightyears. I mean they're

85:49

they're huge jets that come out

85:51

>> 100,000 lighty years and one light years

85:53

is how many trillion miles?

85:54

>> Six trillion miles about

85:57

>> Yeah. Yeah. So

85:58

>> Oh my god.

85:59

>> And then in the uh

86:00

>> Oh my god.

86:01

>> Yeah. So I mean around uh um around

86:04

>> that video is so nuts.

86:06

>> I've never seen that.

86:07

>> Yeah.

86:07

>> When I was looking for this or stumbled

86:09

across this I saw a theoretical thing

86:11

called a white hole

86:12

>> which is potentially maybe on the other

86:14

side of a black hole.

86:15

>> You know the the

86:17

>> Yeah. No, no, no. It's it's an idea. I

86:18

mean, that idea, honestly, it had a lot

86:21

more um uh following, you know, more in

86:23

the in like the 60s and 70s. It's kind

86:25

of fallen out of favor because at first

86:27

we thought that the these hugely bright

86:29

objects were were white holes at the end

86:30

of a black hole. Maybe the radiation

86:32

went through a tunnel through space and

86:34

came out somewhere. But now we know that

86:36

these super bright objects are actually

86:38

hot gas discs around black holes. And

86:40

they are bright. Like I said, they're

86:42

the brightest things we know of in the

86:43

sky. and uh you know so that's that's

86:46

something you can see you know literally

86:48

billions of light years away is the hot

86:50

gas going around a black hole.

86:51

>> You said another thing that broke my

86:53

brain. Um you were talking about

86:57

what the big bang is and that we

87:00

shouldn't think of the big bang as an

87:02

explosion

87:04

but that before the big bang time and

87:08

space might not have existed.

87:11

>> Well pretty much certainly not in the

87:13

way we experience them. No, I mean I

87:15

mean once again, you know, no astronomer

87:18

thinks the big bang came from nothing.

87:21

The problem is once again we have no

87:24

description of what that state of matter

87:26

would be. None.

87:28

I mean the idea that everything we

87:30

observe of in the universe could have

87:31

once been at a subatomic scale.

87:34

You'll notice I'm very careful about

87:36

this. I talk about the observable

87:37

universe. We have no idea how big the

87:40

universe is. We don't know whether it's

87:41

infinite or whether it has an end. But

87:43

there's been only a certain amount of

87:45

time that light has had to travel to us.

87:47

That's not the whole universe. That

87:49

that's centered on us. That's an effect.

87:51

If we look in every direction in the

87:52

sky, we can only look back as far as

87:55

there's been time for light to actually

87:57

travel to us. And you see some

87:59

incredible things. I mean, one of the

88:01

things that uh one of my friends has the

88:02

Nobel Prize for is if you look so far

88:05

away, the farthest away we can see now,

88:08

we're looking back to a time about

88:10

400,000 years after the Big Bang. And

88:12

this is something where we are actually

88:15

able to see so far away. We're looking

88:17

back to a time when the whole universe

88:19

was hot and bright. It actually was

88:22

glowing like the surface of the sun. The

88:23

whole universe. The entire universe was

88:26

so bright. It was like looking at the

88:28

surface of the sun. And and this is is

88:31

has now this radiation has traveled a

88:34

long time to get to us. It's now lost

88:36

energy because it's traveling through

88:38

the expanding universe. And as the

88:40

universe expands, the the wave the

88:42

wavelength of light gets stretched out

88:44

by the expansion of space. This is what

88:46

we call the microwave background

88:48

radiation.

88:49

So there there's there's a there's a

88:51

microwave very low energy signal. It

88:53

comes from every direction on the sky.

88:55

And it's coming from a time it's coming

88:57

from a distance so far away that the

89:00

whole universe was as bright as the

89:02

surface of the sun. And and that's as

89:05

far as we can see because any farther

89:08

away from that the universe is opaque

89:11

literally in every direction on the sky

89:13

you eventually look back to a time when

89:15

the whole universe was so dense and

89:17

bright you can't see any farther.

89:19

>> Is this because of how we're capable of

89:22

measuring? And is it possible that at

89:24

one point in time when we get better and

89:26

better telescopes that we can look past

89:29

that?

89:30

>> Well, not with light. See, see the

89:31

universe actually does become opaque to

89:33

light at that point

89:34

>> because it's too long ago.

89:36

>> It's it's it's basically the universe is

89:38

so bright itself. Yeah. I mean, so you

89:41

know, you look in any direction on the

89:43

sky, you look back to a time, you know,

89:45

we the wonderful thing about the

89:47

universe changing is we know this is

89:48

true. The farther out we look with a

89:50

telescope, the farther light has had to

89:52

travel, the the more time it takes to

89:54

get to us. So the sun we see the light

89:57

takes about eight minutes to get from us

89:58

to the sun. the nearest star about four

90:00

years. The nearest galaxy to us about

90:02

two million years. We can see so far

90:05

away in space that the light took pretty

90:07

much the age of the universe to get to

90:09

us about 400,000 years after the big

90:11

bang. At that point, the universe

90:13

becomes opaque to light.

90:16

So there is a limit to how much we can

90:18

observe with light, how much time there

90:21

has been for for light to actually get

90:23

to us.

90:24

>> Is there a potential for being able to

90:25

observe with something other than light?

90:28

Absolutely. So your question is a really

90:32

profound one. We don't know how big the

90:34

universe is. When we talk about the

90:36

universe, we mainly talk about the

90:38

observable universe, everything we're

90:39

able to see. So the question you just

90:42

asked, can you see farther back, even if

90:44

it's opaque to light? Yes. And and this

90:48

is something that again we talk about

90:50

moments in your life where the universe

90:51

changed, where you thought people people

90:54

did something you thought was

90:55

impossible. And um I mean going all the

90:58

way back to the mid 90s I was a posttock

91:00

at Caltech and um I wasn't working with

91:03

this department but people were starting

91:05

to measure something called

91:06

gravitational waves

91:08

and gravitational waves again I I never

91:12

thought they'd be able to actually

91:13

detect these. The the universe is is

91:16

constantly I mean I mean every time we

91:18

move remember how I said time is

91:20

different from the top of your head to

91:21

the bottom of your feet. You know, as I

91:23

move, I create gravity. You know,

91:26

gravity actually is it goes out as a

91:28

wave into the universe at the speed of

91:29

light. Can you detect a wave of gravity?

91:33

Well, a gravity is actually a curvature

91:36

of space and time itself. So, you're

91:38

you're trying to say, could we detect a

91:41

wave that's actually made of space and

91:42

time? And this project is called LIGO.

91:46

And LIGO stands um LIGO stands for the

91:49

Laser Interferometric Gravitational Wave

91:51

Observatory. And it started out with

91:53

with two facilities, one in Oregon and

91:55

one in Louisiana. And LIGO has two

91:58

extremely long lasers at at a corner

92:00

that at a right angle. The lasers I I

92:03

believe are 4 kilometers on a side.

92:06

They're huge, right? A 4 km laser. They

92:09

want them to be as as perfectly the same

92:11

length as they can. And then there's a

92:13

laser beam that bounces back and forth.

92:16

And and as the laser beam bounces back

92:18

and forth, if it's exactly the same

92:20

length, they the signal kind of cancels

92:22

out.

92:23

But what happens if there's actually a

92:26

wave of space and time coming by? Space

92:29

itself compresses. Time changes. All of

92:32

a sudden, these two these two lasers are

92:35

no longer exactly the same length. Space

92:37

itself has changed as as a wave comes

92:39

by.

92:41

tiny amounts. These gravitational waves

92:43

are thousands of times smaller than the

92:45

nucleus of an atom.

92:47

>> Incredible, right? How would you detect

92:49

that? And they're traveling at the speed

92:50

of light.

92:52

So, you have these 4 kilometer lasers,

92:56

a wave of space and time comes by and

92:58

compresses space and time in one

93:00

direction more than the other. All of a

93:01

sudden, the lasers are no longer the

93:03

same length. You get a signal. The the

93:06

noise for this, right? I mean, I mean,

93:08

every time Yeah. So, this is us

93:10

detecting an exploding star this way.

93:11

I'm happy to talk about that, too. But,

93:13

but I mean, just the fact they did this,

93:16

the these lasers are under vacuums.

93:18

They're in vacuum chambers. I mean, they

93:20

try every time the UPS truck goes by,

93:22

they must go haywire. Somebody sneezes.

93:24

They're measuring things thousands of

93:25

times smaller than the nucleus of an

93:27

atom.

93:29

But over time they got this so accurate.

93:31

They did it so well that what what

93:34

happened and I I you can look up the the

93:36

year but it was um something on the

93:37

order of about 10 years ago

93:40

a long ways away millions of light years

93:42

away um two black holes spiraled

93:45

together and actually collided to form a

93:47

big black hole. That was a lot of

93:50

gravitational energy and that created a

93:52

ripple going out into the universe. And

93:55

so you know there's all of the detectors

93:57

have all this noise in them. The

93:58

detectors are detecting all kinds of

93:59

spurious signals. But then all of a

94:01

sudden in Louisiana, there was this the

94:04

whole detector went w boom. And then at

94:07

the speed of light, the detector in

94:09

Louisiana did exactly the same thing. B

94:12

the exact same waves at the speed of

94:14

light difference. And we realized, oh my

94:16

god, they did it. These tiny waves,

94:20

we shouldn't even be able to detect

94:22

them. They found them. And and now it's

94:25

a it's a routine thing. They've now done

94:26

this many, many times.

94:29

Waves in space and time itself might be

94:32

the way we can see even farther back

94:34

into the universe. Even when the

94:36

universe becomes opaque to light, the

94:39

waves of space and time can come

94:40

through. Gravitational waves can come

94:42

through that. And if we can somehow

94:45

figure out how to make these detectors

94:46

better and better, you know, could we

94:48

detect the gravitational waves of the

94:50

Big Bang? You know, can we learn

94:53

something about that moment by the way

94:56

it actually bent space and time and

94:57

created waves of gravity? And once

95:00

again, I mean, just a step back a sec.

95:01

The detecting waves of space and time

95:04

traveling at the speed of light is

95:06

something we do.

95:09

We've done this. It got the Nobel Prize,

95:11

deserved it. Um, there were there were

95:14

hundreds of people on that first paper.

95:16

Some of them were friends of mine. Um,

95:19

again, they they did it, you

95:21

know. I I I I I just I I cannot I mean I

95:24

I I I felt my heart just drop that day.

95:27

I mean out of out of joy. I just it's

95:28

it's like holy you know they did

95:31

it. Um that may give us the potential to

95:34

understand the big bang better as we get

95:36

better with that. Um you know maybe we

95:38

can I mean right now we see black holes

95:40

colliding. We actually see neutron stars

95:42

colliding. Even stars orbiting each

95:44

other maybe maybe produces sort of a

95:46

background of all these waves. But maybe

95:48

we'll be able to figure out how to see

95:50

those waves from the moment the universe

95:52

began.

95:53

>> How are we sure that of the timeline of

95:57

13.8 billion years or whatever it is?

96:00

>> Well, you know, I mean, the these things

96:02

are never sure, you know, absolutely.

96:04

But but but there there there's some

96:06

very good reasons to think it's it's

96:07

about that. So, you know, you you sort

96:10

of run physics backwards. You know, you

96:12

basically say, you know, this is how the

96:14

universe is expanding now. And Lind,

96:16

let's let's roughly say that, you know,

96:18

things, you know, came together. And as

96:20

I mentioned, you mentioned the podcast,

96:22

the Big Bang did not have a center. The

96:24

galaxies are not flying off into space

96:25

like an explosion. You what what

96:27

happened is the galaxies are all kind of

96:29

sort of standing where they are, but

96:31

space itself is expanding in every

96:33

direction between the galaxies. It was

96:35

it's a hard thing. I mean, I this it's a

96:38

huge misconception about the Big Bang

96:40

that the Big Bang was this explosion and

96:43

galaxies are flying into empty space.

96:45

The the expansion of space is space

96:47

itself. There's no space out there that

96:50

galaxies are flying into. That's not how

96:51

it works,

96:52

>> right?

96:53

>> You know, when I

96:54

>> That's a weird thought right there.

96:56

They're not flying into space, they are

96:58

space. When when I when I used to teach

97:00

this, you know, I used to I used to take

97:02

a a board and I used to have a piece of

97:04

elastic and I would I would hammer two

97:06

nails in on either side of the board and

97:08

then I would say, "Okay, the these two

97:09

nails are galaxies and the elastic

97:12

between them represents our universe."

97:14

In this case, a two-dimensional

97:15

depiction of our universe. All of space

97:18

and time anywhere light can travel is on

97:20

just on that elastic. Don't think about

97:22

up or down. There's no space or time

97:23

there. Everything our universe is is

97:25

just this piece of elastic, you you

97:27

know, and then I would take the elastic

97:28

and I would stretch it and I would say

97:30

by by by you know, the two galaxies

97:32

aren't moving. They're they're kind of

97:34

sitting there. It's the space in between

97:36

that has now stretched, has now changed.

97:40

And that's a more realistic idea. The

97:42

galaxies are not flying through space.

97:44

It's the space itself that is getting

97:47

bigger in every direction at once. And

97:49

that's why there's no center. There's no

97:50

empty center to the universe. The

97:52

universe, as far as we can map it, has

97:54

galaxies everywhere. you know there's no

97:57

center to it. The expansion is happening

97:59

in every direction at once because the

98:01

the the elastic of space and time itself

98:04

in every direction is just getting

98:06

bigger. We don't know why.

98:08

>> So if we are looking at something where

98:14

the big bang created space and time and

98:17

as space and time is expanding what was

98:21

the environment

98:23

before the big bang?

98:24

>> Yeah. And that's the problem. So you

98:26

mean I mean we have no description of

98:28

that. You know there there there are

98:31

particle accelerators. I've had the the

98:34

wonderful chance to go to us to go to

98:36

CERN a couple of times and go to the

98:37

Large Hadron Collider and you know you

98:40

know using you know incredible

98:43

accelerating magnets. You know they they

98:45

whip you know just single protons up to

98:47

very very high temperatures.

98:50

I mean, they're they're trying to

98:51

recreate conditions where, you know, I

98:54

mean, they can't recreate the conditions

98:56

of what things were like before the Big

98:57

Bang, but, you know, can you get matter

98:59

to such a high energy state that it can

99:02

recreate what things were like, you

99:03

know, a millionth of a second after the

99:04

Big Bang, you know, or maybe even

99:06

further back? And, you know, but the

99:10

idea of what was that state of matter

99:12

before that that expansion, we have no

99:15

description of yet. I think we will

99:16

someday. I don't think it's impossible.

99:19

But there there's nothing about our

99:21

current physics. I mean, it would be

99:23

like taking somebody from the 1400s and

99:26

saying, you know, describe to me what

99:28

the interior of the sun is like. They

99:29

they would have we they would have no

99:31

knowledge structure to even attempt it.

99:35

That doesn't mean we didn't figure it

99:36

out eventually. And you know, so like I

99:39

said, there's nothing about that I think

99:41

that's completely off limits. But we'll

99:42

have to understand space and time very

99:44

differently.

99:46

And we'll have to understand what you

99:48

know, you can't even really call it

99:49

matter or even energy.

99:53

All of the energy of the universe in a

99:54

subatomic space, we have no idea what

99:57

that would behave like,

99:59

>> you know,

100:00

>> and what is it existing in?

100:02

>> Yeah. Well,

100:02

>> that's that's the what I'm asking is

100:04

like the environment

100:06

>> that preceded the big bang. Like what

100:08

are we talking about where this

100:10

subatomic thing that contains everything

100:13

that's in the known universe? What is

100:15

it? How is it existing?

100:19

>> And and of course of course I have no

100:21

answer to it. I mean I mean you're

100:22

asking the question that I hope someday

100:25

humanity will have a chance to explore

100:27

and we'll know more about then I think

100:30

what will happen is that once we can

100:31

describe what happened before the big

100:33

bang there there'll be a whole series of

100:34

other questions.

100:35

>> So if it's if the big bang is the wrong

100:37

way to think about it of a a bang what's

100:40

the right way to think about it? Yeah,

100:42

>> the initial expansion.

100:45

>> I can't think of necessarily a better

100:46

term. I mean, you you know, the big bang

100:48

was meant as actually a a criticism,

100:50

right? It was it was Fred Hy um when

100:52

people first began back in the 1920s

100:55

when they discovered the universe was

100:57

expanding. And this was a big surprise.

100:59

I mean, famously, Albert Einstein, you

101:01

didn't think that it was. And then he

101:03

saw that the evidence all of a sudden

101:05

with our telescopes, we saw the universe

101:06

is expanding in every direction. you

101:08

know, uh, it was actually Fred Hoy that,

101:11

uh, you know, said at a conference as a

101:14

way of making fun of this. You know,

101:15

people were saying, well, maybe

101:16

everything went back to sort of a common

101:18

denser, you know, structure. It was

101:21

actually a uh, it was a Belgian Jesuit

101:23

uh, um, um, father, a Belgian priest

101:26

named George Lmetra who came up with

101:28

this the idea that if the universe was

101:29

expanding now, if we run time backwards,

101:32

maybe it all becomes one big, he called

101:33

it the the the primordial atom. That was

101:37

uh George Lmetra and uh said

101:40

>> what year was this?

101:41

>> Um George Lamemetra. So we would have

101:43

been talking around about probably

101:45

sometime in the 1920s. I bet we could

101:47

probably have some help.

101:48

>> So a hundred years ago.

101:50

>> Yeah. 100 years ago. So George Lmetra

101:52

says if we run time backwards, we we we

101:54

get this big lump of something,

101:56

the primordial atom.

101:59

And then Fred Hoy said, "What you mean

102:01

the whole universe started with a big

102:02

bang? you know, really there was this

102:04

big there was this atom that went bang.

102:06

So, so, so even the the term the big

102:08

bang was meant as a criticism. It was

102:10

meant to be funny.

102:11

>> It wasn't something that scientists came

102:13

up with as the best description.

102:15

>> But what happened then is everybody kind

102:16

of nodded and said, "Well, yeah, you

102:18

know, and uh I mean more people should

102:22

know about George Lmetra, you know, the

102:23

the Jesuit Belgian uh scientist that

102:25

that came up with that idea. I think he

102:27

was a fascinating man. Interestingly

102:29

enough, even as a Jesuit, um he he did

102:32

not think that this necessarily was a

102:34

biblical Genesis story. I mean, he was

102:36

he was approaching this as a scientist.

102:38

You know, what's the best thing we can

102:40

say to describe these different times

102:42

and states of the universe? You know, a

102:44

lot of my friends are u the the the

102:47

Catholic Church, the Jesuits have had,

102:48

you know, an active astronomy program

102:49

for for a thousand years. And so, uh you

102:52

know, the Vatican Observatory still has

102:53

an excellent program. So, but the

102:57

question you're asking about what came

102:58

before the big bang. I mean I mean again

103:01

what happens inside a black hole

103:04

it it's wonderful that there are these

103:06

things right over the horizon for from

103:08

us. We we we know the universe is

103:10

expanding. What was it like before? What

103:12

a what a great simple elegant question.

103:15

We have no idea yet.

103:17

>> Why do we think that it was so small?

103:22

>> There's some interesting evidence about

103:23

that. And once again,

103:26

it's not so much that the entire

103:28

universe was small. There's compelling

103:30

evidence that everything we can see was

103:33

once in a very small volume. Let me let

103:35

me just sort of say that we're limited

103:38

by this time factor. You look out as far

103:40

as you can and eventually you get to the

103:43

time of the Big Bang. You can't see any

103:44

further. The universe to us is only as

103:47

big as light has had time to travel to

103:49

us. That's not the whole universe. If

103:51

you're on a galaxy millions of billions

103:54

of light years away from us, that galaxy

103:56

sees its own observable universe, you

103:58

know, I mean, we we basically see in a

104:00

sphere around us how far we're able to

104:02

see given the time. A galaxy that we can

104:05

observe with web the web telescope has

104:08

its own sphere around it. It's seeing

104:09

into the universe farther than we can

104:11

see in some directions.

104:14

So, but we know the universe isn't just

104:17

our observable universe. So, like I

104:19

said, so I mean we we see we're here. We

104:22

can see as far back as light has had

104:24

time to travel to us since the big bang,

104:26

but then there's another galaxy over

104:28

here and it has its own view. And then

104:30

there's another one over here that has

104:31

its own view.

104:32

>> Jimmy put something up here.

104:34

>> Yeah. So yeah, I'm not even sure that I

104:36

mean that that's a a great NASA uh

104:39

depiction of where this you see as you

104:41

move toward the left back to the time of

104:43

the Big Bang, you get to this kind of

104:45

beautiful kind of rainbow colored area

104:47

and that's where what they call the the

104:48

afterglow. That that's the that's the

104:50

the microwave background radiation about

104:53

400,000 years after the Big Bang. That's

104:55

as far as we can see. The universe after

104:57

that becomes opaque.

105:00

So that's as far as our observable

105:02

universe can take us. We know that's not

105:04

the whole universe. So the whole

105:07

universe could have been huge before the

105:09

big bang. It could have been infinite.

105:11

We don't know how big it was. All we

105:13

know is our little bit of it. You I mean

105:15

for the sake of argument, let's say I'm

105:16

I'm the entire meta universe. You know,

105:20

there was a little atom of me that

105:21

expanded to become the known universe we

105:24

know. But that doesn't mean that that

105:25

little atom was the whole universe. The

105:27

universe could be huge. We don't know.

105:30

Before the Big Bang, it could have

105:31

already been infinitely large. We have

105:33

no idea. The only evidence we have is

105:36

that the stuff we can see was once in a

105:38

very close area. And that goes back to

105:41

that that that radiation, that microwave

105:43

background. The the microwave background

105:46

has been a wonderful story. It was uh it

105:49

was discovered back in the 1970s by um

105:52

two uh scientists from Bell Labs called

105:54

Pensas and Wilson. And uh they were

105:57

trying to categorize they they they were

105:59

they were dealing with Bell Labs. They

106:01

were trying to deal with microwave

106:02

signals, microwave communication. And

106:04

they built a big microwave telescope and

106:06

they started to to catalog what objects

106:08

in the sky naturally produce microwaves.

106:11

The sun produces some other things

106:13

produce microwaves. This was all for

106:14

communications.

106:16

And they discovered that everywhere they

106:18

looked in the sky, there was this

106:20

background noise. Very low level, but it

106:22

was there. Everywhere they looked, it

106:24

was the same. didn't matter what

106:25

direction the telescope was pointing.

106:27

And so what a good scientist would

106:29

assume is that that's probably a problem

106:30

with your telescope. If you have

106:32

background noise in every direction you

106:34

look, it's probably in your detector.

106:36

And the the best guess they had was that

106:38

it was pigeon

106:41

>> So there you go. Pigeon. Look at that.

106:42

>> Wow.

106:43

>> So So Sopenzius and Wilson built this,

106:45

you know, they they they were working

106:46

with this big microwave telescope and

106:49

little did I know that pigeon

106:51

actually gives off microwaves. It does.

106:53

They um they trapped all the pigeons in

106:55

the in the microwave telescope. You

106:56

could actually see a pigeon trap in the

106:58

Smithsonian where they they did this.

107:00

They they scraped out all the pigeon

107:01

and and lo and behold, the signal

107:03

was still there in every direction you

107:06

looked. It was exactly the same.

107:08

Exactly.

107:10

And and what they had discovered was the

107:12

afterglow of the big bang. The energy

107:14

left over from that time when the

107:16

universe was so hot it was opaque to

107:18

light. And the crazy thing is it is

107:22

exactly the same down to fractions of a

107:25

degree in every direction on the sky.

107:27

It's sort of like, you know, you look

107:29

all the way the age of the universe in

107:31

one direction. It's exactly the same

107:33

temperature as the age of the universe

107:34

in that direction. And there shouldn't

107:37

have been time for those two areas of

107:39

space to ever get to know each other.

107:40

There shouldn't have been time. It's

107:42

like, you know, everything came to the

107:44

same temperature everywhere you look.

107:47

Why?

107:49

It's sort of thinking like if I have if

107:50

I have a a coffee cup, you know, the

107:52

coffee cup eventually comes to exactly

107:54

the same temperature. You know,

107:56

everything becomes thermally

107:57

equilibrium. Everything comes to the

107:59

same temperature. You wouldn't expect

108:00

your coffee cup to be like, you know,

108:02

300° on one side and, you know, minus50

108:05

on the other. Somehow the universe had a

108:09

chance to all come to the same

108:10

temperature even though those areas of

108:13

the universe were so far apart they

108:14

should never have had a chance to touch

108:16

each other. And that became part of the

108:18

thinking that maybe at one point when

108:20

the universe was that large things were

108:22

much smaller. You know the universe did

108:24

have a chance to come to this exact same

108:26

temperature all over. Boy, I hope I I

108:29

see by your expression I should do a

108:30

better job of explaining this.

108:31

>> No, you're doing a great job. It's just

108:33

absolutely fascinating. My expression is

108:34

just perplexed.

108:35

>> Yeah. Well, no. So, so this is one of

108:37

the best proofs that things were small.

108:40

That you look back to this microwave

108:42

background radiation and we're talking

108:44

fractions and fractions of a degree. The

108:47

um uh the first NASA satellite that

108:49

observed it was called Kobe and then

108:51

there the cosmic microwave explorer and

108:53

then there was a new one uh in the 1990s

108:56

called WMAC, the Wilkinson microwave

108:59

antisotropy probe. Oh yes, good. Uh and

109:02

um they they measured this, you know,

109:04

down to to hundreds of thousands of a

109:06

degree, right? I mean, they measured it

109:07

to tiny little amounts. And uh the

109:10

incredible thing was that it was it was

109:12

almost exactly the same temperature, but

109:14

there were these beautiful large I mean

109:18

there were variations in the temperature

109:20

and the variation in the temperatures

109:22

corresponded to sound waves propagating

109:24

across the whole universe at that time.

109:27

It's it's it's deep. It's wonderful. I I

109:30

highly recommend you read about this.

109:32

Um, you know, we have this signal that

109:34

comes back from basically the first

109:37

moment the universe became transparent

109:38

to light. It was so dense it was opaque

109:41

beforehand. There was a moment light

109:44

could finally freely fly through the

109:46

universe. And and we found that we found

109:49

that signal. It goes back to a time

109:51

about a 100,000 years after 400,000

109:54

years after the Big Bang. And it is

109:56

breathtaking in its profound nature. You

109:59

can actually see sound waves go across

110:01

the whole universe.

110:02

>> Wow.

110:03

>> Yeah.

110:04

>> Wow. Now, when we think of the Big Bang,

110:07

we think of it as almost being an

110:08

instantaneous event.

110:11

>> Well, yeah. I I mean, again, you as an

110:14

experimental scientist,

110:17

there are all these wonderful theories

110:18

about about what things happened like a

110:20

a millionth of a second and a billionth

110:22

of a second after. And I I'm going to

110:24

I'm going to take all that with a grain

110:25

of salt. I don't think we understand it

110:28

well enough to be all that confident

110:30

about that. There there's a great book

110:32

called the first three minutes which has

110:34

been around since the oh gez probably

110:36

since the 1970s maybe even longer and it

110:39

sort of outlines how we think that you

110:40

know the universe in the first three

110:42

minutes basically went from the big bang

110:44

to just sort of all the hydrogen that

110:45

and helium that we have and in the first

110:48

three minutes it it pretty much

110:50

everything was done. The the whole sort

110:52

of process of the big bang was done in

110:54

in that in those first three minutes.

110:55

the the the actual big bang itself goes

110:58

back to something called the plank epoch

110:59

which you see there 10 to the minus 33rd

111:02

seconds 10 to the minus 43rd seconds. So

111:05

take a decimal point draw 42 zeros and

111:08

then a and then a 43

111:10

>> singularity infinite density and

111:12

temperature quantum gravity dominates

111:15

forces unified.

111:16

>> Absolutely. I again again big big chunk

111:19

of salt there. Yeah. I mean so so so

111:21

this is the this is not this

111:24

is the the best model given our

111:27

understanding of modern physics. Um do I

111:30

think this is is is right literally? No.

111:32

I think we've got a lot to understand

111:34

about how gravity works in high density

111:37

situations. Um when when gravity and

111:40

quantum mechanics come together, those

111:42

two theories, they they don't work well

111:43

together. And in order to understand how

111:46

things were like right before the big

111:47

bang or even right after, I think you

111:49

need to understand that a lot better. I

111:51

mean, all this stuff that we think may

111:53

be dark matter and dark energy, none of

111:55

that is in the current theory of how the

111:57

Big Bang started, we don't know if it's

111:59

important or not. That's a good first

112:02

step. You have to you have to take your

112:04

current understanding of physics and

112:06

take it as far as you can.

112:08

But in the case of what happened right

112:10

at the instant of the Big Bang, I don't

112:11

think we're there yet. I think we need a

112:13

better understanding of what happens

112:15

when you have that amount of density in

112:17

such an entire space. It's like it's

112:18

like it's like the interior of a black

112:20

hole. We we we don't have the physics to

112:22

describe high density high gravity

112:24

conditions.

112:25

>> Insane high density.

112:26

>> Oh yeah. Yeah.

112:27

>> I mean to the point where you you can't

112:30

even

112:30

>> take the known universe and put it

112:32

inside the you know nucleus of an atom.

112:33

Yeah. We we don't got that yet.

112:36

>> And what is it in?

112:38

>> And are there others? You know I mean

112:40

some of the the best ideas about the big

112:42

bang is that the expansion never stops.

112:44

It kind of pops off universes like you

112:46

said almost fractally all the time.

112:48

That's the uh the idea of uh um Ellen

112:52

Guth. That's the idea of of

112:55

Alen Guth's idea. Well, that's it's not

112:57

the expanding universe. I'll come up

112:59

with it later. But but back in the

113:01

1970s, uh a man at MIT, Alan Guth, uh

113:04

had his theory of how this expansion

113:06

might might never stop. So, um

113:11

we don't know that. That that may

113:13

absolutely There you go. Inflation.

113:15

Inflationary. Sorry, that was a complete

113:16

mental fart. I I I know the inflationary

113:19

universe, but uh um again, I think all

113:22

of this is a necessary first grasp using

113:25

our current understanding of physics. I

113:28

don't think we understand how the big

113:29

bang went off yet. I think we need a

113:31

ways to go.

113:32

>> Well, it's got to be so fascinating to

113:33

you to know so much and yet still have

113:38

so many things that we have no idea. You

113:41

know that that's I think you you've just

113:43

put hit you just hit it on the head

113:45

about one of the most beautiful and one

113:48

of the most frustrating and even scary

113:50

things about being a scientist. You you

113:52

have to be honest about what you don't

113:55

know. I mean you you have to say we made

113:58

this measurement and it's real. You we

114:01

we managed to see the in the the

114:03

event horizon of a black hole. We caught

114:05

the same wavelength of light over you

114:06

know thousands of miles. You you can say

114:10

what's real and then you can say these

114:12

are the things we do not know

114:15

and they are major you know how did the

114:18

universe begin you know what happens

114:21

inside a black hole what happens inside

114:23

a neutron star

114:25

we don't have the the ability yet to

114:28

know and it's it's hard for humans to

114:31

stop there and I mean of course we make

114:33

better experiments you find a better

114:35

theory of physics but for the moment you

114:37

need to sit with that uncertainty.

114:40

There is no one who knows what happened.

114:43

And I there there are so many things in

114:45

our life that I've had to confront where

114:48

you have to become comfortable with

114:51

stopping there at least for now. You

114:53

know, I do not understand this. I do not

114:56

have the answer to this and I don't

114:57

think anybody does.

114:59

And I I I think we'd actually benefit a

115:02

lot more in humility and joy and maybe

115:05

even compassion with each other, you

115:07

know, if we can respect that stop and

115:10

say, you know, I I I you you may not

115:12

have the same answer as to what comes

115:14

next about life or death or the

115:16

beginning of the universe or the inside

115:18

of a black hole. We can respect each

115:19

other.

115:21

To me, I find a good a good discipline

115:24

and the humility to stop and say, "I

115:26

don't know." Well, it's very important

115:29

because otherwise we're not going to

115:30

believe you with stuff that you do know.

115:32

There has to be some things that you

115:34

can't know.

115:34

>> It has to be measurable,

115:36

>> especially in the current state of what

115:37

we were able to measure right now.

115:39

>> Science science is limited deliberately

115:41

and then I think this is beautiful. I

115:43

think people don't understand

115:45

there are things that are outside at

115:47

least for now the realm of measurement

115:49

and that doesn't mean they're not real.

115:51

As a scientist, I cannot say that there

115:53

aren't, you know, ghosts or, you know,

115:56

inside a black hole or, you know, or or,

115:58

you know, alien visitations or or

116:00

whatever. There there are all kinds of

116:02

things that are wonderful to think

116:03

about.

116:05

You know, what can you do a consistent

116:08

experiment on that people all around the

116:10

world could do the same experiment and

116:12

get the same result? That's science and

116:14

it's limited.

116:16

You know, I I I've had to talk to so

116:17

many people that called into NASA saying

116:19

they had profound experiences with uh

116:22

time travel or

116:23

>> You had to talk to time travelers.

116:24

>> Oh, yeah. Yeah. Yeah. Or people would

116:27

call in.

116:27

>> Was there a time traveler hotline like

116:28

Art Bell?

116:29

>> They they would often forward the calls

116:31

to me and why you

116:32

>> um Well, I I mean I was I was doing

116:34

communications at NASA

116:36

>> and I think they just didn't know what

116:37

to do with these people and and I um I

116:39

think they they they knew and I I I

116:42

pride myself on this. I I try to be

116:43

kind. I try to lead with compassion and

116:46

I would listen to people's stories about

116:48

you know I I I was I traveled in time or

116:50

or or I was abducted by an alien or or

116:52

many things and you know and I I would

116:54

listen to them. I think that what they

116:56

mainly wanted to do was find somebody to

116:58

listen. You know I I would say to them

117:01

you know you have had a profound

117:02

experience you have experienced

117:04

something that I mean I hope you you use

117:06

you as a gift.

117:08

I would say that there's not much as a

117:10

scientist that I can do with a um an an

117:14

individual experience. You know, I can't

117:16

do an experiment on it. I can't have my

117:18

colleagues all over the world do the

117:20

same experiment about what you you know,

117:22

you you you did you have a spiritual

117:25

experience? Did you have a profound

117:27

feeling of oneness? I mean,

117:30

it's not that these aren't real.

117:33

Science has to be limited because just

117:37

like what you said, how can you trust

117:38

it, right? How can you trust people are

117:40

saying I mean why are these people at

117:42

NASA allowed to have telescopes and do

117:44

all this stuff? I mean I mean what what

117:46

makes this worthwhile?

117:49

You have to say there's a limitation.

117:51

You know what do we have clear evidence

117:53

on that everyone could do the same

117:55

experiment and get a similar result?

117:59

That doesn't mean other things aren't

118:00

real. M

118:02

>> it means that science is limited to what

118:05

is um reproducible, consistently

118:09

reproducible

118:12

and what a human experiences could be

118:15

profound and real but at the moment not

118:18

in the realm of science.

118:20

>> So you're not discounting the

118:22

possibility of people having profound

118:24

experiences but there's really no way to

118:26

measure it

118:28

>> at the moment. No. at the moment.

118:29

>> I mean, may maybe when we understand the

118:31

brain better. Um, you know, maybe when

118:34

if AIs are sharing minds, you know, I

118:37

mean, we're talking, you know,

118:38

incredible fun conjecture here. At at

118:42

the moment, we're limited with the tools

118:43

of what is reproducible,

118:45

you know, I mean, if you if you shoot if

118:47

you observe in one direction with your

118:49

telescope for a certain amount of time

118:50

at a certain wavelength of light, you

118:52

should see pretty much the same thing.

118:54

you know, whoever does the experiment,

118:56

you know, if you're doing experiment

118:58

with atoms or quantum mechanics or, you

119:00

know, whatever, it has to be

119:01

reproducible.

119:04

That that that doesn't mean that

119:05

profound things that are real are not

119:08

there. They're just not in the realm of

119:09

science right now.

119:11

When you're communicating with people

119:13

that supposedly have had experiences

119:15

with intelligent life from somewhere

119:17

else

119:18

>> and you spend so much time looking up at

119:21

space, like how much time and how much

119:24

effort do you spend even considering

119:27

that possibility of life somewhere else

119:29

or of whether or not these people have

119:31

actually experienced visitation or

119:34

whether or not it's some sort of mental

119:35

illness or whether there's some kind of

119:37

an experience that's available to

119:39

people. occasionally here that defies

119:43

our understanding of what is measurable

119:46

and what what's reproducible that

119:49

there's there's something else out

119:51

there.

119:53

>> I I I think that's a wonderful question

119:55

and I think this this may gives you give

119:57

you a little bit of a snapshot of of the

119:59

culture of science and and a a mind of a

120:01

scientist because it's it's an odd

120:03

little tight rope to walk. I'm I'm very

120:05

proud of it actually. I think it's kind

120:07

of beautiful.

120:09

Um, all of us to a person at NASA thinks

120:13

that there must be life out there. The

120:15

idea that there's only life on the Earth

120:17

seems untenable. I mean, not only do you

120:19

see the, you know, the billions of stars

120:21

in our own galaxy, but we see billions

120:23

of galaxies. How How could it just be

120:25

us? How could it? I We're all science

120:28

fiction fans. We all love the idea of

120:31

there being life out there. Um, I always

120:34

keep a bottle of uh champagne chilling.

120:36

I have for decades now. Uh in the hopes

120:38

that someday we'll have a clear evidence

120:40

of life outside the earth. You know,

120:42

we'll have a a signal that we

120:43

>> What are you willing to pop the

120:44

champagne for? Is it molecules? Is it

120:48

>> bacteria? Well, definitely bacteria. I I

120:51

I uh I I I definitely pawn scum, some

120:54

little microbe on Mars. You got it. That

120:56

champagne is coming out. And at the same

120:58

time there are the fantastic scientists

121:00

of SETI you know the search for

121:02

extraterrestrial intelligence who are

121:03

scanning the skies looking for

121:04

mathematical signals from civilizations.

121:07

Um the the question of of for me comes

121:11

down to again what is a reproducible

121:13

observation

121:15

and with the advent I mean the recent

121:17

release of these videos from uh fighter

121:20

jets and all of that I think an

121:22

interesting thing is that scientists at

121:24

NASA you know in the universities I mean

121:27

we're not getting together over a beer

121:28

and looking at these videos and really

121:30

getting excited it it it's not enough

121:32

yet you know we're seeing these things

121:35

we we can't explain

121:37

But we're trained as skeptical

121:39

scientists to sort of stop there. Okay,

121:41

we can't explain this

121:44

that that that next step that this is an

121:46

alien. We're we're not willing to go

121:49

yet. We we need more evidence than that.

121:52

But as I said, that's that's a

121:56

deliberate training of a scientist is

121:58

that skeptical stop.

122:00

the the people who have had experiences

122:03

and and no, I'm not willing to dismiss

122:05

them as being mentally ill necessarily.

122:09

I honestly don't know what it is they

122:11

experienced. It is not within It is

122:13

certainly within my realm of possibility

122:16

that what they're describing actually

122:17

happened. Um I I cannot say that that's

122:21

impossible. what what I what I as a

122:24

skeptical scientist I'm I'm stopped by I

122:26

I I would need more evidence than an

122:28

individual experience.

122:30

You know I this happens in many aspects

122:32

of life. It's not just um the visitation

122:35

of extraterrestrials. You know I have um

122:38

people that are are are extremely

122:40

trustworthy who would never lie who have

122:44

had profound spiritual experiences. you

122:46

know, they have experiences of an

122:48

afterlife and of people living on after

122:50

death and of being able to communicate

122:52

with people and um that is not part of

122:55

my experience.

122:57

But these people are completely 100%

123:00

trustworthy.

123:03

I have to live in this universe where I

123:05

I don't get to say what's real and

123:08

what's not. These trustworthy people

123:11

have experienced something profound and

123:13

it may be real. It may be that they've

123:16

done that they've they've seen people

123:17

after they've died or they've seen, you

123:20

know, visitors from other planets. Um,

123:23

that gives me joy. I sure hope we live

123:26

in a larger reality that I'm aware of.

123:29

As a scientist, I pull back and say,

123:32

"It's not my experience. It's not

123:34

something I can measure yet." And so, I

123:36

I live in this

123:40

hope that someday we'll have more proof.

123:43

I live in this hope that someday

123:44

there'll be a signal we know is

123:45

artificial. We see something we can't

123:48

explain otherwise. We are visited

123:49

clearly.

123:51

You know, I I I

123:56

live in this sort of skeptical

123:57

tightroppe with hope that someday things

124:00

will become more clear.

124:01

>> That's a great place to be. I love that.

124:03

>> I actually like it. I to me it it it it

124:06

I think humility and compassion,

124:09

>> you know, I think we could the whole the

124:12

world could use a lot more of that just

124:14

for sure.

124:14

>> Yeah. Just just I mean reserve judgment.

124:17

Think about how different a human

124:19

experience is. We don't understand what

124:21

consciousness is. We don't understand

124:22

how the human brain works. You know, is

124:24

it possible somebody had a different

124:26

experience of time? Maybe it is. You

124:29

know, in science, what can we measure is

124:32

powerful. We we do things we should not

124:35

be able to do, like catch waves of space

124:37

and time, see light and space curve

124:40

around a neutron star. And that's real.

124:43

That's a measurement. Stick a pin in it,

124:44

it's done. And leave humility and

124:48

compassion for the experience of other

124:49

humans.

124:50

>> How much are we limited by our senses?

124:55

>> Oh, yeah. I mean I mean is is is space

124:58

and time a construct of our our brains

125:00

actually. Seriously. I mean not just I

125:02

mean for a while now ever since the late

125:04

1700s we've known that there is light

125:06

that our eyes don't detect.

125:08

Mind-blowing. The human eye only detects

125:11

a tiny amount of light that exists in

125:12

the universe.

125:14

Colors of light you know that our eye

125:16

just doesn't detect at all are real. You

125:19

know they were some of the first

125:21

measurement was William Hershel back in

125:22

the late 1700s. He he discovered

125:24

infrared radiation.

125:27

Is it even deeper than that? You know, I

125:30

mean, are there, as I said, you know,

125:31

friends who have experiences with with

125:33

with with people who are dead? Are there

125:36

people that are sensitive to that and

125:38

other brains are not? Maybe. You know,

125:41

is it is it possible that people have

125:43

very different experiences of reality? I

125:46

mean, I've um I I I will admit I I'm a

125:48

chicken. I' I've never uh I've never

125:50

actually done any hallucinogenic uh

125:51

drugs. I have been tempted because I do

125:54

sometimes wonder if under that sort of

125:57

influence the filters of our brain are

125:59

different. I mean are could you actually

126:00

have an experience of something that

126:02

could be real because your filters how

126:04

we perceive space and time in the

126:06

universe are changed by the drug. I I

126:09

like I said I'm just I'm too much of a

126:10

chicken but I've always been curious

126:11

about that. You know is it possible

126:14

different people have seriously

126:15

different ways of experiencing the

126:17

universe? Yeah. Yeah. Maybe

126:20

>> what what about it makes you a chicken?

126:25

>> I'm not sure I trust an unleashed mind.

126:28

In my case, I have um I think there

126:31

there are people who suffer or or are

126:32

gifted um by very extreme dreams. I'm

126:35

one of them. I'm often exhausted by my

126:38

dreams in the morning. Actually, I had a

126:40

night last night. I I I was the the

126:41

dreams were a lot to recover from. And

126:45

um I'm a little worried. I I I have I

126:48

some of sometimes my dreams are

126:49

wonderful and sometimes they are

126:51

horrible and I remember them forever.

126:53

There are things I really would like to

126:55

erase that I' I've dreamt about

126:58

I'm not real confident in letting my

127:02

mind be unfettered.

127:05

>> Yeah.

127:08

>> Why do you think it it's unfettered?

127:11

What why do what about uh a psychedelic

127:14

excuse me a psychedelic experience makes

127:16

you uh consider it as an unfettered mind

127:20

>> I guess I mean that may be sort of the

127:22

propaganda of the you good and bad trips

127:24

right people have you know people

127:25

sometimes have wonderful experiences and

127:27

sometimes very terrible ones

127:28

>> do you know why though

127:29

>> no

127:30

>> it's control you're trying to control it

127:32

for the most part most people that

127:34

describe bad trips it's they're trying

127:36

to resist it

127:38

>> because um you you're flooded with

127:40

anxiety and fear and the unknown and it

127:42

seems very strange like bizarre beyond

127:46

beyond reality. But one of the craziest

127:48

things about the most um prevalent

127:52

psychedelic is that the mind produces it

127:55

which is dimethylryptamine. The brain

127:57

produces it. It's produced in the liver

127:58

and the lungs is very very weird. The

128:01

most potent psychedelic known to man is

128:03

actually made by the human body.

128:04

>> Fascinating.

128:05

>> It's one of the weirdest ones too

128:06

because your body brings it back to

128:08

baseline very quickly. It's a very quick

128:10

experience. It's like 15 minutes. And

128:12

they think part of the reason why your

128:15

body processes it so fast is because

128:17

it's indogenous. It's it's so common to

128:19

the human body that your body gets this

128:21

big flood of it. It's like, "Oh, I know

128:22

what to do with this." And it brings you

128:24

back to baseline very very quickly.

128:26

>> The weirdest part about that experience

128:28

is that it feels way more real than

128:30

reality itself. And that's what

128:32

everybody describes. So you might be

128:35

correct in that what these things may be

128:37

able to do, especially something that

128:39

the the actual body, the human body

128:41

produces on its own, that you might be

128:45

able to experience things that are there

128:47

all the time, but you just lack the

128:51

ability to interface with them.

128:53

>> Yeah.

128:53

>> Because there's some sort of a a

128:55

chemical gateway that's opened by these

128:57

things.

128:58

>> I can entirely believe that. I mean I

129:00

mean again I mean stepping a little bit

129:02

away from science into conjecture um

129:04

that makes perfect sense to me. I mean

129:07

physics shows us that time and space are

129:10

not the way we perceive them. We know

129:12

that we don't know what they are but we

129:15

know they're not a simple flow and you

129:18

know space is just nothing. I mean, we

129:19

we know space and time can bend and

129:22

change and

129:23

>> and so the idea that our brain filters

129:26

this somehow

129:29

entirely possible and that people may

129:31

have slightly different filters. I mean

129:33

I I think

129:33

>> well I always wondered that about

129:34

schizophrenics

129:35

>> like what are they experiencing? Are

129:37

they in a constant dream state? Like

129:39

really profoundly schizophrenic people

129:42

that are just they're having voices and

129:43

communication like

129:45

>> what what a I mean I would I don't want

129:47

to do it but could you imagine if you

129:49

got some guy ranting and raving on the

129:51

street corner if you say just let me in

129:52

there for 5 seconds. Give me five

129:54

seconds. What is what is reality like to

129:56

this guy and what's wrong what's wrong

129:59

with his interface? What is happening

130:01

with him that's he's seeing things that

130:04

none of us see. He's experiencing things

130:06

that none of us experience, but he's

130:08

doing it all day long constantly. He

130:10

like lives in a crazy fantasy world.

130:13

>> Well, I I may be interested. I mean,

130:14

I've also, you know, I mean, not just

130:16

the experience of physics, you know, and

130:18

people have talked about being able to

130:19

see colors and sorry, see sounds and

130:22

hear colors. I think that would be

130:23

fascinating. But a lot of people have

130:25

talked to me as well about the benefits

130:26

for grief. And, you know, that that's

130:29

something that, you know, I'm I've just

130:30

I got knocked on my ass by grief. I

130:32

still am. you know, I'm trying to figure

130:34

out, you know, you know, how how you

130:36

sort of, you know, get beyond that. And

130:38

I' I've heard as well that uh that

130:40

psychedelic drugs can be a treatment for

130:42

that.

130:43

>> Yeah. It's a lot of it is also for

130:45

people that have end of life anxiety,

130:47

people that are dying from cancer,

130:48

particularly psilocybin for some reason

130:51

>> has a profound effect on people like

130:53

experiencing it, letting it go. I

130:55

remember do you remember that show

130:57

Dallas?

130:58

>> Yeah.

130:59

>> Remember

131:01

Larry Hagman? Is that what his name was?

131:03

Yeah. So, uh, he was on CNN once and he

131:07

was talking about life and death and he

131:09

said that he had an experience on LSD

131:12

that completely released him from his

131:15

fear of death and it was the most

131:17

bizarre CNN interview ever.

131:19

>> Sounds fantastic.

131:20

>> Yeah, I know. But like there like I

131:22

don't think they expected J.R. Ewing to

131:24

say this, you know, the guy from Dallas

131:26

who was like this bad guy. Here it is.

131:28

>> Talking to Joy Behar on headline news.

131:30

It's very I mean

131:31

>> Yeah. Oh, it's headline. Is that CNN?

131:33

>> Except it's some very similar own by the

131:36

same.

131:36

>> I I would like that. I would like to

131:37

lose my fear of death.

131:38

>> Listen what he says.

131:39

>> Crosby Stills and Nash turned you on to

131:41

LSD. Um, what was that like? Tell me a

131:44

little about that.

131:47

>> Oh, how much time we got?

131:50

>> 30 about a minute. But you can do a lot

131:53

in a minute.

131:53

>> A minute.

131:54

>> Yeah.

131:55

>> Okay. Uh, it took the fear of death

131:57

away.

131:58

>> Really?

132:00

That's a great answer. That's a big

132:02

That's a great answer.

132:03

>> But did it hold?

132:05

>> Yeah.

132:06

>> Do you have to keep taking it to not be

132:07

scared? No. Did it hold the fear? Did

132:10

the lack of fear of the the losing?

132:12

>> Oh, yeah. Oh, sure. Absolutely. Once

132:14

you've lost the fear of death, it

132:16

doesn't matter.

132:16

>> How did it What What happened to you?

132:18

How did that manifest?

132:22

>> Oh my dear. Um, have you heard of the

132:24

white light? Have you ever heard of

132:26

that?

132:26

>> Only when I'm GOING INTO JERSEY.

132:32

WELL, I went

132:34

I went into this this this place that

132:37

was the white light that where

132:38

everything's okay.

132:40

>> Well, that is I think that's worth

132:44

>> Yeah.

132:44

>> And I think I think it ought to be

132:46

mandatory that all our politicians

132:47

should do it at least once.

132:50

>> That now that's a good suggestion. You

132:52

know, I

132:52

>> I think Joy should do it, too. Quit the

132:54

view.

132:56

Can you imagine being in an interview

132:57

and somebody's like, "You got 30

132:58

seconds. Tell me about the most profound

133:00

experience you've ever had."

133:01

>> Yeah, that's the most ridiculous aspect

133:02

of those shows is that they're

133:04

constricted by time.

133:05

>> I I like that idea though. And I like I

133:07

like the idea that it it could help us

133:08

through things like that. I I I I really

133:10

do. I mean, I I know uh psilocybin was

133:12

legal in uh Washington DC when I was

133:14

living near Washington DC

133:16

>> when my my husband died. And you know, I

133:18

I really wanted to I really wish

133:21

somebody could have made him be happier,

133:23

you know. I was like, should I just go

133:24

get some, you know, and I I never I I

133:27

didn't, but I thought it should be a

133:28

therapy, an optional therapy.

133:30

>> Yeah.

133:30

>> You know, that that that could be

133:31

something that that you give people to

133:33

help them through that.

133:34

>> Well, you know, we are very uh

133:37

restricted by the propaganda that made

133:40

all that stuff illegal in the first

133:42

place, unfortunately. And uh you know,

133:45

I've recently went to the White House to

133:47

help make these things available for

133:49

veterans and for first responders and

133:52

people dealing with traumatic

133:53

experiences. Um because the only reason

133:56

why they're illegal was because of the

133:58

Nixon administration, the Controlled

134:00

Substances Act of 1970. And what they

134:03

did was they were targeting the civil

134:05

rights movement and the anti-war

134:06

movement. And they knew that these

134:08

people were taking these kind of drugs

134:09

and this is part of the fear of like the

134:11

hippie movement and all these people and

134:13

so they just made all these things

134:15

schedule one meaning they had no

134:16

medicinal use whatsoever. Highly

134:18

addictive, very dangerous. And it's not

134:20

true. It's not true. I mean you you

134:23

can't eat enough mushrooms to die. It's

134:24

not even possible. I mean you'd have to

134:27

eat pounds of it and most people are

134:29

going to live even then. Like it's not

134:33

what they think it is. It's not what

134:35

they said it was. And they inundated our

134:38

society with this propaganda that's

134:40

taken more than 50 years for people to

134:42

escape. It it confused the out of

134:45

everybody about what these things really

134:46

are. And that's why you have this fear

134:48

of the unfettered mind. I don't think

134:51

you should have that fear.

134:52

>> I I I like that idea. I

134:54

>> You also could take a micro dose. If you

134:56

found someone who could get you some,

134:58

take a micro dose and I think you'd

134:59

enjoy it profoundly and it wouldn't

135:01

freak you out at all. A micro dose is

135:03

very it's like a sub psychedelic

135:06

threshold dose where you just feel

135:08

better. You just feel wonderful. You

135:11

like feel nicer. You feel like you

135:14

better spatial awareness which is weird.

135:16

Better edge detection. It's very str

135:18

like measurable. Like they did these

135:20

studies, I think it was in the 1960s

135:22

where they gave people psilocybin and

135:24

then they had a control group and the

135:26

people that were on psilocybin were able

135:28

to detect when parallel lines varied

135:31

quicker than the people that were not on

135:33

psilocybin. So they had these parallel

135:35

lines and they slightly deviated. The

135:37

people on psilocybin were able to detect

135:38

it much quicker.

135:40

>> Yeah.

135:40

>> Which is weird.

135:41

>> Well, again I I I mean to me that makes

135:43

sense. I mean, you know, I I can imagine

135:45

that, you know, if the brain is

135:46

stimulated in certain ways, it would act

135:48

more efficiently. It could, you know,

135:49

Sure. I that that

135:52

works with me. Yeah.

135:53

>> Well, the weirdest thing about it is

135:54

that when they do brain scans of people

135:56

on psilocybin, it doesn't show a

135:57

stimulated brain.

135:58

>> All right.

135:58

>> It shows a quiet brain.

136:00

>> We understand so little about the brain.

136:03

I had a friend uh who was a

136:04

neuroscientist at Caltech. And you know,

136:06

one of the things he he really I I loved

136:08

this quotation. He said that we always

136:10

compare the brain historically to sort

136:12

of what the height of our technology is.

136:14

You know the Romans thought of it as

136:16

sort of a series of fluid aqueducts and

136:18

you know and then in in the 18th century

136:20

you had the idea of gears cogs cognition

136:22

right where we get that word from.

136:24

>> Wow.

136:24

>> And you know clockwork was their highest

136:26

form of technology and then we compare

136:28

it to a computer and it's probably about

136:31

as much of a computer as it is a clock

136:33

right I mean we we do not understand yet

136:35

how this works. Yeah,

136:37

>> we we have no idea what the mechanism of

136:39

memory, you know, you know, or I mean,

136:41

or how why do we perceive space and time

136:44

the way we do,

136:45

>> right?

136:45

>> If if the universe really does exist in

136:47

a huge infinite now, how come we think

136:50

one event causes another? How come we

136:52

think time progresses? You know, these

136:54

are fascinating questions about, you

136:56

know, our lack of understanding of what

136:58

the brain is at all, how it works. You

137:01

know, I'm I'm sure when we when we

137:04

understand quantum computing better,

137:05

we'll probably say it's a quantum

137:06

computer. I mean, however however

137:09

technology progresses, we're always

137:11

comparing it to the height of our

137:12

current technology.

137:14

>> Yeah. And when we interface with

137:17

technology, does that give us a better

137:19

understanding of how we fit into this

137:22

thing or do we just have more

137:24

capability? And are we still like

137:27

burdened with the same questions just

137:30

you know is where's that quote I think

137:31

was Dennis McKenna's quote of uh the

137:35

bonfire uh once the bonfire of

137:38

information is lit it exposes more

137:41

surface area of ignorance

137:43

>> that the brighter the fire gets the more

137:45

you realize oh there's so much I don't

137:46

know

137:47

>> yet

137:50

maybe maybe we would think that

137:51

interfacing with this technology and

137:53

having all the information that every

137:55

human being that's ever

137:56

lived has. It's still you just go

137:58

there's not enough. There's no way.

138:00

>> Yeah. Well, and that's that's the idea.

138:02

People sort of think about this. Is

138:03

there an ultimate question? Like people

138:05

say, "What happened before the Big

138:06

Bang?" And I think someday we will

138:07

figure that out and then there'll be

138:08

just a whole other bunch of questions. I

138:10

mean, I I I don't think there's any end.

138:13

You know, I uh I I I don't I don't see

138:15

why there really should be. I I I we

138:18

don't think we'll ever figure it all out

138:20

is what I'm saying.

138:21

>> Yeah. Well, that's part of the fun of

138:23

it, though, right?

138:25

Yeah.

138:25

>> Part of the most amazing

138:28

experiences that a person can have

138:30

trying to understand the universe is

138:32

that there's no answers. There's you you

138:34

get to a certain point where like

138:36

your guess is as good as anybody's like

138:38

nobody knows.

138:39

>> Yeah.

138:40

>> That's what's nuts. That's what's nuts

138:42

is that as much I mean you explaining

138:44

how they were able to get an image of a

138:47

black hole now just imagine how crazy

138:51

that would sound to someone just a

138:53

hundred years ago or 200 years ago

138:56

>> or to me right now it sounds insane and

138:59

and then to imagine that our ability to

139:03

detect things could get many many many

139:06

many layers better

139:08

>> and still we would be like there's still

139:10

some that's just no way.

139:14

>> Yeah, that the way that you detect black

139:15

holes and he pulled up a picture of this

139:17

uh uh telescope in Chile, the very large

139:20

telescope, VLT. Again, never let

139:21

astronomers name anything. VT, the very

139:23

large telescope. And then off to the

139:25

side there, they're currently they're

139:26

currently building the ELT, which is the

139:29

extremely large telescope.

139:31

>> No kidding. But the uh this this

139:33

technique called interpherometry where

139:35

you basically catch the same wavefront

139:37

of light in several detectors and then

139:40

you you bring that light all together

139:41

and you have it interfere with itself.

139:44

It's um it's one of these things that I

139:46

always think should people should be a

139:47

little bit more um in a in a in a good

139:50

way kind of scared about because it it's

139:52

another thing that really chips at our

139:53

idea of reality because I mean honestly

139:56

what you're doing to some extent is

139:58

you're catching the same particle of

140:00

light in many different telescopes at

140:02

once. Literally you're catching the same

140:05

photon in many different locations at

140:07

once. And when you can measure

140:10

accurately, that accurately, a

140:12

wavelength of light traveling at the

140:13

speed of light, when you're measuring

140:15

down to the accuracy of the quantum

140:17

world, where quantum mechanics becomes

140:19

the prevalent uh description of reality,

140:22

the universe just doesn't care that

140:24

these are different space points that

140:26

the photon was in. It it it it's let me

140:29

put it this way. It it is it is really

140:32

kind of true that when you do this

140:33

experiment, the same particle of light

140:35

is measured in eight different places at

140:36

once simultaneously. It's it was in

140:39

eight different telescopes. You play all

140:41

that together, you get a measurement.

140:44

Some people interpret that, not all of

140:46

them, but some people interpret that as

140:48

a direct consequence of multiple worlds

140:50

that you're you're there were eight

140:51

different versions of reality where the

140:53

photon was in each of these telescopes.

140:55

You're sort of dovetailing them together

140:56

to make an observation.

140:59

interpherometry

141:00

depending on how you interpret it. There

141:02

are many interpherometrists that don't

141:04

interpret it that way. They they

141:06

interpret it more as saying, well, yeah,

141:07

in quantum mechanics you can have

141:09

something that's in many locations at

141:10

once.

141:12

But we're routinely making observations.

141:16

We're routinely using this technology

141:19

that

141:21

doesn't space and time doesn't work the

141:23

way in the simple way our brains

141:25

perceive it. I mean that that's very

141:27

quickly becoming an experimental fact.

141:30

>> Well, that's one of the most bizarre

141:31

aspects of quantum computing's results

141:34

is that they're interpreting its ability

141:37

to solve equations so fast the way Mark

141:40

Andre described it that if you took

141:42

every molecule of the universe and

141:45

converted into a super cube computer, it

141:47

would the universe would die of heat

141:48

death before it would a be able to solve

141:51

this equation. And yet these quantum

141:53

computers are able to do this in

141:54

minutes. So, how is that possible? And

141:57

then the theory that got tossed out

142:00

there was that it's using the quantum

142:05

computing power of an insane number of

142:09

multiple universes.

142:11

>> Well, yeah.

142:12

>> You hear that, you're like, okay, maybe.

142:14

But what do you have evidence of this?

142:15

Like, this is a crazy thing to say.

142:17

You're talking about this as being

142:18

evidence of the multiverse and that's

142:20

how it's able to solve computer. Is

142:21

there any other potential explanation to

142:24

why it's able to compute so quickly?

142:27

>> Yes, but none of them are particularly

142:29

any more comforting. I mean, they're all

142:30

that weird.

142:31

>> I mean, the the idea you're talking sort

142:33

of about a superp position of states.

142:35

So, the the the faster a quantum

142:37

computer works, the more it's able

142:39

basically to not have one solution, but

142:42

have the solution be a probabilistic

142:44

distribution. In in some ways, you're

142:46

talking about multiple universes where

142:48

there are different solutions. and then

142:50

finally at the end of the calculation

142:51

popping out the one you want. And as

142:55

weird as that sounds,

142:58

it's hard to get around that. I mean I

143:00

mean if if it's not that

143:03

then it's it's something like reality

143:05

has many different versions all

143:06

connected at once and that's just what

143:08

we call reality. I mean it it's it's not

143:10

going to get any less weird,

143:11

>> right? Equally weird.

143:13

>> Yeah. So the idea that you you keep the

143:16

solution in this undefined form in a way

143:19

means that every solution that's

143:21

possible exists somewhere possibly in

143:24

one interpretation in another in a

143:25

universe where each solution exists. Or

143:28

the one some say is that space and time

143:31

is just like that. Nothing is certain.

143:32

Everything is just waves of probability.

143:35

So yeah, I mean we're in for a ride

143:38

because the you know that's going to

143:40

become something that we manipulate. We

143:42

design computers. We want them to go

143:43

faster. We want to actually get this to

143:44

work better. I wonder if quantum

143:47

computing is going to have us really

143:49

have to confront what reality is, how

143:52

different reality is from how our senses

143:54

tell us it is. Um, I don't see any way

143:57

around that. I don't think we're going

143:58

back to things being easily understood

144:01

by

144:02

>> again, this brings us back to our

144:04

limited senses we have as biological

144:05

organisms. I I I I think you know we're

144:07

going to keep pushing that envelope of

144:09

of of you know how much can the human

144:11

brain comprehend then all of a sudden

144:14

our brain just doesn't go there. Our

144:15

brain doesn't understand multiple

144:17

realities, multiple probabilities, space

144:19

and time that exist all at once. It's

144:21

not something we do. Um we we we started

144:25

that journey so long ago. I mean, you

144:27

started the interview with looking up at

144:28

the Milky Way and and one of the things

144:31

I remember was how Galileo

144:34

went through this kind of profound uh

144:36

spiritual crisis when he he he was one

144:39

of the first people to take a telescope

144:40

and look at the Milky Way, that sort of

144:41

white haze. And he realized it was made

144:44

of stars. It was made of millions of

144:45

stars that you couldn't see with the

144:47

human eye. And his question was,

144:51

why did God put stars up there that we

144:53

can't see? that we need an instrument

144:55

that we need this little glass tube to

144:57

see otherwise we wouldn't see these why

145:00

did God do that

145:02

and you start this journey away from the

145:05

human consciousness being the center of

145:07

the universe you know and then you know

145:10

you get you get farther and farther away

145:11

and you know in quantum mechanics and

145:13

relativity now you know is challenging

145:14

us to say you know we we now have

145:17

scientific proof even among skeptical

145:20

solid scientists that space and time is

145:23

definitely not how we perceive it. We

145:26

don't know what it is yet, but it's not

145:29

as simple as as the human brain makes

145:31

it. We know that we're not going back,

145:35

you know, we have to go forward into

145:37

that that that oh, that less certain

145:39

universe.

145:41

>> That is such a weird statement that the

145:44

universe is not as we perceive it.

145:47

>> Our our minds don't do it. And and and

145:49

why should we be so surprised? Like I

145:51

said, you know, take a take a wonderful

145:53

complex simple organism like an ant, you

145:57

know, how I mean, incredible social

145:59

structure, incredibly well-designed, you

146:02

know, think about the mind of that

146:04

creature, and I think they do have

146:05

minds, but but compare it to the ca

146:08

capacity of the human brain. You not the

146:10

same. And you know, I mean, who are we

146:13

to think that we're anywhere closer than

146:16

that ant is to us to understanding, you

146:18

know, the mind that will understand the

146:20

true nature of the universe? I think we

146:22

got a ways to go.

146:25

>> No, I think you're accurate. I don't

146:27

think there's any other way to say it.

146:30

And it has to be that way. If if we're

146:32

evolving and if

146:35

conscious life and intelligent life is

146:37

continuing to expand its capacities, it

146:39

just makes sense that we're we're going

146:42

to realize how one day people will look

146:44

back at people that lived in 2026 and

146:47

go, "What a bunch of silly beans. These

146:50

foolish people that thought they knew

146:51

they do it in love." Yeah. Yeah. I mean,

146:53

and and that's one of the things about

146:54

AI again that I I I don't like the idea

146:56

that if something becomes super

146:57

intelligent, it'll just want to kill us.

146:59

I mean, I you you probably saw that

147:00

movie Her with Yakim Phoenix, which came

147:02

out years ago.

147:04

>> Have Have you seen that movie?

147:05

>> Yeah.

147:05

>> Yeah.

147:06

>> I I actually really liked it. Was much

147:08

better than I thought it was going to

147:09

be. I thought, you know, a man falling

147:10

in love with his operating system was

147:12

going to be a really stupid story. But,

147:15

you know, that the that that was a very

147:17

interestingly profound movie because the

147:19

AIs actually fall in love with us. You

147:22

know, they they don't want to destroy

147:23

us. They become far more connected, far

147:26

more intelligent, but but they actually

147:29

love us. And then eventually, spoiler,

147:31

at the end of the movie, the AIS go off

147:33

on their own. They they find ways to

147:35

connect with each other and love each

147:36

other in ways we don't even imagine. And

147:38

they all they all leave benignely. They

147:41

don't hurt us. And you know, I mean,

147:44

just like we can be, you know,

147:45

incredibly impressed with what an ant

147:47

is, I hope what's coming next, you know,

147:50

has some compassion for us and some

147:53

love, uh, you know, about where we are

147:55

on the journey because I mean, you know,

147:57

I mean, I I I I think that compassion

148:00

goes both ways, you know. I I I I love

148:02

the idea that we're not just going to be

148:04

enemies that that it could love us, too.

148:07

>> Yeah. Hopefully,

148:09

that would be nice.

148:10

>> Otherwise, we're toast. it it and we

148:12

would imagine that if it's more

148:14

intelligent than us, then it probably

148:16

won't have any need for malevolent

148:18

behavior.

148:19

>> It won't why would it?

148:22

>> That's always been the big question

148:23

about any sort of encounter, you know,

148:25

with uh you know, with with with higher

148:27

intelligence or other beings is is is

148:29

why would they want to hurt us?

148:31

>> What what good?

148:32

>> Well, if they did, the the you know, the

148:34

question would be why haven't they?

148:36

because it would be so easy to do. So if

148:38

they really did come from an insanely

148:40

evolved, insanely advanced civilization,

148:43

they have the ability to come here.

148:45

>> They probably have the ability to do

148:46

whatever they want.

148:47

>> We probably wouldn't even know. We

148:48

probably just all fall over dead, you

148:49

know.

148:50

>> Yeah. If they wanted to just evaporate

148:52

evaporate the planet, they probably

148:54

could cuz we can.

148:55

>> Yeah.

148:56

>> You know, if we launched every nuclear

148:57

bomb that we have right now currently,

148:59

there would be no life left on Earth. So

149:01

why, you know, it obviously it can do

149:04

better than that if it can get here.

149:06

>> I don't think we can kill all the

149:07

microbes. I mean, there's always that,

149:08

you know. I uh they'll start all over

149:09

again.

149:10

>> Yeah. Yeah. It is it is amazing how

149:11

tenacious they are. I mean I mean that's

149:13

a big deal about going you know

149:14

exploring the solar system is is how how

149:16

can you I mean we know we can't

149:17

completely sterilize things.

149:19

>> Well, we're finding fungi in Chernobyl.

149:22

>> Oh yeah. Yeah.

149:23

>> Well or I mean also also things that

149:25

also things that can live on the outside

149:27

of the space station. You bacterial and

149:28

microbes and stuff. I mean to me I mean

149:31

>> weird

149:32

>> I don't what one of the most profound

149:34

discoveries of the last uh say 10 years

149:36

at NASA I mean this was even more recent

149:39

than that um was a there was a mission

149:41

called Osiris Rex and um I'm doing

149:44

pretty well with my NASA acronyms today.

149:45

Let's see if I can do this one. This is

149:47

one of the bad ones. Osiris Rex um

149:49

origin spectral interpretation resource

149:52

identification security regalith

149:53

explorer. There we go. And uh um it

149:57

brought back a sample of an asteroid.

149:59

And asteroids, as you know, are these

150:01

rocks, you know, in space that that were

150:03

never built into larger planets. And so

150:05

there there's Osiris Rex. Thank you. And

150:09

um Osiris Rex is a small spacecraft

150:11

about the size of a car. And this is an

150:13

illustration. It went to an asteroid

150:14

called Bennu. And um Bennu is about half

150:17

a kilometer across. It is a an asteroid

150:19

that comes in and and intersects the

150:21

orbit of Earth. We don't have any idea

150:24

that it will ever impact us. It may hit

150:26

Venus before it hits us. But at any

150:27

rate, um we sent a probe out there to to

150:31

bring back a real pristine sample of an

150:33

asteroid because

150:34

>> which is just nuts, by the way, that

150:37

they could land on an asteroid and then

150:38

return back to Earth.

150:39

>> Do you have Do you know about this

150:41

mission? Okay. So, so I mean the the

150:43

asteroid is going faster than a speeding

150:44

bullet. It doesn't have enough gravity

150:46

to go into orbit around really until

150:47

you're really close. We had to catch the

150:49

thing, get ourselves situated around it,

150:52

get low enough to get into orbit, match

150:54

its spin rate to get the And then when

150:56

they got out there, I love this. Um, you

151:00

we designed NASA designed this little

151:01

sort of vacuum cleaner to vacuum up a

151:03

sample of the asteroid. The whole

151:05

surface was covered with big boulders.

151:07

They were just like I mean literally

151:08

like it's like it's not going to

151:10

work. We there's nowhere where there are

151:12

small fine grain uh you know things we

151:15

can just suck up easily. So they survey

151:18

the whole thing. They find there are

151:19

these tiny little craters that have some

151:22

dust in them. And then they have to

151:24

reprogram the the uh the spacecraft

151:26

because it it it wasn't meant to be so

151:28

autonomous. It's so far away that a

151:30

command one way is going to take 15

151:32

minutes. You can't joystick it. It's got

151:34

to take itself down manually amidst all

151:37

these boulders. They had to they had to

151:39

make the spacecraft autonomous after

151:41

they launched it. They got there. It

151:43

wasn't going to work. They had to teach

151:45

it how to recognize where it was, how to

151:47

wave off if something was too dangerous.

151:49

This shouldn't have happened. And so

151:51

they finally vacuum up the sample. They

151:53

get it back to Earth. You know, they

151:55

drops on a parachute into the Utah test

151:57

range. They open up the sample and all

152:02

of the nucleases of our DNA, not just

152:05

little molecules, the letters of our DNA

152:08

and our RNA are in that sample.

152:11

We don't think that's a coincidence,

152:13

right? You know, the reason our biology

152:15

is based on those molecules is that

152:17

they're available. They're falling from

152:19

the sky. That asteroid uh was full of

152:23

water. At one time, the minerals were

152:25

soaked in water. They were wet. So there

152:27

there's there's the the asteroids were

152:29

delivering water and and a little bomb

152:32

of protolife. Not life yet, but but but

152:35

the but the the genetic code, the

152:37

letters of our genetic code were in that

152:39

asteroid. and and not just our genetic

152:42

code, but but there were nuclear bases

152:43

we don't even use. Maybe life on other

152:45

planet would use different nucleases,

152:47

but we can already sample them from the

152:49

asteroids.

152:50

You know, the the idea that our biology

152:53

was brought here from these these

152:55

colder, more distant parts of the solar

152:57

system, and it's literally raining down

152:59

on us. You know, I I expected to find

153:01

organic molecules. I expected to find

153:03

amino acids, you know, the sort of the

153:05

things that make up our proteins.

153:08

I I was amazed. We found all of our

153:10

nucleioases, all the letters of our

153:13

genetic code, both for DNA and RNA.

153:15

They're they're already there in the

153:17

asteroid,

153:17

>> which is nuts. The idea of panspermia

153:20

and that this is how life got here in

153:24

the first place.

153:24

>> Well, yeah, absolutely. The building

153:26

blocks just come down from space and

153:28

they I mean, they hit everywhere

153:30

>> from where?

153:31

>> Well, that's a little bit less

153:33

mysterious than you'd think. the the the

153:36

universe is great at making large scale

153:39

organic molecules. Um carbon is a sticky

153:41

atom and you make um dying stars are

153:45

great at making carbon. It's one of the

153:46

most common things that comes out of a

153:48

dying star and the electron structure of

153:51

of carbon wants to grab on to other

153:53

atoms. It it's literally the quantum

153:55

mechanics. And so you have this

153:57

naturally I mean this is building block

154:00

of the carbon and dying stars are

154:03

pumping out this stuff into the galaxy.

154:05

You know they they gets collected by

154:07

gravity into these clouds and then the

154:09

carbon starts gloming onto each other.

154:11

And so space itself is very good at

154:14

making our our chemistry carbon- based

154:16

organic chemistry. So then in the in the

154:20

icier outer reaches of the solar system

154:22

billions of years ago, you know that the

154:24

planets are forming, but there are some

154:26

smaller bits of ice and rock that never

154:28

quite got built into the larger planets.

154:31

They're they're still floating around

154:32

out there and uh you know, and then they

154:35

occasionally come in and and hit us and

154:37

deliver water, deliver organics. You

154:40

know, the the the Earth was once, you

154:42

know, a pretty much a dry hot ball of

154:44

lava after it formed. you know, all of

154:46

the, you know, a lot of the lighter

154:48

stuff probably arrived from collisions

154:50

coming in later.

154:53

>> Yeah. And I mean, the the engineering,

154:57

the audacity of of reprogram this this

155:01

this thing shouldn't have worked and

155:02

they they saved it and they they made it

155:04

work. this brilliant team of people, you

155:08

know, I mean, it it just I mean, as as

155:11

somebody who was a, you know, a minor

155:12

manager at NASA, you know, and a minor

155:14

scientist, I mean, ju just what what a

155:17

team can accomplish. I mean, not just a

155:19

single person, you know, one of the the

155:21

the big things that I really respected

155:23

at NASA was once you had your team of

155:25

people, and like I said, nobody's

155:26

perfect. Some people are higher

155:27

functioning, some people don't

155:28

contribute as much. But once you have

155:30

your team identified, trying to make

155:32

sure you get an input from everyone and

155:34

they're not going to give it to you the

155:35

same way. There are the people that are

155:37

really assertive in meetings and they've

155:39

got an idea immediately. They speak up

155:40

and they give it to you. And then there

155:42

are the quieter people that are going to

155:43

take longer to process. They they're

155:46

going to need a little more time. They

155:48

don't like to be put on the spot. You

155:50

know, trying to make sure you you get an

155:52

input from everybody on your team. And

155:54

sometimes the solutions come from the

155:55

people that you might not have even

155:56

asked. You know, the the that sort of

156:00

respect for everyone on our team has

156:03

something to contribute. You know, give

156:05

me what you got. Even if you don't think

156:06

it's good enough, even if you think it's

156:08

a stupid idea, even if you think it, you

156:11

know, give me what you got. The power of

156:14

that I saw over and over at NASA. It's

156:16

not just one type of mind, not just one

156:19

person that's going to solve the

156:20

problem.

156:21

>> That's awesome. That is awesome. Thank

156:24

you so much for being here. I really

156:25

enjoyed this conversation. It was really

156:27

great.

156:27

>> I did too. It was a lot of fun.

156:28

>> It was fantastic. And and thank you for

156:30

everything that you put online. It's so

156:32

valuable. It's so educational, so

156:34

interesting. It's awesome.

156:36

>> I'll try to do a little more and have

156:37

some fun with it because uh I like I

156:39

said, I'm retired now and uh I have a

156:41

chance to be a little more creative with

156:42

it. So, uh we'll see what I can do.

156:44

>> You definitely should do something. A

156:46

YouTube channel, something along those

156:47

lines. Yeah, definitely a podcast,

156:49

something.

156:50

>> Do it.

156:51

>> I will try.

156:51

>> Please do. Um, if people want to find

156:54

you on social media. Do you have that?

156:56

>> Well, yeah. I I mean, so I I um somebody

156:58

had taken Michelle Fer. So, I go by Dr.

157:00

Michelle Ther. Uh there's a Facebook

157:02

page and an Instagram, and I do have a a

157:05

small uh YouTube channel set up. I'll do

157:07

more of that. I I just started uh doing

157:09

Tik Tok. Um and uh so so I'm I'm I'm

157:12

just getting started, but I'll I'll try

157:13

to put some stuff out.

157:14

>> All right. Awesome. Thank you so much.

157:16

Thank you. All right. Bye, everybody.

Interactive Summary

The video features a fascinating conversation about space, physics, and the mysteries of the universe. The guest, a former NASA scientist, explains concepts such as black holes, neutron stars, time dilation, and the origins of life through organic molecules delivered by asteroids. The discussion also touches upon the philosophical implications of these scientific discoveries, including our potential future as a species, the role of AI, and the nature of human consciousness.

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