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<v Speaker 1>Hey, everyone, This is Katie Mack, your friendly neighborhood cosmologist

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<v Speaker 1>and connoisseur of cosmic catastrophes. It's been a while since

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<v Speaker 1>I've talked to on ologies, and a lot of things

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<v Speaker 1>have been happening since that time. I have published a

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<v Speaker 1>book called The End of Everything, Astrophysically Speaking, which is

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<v Speaker 1>all about different ways the universe might end and what

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<v Speaker 1>those would look like. And I've moved to a new place.

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<v Speaker 1>When I recorded this, I was just about to start

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<v Speaker 1>a job at North Carolina State University, where I was

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<v Speaker 1>an assistant professor of physics, and about a year ago

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<v Speaker 1>I moved to the Perimeter Institute for Theoretical Physics in Ontario, Canada,

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<v Speaker 1>and there I have a really cool job title, which

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<v Speaker 1>is the Hawking Chair in Cosmology and Science Communication. And

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<v Speaker 1>at the Perimeter Institute, I continue my research on dark matter,

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<v Speaker 1>and I work on a number of other early universe

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<v Speaker 1>kinds of questions, and I do a bunch of public

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<v Speaker 1>engagement outreach things like that, give a lot of talks,

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<v Speaker 1>I do radio things, and I'm working on a new

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<v Speaker 1>book which will come out in a couple of years

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<v Speaker 1>that's about particle physics. So this episode is an episode

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<v Speaker 1>from twenty seventeen. The end of twenty seventeen, and a

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<v Speaker 1>lot has happened in physics since then. In terms of

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<v Speaker 1>what I talked about on the episode, there's a bit

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<v Speaker 1>of an update for the Ligo experiment. At the time,

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<v Speaker 1>there were just a handful of detections of black holes

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<v Speaker 1>colliding and other galaxies, which is just amazing. But now

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<v Speaker 1>there have been something like ninety detections of black holes

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<v Speaker 1>colliding in other galaxies. There'll be some discussion in the

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<v Speaker 1>episode about gravitational waves that we see from those. Another

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<v Speaker 1>thing that we talked about is super massive black holes

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<v Speaker 1>and what they would look like if you could see them,

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<v Speaker 1>and in the movie Interstellar there was a simulation of

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<v Speaker 1>what that would look like. Since then, astronomers I've actually

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<v Speaker 1>seen that they've actually seen the light from stuff falling

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<v Speaker 1>into black holes and the black hole shadow that's produced

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<v Speaker 1>when the light gets eaten by the black holes. So

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<v Speaker 1>there's an experiment called the Event Horizon Telescope project where

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<v Speaker 1>astronomers basically linked together telescopes all over the world and

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<v Speaker 1>created an image of a couple of supermassive black holes. So, yeah,

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<v Speaker 1>really exciting stuff. Check out those things, and I hope

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<v Speaker 1>you enjoy this little blast from the past of cosmology.

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<v Speaker 2>Hey, welcome to Ologies. I'm your Allie Warren, the host.

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<v Speaker 2>Now each week I sit down with an ologist, I

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<v Speaker 2>ask why do they love what they do? What is

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<v Speaker 2>your deal? What should we know about it? And this

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<v Speaker 2>week we cover the whole fucking universe which has existed

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<v Speaker 2>and it's expanding and you're floating in it and you're

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<v Speaker 2>made out of particles and matter and forces we don't

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<v Speaker 2>even understand, and maybe there are multiverses and is this reality?

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<v Speaker 2>And what are you doing here? And does anything matter?

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<v Speaker 2>And of course it does. But should you be afraid

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<v Speaker 2>of wearing bright lipstick or dancing in public? Probably not. No,

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<v Speaker 2>in the scope of things, and the scope of things

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<v Speaker 2>is really it's giant. It's called cosmology. Now, if you

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<v Speaker 2>think that you listen to this episode already because you

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<v Speaker 2>learn some stuff about beard care and face wash, think again, suckers.

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<v Speaker 2>That was cosmetology. This week is cosmology, the study of

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<v Speaker 2>the cosmos. And so when I say this episode is

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<v Speaker 2>like everything, it's actually everything. It's the whole universe. It's

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<v Speaker 2>it's a lot, it's a lot, it's so much it's

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<v Speaker 2>a two parter. It's a two fur So this week

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<v Speaker 2>we'll get the nuts and bolts of what astrophysics is,

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<v Speaker 2>and after about an hour you will walk away cocktail

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<v Speaker 2>party literate on goddamn astrophysics. Kind of I don't know.

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<v Speaker 2>I'm learning here with you. Of all the episodes I've done,

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<v Speaker 2>this was probably the one I knew the least about.

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<v Speaker 2>So let's learn together, shall we? Part two of this now?

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<v Speaker 2>Next week? Are your questions submitted via Patreon and the

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<v Speaker 2>Ologies Podcast Facebook group. Y'all had good ones. Next week

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<v Speaker 2>will address them now. The etymology of cosmology Cosmos with

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<v Speaker 2>a K is the kicky little Greek word for world

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<v Speaker 2>or order. So cosmology is a study of planets and such, sure,

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<v Speaker 2>but also why and what and how? Where? What's huh?

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<v Speaker 2>It's the study of what. This week's cosmologist is someone

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<v Speaker 2>I've had a fawning Twitter fascination with for a while,

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<v Speaker 2>and I met through a group of science friends I love,

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<v Speaker 2>known to some as the nerd Brigade. Were kind of

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<v Speaker 2>like a gang but with a website. But I was

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<v Speaker 2>always kind of intimidated by her because she is, in

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<v Speaker 2>her own words, an academic nomad and She continent hops

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<v Speaker 2>while studying particle physics and black holes and gravitational waves,

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<v Speaker 2>and she hangs out with Stephen Hawking. So when I

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<v Speaker 2>met her through friends, I usually just sat at brunch

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<v Speaker 2>like a barnacle and tried to look away when she

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<v Speaker 2>caught me staring at her, so I asked her to

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<v Speaker 2>be on the podcast. She said yes, and I immediately

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<v Speaker 2>started perspiring. So she came to my apartment. We sat down,

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<v Speaker 2>and my usual hour interview stretched to almost two, hence

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<v Speaker 2>the two parter. Hours before she politely reminded me that

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<v Speaker 2>we were supposed to be meeting people for a movie

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<v Speaker 2>and we should stop. I'm so so glad we did

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<v Speaker 2>this podcast because I got to know her even better

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<v Speaker 2>as a friend, which, y'all, I'm going to be cheesy

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<v Speaker 2>and say it's a true honor. So in this episode,

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<v Speaker 2>you'll learn about the things that make you you, and

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<v Speaker 2>the stars that exploded to make the things that make you,

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<v Speaker 2>and the scale of our existence in space, and what

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<v Speaker 2>it feels like to be heckled by Stephen Hawking and

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<v Speaker 2>if this is real life, and if astrophysicists are just

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<v Speaker 2>like making bullshit up that the rest of us just

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<v Speaker 2>accept because we're like, man, I don't even know how

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<v Speaker 2>to read these equations. So okay, So you'll get at

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<v Speaker 2>the very least a loose grasp on just the whole

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<v Speaker 2>of existence and maybe steel yourself to be the biggest

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<v Speaker 2>you you want to be, and more importantly, get to

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<v Speaker 2>know better one of the world's finest voices in cosmology.

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<v Speaker 2>You know her as astro Kti on Twitter aka astrophysicist

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<v Speaker 2>Katie mac. So take me back to defining some stuff

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<v Speaker 2>because as a layman, as a lay woman over here,

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<v Speaker 2>a lay human, Yes, I don't know the difference between

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<v Speaker 2>a physicist, an astrophysicist, a particle physicist, an experimentalist, a cosmologist,

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<v Speaker 2>and an astronomer. I don't know what those are, and

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<v Speaker 2>I'm either going to have to Wikipedia this or I

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<v Speaker 2>can have you give me a down.

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<v Speaker 1>So these things are, they're a little bit like fluid,

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<v Speaker 1>these definitions. So astronomer is basically somebody who studies space

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<v Speaker 1>in some way. And usually when people say astronomer versus astrophysicists,

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<v Speaker 1>usually astronomer is like more on the observational side or

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<v Speaker 1>sort of describing stuff in space. Astrophysicists is more about

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<v Speaker 1>like trying to understand how the physics of the thing

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<v Speaker 1>in space works. So you can be an astrophysicist trying

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<v Speaker 1>to understand how galaxies form, for example, and so you're

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<v Speaker 1>applying physics to this stuff in space. If you're a

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<v Speaker 1>particle physicist, you're working on like how particle interactions work,

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<v Speaker 1>so like you know anomsmasters and things. Large Tadron Collider

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<v Speaker 1>exposon usually. I mean the like classic particle experiment is

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<v Speaker 1>you take two particles and you smash them together and

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<v Speaker 1>you see what comes out. That's what the Large tadronical

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<v Speaker 1>is doing.

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<v Speaker 2>Now. The LHC, that's what you call the Large Hadron

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<v Speaker 2>Collider when y'all are tight. So you've maybe heard of it,

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<v Speaker 2>you kind of know, like it's a thing in Europe,

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<v Speaker 2>maybe has something to do with atoms. I looked into it.

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<v Speaker 2>The Large Hadron Collider is located near the France Switzerland border,

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<v Speaker 2>and it's a circular tunnel. It's over five hundred feet

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<v Speaker 2>deep in some parts, and it's seventeen miles around. It

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<v Speaker 2>is the largest machine in the world. So this thing

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<v Speaker 2>consists of over twelve hundred magnets and they're cooled to

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<v Speaker 2>a temperature colder than outer space, and then the magnets

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<v Speaker 2>accelerate protons to almost the speed of light, and then

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<v Speaker 2>the protons are bashed together. It's very punk rock, very expensive.

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<v Speaker 2>The LHC was mostly completed in two thousand and eight.

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<v Speaker 2>Over ten thousand scientists and engineers worked on it. Now

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<v Speaker 2>in photos it looks kind of like a giant, well

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<v Speaker 2>lit subway tunnel, but with less p and rap. If

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<v Speaker 2>you're like, I can't remember what a proton is because

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<v Speaker 2>I'm not required to anymore I'm not in school, don't worry.

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<v Speaker 2>Neither did I. I had to google, like how does

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<v Speaker 2>an atom work? I forgot, so I'll brush you up.

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<v Speaker 2>So matter is stuff, and molecules are some atoms stuck together.

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<v Speaker 2>Atoms are made of a nucleus, which is a little

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<v Speaker 2>cluster of neutrons and protons. Protons have a positive charge,

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<v Speaker 2>pro electrons have an equal negative charge, and electrons are

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<v Speaker 2>bebopping zooming around whirling derbish style outside of the nucleus.

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<v Speaker 2>So the neutrons and protons, which are the ones that

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<v Speaker 2>are just cuddling in the nucleus, those are made of

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<v Speaker 2>smaller particles called quarks, and the quarks come in a

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<v Speaker 2>couple different varieties. So what gives these particles their mass?

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<v Speaker 2>What are they? Where do they come from? We've got

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<v Speaker 2>all these little tiny things that make up matter. Okay,

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<v Speaker 2>so I heard it explained that there's a field called

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<v Speaker 2>the Higgs field. It's named after one alive and well

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<v Speaker 2>Scotsman physicist named Peter Higgs. And how a particle interacts

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<v Speaker 2>with the Higgs field gives it its mass, kind of

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<v Speaker 2>like drag in water. So Higgs bosons are particles. They're

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<v Speaker 2>an excitation of the Higgs field. It's kind of like

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<v Speaker 2>a drop of water splashing from an ocean. So the

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<v Speaker 2>Large Hadron Collider smashed protons together to see if they

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<v Speaker 2>could prove that the Higgs boson exists. And guess what,

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<v Speaker 2>bitches it does. You're not bitches. Some people call this

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<v Speaker 2>the God particle because it's so fundamental to all matter

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<v Speaker 2>in the universe. Does doctor Higgs like this name? No,

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<v Speaker 2>he's an atheist. He thinks it sucks. And the guy

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<v Speaker 2>who coined it the god particle actually wanted to call

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<v Speaker 2>it the goddamn particle, but his publisher made him change

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<v Speaker 2>it in a book. So the Large Hadron Collider one

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<v Speaker 2>of the things it does smashes these protons together into

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<v Speaker 2>smaller things to figure out why matter has mass. There

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<v Speaker 2>you go. Also, the large hadron collider accidentally has its

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<v Speaker 2>name spelled wrong on its own website as large hard

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<v Speaker 2>on collider Once would be mortifying. But what if they

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<v Speaker 2>did it more than once, like twice or five times?

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<v Speaker 2>That's impossible, is it? Because a search on their site

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<v Speaker 2>revealed they'd spelled it large hard on collider one hundred

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<v Speaker 2>and sixty five times. Thank god particle for that. That's

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<v Speaker 2>just precious. So whenever you're like, I don't understand this stuff,

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<v Speaker 2>maybe I'm not smart enough, just think someone typed in

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<v Speaker 2>large hard on collider over one hundred and fifty times

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<v Speaker 2>and they built the thing. So how else do people

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<v Speaker 2>figure this shit out? About very important things that we

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<v Speaker 2>can't see?

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<v Speaker 1>But there are other ways to do particle physics measuring

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<v Speaker 1>how particles interact with each other, throwing particles that other things,

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<v Speaker 1>accelerating stuff, and seeing what happens. All of that kind

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<v Speaker 1>of stuff. On the experimental side and on the theory side,

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<v Speaker 1>it's a lot about trying to understand like the fundamental

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<v Speaker 1>forces of nature, so like how how atoms hold together,

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<v Speaker 1>how you know, particles can change into other particles in

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<v Speaker 1>certain conditions. How gravity fits into all that, which it

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<v Speaker 1>doesn't at the moment theoretically, Okay, okay, it's very hard

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<v Speaker 1>to get gravity and particle physics to work together. This

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<v Speaker 1>is kind of yeah, it's it's sort of. This may

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<v Speaker 1>be another topic, but like, this is the reason string

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<v Speaker 1>theory was invented.

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<v Speaker 2>Real quick, what is string theory? Well, in a very

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<v Speaker 2>quark sized, tiny nutshell, the premise of string theory is

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<v Speaker 2>that basic objects are not point like, but they're string like.

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<v Speaker 2>So a quark might be made of a loop that

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<v Speaker 2>kind of vibrates and moves around. Every kind of particle

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<v Speaker 2>is like a different wiggly string. So why does anyone care?

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<v Speaker 2>Why are people so horny for string theory? Well, number one,

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<v Speaker 2>it's from the eighties, and maybe this is like the

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<v Speaker 2>scrunchy of particle physics. I don't know. More importantly, string

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<v Speaker 2>theory is a theory that works with both Einstein's general

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<v Speaker 2>relativity and that mister Einstein pose that what we perceive

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<v Speaker 2>as the force of gravity is the curvature of space

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<v Speaker 2>and time. More on that in a minute, and quantum mechanics,

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<v Speaker 2>which is the physics of the tiniest building blocks that exist.

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<v Speaker 2>So remember those quirks that made up protons and neutrons,

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<v Speaker 2>what are those made of? Maybe these string like loops

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<v Speaker 2>of matter. Every time I hear string theory mentioned, I

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<v Speaker 2>think of string cheese. I cannot And I was writing

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<v Speaker 2>and researching this episode, and I found myself on a

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<v Speaker 2>website like two thirty in the morning learning that string cheese,

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<v Speaker 2>as we know what, was invented in Wisconsin in nineteen

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<v Speaker 2>seventy six. And the way they get it to string

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<v Speaker 2>is to heat it to one hundred and forty degrees fahrenheit,

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<v Speaker 2>and that aligns all the proteins. Also, the first iterations

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<v Speaker 2>of string cheese were bigger and chunkier and served to

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<v Speaker 2>drunks in bars. Should we get back to physics, Okay, I'm.

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<v Speaker 1>Sorry, And this is like the big question in physics

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<v Speaker 1>is that, like, so, there there are a few sort

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<v Speaker 1>of fundamental forces of nature. Right, there's electromagnetism, there's that,

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<v Speaker 1>and that's like light and you know, like static cling

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<v Speaker 1>and and all of those kinds of things, right, and

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<v Speaker 1>and magnetism, and then there's the weak nuclear force, which

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<v Speaker 1>has to do with like how particles decay in radioactivity

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<v Speaker 1>that kind of thing, and how particles can change into

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<v Speaker 1>other particles under certain conditions. There's the strong nuclear force

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<v Speaker 1>and that holds particles together in the centers of atoms. Okay,

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<v Speaker 1>and those all kind of make sense together theoretically, like

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<v Speaker 1>you can write down equations that make those all fit

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<v Speaker 1>in some way more or less.

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<v Speaker 2>When Katie says you can write down equation that make

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<v Speaker 2>those all fit, I appreciate her being inclusive with the

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<v Speaker 2>second person, but I cannot write down equations to make

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<v Speaker 2>those all fit in some way. I cannot do that.

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<v Speaker 1>But then there's gravity, and gravity just doesn't follow any

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<v Speaker 1>of the same rules. It's like it's very hard to put

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<v Speaker 1>together a theory that includes those the fundamental forces of

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<v Speaker 1>particle physics and gravity.

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<v Speaker 2>So so it's gravity like the bad boy in a

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<v Speaker 2>teen drama. It's just like it's just not following any rules.

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<v Speaker 1>It's weird. It's like like gravity is all about space time,

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<v Speaker 1>you know, so gravity like, so the theory of gravity

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<v Speaker 1>that we have is Einstein's theory of relativity, so general relativity.

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<v Speaker 1>This is the theory of gravity where.

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<v Speaker 2>Okay, yeah, ready, heres Einstein. Here's how the universe of

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<v Speaker 2>which you are a part works.

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<v Speaker 1>The basic picture is that you can think of space

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<v Speaker 1>as this malleable thing, and if you have something that

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<v Speaker 1>has mass, it creates like a dentist space sort of

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<v Speaker 1>bends space around it, okay, and so other things moving

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<v Speaker 1>past will respond to that and like fall into that dent.

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<v Speaker 1>And that's like how gravitational attraction works. You can think

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<v Speaker 1>of it in this geometric way, okay, and it works

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<v Speaker 1>really well like geometrically to think of it like that.

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<v Speaker 1>But then there are fundamental principles that happen in that,

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<v Speaker 1>like the speed of light as a limiting factor and

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<v Speaker 1>all sorts of things like that, so only certain paths

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<v Speaker 1>things can follow and everything. But then the particle physics stuff,

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<v Speaker 1>like all the equations of particle physics are done without

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<v Speaker 1>thinking about gravity because on those scales, like gravity isn't important.

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<v Speaker 1>It's a really really weak force, okay. But also like

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<v Speaker 1>there are the way that the particle physics is formulated

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<v Speaker 1>in the standard Model of particle physics, which is what

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<v Speaker 1>we use to talk about all these interactions, it doesn't

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<v Speaker 1>have the same like it doesn't follow the same rules

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<v Speaker 1>as gravity, Like there are ways in which the whole

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<v Speaker 1>like speed of light thing is violated in one way

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<v Speaker 1>that you can formulate how particles move around, which is

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<v Speaker 1>kind of like there's kind of like there's this way

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<v Speaker 1>of formulating it where a particle going from point A

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<v Speaker 1>to point B passes through every possible path on the

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<v Speaker 1>way between point A and point B, and it's only

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<v Speaker 1>by by using that idea that you get the right

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<v Speaker 1>answer for how that particle is moving in the particle

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<v Speaker 1>physics point of view. And that doesn't work with relativity.

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<v Speaker 1>So there are a couple of things like that where

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<v Speaker 1>like quantum mechanics and relativity just do not like each

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<v Speaker 1>other really, And it gets especially problematic when you get

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<v Speaker 1>to black hole because a black hole is this very

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<v Speaker 1>like intense gravitational system HM. It's basically a dent in

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<v Speaker 1>space time that's so deep that like everything falls into

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<v Speaker 1>it if it gets close enough. But at the edge

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<v Speaker 1>of a black hole, the event horizon, you have this

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<v Speaker 1>weird quantum mechanical thing happening where you can have like

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<v Speaker 1>particles evaporating off of it, and that sets like a

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<v Speaker 1>sort of scale of the black hole, and that means

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<v Speaker 1>there's quantum mechanics happening in a strong gravitational system and

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<v Speaker 1>then just everything breaks. It just goes totally haywire, because

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<v Speaker 1>if you look at it from a gravitational point of view,

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<v Speaker 1>like a relativity point of view, you should see nothing

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<v Speaker 1>at all interesting happening when you when you fall into

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<v Speaker 1>the black hole, like aside from like you're you're killed

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<v Speaker 1>by the gravity, but like you don't see like nothing

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<v Speaker 1>weird happens when you pass the horizon. But from a

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<v Speaker 1>particle physics point of view, like there there might be

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<v Speaker 1>like this like firewall, like there might be like a

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<v Speaker 1>sort of like boundary of intense radiation there. Because of

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<v Speaker 1>the way you have to think about how the particle

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<v Speaker 1>physics works. This is a complicated story, but.

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<v Speaker 2>Basically the astrophysics typically is yeah, I'm not explaining it

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<v Speaker 2>very well, but but basically.

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<v Speaker 1>Like like basically, when you get to that point when

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<v Speaker 1>you have a black hole that has an evaporation happening

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<v Speaker 1>where particles are coming off the edge of the event horizon,

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<v Speaker 1>one way of looking at it says that that that

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<v Speaker 1>means that whatever you fought through into the black hole,

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<v Speaker 1>you can't ever find out what it was. That information

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<v Speaker 1>is destroid. But quantum mechanics like the particle point of

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<v Speaker 1>view says you can't do that, and so there has

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<v Speaker 1>to be some kind of loophole and then gravity doesn't

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<v Speaker 1>like that and you just you just end up with chaos.

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<v Speaker 1>And so there's this there's this big problem called the

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<v Speaker 1>black hole information paradox, which has been around forever, and

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<v Speaker 1>every once in a while somebody's like, oh, I solved it,

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<v Speaker 1>and then it's really complicated and people don't really understand

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<v Speaker 1>how that works.

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<v Speaker 2>Has anyone actually solved that?

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<v Speaker 1>I mean, I so technically I'm just not qualified to

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<v Speaker 1>know that for sure, because it requires understanding quantum gravity

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<v Speaker 1>in a way that I do not. But there have

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<v Speaker 1>been some solution suggested, but in general there's still a

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<v Speaker 1>lot of discussion. So I don't know.

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<v Speaker 2>Okay, wait, so what does a cosmologist do.

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<v Speaker 1>Cosmologist just means you study the universe as a whole, right,

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<v Speaker 1>so you study maybe the beginning of the universe, the

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<v Speaker 1>end of the universe, how it changes over time. But

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<v Speaker 1>you can be a physicist cosmologist or an astronomer cosmologist,

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<v Speaker 1>and those are different and and it's culturally different, like

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<v Speaker 1>but the so if you if you're a physicist, if

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<v Speaker 1>you hang out with particle physics people and you say

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<v Speaker 1>you're a cosmologists, then then the implication is that you

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<v Speaker 1>work on like the beginning of the universe and the

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<v Speaker 1>forces of nature and maybe the end of the universe

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<v Speaker 1>something like that. If you hang out with astrophysicists and

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<v Speaker 1>you say you're a cosmologist, then you just study things

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<v Speaker 1>that are really far away, or you study, you know,

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<v Speaker 1>some something you know more fundamental. But you can be

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<v Speaker 1>a cosmologist in astrophysics and you're a cosmologist because you

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<v Speaker 1>study very very distant galaxies. The reason that counts as

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<v Speaker 1>cosmology is because that means you're studying the very distant

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<v Speaker 1>past of the universe.

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<v Speaker 2>So there are different flavors of cosmology, but they're all

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<v Speaker 2>kind of linked, at least in my opinion, by like,

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<v Speaker 2>oh where are we? What are we? What are we

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<v Speaker 2>made of? AKA, it's a branch of astronomy that involves

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<v Speaker 2>the origin and evolution of the universe. That's a less

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<v Speaker 2>panicky way to put it.

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<v Speaker 1>And so then you're studying like how the universe has

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<v Speaker 1>changed over time. So there are kind of different ways

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<v Speaker 1>of doing it. And I've done all of those different

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<v Speaker 1>kinds of cosmology. I guess because I've spent my time

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<v Speaker 1>kind of bouncing back and forth between the particle physics

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<v Speaker 1>and the astrophysics communities. So I've worked on you know,

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<v Speaker 1>the Big Bang and like theories of the early universe,

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<v Speaker 1>and I've worked on distant galaxies and how galaxies form.

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<v Speaker 1>And I've worked on black holes and weird stuf like

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<v Speaker 1>cosmic strings and just all sorts of things.

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<v Speaker 2>What is a cosmic string?

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<v Speaker 1>A cosmic string is kind of like a sort of

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<v Speaker 1>line or wiggly line of energy that stretches across the cosmos.

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<v Speaker 1>Might not exist, probably doesn't exist, but there could be

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<v Speaker 1>this like whole network of strings of Like it's kind

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<v Speaker 1>of like if you think of like a black hole,

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<v Speaker 1>but you like stretch it out across the whole universe.

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<v Speaker 1>You get It's kind of like that, what does it do? What?

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<v Speaker 3>It?

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<v Speaker 1>So really interesting things. So if you have two cosmic

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<v Speaker 1>strings and they cross each other they collide, they can

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<v Speaker 1>like reconnect in a different way. So you can have

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<v Speaker 1>two cosmic strings that are about to collide and then

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<v Speaker 1>they they like change so that now you have two

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<v Speaker 1>sort of loops of cosmic strings. They're going intopposite directions, like,

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<v Speaker 1>so they sort of pass through each other by branching

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<v Speaker 1>off in this weird way.

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<v Speaker 2>So cosmic strings may or may not exist. Now, if

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<v Speaker 2>they do exist, some theorists have used them to maybe

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<v Speaker 2>catch out some stuff about time travel. Please figure that out,

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<v Speaker 2>please fix some stuff. Thank you.

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<v Speaker 1>And you can make a loop of cosmic string, and

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<v Speaker 1>then that loop of cosmic string will like wiggle around

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<v Speaker 1>and make gravitational radiation and disappear into nothingness. And if

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<v Speaker 1>you have a cosmic string, like if you have a

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<v Speaker 1>cosmic string between you and some distant galaxy, then you

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<v Speaker 1>might see two pictures of that galaxy because it like

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<v Speaker 1>splits the space kind of. It's really cool.

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<v Speaker 2>Now, how much do you think about all of this

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<v Speaker 2>in your day to day life? And like when you're

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<v Speaker 2>deciding if you should upgrade your rental car and like

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<v Speaker 2>if you should cut bangs and what happens to your

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<v Speaker 2>molecules after you die? Like how much do you let

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<v Speaker 2>this kind of get to your own existence?

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<v Speaker 1>H Yeah, somebody asked me that the other day, Like

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<v Speaker 1>how much do I like get sort of just overwhelmed

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<v Speaker 1>by these ideas or whatever? It's not very often like

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<v Speaker 1>most of the time this is like, this is fun

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<v Speaker 1>stuff to work on, but like most of this time,

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<v Speaker 1>it feels more like some kind of combination of science

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<v Speaker 1>fiction and a fun puzzle, you know. So like I'm

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<v Speaker 1>trying to solve a problem, I'm trying to calculate something

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<v Speaker 1>and trying to come up with a new idea for

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<v Speaker 1>how to do something, and so it's like a puzzle.

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<v Speaker 1>It's like some kind of neat thing to work out.

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<v Speaker 1>And I don't think of it as connecting to my

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<v Speaker 1>own life or existence because it's way far away or

418
00:24:29.200 --> 00:24:32.039
<v Speaker 1>way in the past, or you know, probably doesn't exist

419
00:24:32.119 --> 00:24:35.680
<v Speaker 1>or whatever. Right, But then every once in a while,

420
00:24:35.720 --> 00:24:37.759
<v Speaker 1>like I'll be I'll be thinking about this stuff and

421
00:24:37.799 --> 00:24:41.440
<v Speaker 1>I'll be like, oh my god, Like there's this stuff

422
00:24:41.480 --> 00:24:45.880
<v Speaker 1>is out there. Like I'll be thinking about black holes

423
00:24:46.200 --> 00:24:50.640
<v Speaker 1>or gravitational waves or like the inflation period in the

424
00:24:50.720 --> 00:24:52.759
<v Speaker 1>early universe or something like that, and I'll be like

425
00:24:52.839 --> 00:24:54.799
<v Speaker 1>I'll have to like hold on to something and be like,

426
00:24:54.880 --> 00:25:00.119
<v Speaker 1>oh God, because these are huge, like mind bendingly the

427
00:25:00.359 --> 00:25:06.480
<v Speaker 1>intense forces and massive things and like the kinds of

428
00:25:06.759 --> 00:25:10.720
<v Speaker 1>energies and the kinds of like force and just I

429
00:25:10.759 --> 00:25:14.519
<v Speaker 1>don't know, the explosions and everything. It's just we cannot

430
00:25:14.519 --> 00:25:17.960
<v Speaker 1>comprehend this stuff. I mean, the Earth is really tiny

431
00:25:18.000 --> 00:25:21.759
<v Speaker 1>and really unimportant, like in a big way. So okay,

432
00:25:22.599 --> 00:25:28.640
<v Speaker 1>you know, there's there's this. There's this famous photograph, the

433
00:25:28.680 --> 00:25:31.160
<v Speaker 1>pale Blue Dot. Yes, huh yeah, so this is a

434
00:25:31.200 --> 00:25:34.000
<v Speaker 1>picture that was taken by the Voyager spacecraft.

435
00:25:34.200 --> 00:25:36.880
<v Speaker 2>So the Pale Blue Dot photo was taken on Valentine's

436
00:25:36.920 --> 00:25:40.440
<v Speaker 2>Day in nineteen ninety as Voyager one was leaving the

437
00:25:40.519 --> 00:25:43.759
<v Speaker 2>Solar System, it was like bye bye, I'm out, and

438
00:25:43.920 --> 00:25:47.160
<v Speaker 2>astronomer Carl Sagan said, Yo, let's turn that lens around.

439
00:25:47.319 --> 00:25:49.000
<v Speaker 2>Let's take a pick of all of us far away.

440
00:25:49.079 --> 00:25:51.440
<v Speaker 2>What do you say, might as well? And it was

441
00:25:51.920 --> 00:25:58.720
<v Speaker 2>three point seven billion miles away. It's little galaxy's longest range.

442
00:25:58.720 --> 00:26:01.799
<v Speaker 2>Selfie this to itself. It looks like you accidentally took

443
00:26:01.839 --> 00:26:04.720
<v Speaker 2>like a blurry image of a few Christmas lights and

444
00:26:04.759 --> 00:26:07.000
<v Speaker 2>there was like a speck of dust on your lens.

445
00:26:07.400 --> 00:26:10.559
<v Speaker 2>Those lights are just a few scattered rays of sun.

446
00:26:10.960 --> 00:26:13.759
<v Speaker 2>And someone would have to point out that that dust

447
00:26:14.119 --> 00:26:18.359
<v Speaker 2>is our planet is such a tiny speck. And I'll

448
00:26:18.440 --> 00:26:21.000
<v Speaker 2>let Carl Sagan put this in context.

449
00:26:21.279 --> 00:26:27.160
<v Speaker 4>He's the pro here, that's here, that's home, that's us

450
00:26:27.839 --> 00:26:33.079
<v Speaker 4>on it. Everyone You love, everyone you know, everyone you

451
00:26:33.200 --> 00:26:37.720
<v Speaker 4>ever heard of, every human being whoever was, lived out

452
00:26:37.759 --> 00:26:44.000
<v Speaker 4>their lives, the aggregate of our joy and suffering, thousands

453
00:26:44.039 --> 00:26:49.720
<v Speaker 4>of confident religions, ideologies, and economic doctrines, every hunter and forager,

454
00:26:50.559 --> 00:26:54.640
<v Speaker 4>every hero and coward, every creator and destroyer of civilization,

455
00:26:55.720 --> 00:27:00.119
<v Speaker 4>every king and peasant, every young couple in love, every

456
00:27:00.160 --> 00:27:06.440
<v Speaker 4>mother and father, hopeful child, inventor and explorer, every teacher

457
00:27:06.559 --> 00:27:12.920
<v Speaker 4>of morals, every corrupt politician, every superstar, every supreme leader,

458
00:27:13.440 --> 00:27:16.559
<v Speaker 4>every saint and sinner in the history of our species

459
00:27:17.400 --> 00:27:23.880
<v Speaker 4>lived there on a mote of dust, suspended in a sunbeam.

460
00:27:24.200 --> 00:27:29.119
<v Speaker 4>The Earth is a very small stage in a fast

461
00:27:29.880 --> 00:27:31.279
<v Speaker 4>cosmic arena.

462
00:27:32.119 --> 00:27:34.759
<v Speaker 1>Sometimes when I give talks about cosmology, I'll end with

463
00:27:34.799 --> 00:27:37.640
<v Speaker 1>this picture, and I'll be like, you know, just thinking

464
00:27:37.680 --> 00:27:42.000
<v Speaker 1>about how vast the universe is and how really insignificant

465
00:27:42.119 --> 00:27:46.079
<v Speaker 1>we are, and it's and the insignificant is even deeper

466
00:27:46.119 --> 00:27:47.960
<v Speaker 1>than just what you see from that picture, because in

467
00:27:48.000 --> 00:27:49.559
<v Speaker 1>that picture you see like there's a whole lot of

468
00:27:49.559 --> 00:27:52.400
<v Speaker 1>empty space, and then there's a little tiny rock and

469
00:27:52.440 --> 00:27:55.200
<v Speaker 1>we're on that little tiny rock, right, and there's a

470
00:27:55.240 --> 00:27:58.400
<v Speaker 1>lot of space. But it's even worse than that because

471
00:27:59.480 --> 00:28:02.559
<v Speaker 1>because not only are we not the center of like

472
00:28:02.880 --> 00:28:05.400
<v Speaker 1>the universe or a galaxy or a solitist or anything

473
00:28:05.440 --> 00:28:08.319
<v Speaker 1>like that, the matter that we're made of is also

474
00:28:08.400 --> 00:28:13.200
<v Speaker 1>really unimportant because because like like just the kind of

475
00:28:13.200 --> 00:28:15.160
<v Speaker 1>stuff that we are and that we can understand and

476
00:28:15.160 --> 00:28:19.240
<v Speaker 1>interact with. Regular matter is like five percent of the universe.

477
00:28:19.759 --> 00:28:23.559
<v Speaker 1>So most of the universe is something called dark energy

478
00:28:23.599 --> 00:28:25.559
<v Speaker 1>that we really don't understand, but it's some sort of

479
00:28:26.000 --> 00:28:29.200
<v Speaker 1>mysterious stuff that's making the universe expand faster and faster,

480
00:28:29.279 --> 00:28:31.599
<v Speaker 1>and it's going to take over eventually. And then there's

481
00:28:31.680 --> 00:28:34.720
<v Speaker 1>dark matter, which is some kind of invisible matter that

482
00:28:35.119 --> 00:28:37.200
<v Speaker 1>is most of what the galaxy is made of and

483
00:28:37.240 --> 00:28:39.039
<v Speaker 1>most of what all galaxies are made of. So like

484
00:28:39.079 --> 00:28:41.519
<v Speaker 1>our galaxy, you know, we think of it as like

485
00:28:41.559 --> 00:28:44.599
<v Speaker 1>this pretty disc of stars, but it's actually embedded in

486
00:28:44.640 --> 00:28:48.200
<v Speaker 1>this invisible blob of extra stuff that we can't see,

487
00:28:48.240 --> 00:28:50.720
<v Speaker 1>and that blob is way bigger than the stuff that

488
00:28:50.759 --> 00:28:53.119
<v Speaker 1>we can actually see. So dark matter is like eighty

489
00:28:53.119 --> 00:28:54.960
<v Speaker 1>five percent of the matter in the universe or something

490
00:28:55.000 --> 00:28:56.960
<v Speaker 1>like that, oh my god. And then dark energy is

491
00:28:57.000 --> 00:28:59.880
<v Speaker 1>like seventy percent of all of the stuff in the universe.

492
00:29:00.359 --> 00:29:04.000
<v Speaker 1>Like so so then we're this like little tiny five

493
00:29:04.000 --> 00:29:06.960
<v Speaker 1>percent slices, and that's just the kind of matter that

494
00:29:07.000 --> 00:29:09.720
<v Speaker 1>we can understand, that we can do experiments on, that

495
00:29:09.720 --> 00:29:12.559
<v Speaker 1>we can see or touch or interact with in any

496
00:29:12.759 --> 00:29:19.680
<v Speaker 1>reasonable way. And then it's like, not only not only

497
00:29:19.720 --> 00:29:21.680
<v Speaker 1>are we like a tiny speck of dust on a

498
00:29:21.680 --> 00:29:24.720
<v Speaker 1>tiny speck of dust, Like who's you know, Like we

499
00:29:24.799 --> 00:29:27.920
<v Speaker 1>are so insignificant, Like the universe doesn't even it doesn't

500
00:29:27.920 --> 00:29:31.440
<v Speaker 1>even matter that we're like that our kind of stuff

501
00:29:31.480 --> 00:29:31.839
<v Speaker 1>is there.

502
00:29:31.920 --> 00:29:34.440
<v Speaker 2>You know, the best thing about this conversation is, yeah,

503
00:29:34.759 --> 00:29:38.119
<v Speaker 2>I'm I'm having it with a cosmologist and like an astrophysicist,

504
00:29:38.400 --> 00:29:40.519
<v Speaker 2>but I could also be having the same conversation with

505
00:29:40.680 --> 00:29:43.000
<v Speaker 2>any of my college roommates who had like a seven

506
00:29:43.000 --> 00:29:47.759
<v Speaker 2>foot bong in the garage. When astrophysicists and cosmologists get together, yeah,

507
00:29:48.039 --> 00:29:50.039
<v Speaker 2>is it just kind of like a round robin of

508
00:29:50.079 --> 00:29:53.640
<v Speaker 2>like stoner existentialism, like because they feel like there's such

509
00:29:53.640 --> 00:29:59.000
<v Speaker 2>a fine line, like and then you're either incredibly incredibly

510
00:29:59.039 --> 00:30:01.839
<v Speaker 2>smart and thoughtful and knowledgeable about this stuff, or you're

511
00:30:01.920 --> 00:30:04.599
<v Speaker 2>just like you've just numbed yourself enough or you allow

512
00:30:04.599 --> 00:30:06.000
<v Speaker 2>yourself to think about it, and then and it's like

513
00:30:06.119 --> 00:30:08.640
<v Speaker 2>the Bell curve. There's this big white swath of people

514
00:30:08.640 --> 00:30:10.519
<v Speaker 2>who are like I can't even think about it. It's

515
00:30:10.599 --> 00:30:12.079
<v Speaker 2>too much, you know.

516
00:30:12.599 --> 00:30:16.119
<v Speaker 1>I mean, so when I do get together with other

517
00:30:16.160 --> 00:30:19.880
<v Speaker 1>cosmologists and we talk shop, it's usually very very technical,

518
00:30:20.440 --> 00:30:23.559
<v Speaker 1>and so we don't get into this stuff at all,

519
00:30:23.599 --> 00:30:26.440
<v Speaker 1>like we're it's it's usually you know, we're just talking

520
00:30:26.480 --> 00:30:29.720
<v Speaker 1>about we're talking in a lot of jargon about like

521
00:30:29.759 --> 00:30:32.480
<v Speaker 1>some measurement or something, and we're throwing out numbers and

522
00:30:32.519 --> 00:30:34.920
<v Speaker 1>we're trying to like figure out like is this a

523
00:30:34.920 --> 00:30:37.799
<v Speaker 1>reasonable measurement to make or whatever, Like what kind of

524
00:30:37.799 --> 00:30:41.799
<v Speaker 1>plot can we make to you know, to illustrate this point,

525
00:30:41.880 --> 00:30:44.079
<v Speaker 1>or what kind of calculation should we do, or like

526
00:30:44.119 --> 00:30:48.240
<v Speaker 1>what's the important variable? It would not be interesting to

527
00:30:48.759 --> 00:30:51.640
<v Speaker 1>somebody who is not in the field. So it's really

528
00:30:51.720 --> 00:30:53.799
<v Speaker 1>only when I'm talking about people who are not in

529
00:30:53.880 --> 00:30:58.440
<v Speaker 1>cosmology where like I have these moments of like, oh god,

530
00:30:59.119 --> 00:31:02.599
<v Speaker 1>you know, but the thing I mean, but it's it's

531
00:31:02.599 --> 00:31:04.480
<v Speaker 1>a little bit dangerous to talk about this stuff though,

532
00:31:04.519 --> 00:31:08.400
<v Speaker 1>because then sometimes people get the idea that we really

533
00:31:08.440 --> 00:31:10.640
<v Speaker 1>are just kind of sitting around making stuff up, you know,

534
00:31:11.200 --> 00:31:14.880
<v Speaker 1>like and so then people think like, oh, I can

535
00:31:14.920 --> 00:31:17.440
<v Speaker 1>be a cosmologist, Like what if the universe is shaped

536
00:31:17.480 --> 00:31:19.559
<v Speaker 1>like a football? You know, And I think that that

537
00:31:19.640 --> 00:31:24.839
<v Speaker 1>the sort of disconnect there is that like the ideas themselves,

538
00:31:25.039 --> 00:31:27.200
<v Speaker 1>if they're not backed up by the data or by

539
00:31:27.319 --> 00:31:30.319
<v Speaker 1>like a very rigorous model, are really not that important.

540
00:31:31.400 --> 00:31:35.119
<v Speaker 1>Like once we have data and we have some kind

541
00:31:35.119 --> 00:31:38.359
<v Speaker 1>of unifying theory that says that this is probably the

542
00:31:38.359 --> 00:31:42.279
<v Speaker 1>way things are, then it's like super cool, right, But

543
00:31:43.839 --> 00:31:45.920
<v Speaker 1>if somebody had said, like, oh, you know, maybe the

544
00:31:46.000 --> 00:31:48.279
<v Speaker 1>universe is like this, like we don't really know what

545
00:31:48.319 --> 00:31:50.079
<v Speaker 1>to do with that, and it does, it's not really

546
00:31:50.119 --> 00:31:54.279
<v Speaker 1>helpful and you can't just spitball like yeah, yeah exactly,

547
00:31:54.359 --> 00:31:57.480
<v Speaker 1>like like you have to. It has to be connected

548
00:31:57.519 --> 00:32:01.440
<v Speaker 1>to something we can test or or write down mathematically

549
00:32:02.279 --> 00:32:05.440
<v Speaker 1>or else. It just it's kind of not helpful, which is,

550
00:32:05.759 --> 00:32:08.160
<v Speaker 1>you know, it's a bummer. But once you do have

551
00:32:08.400 --> 00:32:11.400
<v Speaker 1>the sort of mathematical tools and stuff and you can

552
00:32:11.400 --> 00:32:14.720
<v Speaker 1>speak that language, you know, then you can get really

553
00:32:14.720 --> 00:32:17.680
<v Speaker 1>creative and then you can just do really fun things.

554
00:32:18.440 --> 00:32:21.160
<v Speaker 1>So like, I have a project I'm working on that

555
00:32:21.240 --> 00:32:25.079
<v Speaker 1>has to do with I have a few interesting projects. Actually,

556
00:32:25.799 --> 00:32:29.119
<v Speaker 1>So I have one. So here's one that it could

557
00:32:29.119 --> 00:32:31.680
<v Speaker 1>be fun. So it has to do with black holes

558
00:32:31.839 --> 00:32:37.200
<v Speaker 1>and galaxies and the bending of space. Okay, so every

559
00:32:37.279 --> 00:32:40.319
<v Speaker 1>time there's a massive object, it bends space around it,

560
00:32:40.400 --> 00:32:42.960
<v Speaker 1>and so that means that light when it goes past

561
00:32:43.440 --> 00:32:46.519
<v Speaker 1>bends around so like a lens, Like the massive object

562
00:32:46.519 --> 00:32:48.440
<v Speaker 1>acts like a lens for light, and so light gets

563
00:32:48.440 --> 00:32:52.160
<v Speaker 1>bent around. So there's this way to study like what

564
00:32:52.279 --> 00:32:56.000
<v Speaker 1>galaxies are made of by having a very bright light

565
00:32:56.119 --> 00:32:59.680
<v Speaker 1>behind the galaxy, like really far away and looking at

566
00:32:59.680 --> 00:33:03.640
<v Speaker 1>how that light like bends around inside that galaxy and

567
00:33:03.720 --> 00:33:06.519
<v Speaker 1>like how the light fluctuates as things move and stuff

568
00:33:06.559 --> 00:33:10.440
<v Speaker 1>like that. And that's called gravitational microlensing in this case

569
00:33:10.720 --> 00:33:13.000
<v Speaker 1>the kind of thing I'm working on, but the details

570
00:33:13.000 --> 00:33:17.440
<v Speaker 1>aren't important, but it's this thing where like the thing

571
00:33:17.440 --> 00:33:19.279
<v Speaker 1>that's making the bright light is also a black hole.

572
00:33:20.400 --> 00:33:22.519
<v Speaker 1>Because it turns out when you have a super massive

573
00:33:22.519 --> 00:33:25.119
<v Speaker 1>black hole, like billions of times as massive as the sun,

574
00:33:26.240 --> 00:33:30.119
<v Speaker 1>those things can be pulling matter into themselves and that

575
00:33:30.160 --> 00:33:34.480
<v Speaker 1>matter lights up like a whirlpool of stuff what, and

576
00:33:34.519 --> 00:33:36.880
<v Speaker 1>it can make this incredibly bright light that you can

577
00:33:36.920 --> 00:33:41.400
<v Speaker 1>see like across the universe. And so we use that

578
00:33:41.599 --> 00:33:45.279
<v Speaker 1>as like a back light to study this stuff in

579
00:33:45.359 --> 00:33:48.559
<v Speaker 1>a more nearby galaxy to find out how many black

580
00:33:48.599 --> 00:33:50.039
<v Speaker 1>holes there are in that galaxy.

581
00:33:50.400 --> 00:33:53.359
<v Speaker 5>So black holes make lights sometimes. Yeah, it's supposed to

582
00:33:53.400 --> 00:33:56.079
<v Speaker 5>be confusing. Yeah, it's like I think, I mean, I

583
00:33:56.119 --> 00:33:58.200
<v Speaker 5>think it's like it's one of these things. It's like

584
00:33:58.200 --> 00:34:00.640
<v Speaker 5>the biggest misconception about black holes is that they're dark.

585
00:34:00.839 --> 00:34:03.200
<v Speaker 5>Usually they're not, like the ones we know about are

586
00:34:03.279 --> 00:34:06.359
<v Speaker 5>usually not dark, and it's it's yeah, it's because they're not.

587
00:34:06.599 --> 00:34:10.679
<v Speaker 5>It's it's because like technically the black hole itself can't

588
00:34:10.719 --> 00:34:13.840
<v Speaker 5>be seen, but it's doing so much that it like

589
00:34:14.000 --> 00:34:17.880
<v Speaker 5>affects everything around it. And so usually you can see

590
00:34:17.880 --> 00:34:21.840
<v Speaker 5>black holes because they're like really destructive and like the

591
00:34:21.920 --> 00:34:24.360
<v Speaker 5>stuff is falling into them, kind of like if you

592
00:34:25.639 --> 00:34:28.440
<v Speaker 5>if you had a drain at the bottom of a bathtub,

593
00:34:28.480 --> 00:34:31.719
<v Speaker 5>uh huh, Like you might not be able to see

594
00:34:31.840 --> 00:34:34.519
<v Speaker 5>the drain through like the you know, bubbles or something,

595
00:34:34.559 --> 00:34:37.440
<v Speaker 5>but you can see that there's like a whirlpool of

596
00:34:37.480 --> 00:34:38.840
<v Speaker 5>stuff falling in at that point.

597
00:34:39.280 --> 00:34:39.760
<v Speaker 2>Oh man.

598
00:34:39.840 --> 00:34:43.440
<v Speaker 1>And that's how we see black holes in space usually,

599
00:34:43.679 --> 00:34:46.000
<v Speaker 1>is we see that they're they're pulling in a lot

600
00:34:46.039 --> 00:34:48.320
<v Speaker 1>of matter and so they like that matter lights up

601
00:34:48.760 --> 00:34:50.599
<v Speaker 1>and so once it goes into the black hole, we

602
00:34:50.639 --> 00:34:52.760
<v Speaker 1>can't see it, but it spends a lot of time

603
00:34:52.760 --> 00:34:54.280
<v Speaker 1>whirling around really fast.

604
00:34:54.559 --> 00:34:57.239
<v Speaker 2>It's like an intergalactic garbage disposal.

605
00:34:57.360 --> 00:34:59.639
<v Speaker 1>That yeah, yeah, and it can be. It's some of

606
00:34:59.639 --> 00:35:01.960
<v Speaker 1>the bright things in the universe are are black holes.

607
00:35:02.000 --> 00:35:04.079
<v Speaker 1>We call them quasars when they're when they're the super

608
00:35:04.079 --> 00:35:08.320
<v Speaker 1>massive ones and they're pulling matter in like that, and

609
00:35:08.519 --> 00:35:12.159
<v Speaker 1>and we have so so that's like those are for

610
00:35:12.360 --> 00:35:14.599
<v Speaker 1>black holes that are like millions or billions of times

611
00:35:14.599 --> 00:35:15.639
<v Speaker 1>as massive as the Sun.

612
00:35:15.960 --> 00:35:17.559
<v Speaker 2>And how far away are those puppets?

613
00:35:17.760 --> 00:35:22.760
<v Speaker 1>All right? Well, okay, super massive black holes, the ones

614
00:35:22.800 --> 00:35:24.679
<v Speaker 1>I was just talking about millions or billions of times

615
00:35:24.719 --> 00:35:28.840
<v Speaker 1>the mass of the Sun. Those seem to exist at

616
00:35:28.880 --> 00:35:32.280
<v Speaker 1>the centers of pretty much every reasonably sized galaxy we

617
00:35:32.360 --> 00:35:33.119
<v Speaker 1>know about.

618
00:35:33.239 --> 00:35:36.159
<v Speaker 2>At the centers, yes, so including ours?

619
00:35:36.639 --> 00:35:40.320
<v Speaker 1>Yes, really, yes, so our galaxy.

620
00:35:40.440 --> 00:35:44.280
<v Speaker 2>Okay, quick note, let's do a few cosmological basics. Our

621
00:35:44.320 --> 00:35:47.639
<v Speaker 2>galaxy is the Milky Way, right, And this next analogy

622
00:35:47.679 --> 00:35:51.079
<v Speaker 2>I got right off of NASA's Night Sky website, which

623
00:35:51.079 --> 00:35:54.239
<v Speaker 2>I think is for children, but it's so helpful. So okay,

624
00:35:54.280 --> 00:35:59.000
<v Speaker 2>imagine our sun. It's one star among hundreds of billions

625
00:35:59.039 --> 00:36:02.119
<v Speaker 2>of stars in our milky right, So if we shrink

626
00:36:02.199 --> 00:36:04.320
<v Speaker 2>the Sun down to smaller than a grain of sand,

627
00:36:04.840 --> 00:36:10.239
<v Speaker 2>our little solar system Venus, Mercury Earth, all of those

628
00:36:10.559 --> 00:36:13.079
<v Speaker 2>would be small enough to fit the whole solar system

629
00:36:13.079 --> 00:36:15.519
<v Speaker 2>in the palm of your hand. Now, on that scale,

630
00:36:15.559 --> 00:36:18.360
<v Speaker 2>with our solar system in your hand, the Milky Way

631
00:36:18.400 --> 00:36:21.960
<v Speaker 2>galaxy would be the size of North America. And the

632
00:36:22.000 --> 00:36:26.239
<v Speaker 2>Milky Way's big. But our next, our neighbor and Drameda galaxy,

633
00:36:26.440 --> 00:36:28.960
<v Speaker 2>it's about twice as big as the Milky Way. Scale

634
00:36:29.360 --> 00:36:31.960
<v Speaker 2>is important here, I suppose. But at the center of

635
00:36:31.960 --> 00:36:33.880
<v Speaker 2>our galaxy there's a black hole.

636
00:36:34.440 --> 00:36:37.159
<v Speaker 1>So the Milky Way is like a disc of stars

637
00:36:37.159 --> 00:36:39.199
<v Speaker 1>and gas and dusts and stuff, and we're sort of

638
00:36:39.239 --> 00:36:43.119
<v Speaker 1>out toward an edge, and at the center there's a

639
00:36:43.159 --> 00:36:45.000
<v Speaker 1>bulge of stars and gas and dust, and then at

640
00:36:45.000 --> 00:36:47.199
<v Speaker 1>the middle of that there's a black hole. It's four

641
00:36:47.239 --> 00:36:50.239
<v Speaker 1>million times as massive as the Sun. I didn't know that.

642
00:36:50.280 --> 00:36:52.480
<v Speaker 1>Do we have a name for it, Yeah, yeah, we

643
00:36:52.480 --> 00:36:55.400
<v Speaker 1>have a name for it. We call it Sagittarius a star, okay,

644
00:36:55.639 --> 00:36:58.559
<v Speaker 1>which is a silly same. It's because it's the kind

645
00:36:58.599 --> 00:37:01.880
<v Speaker 1>of I think it was, like I think a radio source,

646
00:37:02.239 --> 00:37:05.840
<v Speaker 1>and because it was pulling in some matter and so

647
00:37:05.920 --> 00:37:07.519
<v Speaker 1>it was lighting up in the radio a little bit,

648
00:37:07.559 --> 00:37:09.800
<v Speaker 1>and so ours is not pulling in very much matter

649
00:37:09.800 --> 00:37:12.280
<v Speaker 1>at all, like very occasionally it'll lead a little blobb

650
00:37:12.280 --> 00:37:15.559
<v Speaker 1>of gas and the astronomers get super excited, but like

651
00:37:15.599 --> 00:37:18.800
<v Speaker 1>there's very little happening with it, but it does. It

652
00:37:18.880 --> 00:37:23.239
<v Speaker 1>is really big, and it's got a bunch of stars

653
00:37:23.320 --> 00:37:25.920
<v Speaker 1>orbiting really closely around it, and so you can actually

654
00:37:25.960 --> 00:37:30.599
<v Speaker 1>go online and see like data follow like tracing out

655
00:37:30.679 --> 00:37:33.159
<v Speaker 1>the paths of some of these stars and you can

656
00:37:33.159 --> 00:37:36.119
<v Speaker 1>see them like whip around as they go really close

657
00:37:36.119 --> 00:37:37.679
<v Speaker 1>to the black hole in their orbits. So some of

658
00:37:37.679 --> 00:37:39.480
<v Speaker 1>them have these orbits that they're really far away in

659
00:37:39.480 --> 00:37:41.360
<v Speaker 1>and they come in really close and they go boom

660
00:37:41.400 --> 00:37:43.760
<v Speaker 1>like that right around the black hole. And so you

661
00:37:43.800 --> 00:37:45.840
<v Speaker 1>can figure out exactly like how big it is and

662
00:37:45.880 --> 00:37:48.239
<v Speaker 1>where it is by watching these stars go around it

663
00:37:48.239 --> 00:37:48.840
<v Speaker 1>really quickly.

664
00:37:48.960 --> 00:37:51.440
<v Speaker 2>So I did a little looking, and if you google

665
00:37:51.840 --> 00:37:56.760
<v Speaker 2>European Southern Observatory and s AS in SAM too, you'll

666
00:37:56.760 --> 00:37:58.519
<v Speaker 2>find this, Oh my god, like a rim shot in

667
00:37:58.559 --> 00:37:59.599
<v Speaker 2>a basketball game, like.

668
00:37:59.599 --> 00:38:02.360
<v Speaker 1>Yeah, yeah, yeah, yeah, like that, except it comes back around.

669
00:38:02.400 --> 00:38:04.840
<v Speaker 1>You know, it's on an orbit. So yeah, so there's

670
00:38:04.880 --> 00:38:08.239
<v Speaker 1>stuff orbiting really close. So that black hole, that one

671
00:38:08.360 --> 00:38:13.360
<v Speaker 1>is like, well, let's see, it's eight thousand parsecs away.

672
00:38:13.519 --> 00:38:16.559
<v Speaker 1>I don't know how much that is. A parsec is

673
00:38:16.559 --> 00:38:19.960
<v Speaker 1>about three something light years. So a light year is

674
00:38:20.039 --> 00:38:23.400
<v Speaker 1>how far? How far to how far light travels.

675
00:38:23.000 --> 00:38:23.440
<v Speaker 4>In a year?

676
00:38:24.039 --> 00:38:26.880
<v Speaker 1>Right, So light moves very quickly, so that's a very

677
00:38:26.920 --> 00:38:32.239
<v Speaker 1>long way. So for example, light travels it takes light

678
00:38:32.400 --> 00:38:36.360
<v Speaker 1>eight minutes to get between the Sun and us. There's

679
00:38:36.400 --> 00:38:38.239
<v Speaker 1>a rule of thumb. Actually, if you want to know

680
00:38:38.400 --> 00:38:41.679
<v Speaker 1>how far how fast light speed is, it goes about

681
00:38:41.920 --> 00:38:43.360
<v Speaker 1>a foot per nanosecond.

682
00:38:43.760 --> 00:38:45.480
<v Speaker 2>A foot per nanosecond.

683
00:38:45.599 --> 00:38:48.280
<v Speaker 5>Yes, oh that's easy to calculate, Yeah, just to punch

684
00:38:48.280 --> 00:38:50.679
<v Speaker 5>of zeros, right, yeah, put a zero on it.

685
00:38:50.800 --> 00:38:53.280
<v Speaker 1>Yeah, yeah, it's easy. But it's kind of cool because

686
00:38:53.280 --> 00:38:55.320
<v Speaker 1>then you can like you can say, like, if somebody

687
00:38:55.400 --> 00:38:56.880
<v Speaker 1>is like ten feet away from you, they are ten

688
00:38:56.960 --> 00:38:58.239
<v Speaker 1>nanoseconds in the past.

689
00:38:59.320 --> 00:39:03.119
<v Speaker 2>They're ten seconds in the past. Oh man, I'm gonna

690
00:39:03.119 --> 00:39:03.599
<v Speaker 2>trip out.

691
00:39:04.079 --> 00:39:08.159
<v Speaker 1>I'm so like, we're like three nanoseconds apart right now.

692
00:39:08.320 --> 00:39:14.719
<v Speaker 2>Weird. It's so weird. It's great though, And I learned

693
00:39:14.719 --> 00:39:16.719
<v Speaker 2>this recently and I've already forgotten it, which is embarrassing.

694
00:39:16.960 --> 00:39:23.000
<v Speaker 2>The distance between us and the Sun is a certain

695
00:39:23.559 --> 00:39:24.320
<v Speaker 2>what is the U?

696
00:39:24.800 --> 00:39:26.800
<v Speaker 1>Oh, that's an astronomical unit.

697
00:39:26.960 --> 00:39:27.960
<v Speaker 2>Astronomical unit.

698
00:39:28.039 --> 00:39:29.800
<v Speaker 1>Yeah, that was the distance between us and the Sun.

699
00:39:29.960 --> 00:39:32.079
<v Speaker 2>I just learned that and then completely forgot it all

700
00:39:32.079 --> 00:39:33.400
<v Speaker 2>in this span of a couple of weeks.

701
00:39:33.960 --> 00:39:36.039
<v Speaker 1>It's okay, there's no reason to know that stuff.

702
00:39:36.519 --> 00:39:38.239
<v Speaker 2>I want to know a little bit more about when

703
00:39:38.239 --> 00:39:40.079
<v Speaker 2>you were a kid. By the time Katie was about

704
00:39:40.159 --> 00:39:43.920
<v Speaker 2>ten years old, she was inspired to pursue some form

705
00:39:43.960 --> 00:39:47.679
<v Speaker 2>of cosmology, and she was already a fan of British

706
00:39:47.719 --> 00:39:52.760
<v Speaker 2>cosmologists and theoretical physicist Stephen Hawking. She was already hip

707
00:39:52.800 --> 00:39:55.320
<v Speaker 2>to him. She's like, I know this dude now. If

708
00:39:55.320 --> 00:39:57.559
<v Speaker 2>you need a quick brush up on him as a person.

709
00:39:58.000 --> 00:40:03.159
<v Speaker 2>After this podcast, watch the twenty fourteen Eddy Redmain film

710
00:40:03.280 --> 00:40:04.280
<v Speaker 2>The Theory of Everything.

711
00:40:04.519 --> 00:40:09.280
<v Speaker 1>A cosmologist. What's that? I study? The marriage of space

712
00:40:09.400 --> 00:40:10.920
<v Speaker 1>and time.

713
00:40:10.400 --> 00:40:14.679
<v Speaker 2>The perfect couple. Or you can just watch the trailer

714
00:40:14.719 --> 00:40:18.519
<v Speaker 2>and start crying like somebody you know. Now, if thinking

715
00:40:18.519 --> 00:40:21.480
<v Speaker 2>about living on a dust moat floating in a sunbeam

716
00:40:21.880 --> 00:40:23.519
<v Speaker 2>was an inspiration to do what you want to do

717
00:40:23.559 --> 00:40:26.840
<v Speaker 2>in life, consider a human who's figuring out the mysteries

718
00:40:26.840 --> 00:40:30.960
<v Speaker 2>of the cosmos, doing computations and cracking theories about which

719
00:40:31.119 --> 00:40:35.079
<v Speaker 2>I can't even comprehend. The first paragraph of the Wikipedia

720
00:40:35.119 --> 00:40:38.800
<v Speaker 2>page also while living with als, Katie is one of

721
00:40:38.880 --> 00:40:42.800
<v Speaker 2>several billion people inspired by Stephen Hawking. What was it

722
00:40:42.800 --> 00:40:45.840
<v Speaker 2>that Stephen Hawking did or what did you How did

723
00:40:45.880 --> 00:40:47.480
<v Speaker 2>you become aware of him? And how did you kind

724
00:40:47.480 --> 00:40:48.360
<v Speaker 2>of absorb what he did?

725
00:40:48.639 --> 00:40:50.920
<v Speaker 1>Oh, I'm not sure how I became aware of him.

726
00:40:50.960 --> 00:40:52.880
<v Speaker 1>I think that you know, he was on TV every

727
00:40:52.880 --> 00:40:55.360
<v Speaker 1>once in a while, and I had a Brief History

728
00:40:55.400 --> 00:40:59.559
<v Speaker 1>of Time the book, and I read that, and I

729
00:40:59.679 --> 00:41:02.239
<v Speaker 1>just like, I don't know, Like I was interested in

730
00:41:02.280 --> 00:41:05.480
<v Speaker 1>black holes, and I was interested in like the Big Bang.

731
00:41:05.400 --> 00:41:08.760
<v Speaker 2>The Big Bang theory being that the universe began those

732
00:41:08.800 --> 00:41:12.480
<v Speaker 2>thirteen billion years ago with high temperatures and high density,

733
00:41:12.599 --> 00:41:18.159
<v Speaker 2>it's continued to expand Also note if you google Big

734
00:41:18.159 --> 00:41:22.840
<v Speaker 2>Bang theory, all roads lead to Sheldon, So just be

735
00:41:23.000 --> 00:41:26.840
<v Speaker 2>cash call it big bang as far as Wikipedia is concerned.

736
00:41:26.960 --> 00:41:29.000
<v Speaker 1>And so I would read about that stuff. And Stephen

737
00:41:29.039 --> 00:41:32.280
<v Speaker 1>Hawking was a big figure in those those areas, and

738
00:41:32.719 --> 00:41:34.760
<v Speaker 1>he was he was doing a lot of science, communication

739
00:41:35.599 --> 00:41:40.119
<v Speaker 1>and he would visit cal Tech every once in a while,

740
00:41:40.719 --> 00:41:43.119
<v Speaker 1>and I was growing up in LA and St. Long Beach,

741
00:41:43.199 --> 00:41:46.039
<v Speaker 1>and so I would sometimes, like my mom would take

742
00:41:46.039 --> 00:41:49.639
<v Speaker 1>me to see talks by physicists because I was super

743
00:41:49.639 --> 00:41:53.159
<v Speaker 1>excited about these things. And so I remember seeing talked

744
00:41:53.159 --> 00:41:55.920
<v Speaker 1>by him, I remember seeing up talk by Paul Davies

745
00:41:56.000 --> 00:42:01.039
<v Speaker 1>and like, you know, just prominent theorists give talk sometimes,

746
00:42:01.039 --> 00:42:02.719
<v Speaker 1>and somehow my mom would find out about them and

747
00:42:02.760 --> 00:42:05.519
<v Speaker 1>take me along because she's she's really into science and

748
00:42:05.519 --> 00:42:07.679
<v Speaker 1>science fiction and physics and everything.

749
00:42:08.119 --> 00:42:10.119
<v Speaker 2>Have you gotten to meet Have you gotten to meet

750
00:42:10.199 --> 00:42:10.880
<v Speaker 2>stupid Hawking?

751
00:42:11.119 --> 00:42:16.199
<v Speaker 1>Yeah? Yeah, So when I was at Cambridge. So I

752
00:42:16.239 --> 00:42:19.320
<v Speaker 1>spent a year at Cambridge during grad school just kind

753
00:42:19.320 --> 00:42:21.400
<v Speaker 1>of visiting and working with people on some research. And

754
00:42:21.440 --> 00:42:24.480
<v Speaker 1>I was mostly based in his department and my office

755
00:42:24.639 --> 00:42:28.480
<v Speaker 1>was like directly below his. Yeah, and we were in

756
00:42:28.519 --> 00:42:31.960
<v Speaker 1>the same like research group basically, I mean like like

757
00:42:32.000 --> 00:42:34.440
<v Speaker 1>we didn't talk, like we weren't. I wasn't in his

758
00:42:34.480 --> 00:42:36.440
<v Speaker 1>research group, but we were in the same as the

759
00:42:36.480 --> 00:42:38.880
<v Speaker 1>center for the article cosmology, and like we were both

760
00:42:38.920 --> 00:42:41.119
<v Speaker 1>based there. So there were you know, half a dozen

761
00:42:41.480 --> 00:42:43.400
<v Speaker 1>professors who were involved to that. He was one of them,

762
00:42:43.400 --> 00:42:47.360
<v Speaker 1>and I was a grad student visiting, and so I

763
00:42:47.360 --> 00:42:49.599
<v Speaker 1>would go to all these like you know, meetings and

764
00:42:49.639 --> 00:42:54.639
<v Speaker 1>the coffee and stuff. And shortly after I was shortly

765
00:42:54.679 --> 00:42:58.679
<v Speaker 1>after I started being a visitor there, somebody asked me

766
00:42:58.719 --> 00:43:02.559
<v Speaker 1>to do one of the like lunch seminars.

767
00:43:02.760 --> 00:43:05.960
<v Speaker 2>So basically, if you're a physicist and you're visiting another department,

768
00:43:06.360 --> 00:43:08.519
<v Speaker 2>you're kind of obligated to give a talk. That's kind

769
00:43:08.519 --> 00:43:11.519
<v Speaker 2>of how it works. So they say, hey, can you

770
00:43:11.559 --> 00:43:13.639
<v Speaker 2>give a talk. She's like, yeah, I'll give a talk

771
00:43:13.679 --> 00:43:17.559
<v Speaker 2>for the Thursday lunch seminar. So she does it, and.

772
00:43:17.639 --> 00:43:20.000
<v Speaker 1>It turns out that it was the lunch seminar that

773
00:43:20.199 --> 00:43:25.400
<v Speaker 1>like Hawking goes to. I'm getting ready to give the talk,

774
00:43:25.679 --> 00:43:28.280
<v Speaker 1>and I see like several of my professors in the

775
00:43:28.320 --> 00:43:32.679
<v Speaker 1>audience like looking expectantly at me, and this is when

776
00:43:32.719 --> 00:43:36.880
<v Speaker 1>I'm like freaking out. But he wasn't there. Hawking wasn't there.

777
00:43:36.920 --> 00:43:39.480
<v Speaker 1>So I was like, it's fine, it's fine, and I'm

778
00:43:39.519 --> 00:43:41.079
<v Speaker 1>getting ready to give the talk, and then I hear

779
00:43:41.119 --> 00:43:43.519
<v Speaker 1>this like beep beep beep.

780
00:43:44.199 --> 00:43:47.159
<v Speaker 2>Oh my god, my stomach is cramping just hearing this.

781
00:43:47.639 --> 00:43:50.800
<v Speaker 1>And he shows up. Oh gets so much worse. Oh god,

782
00:43:51.280 --> 00:43:54.360
<v Speaker 1>So I've told this story before, but it's it's still

783
00:43:54.519 --> 00:43:58.559
<v Speaker 1>it's still like is it makes me like sweat? So

784
00:43:58.559 --> 00:44:00.840
<v Speaker 1>so I was, I was getting ready to give the talk,

785
00:44:00.880 --> 00:44:03.480
<v Speaker 1>and so I start the talk, like I put up

786
00:44:03.480 --> 00:44:06.599
<v Speaker 1>the title slide, and I was the topic was primordial

787
00:44:06.639 --> 00:44:09.920
<v Speaker 1>black holes, which is a concept that Hawking came up

788
00:44:09.960 --> 00:44:15.320
<v Speaker 1>with along with some other people and pressure. Yeah, And

789
00:44:15.400 --> 00:44:18.119
<v Speaker 1>as I'm starting, like as I after I introduced the

790
00:44:18.159 --> 00:44:22.519
<v Speaker 1>title and stuff, I hear this this voice say and

791
00:44:22.599 --> 00:44:26.559
<v Speaker 1>it was his voice, and I was like, and everybody

792
00:44:26.679 --> 00:44:29.119
<v Speaker 1>kind of laughed, you know, and I thought maybe he

793
00:44:29.280 --> 00:44:32.320
<v Speaker 1>was like thanking me for talking about the thing that

794
00:44:32.360 --> 00:44:34.159
<v Speaker 1>he invented, you know. But I don't know. And you

795
00:44:34.199 --> 00:44:37.559
<v Speaker 1>can't ask him to elaborate because he's his speech is

796
00:44:37.679 --> 00:44:40.679
<v Speaker 1>very like slow. So he uses this machine thing and

797
00:44:40.719 --> 00:44:42.320
<v Speaker 1>it just it's very slow.

798
00:44:42.760 --> 00:44:44.159
<v Speaker 2>At tracks his eye movements.

799
00:44:44.719 --> 00:44:47.639
<v Speaker 1>Yeah, well no, not exactly. It tracks there's a little

800
00:44:47.639 --> 00:44:50.000
<v Speaker 1>sensor that looks at his cheek, okay, and so he

801
00:44:50.079 --> 00:44:53.719
<v Speaker 1>kind of winks and that like selects words on this

802
00:44:53.920 --> 00:44:56.199
<v Speaker 1>like list and it takes a couple of minutes per

803
00:44:56.199 --> 00:44:59.800
<v Speaker 1>words sometimes, right, So you weren't like I couldn't elaborate. Yeah, yeah,

804
00:45:00.000 --> 00:45:03.079
<v Speaker 1>So I had, so, so I just kept going and

805
00:45:03.119 --> 00:45:06.400
<v Speaker 1>then eventually like I heard it again yes or later

806
00:45:06.480 --> 00:45:10.239
<v Speaker 1>on oh, or I don't know, or just random things

807
00:45:10.280 --> 00:45:12.000
<v Speaker 1>as I'm going, And every time, like I'd look at

808
00:45:12.079 --> 00:45:14.119
<v Speaker 1>him and I'd be like, you know, but he would

809
00:45:14.199 --> 00:45:16.320
<v Speaker 1>just kind of look blankly at me. And the person

810
00:45:16.360 --> 00:45:18.199
<v Speaker 1>who was like taking care of him is the lunch seminar,

811
00:45:18.280 --> 00:45:20.000
<v Speaker 1>so the person who was taking care of him like feedium,

812
00:45:20.039 --> 00:45:21.760
<v Speaker 1>and she just kind of looked blankly at me, and

813
00:45:21.840 --> 00:45:23.960
<v Speaker 1>like I had no idea what was going on, and

814
00:45:24.039 --> 00:45:27.480
<v Speaker 1>so I would just kind of pause and then continue.

815
00:45:27.760 --> 00:45:29.639
<v Speaker 1>I guess, like what am I gonna do?

816
00:45:30.760 --> 00:45:31.880
<v Speaker 2>What was happening here?

817
00:45:31.960 --> 00:45:34.480
<v Speaker 1>Had no idea, And I was so nervous, and like

818
00:45:34.559 --> 00:45:37.320
<v Speaker 1>all the professors were there, and already one of the

819
00:45:37.360 --> 00:45:39.599
<v Speaker 1>other professors had been like asking a whole bunch of

820
00:45:39.599 --> 00:45:42.239
<v Speaker 1>really tough questions on like the second slide, so I

821
00:45:42.280 --> 00:45:43.639
<v Speaker 1>was already like freaked out.

822
00:45:43.920 --> 00:45:48.880
<v Speaker 2>Just imagine being in this situation. It's a nightmare. It's

823
00:45:48.920 --> 00:45:51.480
<v Speaker 2>like the best nightmare ever.

824
00:45:51.880 --> 00:45:54.159
<v Speaker 1>But like I answered the questions and that he seemed

825
00:45:54.159 --> 00:45:56.880
<v Speaker 1>to be okay with it. So I finished the talk

826
00:45:57.079 --> 00:46:00.440
<v Speaker 1>and Hawking left and he hadn't asked any questions. And

827
00:46:01.199 --> 00:46:04.239
<v Speaker 1>I asked one of the seminar organizers, like, what what

828
00:46:04.280 --> 00:46:07.199
<v Speaker 1>was that? And he was like, oh, well, when he

829
00:46:07.280 --> 00:46:10.760
<v Speaker 1>eats the machine, my step one is chewing and it

830
00:46:10.920 --> 00:46:14.480
<v Speaker 1>just picks random stuff from like the quick select menu.

831
00:46:16.239 --> 00:46:19.199
<v Speaker 1>So nothing to do with you at all. It was

832
00:46:19.320 --> 00:46:21.719
<v Speaker 1>just like it was just like, here's the you know,

833
00:46:21.760 --> 00:46:24.320
<v Speaker 1>here's the most common phrases. Guess no, maybe I don't know.

834
00:46:24.360 --> 00:46:24.920
<v Speaker 1>I don't think so.

835
00:46:26.360 --> 00:46:29.000
<v Speaker 2>Oh my god, this is like the worst deodorant ad ever,

836
00:46:29.239 --> 00:46:32.639
<v Speaker 2>Like this is the most stressful situation you could possibly

837
00:46:32.719 --> 00:46:33.119
<v Speaker 2>ever be.

838
00:46:33.719 --> 00:46:36.360
<v Speaker 1>Oh my god. And like they could have told me.

839
00:46:36.719 --> 00:46:40.320
<v Speaker 2>Yeah, they could have given you every time, Oh my god.

840
00:46:40.760 --> 00:46:43.960
<v Speaker 1>They just like they just didn't mention it.

841
00:46:44.079 --> 00:46:45.840
<v Speaker 2>Any word on whether or not he liked your talk.

842
00:46:46.280 --> 00:46:47.000
<v Speaker 1>I have no idea.

843
00:46:47.239 --> 00:46:51.320
<v Speaker 2>Oh god, could you ever tell him that you went

844
00:46:51.360 --> 00:46:53.679
<v Speaker 2>into cosmology because of him?

845
00:46:53.960 --> 00:46:54.960
<v Speaker 1>I don't.

846
00:46:55.119 --> 00:46:55.360
<v Speaker 5>Well.

847
00:46:56.440 --> 00:47:01.119
<v Speaker 1>So the first time I met him, when I was sixty, oh,

848
00:47:01.360 --> 00:47:04.880
<v Speaker 1>just by fourteen fourteen, baby baby, I did tell him

849
00:47:04.880 --> 00:47:06.400
<v Speaker 1>then that I was a big fan.

850
00:47:06.719 --> 00:47:10.800
<v Speaker 2>So Hawking was at cal Tech and Katie got her

851
00:47:10.840 --> 00:47:13.559
<v Speaker 2>mom to drive her and a friend there to hear

852
00:47:13.639 --> 00:47:16.199
<v Speaker 2>him speak, and afterward they were walking the same way

853
00:47:16.239 --> 00:47:18.519
<v Speaker 2>that he was going when they were leaving, and she

854
00:47:18.639 --> 00:47:20.079
<v Speaker 2>was too nervous to say hi.

855
00:47:20.280 --> 00:47:23.000
<v Speaker 1>I my friend went up to him and said, my

856
00:47:23.079 --> 00:47:26.119
<v Speaker 1>friend would like to speak to you. She had a wingman,

857
00:47:27.840 --> 00:47:29.760
<v Speaker 1>so I went up and said that I was a

858
00:47:29.800 --> 00:47:32.800
<v Speaker 1>big fan and I enjoyed his work, and I thanked him,

859
00:47:32.840 --> 00:47:33.719
<v Speaker 1>and he said.

860
00:47:33.599 --> 00:47:34.760
<v Speaker 2>Thank you very much.

861
00:47:35.079 --> 00:47:35.519
<v Speaker 4>Oh.

862
00:47:36.239 --> 00:47:38.559
<v Speaker 2>Now, what happens to you when you get that? Because

863
00:47:38.599 --> 00:47:41.800
<v Speaker 2>you're really I mean, I'm not going to fangirl right here,

864
00:47:41.840 --> 00:47:43.360
<v Speaker 2>I'll do it in the intro. But you're like a

865
00:47:43.480 --> 00:47:46.800
<v Speaker 2>very big voice in science communication. You're like, you're a

866
00:47:46.960 --> 00:47:51.000
<v Speaker 2>very well known astrophysicist, cosmologist. How do you feel when

867
00:47:51.000 --> 00:47:52.679
<v Speaker 2>people come up to you and say I was inspired

868
00:47:52.679 --> 00:47:55.400
<v Speaker 2>to study this or you've changed my course, Like, what

869
00:47:55.480 --> 00:47:56.639
<v Speaker 2>kind of reactions do you get?

870
00:47:56.880 --> 00:48:00.440
<v Speaker 1>It's I mean, it doesn't so it's not I'm not

871
00:48:01.000 --> 00:48:03.480
<v Speaker 1>like Stephen Hawking, Like I'm not that level of famous

872
00:48:03.519 --> 00:48:06.199
<v Speaker 1>and I'm not that level of like important in physics

873
00:48:06.199 --> 00:48:08.760
<v Speaker 1>and stuff and and you know, so it's it's kind

874
00:48:08.760 --> 00:48:11.199
<v Speaker 1>of a different thing. But I do you know, sometimes

875
00:48:11.199 --> 00:48:16.679
<v Speaker 1>people do like tell me that they like So one

876
00:48:16.719 --> 00:48:18.840
<v Speaker 1>of the messages I've gotten a couple of times is

877
00:48:19.079 --> 00:48:24.239
<v Speaker 1>a like a teenage girl will say that she didn't

878
00:48:24.239 --> 00:48:27.599
<v Speaker 1>think she could do astrophysics, but she really loved it,

879
00:48:27.639 --> 00:48:29.960
<v Speaker 1>and then she saw what I was saying on Twitter

880
00:48:30.079 --> 00:48:32.760
<v Speaker 1>or something, or she saw me speak and then she

881
00:48:32.800 --> 00:48:34.159
<v Speaker 1>decided she was going to go for it.

882
00:48:34.280 --> 00:48:34.559
<v Speaker 2>Wow.

883
00:48:35.159 --> 00:48:39.440
<v Speaker 1>So I do get that sometimes and I like my

884
00:48:39.519 --> 00:48:42.159
<v Speaker 1>feelings don't know what to do with that. Yeah, but

885
00:48:42.440 --> 00:48:45.280
<v Speaker 1>it's really it's really sweet and.

886
00:48:45.320 --> 00:48:47.639
<v Speaker 2>Throwing in a black hole no feelings.

887
00:48:47.719 --> 00:48:51.599
<v Speaker 1>He I mean, it is really sweet. It's really like

888
00:48:52.320 --> 00:48:55.320
<v Speaker 1>rewarding when that happens, and it it makes me feel

889
00:48:55.320 --> 00:48:58.280
<v Speaker 1>like maybe, like this stuff is maybe the stuff I'm

890
00:48:58.320 --> 00:49:01.079
<v Speaker 1>doing is worthwhile. When we'll say stuff like that, or

891
00:49:01.119 --> 00:49:03.599
<v Speaker 1>like a little kid will sometimes say that they want

892
00:49:03.599 --> 00:49:05.960
<v Speaker 1>to be an astrophysicist or something, and they'll be really

893
00:49:05.960 --> 00:49:08.320
<v Speaker 1>excited to meet me, like I was. I was in

894
00:49:08.400 --> 00:49:12.679
<v Speaker 1>Raleigh a couple of weeks ago, and I was I

895
00:49:12.719 --> 00:49:14.280
<v Speaker 1>was sitting in a cafe and I was wearing my

896
00:49:14.400 --> 00:49:17.239
<v Speaker 1>NASA jacket with a little NASA badge on it that

897
00:49:17.320 --> 00:49:18.320
<v Speaker 1>I got JPL.

898
00:49:18.760 --> 00:49:22.239
<v Speaker 2>JPL, by the way, is NASA's Jet Propulsion Laboratory and

899
00:49:22.280 --> 00:49:26.559
<v Speaker 2>it's nestled in the Golden Hills of Pasadena, California, and

900
00:49:26.599 --> 00:49:30.559
<v Speaker 2>it's responsible for things like rovers on Mars, and according

901
00:49:30.559 --> 00:49:34.159
<v Speaker 2>to press materials, JPL's function is to engineer and fabricate

902
00:49:34.320 --> 00:49:37.920
<v Speaker 2>cool ass shit. That's like so dope, that's very bold.

903
00:49:38.000 --> 00:49:40.719
<v Speaker 2>NASA I also do not fact check that part, and

904
00:49:40.760 --> 00:49:42.320
<v Speaker 2>it's not true.

905
00:49:42.719 --> 00:49:44.880
<v Speaker 1>And this little girl came up to me and she

906
00:49:45.000 --> 00:49:49.239
<v Speaker 1>was probably like eight or something, and she asked me

907
00:49:49.280 --> 00:49:51.159
<v Speaker 1>if I work for NASA, and I said, I don't

908
00:49:51.159 --> 00:49:56.079
<v Speaker 1>work VANASA, but I am an astrophysicist, and so we'd

909
00:49:56.199 --> 00:49:58.199
<v Speaker 1>like talked a little bit, and she said that she

910
00:49:58.320 --> 00:50:00.639
<v Speaker 1>really is into space and and I was like, well,

911
00:50:00.679 --> 00:50:02.960
<v Speaker 1>I'm giving a talk at the museum in a couple

912
00:50:03.000 --> 00:50:05.360
<v Speaker 1>of days. You can come and hear my talk. And

913
00:50:05.559 --> 00:50:07.920
<v Speaker 1>so she and her mom came to my talk and

914
00:50:08.519 --> 00:50:11.000
<v Speaker 1>she asked a question and it was just really sweet,

915
00:50:11.119 --> 00:50:14.719
<v Speaker 1>and I was like, oh, what was her question? I

916
00:50:14.760 --> 00:50:17.719
<v Speaker 1>think her I think her question was about like what's

917
00:50:17.760 --> 00:50:20.800
<v Speaker 1>inside a black hole m hm, which is a good question.

918
00:50:20.760 --> 00:50:22.039
<v Speaker 2>Like a bunch of space garbage.

919
00:50:22.280 --> 00:50:24.599
<v Speaker 1>Well, yeah, so it's I mean, that's it's not as

920
00:50:24.639 --> 00:50:27.800
<v Speaker 1>straightforward answer really, because once stuff goes inside the black hole,

921
00:50:27.840 --> 00:50:29.719
<v Speaker 1>it has to go straight to the singularity and it

922
00:50:29.760 --> 00:50:32.400
<v Speaker 1>can't do anything else. And so then does it really

923
00:50:32.400 --> 00:50:35.639
<v Speaker 1>exist at that point? Like that's kind of subtle, but anyways,

924
00:50:35.679 --> 00:50:37.960
<v Speaker 1>a good question. And apparently like she was talking about

925
00:50:37.960 --> 00:50:40.239
<v Speaker 1>the talk later on, and I was like, okay, you know,

926
00:50:40.280 --> 00:50:41.440
<v Speaker 1>I inspired somebody.

927
00:50:41.559 --> 00:50:43.360
<v Speaker 2>She's going to be in your department later and give

928
00:50:43.400 --> 00:50:48.199
<v Speaker 2>a talk a your live sham explained the singularity.

929
00:50:48.400 --> 00:50:52.039
<v Speaker 1>Oh yeah, yeah. So a singularity is so it comes

930
00:50:52.119 --> 00:50:54.039
<v Speaker 1>up in the context of the Big Bang and in

931
00:50:54.079 --> 00:50:57.760
<v Speaker 1>the context of a black hole. A singularity is like

932
00:50:58.000 --> 00:51:04.760
<v Speaker 1>a point of infinite density. Okay. Usually in physics, when

933
00:51:04.800 --> 00:51:07.480
<v Speaker 1>you have a singularity, I mean a singularity basically means

934
00:51:07.559 --> 00:51:10.880
<v Speaker 1>it's a point where something infinite happens, like where things

935
00:51:10.920 --> 00:51:14.440
<v Speaker 1>diverge in some way. And usually when that happens in physics,

936
00:51:14.440 --> 00:51:16.920
<v Speaker 1>it means you've done something wrong, okay, and it's a

937
00:51:16.960 --> 00:51:19.679
<v Speaker 1>sign that the theory is broken and you just can't

938
00:51:19.719 --> 00:51:22.000
<v Speaker 1>deal with that because it is none of the none

939
00:51:22.039 --> 00:51:26.679
<v Speaker 1>of the theory like really works at a point of infinite anything, Okay.

940
00:51:27.880 --> 00:51:30.159
<v Speaker 1>In the black hole, like the way that black holes

941
00:51:30.199 --> 00:51:32.039
<v Speaker 1>are defined and the way that we understand how the

942
00:51:32.079 --> 00:51:34.559
<v Speaker 1>gravity works, there really should be a singularity at the

943
00:51:34.559 --> 00:51:38.119
<v Speaker 1>center of the black hole, and everything has to move

944
00:51:38.159 --> 00:51:41.000
<v Speaker 1>toward it. So so the you know, the black hole

945
00:51:41.000 --> 00:51:43.320
<v Speaker 1>has this is this thing that like, the way you

946
00:51:43.360 --> 00:51:45.000
<v Speaker 1>make a black hole, you get back up.

947
00:51:45.239 --> 00:51:46.840
<v Speaker 2>Yeah, no, backup, because they're like, where do they come from?

948
00:51:46.840 --> 00:51:47.280
<v Speaker 2>What's the deal?

949
00:51:47.440 --> 00:51:48.880
<v Speaker 1>Yeah, So the way you make a black hole is

950
00:51:48.880 --> 00:51:51.840
<v Speaker 1>you take a really massive star and you wait a

951
00:51:51.840 --> 00:51:56.679
<v Speaker 1>while millions of years, and the star will explode and

952
00:51:57.199 --> 00:51:59.280
<v Speaker 1>the core of the star will collapse on itself. And

953
00:51:59.320 --> 00:52:03.360
<v Speaker 1>if it's massive enough, then I mean the reason that

954
00:52:03.400 --> 00:52:05.920
<v Speaker 1>the star didn't collapse before is because it had nuclear

955
00:52:05.920 --> 00:52:08.840
<v Speaker 1>burning happening. It was kind of keeping it puffed up, okay, right,

956
00:52:09.440 --> 00:52:11.480
<v Speaker 1>and so you had this energy source that's sort of

957
00:52:11.480 --> 00:52:13.599
<v Speaker 1>pushing against it, kind of like if you have like

958
00:52:13.639 --> 00:52:17.320
<v Speaker 1>a balloon in the air inside is pushing the plastic,

959
00:52:17.559 --> 00:52:21.760
<v Speaker 1>the rubber out. Right. When the star explodes, there's nothing

960
00:52:21.800 --> 00:52:26.519
<v Speaker 1>to keep it from collapsing under its own gravity. You know,

961
00:52:26.320 --> 00:52:28.800
<v Speaker 1>you get to a point where there's you can't do

962
00:52:28.920 --> 00:52:29.440
<v Speaker 1>any more.

963
00:52:29.719 --> 00:52:33.440
<v Speaker 2>Nuclear fusion, So nuclear fusion is when atoms join to

964
00:52:33.480 --> 00:52:36.320
<v Speaker 2>become a different kind of atom and they give off

965
00:52:36.519 --> 00:52:40.320
<v Speaker 2>energy in the process, like two hydrogens becoming a helium

966
00:52:40.679 --> 00:52:44.440
<v Speaker 2>and giving off energy. Now, this happens with atoms up

967
00:52:44.480 --> 00:52:47.800
<v Speaker 2>to the size of iron, at which point that fusion

968
00:52:47.920 --> 00:52:49.280
<v Speaker 2>starts to take energy.

969
00:52:49.440 --> 00:52:51.880
<v Speaker 1>You can't get any more energy out of those processes

970
00:52:51.920 --> 00:52:53.840
<v Speaker 1>because you've gotten to a point where you've just the

971
00:52:53.880 --> 00:52:57.519
<v Speaker 1>whole center of the star is iron basically, and it

972
00:52:58.000 --> 00:53:00.480
<v Speaker 1>can't go farther than that. And so then you have

973
00:53:00.519 --> 00:53:03.239
<v Speaker 1>this like huge chunk of iron that's not being held

974
00:53:03.280 --> 00:53:05.400
<v Speaker 1>up by anything, and so it starts to collapse under

975
00:53:05.400 --> 00:53:08.159
<v Speaker 1>its own gravity. Like that stuff just falls in and

976
00:53:08.199 --> 00:53:10.440
<v Speaker 1>it has to go toward the center, and it has

977
00:53:10.480 --> 00:53:13.159
<v Speaker 1>to keep going toward the center, and it can't go

978
00:53:13.199 --> 00:53:16.480
<v Speaker 1>any other direction, and so you end up with this singularity,

979
00:53:16.760 --> 00:53:20.559
<v Speaker 1>this point of infinite density. Technically, what is this shape?

980
00:53:20.639 --> 00:53:20.719
<v Speaker 4>Like?

981
00:53:20.840 --> 00:53:23.840
<v Speaker 2>Is it like an ice cream cone that has an

982
00:53:23.880 --> 00:53:25.039
<v Speaker 2>infinite tail?

983
00:53:25.199 --> 00:53:27.320
<v Speaker 1>Or what is I mean? You can visualize it that

984
00:53:27.360 --> 00:53:29.719
<v Speaker 1>way if you think about it in terms of like

985
00:53:29.760 --> 00:53:33.400
<v Speaker 1>a two D analog. Like usually when we think of

986
00:53:33.400 --> 00:53:35.719
<v Speaker 1>space time, like the pictures are always like a big

987
00:53:35.800 --> 00:53:36.800
<v Speaker 1>rub rubber sheet.

988
00:53:37.000 --> 00:53:42.199
<v Speaker 2>The rubber sheet visual is so helpful for comprehending space time.

989
00:53:43.960 --> 00:53:47.480
<v Speaker 2>But also when I think of rubber sheets, usually the

990
00:53:47.559 --> 00:53:52.280
<v Speaker 2>situation is not comfortable. It's either like an awkward graded

991
00:53:52.440 --> 00:53:57.880
<v Speaker 2>school slumber party, explanation or some suburban dungeon kink that

992
00:53:58.000 --> 00:54:04.519
<v Speaker 2>sounds exasperate at best. But for space, rubber sheets thumbs up.

993
00:54:04.800 --> 00:54:06.320
<v Speaker 1>And you have this big rubber sheet and you put

994
00:54:06.320 --> 00:54:09.639
<v Speaker 1>a bowling ball in one spot and that bends around,

995
00:54:09.840 --> 00:54:11.639
<v Speaker 1>and so then when you take your tennis ball and

996
00:54:11.639 --> 00:54:13.039
<v Speaker 1>you try and roll it past the bowling ball, it

997
00:54:13.039 --> 00:54:15.079
<v Speaker 1>makes a little orbit and falls in right. Wow, this

998
00:54:15.159 --> 00:54:18.920
<v Speaker 1>is the usual visualization for space time. But that doesn't

999
00:54:18.920 --> 00:54:21.800
<v Speaker 1>have the right number of dimensions because space is space

1000
00:54:21.880 --> 00:54:24.400
<v Speaker 1>is three dimensional, and then you can think of time

1001
00:54:24.480 --> 00:54:27.119
<v Speaker 1>as another dimension, but that's kind of separate thing.

1002
00:54:27.360 --> 00:54:29.360
<v Speaker 2>I am curious about time as a fourth dimension.

1003
00:54:29.360 --> 00:54:31.639
<v Speaker 1>Okay, we can talk about that, Okay, but.

1004
00:54:31.480 --> 00:54:33.840
<v Speaker 2>We're going to take a quick break for sponsors of

1005
00:54:33.880 --> 00:54:36.559
<v Speaker 2>the show. Sponsors. Why sponsors, You know what they do?

1006
00:54:36.679 --> 00:54:39.639
<v Speaker 2>They help us give money to different charities every week.

1007
00:54:39.840 --> 00:54:42.199
<v Speaker 2>So if you want to know where Ologies gives our money,

1008
00:54:42.360 --> 00:54:44.880
<v Speaker 2>you can go to alleyword dot com and look for

1009
00:54:44.920 --> 00:54:48.039
<v Speaker 2>the tab Ologies gives back. There's like one hundred and

1010
00:54:48.039 --> 00:54:51.119
<v Speaker 2>fifty different charities that we've given to already, with more

1011
00:54:51.320 --> 00:54:53.280
<v Speaker 2>every single week. So if you need a place to

1012
00:54:53.320 --> 00:54:54.719
<v Speaker 2>go donate a little bit of money. But you're not

1013
00:54:54.800 --> 00:54:57.920
<v Speaker 2>sure where to go. Those are all picked biologists who

1014
00:54:57.960 --> 00:55:01.440
<v Speaker 2>work in those fields, and this ad break allows us

1015
00:55:01.480 --> 00:55:04.760
<v Speaker 2>to give a ton of money to them. So thanks

1016
00:55:04.840 --> 00:55:08.719
<v Speaker 2>for listening and thank sponsors. Okay, I'm sorry, I have

1017
00:55:08.960 --> 00:55:10.639
<v Speaker 2>so many questions.

1018
00:55:10.280 --> 00:55:13.639
<v Speaker 1>But anyway, So, if space is three dimensional, then the

1019
00:55:13.679 --> 00:55:17.159
<v Speaker 1>way gravity like works on it is that it kind

1020
00:55:17.199 --> 00:55:20.639
<v Speaker 1>of like pulls space inward toward itself. So like a

1021
00:55:20.639 --> 00:55:23.400
<v Speaker 1>massive thing kind of pulls space inward toward itself. So

1022
00:55:24.440 --> 00:55:26.920
<v Speaker 1>in the context of a black hole, it would be

1023
00:55:26.960 --> 00:55:29.800
<v Speaker 1>like a place where space gets really scrunched up, right,

1024
00:55:30.199 --> 00:55:32.159
<v Speaker 1>But it's easier to think about it in the two

1025
00:55:32.199 --> 00:55:34.039
<v Speaker 1>dimensional case. So it would be like you have your

1026
00:55:34.119 --> 00:55:37.199
<v Speaker 1>rubber sheet and you pinch a piece of that rubber

1027
00:55:37.239 --> 00:55:38.440
<v Speaker 1>sheet and you just pull it down, and you just

1028
00:55:38.480 --> 00:55:41.519
<v Speaker 1>keep pulling it down, and it just goes to a

1029
00:55:41.519 --> 00:55:43.679
<v Speaker 1>point and it's like, you know, forever, and it gets

1030
00:55:43.679 --> 00:55:47.719
<v Speaker 1>deeper and narrower whatever. Right, So you can think about

1031
00:55:47.760 --> 00:55:49.320
<v Speaker 1>it like that, But then you think about like a

1032
00:55:49.360 --> 00:55:51.320
<v Speaker 1>three dimensional analog, and your brain kind of breaks and

1033
00:55:51.360 --> 00:55:55.159
<v Speaker 1>it's righter. But yeah, so it's basically a place where

1034
00:55:55.199 --> 00:55:59.000
<v Speaker 1>space is really super curved, okay, really super bent inward

1035
00:55:59.639 --> 00:56:04.000
<v Speaker 1>and so there's a point. So if you think again

1036
00:56:04.039 --> 00:56:07.400
<v Speaker 1>about the two D kind of thing, the rubber sheet,

1037
00:56:07.880 --> 00:56:11.039
<v Speaker 1>you can you can still move past. Like you if

1038
00:56:11.039 --> 00:56:13.599
<v Speaker 1>you have your your like little hole that you pulled

1039
00:56:13.599 --> 00:56:15.320
<v Speaker 1>down on a rubber sheet, you can still take your

1040
00:56:15.360 --> 00:56:17.639
<v Speaker 1>tennis ball and roll it past that and it'll keep going.

1041
00:56:17.880 --> 00:56:20.000
<v Speaker 1>But if it gets too close, it'll fall in and

1042
00:56:20.000 --> 00:56:22.039
<v Speaker 1>there's nothing you can do about it, and it'll always

1043
00:56:22.079 --> 00:56:25.679
<v Speaker 1>go toward the deepest point. And so that's like there's

1044
00:56:25.719 --> 00:56:29.159
<v Speaker 1>this horizon, this, this distance from this from that singularity

1045
00:56:29.440 --> 00:56:31.679
<v Speaker 1>where if you get closer than that, you will fall

1046
00:56:31.679 --> 00:56:33.800
<v Speaker 1>in no matter what, and you will just keep going

1047
00:56:33.840 --> 00:56:36.960
<v Speaker 1>and you can't ever escape, and light itself will fall

1048
00:56:37.000 --> 00:56:41.239
<v Speaker 1>into because light follows the curve of space, and so

1049
00:56:41.519 --> 00:56:43.800
<v Speaker 1>if space is curved enough, then light will just follow

1050
00:56:43.800 --> 00:56:47.280
<v Speaker 1>that curve all the way down. Oh man, so once

1051
00:56:47.559 --> 00:56:50.239
<v Speaker 1>you know, so you throw flo flashlight into a black hole,

1052
00:56:50.280 --> 00:56:52.559
<v Speaker 1>like that light never comes out again. It just goes

1053
00:56:52.679 --> 00:56:55.679
<v Speaker 1>that that light beam. No matter which direction the flashlight

1054
00:56:55.760 --> 00:56:57.719
<v Speaker 1>is facing, the light beam will bend toward the center.

1055
00:56:58.199 --> 00:57:00.199
<v Speaker 2>And what is that danger zone called.

1056
00:57:00.639 --> 00:57:02.960
<v Speaker 1>The event Horizonka, that is the event, Yeah, that's the

1057
00:57:03.000 --> 00:57:06.320
<v Speaker 1>event horizon. I mean you should probably stay farther than

1058
00:57:06.360 --> 00:57:11.039
<v Speaker 1>the events event in general, because other bad things can

1059
00:57:11.079 --> 00:57:12.559
<v Speaker 1>happen to you if you get close to the black hole.

1060
00:57:12.599 --> 00:57:16.199
<v Speaker 2>If you listen to Ology's episode one Volcanology and thought

1061
00:57:16.559 --> 00:57:19.840
<v Speaker 2>jumping into a volcano was intense, like hang on to

1062
00:57:19.880 --> 00:57:20.719
<v Speaker 2>your butts right now.

1063
00:57:20.920 --> 00:57:24.280
<v Speaker 1>I mean, so for one thing, that most of the

1064
00:57:24.519 --> 00:57:26.639
<v Speaker 1>most of the ones that we've seen directly with light

1065
00:57:26.800 --> 00:57:30.679
<v Speaker 1>are pulling in matter, right, and so that means that

1066
00:57:30.719 --> 00:57:33.280
<v Speaker 1>there's a lot of hot stuff falling into the black

1067
00:57:33.320 --> 00:57:36.840
<v Speaker 1>hole in the form of a disk, And so that'll

1068
00:57:36.960 --> 00:57:39.280
<v Speaker 1>radiate you to death if you get too close. And

1069
00:57:39.320 --> 00:57:41.639
<v Speaker 1>then if you if you get close, if it's a

1070
00:57:41.639 --> 00:57:44.280
<v Speaker 1>small enough black hole, then when you get close, the

1071
00:57:44.280 --> 00:57:47.400
<v Speaker 1>tidal forces will kill you. So tidal force is where

1072
00:57:47.440 --> 00:57:50.960
<v Speaker 1>you have like it's where you have more more gravity.

1073
00:57:51.159 --> 00:57:53.239
<v Speaker 1>The gravity is pulling stronger on part of you than

1074
00:57:53.280 --> 00:57:56.480
<v Speaker 1>another part. So like if like if you imagine, you

1075
00:57:56.519 --> 00:58:00.519
<v Speaker 1>know you're falling feet first toward a black hole, the

1076
00:58:00.599 --> 00:58:03.559
<v Speaker 1>gravity goes the strength of the gravity goes up so

1077
00:58:03.679 --> 00:58:07.840
<v Speaker 1>steeply because it's such a compact steep thing, then your

1078
00:58:07.840 --> 00:58:10.119
<v Speaker 1>feet will be pulled on much more tightly than your head,

1079
00:58:10.119 --> 00:58:13.000
<v Speaker 1>and you'll be stretched out and it's it's there's a

1080
00:58:13.039 --> 00:58:19.599
<v Speaker 1>word for it. It's called spaghettification. It's actually called that. Yeah. Yeah,

1081
00:58:19.119 --> 00:58:22.559
<v Speaker 1>so you have to watch out for spaghettification if you

1082
00:58:22.599 --> 00:58:24.679
<v Speaker 1>got too close to a black hole. Who the hell?

1083
00:58:24.800 --> 00:58:27.840
<v Speaker 1>Maybe I don't know, I don't know. I mean Hawking

1084
00:58:27.920 --> 00:58:29.639
<v Speaker 1>uses it, I don't and maybe he came up with it.

1085
00:58:29.639 --> 00:58:30.400
<v Speaker 1>I'm not really sure.

1086
00:58:30.559 --> 00:58:32.920
<v Speaker 2>Oh my god. But of all of the things to

1087
00:58:32.960 --> 00:58:33.599
<v Speaker 2>call it.

1088
00:58:33.679 --> 00:58:37.679
<v Speaker 1>Yeah, of all the turns you to spaghetti, I don't know,

1089
00:58:37.800 --> 00:58:39.960
<v Speaker 1>Like that's just what else are you gonna call it?

1090
00:58:40.000 --> 00:58:45.960
<v Speaker 1>Like it's title disruption? But I love it the most. Yeah.

1091
00:58:46.400 --> 00:58:50.079
<v Speaker 2>Spaghnification was indeed coined by Hawking in his book A

1092
00:58:50.119 --> 00:58:54.000
<v Speaker 2>Brief History of Time, And if you happen to Google

1093
00:58:54.039 --> 00:58:58.480
<v Speaker 2>image search this you will find a bounty of photoshopped

1094
00:58:58.480 --> 00:59:03.079
<v Speaker 2>images of astronauts being tapered into space noodles by cosmic forces.

1095
00:59:03.519 --> 00:59:07.119
<v Speaker 2>I'm so impressed by this astrophysical whimsy.

1096
00:59:07.320 --> 00:59:11.079
<v Speaker 1>Yeah, there are a lot of really silly names in astronomy.

1097
00:59:11.239 --> 00:59:12.559
<v Speaker 2>Who gets to name this stuff?

1098
00:59:13.480 --> 00:59:15.840
<v Speaker 1>Whoever comes up with it? I mean, people come up

1099
00:59:15.880 --> 00:59:18.119
<v Speaker 1>with a name it, but like sometimes the community names it,

1100
00:59:18.159 --> 00:59:22.159
<v Speaker 1>Like the Big Bang that was a joke, like that

1101
00:59:22.400 --> 00:59:24.599
<v Speaker 1>the word was a joke, the term the big bang,

1102
00:59:24.679 --> 00:59:26.599
<v Speaker 1>like somebody came up with the idea that you know,

1103
00:59:26.679 --> 00:59:31.199
<v Speaker 1>the universe started small and has been expanding, and somebody

1104
00:59:31.280 --> 00:59:35.159
<v Speaker 1>was like, oh, the big bang, and that it stuck.

1105
00:59:35.559 --> 00:59:37.239
<v Speaker 2>No, it was a throwaway.

1106
00:59:37.440 --> 00:59:38.760
<v Speaker 1>Yeah, it was like it was mocking.

1107
00:59:39.159 --> 00:59:40.840
<v Speaker 2>Did that person get pissed and it stuck?

1108
00:59:41.840 --> 00:59:42.440
<v Speaker 1>I'm not sure?

1109
00:59:42.519 --> 00:59:47.280
<v Speaker 2>Okay. So English astronomer Fred Hoyle coined the term big Bang.

1110
00:59:47.519 --> 00:59:50.719
<v Speaker 2>It was during a radio broadcast in the late nineteen

1111
00:59:50.800 --> 00:59:53.840
<v Speaker 2>forties and it was kind of an accident. Now the

1112
00:59:53.920 --> 00:59:57.920
<v Speaker 2>story is he's so bent that it's stuck, but apparently

1113
00:59:57.920 --> 01:00:02.360
<v Speaker 2>he denies that. So drama in terms of what in

1114
01:00:02.440 --> 01:00:05.400
<v Speaker 2>terms of what your output is, You're you're a professor,

1115
01:00:05.519 --> 01:00:07.960
<v Speaker 2>you give talks, you travel all over the world, Like

1116
01:00:08.079 --> 01:00:11.920
<v Speaker 2>what is your big goal as a cosmologist? Like do

1117
01:00:11.960 --> 01:00:14.800
<v Speaker 2>you want to write an encyclopedia about cosmology? Like what's

1118
01:00:14.840 --> 01:00:16.119
<v Speaker 2>your what's your endgame?

1119
01:00:16.360 --> 01:00:19.159
<v Speaker 1>So what my goal? Uh? I mean I want to

1120
01:00:19.199 --> 01:00:21.960
<v Speaker 1>figure stuff out, but I don't have like there's not

1121
01:00:22.079 --> 01:00:24.719
<v Speaker 1>like one thing where it's like I must solve this problem.

1122
01:00:24.840 --> 01:00:29.000
<v Speaker 1>I kind of like, uh, just working on whatever fun

1123
01:00:29.039 --> 01:00:32.400
<v Speaker 1>stuff comes up, which is not what you're supposed.

1124
01:00:32.039 --> 01:00:34.119
<v Speaker 2>To do, but it's what you like.

1125
01:00:34.400 --> 01:00:36.079
<v Speaker 1>It's always what I like. I mean. So the big

1126
01:00:36.119 --> 01:00:37.559
<v Speaker 1>thing I'm working on right now has to do with

1127
01:00:37.639 --> 01:00:41.360
<v Speaker 1>dark matter. So dark matter is this invisible stuff, you know,

1128
01:00:42.639 --> 01:00:45.760
<v Speaker 1>And it's possible that dark matter has this weird property

1129
01:00:45.800 --> 01:00:48.079
<v Speaker 1>where if you take a dark matter particle and another

1130
01:00:48.159 --> 01:00:51.760
<v Speaker 1>dark matter particle and you you like, collide them into

1131
01:00:51.760 --> 01:00:54.079
<v Speaker 1>each other in just the right way, they'll annihilate and

1132
01:00:54.119 --> 01:00:58.280
<v Speaker 1>create other kinds of particles. So that's a possibility. And

1133
01:00:58.360 --> 01:01:00.960
<v Speaker 1>if that's the case, if that the thing that happens,

1134
01:01:01.079 --> 01:01:03.320
<v Speaker 1>then it can mess with how the first stars and

1135
01:01:03.360 --> 01:01:06.840
<v Speaker 1>galaxies form, because those form and like blobs of dark matter,

1136
01:01:07.440 --> 01:01:11.320
<v Speaker 1>and the formation of those is kind of delicate because

1137
01:01:11.360 --> 01:01:13.119
<v Speaker 1>you have to get the right balance of the gravity

1138
01:01:13.159 --> 01:01:15.360
<v Speaker 1>and the gas and all this stuff. So if dark

1139
01:01:15.400 --> 01:01:18.440
<v Speaker 1>matter is going and like annihilating all the time, then

1140
01:01:18.519 --> 01:01:21.480
<v Speaker 1>that sort of messes with that balance, and so it

1141
01:01:21.519 --> 01:01:23.840
<v Speaker 1>can change the way the first stars and galaxies form,

1142
01:01:23.840 --> 01:01:26.280
<v Speaker 1>and then we can look for the evidence of that

1143
01:01:26.400 --> 01:01:28.880
<v Speaker 1>with telescopes. So this is the kind of problem that

1144
01:01:28.920 --> 01:01:31.119
<v Speaker 1>I like, where you have like a sort of fundamental

1145
01:01:31.199 --> 01:01:33.280
<v Speaker 1>particle physics problem and then you try and figure out

1146
01:01:33.280 --> 01:01:34.440
<v Speaker 1>how to look for it with telescopes.

1147
01:01:34.800 --> 01:01:36.679
<v Speaker 2>So what is your work involved. Do you have like

1148
01:01:36.719 --> 01:01:41.079
<v Speaker 2>a moleskin that's just filled with like gobbledygook equations or

1149
01:01:41.119 --> 01:01:43.400
<v Speaker 2>are you working on a computer with data sets like

1150
01:01:43.440 --> 01:01:46.079
<v Speaker 2>when you're like when you get down to work, what

1151
01:01:46.119 --> 01:01:46.840
<v Speaker 2>does that look like?

1152
01:01:47.280 --> 01:01:50.119
<v Speaker 1>So I do have my moleskin with full of equations

1153
01:01:50.159 --> 01:01:53.840
<v Speaker 1>over there. I brought it with me, so I have that.

1154
01:01:55.880 --> 01:01:58.519
<v Speaker 1>I also have a whole bunch of code that I've

1155
01:01:58.519 --> 01:02:01.519
<v Speaker 1>written to try to solve some of these equations that

1156
01:02:01.559 --> 01:02:04.400
<v Speaker 1>are in the moleskin. I mean, so the usual thing

1157
01:02:04.519 --> 01:02:09.280
<v Speaker 1>is like, Okay, you talk to people who work on

1158
01:02:09.440 --> 01:02:12.760
<v Speaker 1>similar things, and you try and come up with like

1159
01:02:12.880 --> 01:02:15.599
<v Speaker 1>what is how can we answer this question? Or what

1160
01:02:15.679 --> 01:02:18.199
<v Speaker 1>is a question we can answer with this observation, or

1161
01:02:18.280 --> 01:02:20.719
<v Speaker 1>like what would be a cool thing that might happen

1162
01:02:20.760 --> 01:02:22.239
<v Speaker 1>that we could find out if it does happen.

1163
01:02:22.440 --> 01:02:25.400
<v Speaker 2>So then physicists talk to each other and write sut

1164
01:02:25.519 --> 01:02:29.159
<v Speaker 2>down and look at papers and write down more equations.

1165
01:02:29.440 --> 01:02:31.920
<v Speaker 2>And I was kind of surprised to realize how collaborative

1166
01:02:31.960 --> 01:02:34.199
<v Speaker 2>this could be. I always imagine physicists needed to be

1167
01:02:34.239 --> 01:02:38.519
<v Speaker 2>like sequestered in a well appointed lab or a classy

1168
01:02:38.679 --> 01:02:41.400
<v Speaker 2>den to just think clearly, but now there's like a

1169
01:02:41.400 --> 01:02:42.480
<v Speaker 2>lot of chatting happening.

1170
01:02:42.719 --> 01:02:45.719
<v Speaker 1>And then once you figure out like what equations you

1171
01:02:45.760 --> 01:02:48.679
<v Speaker 1>need to solve and what things you need to calculate,

1172
01:02:48.719 --> 01:02:51.480
<v Speaker 1>then you go to the computer and you write code

1173
01:02:52.360 --> 01:02:56.239
<v Speaker 1>to calculate those things and to put out numbers and

1174
01:02:56.599 --> 01:02:59.840
<v Speaker 1>draw graphs, and then you see if you have something

1175
01:02:59.840 --> 01:03:00.599
<v Speaker 1>interesting or.

1176
01:03:00.559 --> 01:03:03.440
<v Speaker 2>Not, if it all kind of clicks yeah, yeah, and.

1177
01:03:03.360 --> 01:03:06.199
<v Speaker 1>You see if like, you know, does this tell us

1178
01:03:06.239 --> 01:03:08.400
<v Speaker 1>that this is going to be an interesting technique to

1179
01:03:08.400 --> 01:03:12.039
<v Speaker 1>test the sery or not. And then depending on you know,

1180
01:03:12.280 --> 01:03:16.039
<v Speaker 1>because this is all theoretical work. Sometimes sometimes you find well,

1181
01:03:16.079 --> 01:03:18.079
<v Speaker 1>this is just really uninteresting and nobody's going to care,

1182
01:03:18.119 --> 01:03:21.159
<v Speaker 1>so I'm not going to write it up. Sometimes you're like, well,

1183
01:03:21.320 --> 01:03:23.360
<v Speaker 1>you know, it turns out you can't measure this thing

1184
01:03:23.400 --> 01:03:25.400
<v Speaker 1>with this technique, but we should write that down anyway,

1185
01:03:25.480 --> 01:03:29.599
<v Speaker 1>because people might have tried otherwise. And then sometimes it's like, oh,

1186
01:03:29.639 --> 01:03:32.239
<v Speaker 1>we can measure this thing with this thing and that'll

1187
01:03:32.280 --> 01:03:34.159
<v Speaker 1>be a really interesting result and we'll get a better

1188
01:03:34.199 --> 01:03:36.719
<v Speaker 1>answer than anybody's gotten before. So we're going to write

1189
01:03:36.719 --> 01:03:38.000
<v Speaker 1>it up and be really happy about it.

1190
01:03:38.159 --> 01:03:40.760
<v Speaker 2>And then you go toward writing it up and publishing it.

1191
01:03:40.920 --> 01:03:43.239
<v Speaker 1>Yeah. Yeah, and then and then you write the paper,

1192
01:03:43.280 --> 01:03:45.320
<v Speaker 1>and then you publish the paper, and then you know,

1193
01:03:45.480 --> 01:03:47.440
<v Speaker 1>or you send it to the journal, and the journals

1194
01:03:47.639 --> 01:03:50.239
<v Speaker 1>the editors or the referees are like, yeah, you should

1195
01:03:50.239 --> 01:03:52.000
<v Speaker 1>do this differently, and so you do that differently, and

1196
01:03:52.039 --> 01:03:53.599
<v Speaker 1>then eventually it gets published.

1197
01:03:54.039 --> 01:03:56.760
<v Speaker 2>What is the craziest paper that you've ever had published?

1198
01:03:56.760 --> 01:03:59.320
<v Speaker 2>When the title of the craziest paper, because just looking

1199
01:03:59.360 --> 01:04:02.480
<v Speaker 2>at paper is yeah, so funny to me because they're

1200
01:04:02.719 --> 01:04:04.199
<v Speaker 2>so specific and wonderful.

1201
01:04:04.559 --> 01:04:06.159
<v Speaker 1>I mean, I guess it depends on what you mean.

1202
01:04:06.239 --> 01:04:11.320
<v Speaker 1>I wrote a paper called known Unknowns of dark Matter

1203
01:04:11.320 --> 01:04:13.760
<v Speaker 1>Annihilation over Cosmic Time.

1204
01:04:14.679 --> 01:04:18.039
<v Speaker 2>That sounds like the best like Norwegian metal album ever.

1205
01:04:18.599 --> 01:04:21.599
<v Speaker 1>It was like, well, yeah, so that was all about

1206
01:04:21.639 --> 01:04:24.039
<v Speaker 1>like what we know we don't know about this problem.

1207
01:04:24.159 --> 01:04:29.000
<v Speaker 1>M h. I've calculated a bunch of stuff. I've I

1208
01:04:29.199 --> 01:04:36.039
<v Speaker 1>had some papers about, uh, like axions and and those

1209
01:04:36.039 --> 01:04:38.639
<v Speaker 1>are theoretical particles that are super cool.

1210
01:04:39.280 --> 01:04:41.360
<v Speaker 2>Is there an upper limit to how many words your

1211
01:04:41.400 --> 01:04:42.480
<v Speaker 2>paper title can be?

1212
01:04:43.039 --> 01:04:44.559
<v Speaker 1>Yeah, you don't want to. I mean you kind of

1213
01:04:44.559 --> 01:04:46.880
<v Speaker 1>wanted to be punchy, right, like like the whole Known

1214
01:04:46.960 --> 01:04:49.840
<v Speaker 1>Unknowns thing is I wanted it to be like eye catching.

1215
01:04:49.719 --> 01:04:51.559
<v Speaker 2>Right, it's good marketing.

1216
01:04:51.840 --> 01:04:54.480
<v Speaker 1>Yeah, yeah, So you got to think about marketing to

1217
01:04:54.519 --> 01:04:57.199
<v Speaker 1>some degree, and you don't want it to be a

1218
01:04:57.199 --> 01:04:58.920
<v Speaker 1>long title because people are going to be skimming it.

1219
01:04:59.039 --> 01:05:01.559
<v Speaker 2>This part is it's crazy. It's like trying to buy

1220
01:05:01.559 --> 01:05:04.679
<v Speaker 2>Beyonce tickets. So the way that people find papers to

1221
01:05:04.719 --> 01:05:08.400
<v Speaker 2>read is every day, every weekday. The website, it's a

1222
01:05:08.800 --> 01:05:13.199
<v Speaker 2>r xiv dot org. There's like one hundred new papers

1223
01:05:13.239 --> 01:05:15.119
<v Speaker 2>about astronomy and physics and math and stuff.

1224
01:05:15.239 --> 01:05:19.000
<v Speaker 1>So the way that people find papers to read is

1225
01:05:19.280 --> 01:05:26.639
<v Speaker 1>every day, every single day, every weekday. The archive website,

1226
01:05:26.920 --> 01:05:29.599
<v Speaker 1>it's a r xiv is how it's spelled, but we

1227
01:05:29.679 --> 01:05:33.880
<v Speaker 1>call it the archive. The archive website displays like one

1228
01:05:33.960 --> 01:05:38.800
<v Speaker 1>hundred papers, new papers about astronomy, and there's just a

1229
01:05:38.840 --> 01:05:41.400
<v Speaker 1>list and the titles. So those the titles and the

1230
01:05:41.440 --> 01:05:43.639
<v Speaker 1>authors and maybe like the abstract depending on how you

1231
01:05:43.679 --> 01:05:49.239
<v Speaker 1>read the archive. And if you're a responsible astronomer, then

1232
01:05:49.320 --> 01:05:52.559
<v Speaker 1>every morning you wake up and you read the archive

1233
01:05:52.599 --> 01:05:55.320
<v Speaker 1>and you skim the papers and the and the abstracts,

1234
01:05:55.320 --> 01:05:57.199
<v Speaker 1>and you see which ones are relevant to your work,

1235
01:05:57.360 --> 01:05:59.639
<v Speaker 1>and then you you know, open those and read you

1236
01:05:59.639 --> 01:06:02.159
<v Speaker 1>know ski those papers and find out if like they

1237
01:06:02.199 --> 01:06:04.880
<v Speaker 1>tell you something interesting, you get information. This is how

1238
01:06:04.880 --> 01:06:07.199
<v Speaker 1>you keep up with the fields. So much work, it's

1239
01:06:07.199 --> 01:06:10.159
<v Speaker 1>so much work. It's heck of a lot of work.

1240
01:06:10.199 --> 01:06:12.880
<v Speaker 1>And if you're somebody who maybe does you know particle

1241
01:06:12.920 --> 01:06:15.840
<v Speaker 1>theory stuff as well, then there's a whole other archive

1242
01:06:15.960 --> 01:06:18.920
<v Speaker 1>for like particle theory and then particle phenomenology, which is

1243
01:06:18.960 --> 01:06:21.960
<v Speaker 1>more like the phenomenology is like where you try and

1244
01:06:21.960 --> 01:06:24.239
<v Speaker 1>figure out what you would see in this in the

1245
01:06:24.360 --> 01:06:27.079
<v Speaker 1>universe that's closer to what I do. So then if

1246
01:06:27.119 --> 01:06:30.000
<v Speaker 1>I if you're trying to read particle theory and phenomenology

1247
01:06:30.119 --> 01:06:33.199
<v Speaker 1>and astronomy, you can get like one hundred and fifty

1248
01:06:33.199 --> 01:06:34.760
<v Speaker 1>papers or something every day.

1249
01:06:34.960 --> 01:06:35.760
<v Speaker 2>It's a black hole.

1250
01:06:36.119 --> 01:06:37.679
<v Speaker 1>It's just it's impossible to keep up.

1251
01:06:37.719 --> 01:06:38.320
<v Speaker 2>Oh my god.

1252
01:06:38.440 --> 01:06:42.000
<v Speaker 1>But anyway, so because of that, you want your paper

1253
01:06:42.039 --> 01:06:46.199
<v Speaker 1>title to be punchy and eye catching. But the other thing,

1254
01:06:46.320 --> 01:06:49.719
<v Speaker 1>so there's a this is like so totally inside baseball,

1255
01:06:49.760 --> 01:06:53.760
<v Speaker 1>but there's there's this ridiculous thing that happens.

1256
01:06:53.840 --> 01:06:56.559
<v Speaker 2>So the order of the papers as they appear on

1257
01:06:56.599 --> 01:07:00.280
<v Speaker 2>the website is determined just by what time they were

1258
01:07:00.320 --> 01:07:05.159
<v Speaker 2>sent in and after not too long, these are literal geniuses.

1259
01:07:05.239 --> 01:07:07.320
<v Speaker 2>They were like, duh, there's.

1260
01:07:07.159 --> 01:07:11.079
<v Speaker 1>A cutoff time of like four pm and sometimes on

1261
01:07:11.159 --> 01:07:14.079
<v Speaker 1>I don't remember which one, where if you get your

1262
01:07:14.119 --> 01:07:17.360
<v Speaker 1>paper in as close as possible after that time, it

1263
01:07:17.360 --> 01:07:20.360
<v Speaker 1>will appear at the top of the archive. And so

1264
01:07:20.440 --> 01:07:23.159
<v Speaker 1>there's this you can people have written papers about like

1265
01:07:23.280 --> 01:07:27.559
<v Speaker 1>the spike insubmission times, where like everybody's trying to get

1266
01:07:27.599 --> 01:07:31.039
<v Speaker 1>like four you know, a clock zero zero one second,

1267
01:07:31.119 --> 01:07:33.679
<v Speaker 1>Like they all want to get it like exactly at

1268
01:07:33.719 --> 01:07:35.679
<v Speaker 1>that moment so that their paper will be on the

1269
01:07:35.679 --> 01:07:37.159
<v Speaker 1>top of the list. Because a lot of people, you know,

1270
01:07:37.360 --> 01:07:39.199
<v Speaker 1>like they open the archive and then they just get

1271
01:07:39.199 --> 01:07:41.480
<v Speaker 1>like exhausted by the time they've gone through five favors,

1272
01:07:41.519 --> 01:07:43.079
<v Speaker 1>and so they don't get to the end of the list.

1273
01:07:43.159 --> 01:07:48.840
<v Speaker 1>And so there's this ridiculous, like this ridiculous ritual of

1274
01:07:49.000 --> 01:07:51.159
<v Speaker 1>when you're when you submit your paper to the archive,

1275
01:07:51.239 --> 01:07:53.320
<v Speaker 1>you try and like you watch the clock and you

1276
01:07:53.440 --> 01:07:55.960
<v Speaker 1>try and hit the submit button at exactly the right moment.

1277
01:07:56.039 --> 01:07:58.639
<v Speaker 2>That makes me so anxious. Yeah, it's like when someone

1278
01:07:58.679 --> 01:08:01.079
<v Speaker 2>people comment first a YouTube videation.

1279
01:08:01.159 --> 01:08:04.599
<v Speaker 1>It should be randomized because like it's also been shown

1280
01:08:04.639 --> 01:08:07.039
<v Speaker 1>that it does matter in terms of like citations.

1281
01:08:07.199 --> 01:08:08.159
<v Speaker 2>That's not right.

1282
01:08:08.239 --> 01:08:08.920
<v Speaker 1>It's not right.

1283
01:08:09.039 --> 01:08:12.519
<v Speaker 2>Oh my god. Yeah, oh wait, what was a question

1284
01:08:12.559 --> 01:08:14.119
<v Speaker 2>that I had right on top of that? It was

1285
01:08:14.159 --> 01:08:15.280
<v Speaker 2>definitely a stupid question.

1286
01:08:16.399 --> 01:08:17.920
<v Speaker 1>I don't think any questions are stupid.

1287
01:08:18.119 --> 01:08:18.680
<v Speaker 2>Are you sure?

1288
01:08:18.920 --> 01:08:21.479
<v Speaker 1>I think these are good questions. These are important questions

1289
01:08:21.520 --> 01:08:24.880
<v Speaker 1>because like what it doesn't like you know, these are

1290
01:08:25.119 --> 01:08:27.800
<v Speaker 1>like if you're asking questions about something because you're not

1291
01:08:27.840 --> 01:08:29.479
<v Speaker 1>an expert in that field, Like you can't be an

1292
01:08:29.520 --> 01:08:32.039
<v Speaker 1>expert in every field. If I ask questions about entomology,

1293
01:08:32.079 --> 01:08:35.920
<v Speaker 1>I'm gonna have no idea what's going on? Okay, I'm like,

1294
01:08:36.000 --> 01:08:38.159
<v Speaker 1>I'm still trying to remember what the difference beviews between

1295
01:08:38.159 --> 01:08:40.359
<v Speaker 1>a bug and not a bug, right, Like, I don't know.

1296
01:08:41.039 --> 01:08:42.840
<v Speaker 2>I'll give you some clearance on that, okay. But the

1297
01:08:42.840 --> 01:08:48.279
<v Speaker 2>problem is is you study the universe? Yes, so could

1298
01:08:48.359 --> 01:08:52.159
<v Speaker 2>your field be any broader? Like no, no, it could

1299
01:08:52.239 --> 01:08:53.760
<v Speaker 2>not literally everything.

1300
01:08:54.239 --> 01:08:56.439
<v Speaker 1>Yeah, And this can be a problem too, Like when

1301
01:08:56.439 --> 01:09:01.560
<v Speaker 1>I give talks, I have to be prepared for anything

1302
01:09:01.560 --> 01:09:03.760
<v Speaker 1>from the questions, and that used to just freak me

1303
01:09:03.800 --> 01:09:05.359
<v Speaker 1>out a lot, and now I just feel like like

1304
01:09:05.439 --> 01:09:08.239
<v Speaker 1>I just have to I have to read as widely

1305
01:09:08.279 --> 01:09:11.600
<v Speaker 1>as possible, and sometimes I'll be like, I have no idea,

1306
01:09:12.079 --> 01:09:15.439
<v Speaker 1>but like I gave the talk about gravitational waves in

1307
01:09:15.600 --> 01:09:18.359
<v Speaker 1>Raleigh the other week and one of the questions was,

1308
01:09:19.720 --> 01:09:21.920
<v Speaker 1>tell me about the Great Red Spot on Jupiter. And

1309
01:09:21.960 --> 01:09:30.600
<v Speaker 1>I was like, it's a storm, it's been shrinking. There's

1310
01:09:30.640 --> 01:09:33.399
<v Speaker 1>a spacecraft looking at it. You should maybe talk to

1311
01:09:33.479 --> 01:09:36.119
<v Speaker 1>somebody who studies about that.

1312
01:09:36.399 --> 01:09:39.640
<v Speaker 2>The Great Red Spot, by the way, that's its actual name.

1313
01:09:39.720 --> 01:09:42.319
<v Speaker 2>It's a little on the nose. Also, people mix it

1314
01:09:42.399 --> 01:09:46.159
<v Speaker 2>up sometimes with the Great Dark Spot, which was near

1315
01:09:46.239 --> 01:09:50.119
<v Speaker 2>Jupiter's northern Paul. So y'all call me, let me name

1316
01:09:50.159 --> 01:09:53.520
<v Speaker 2>some of these things. Also, how did Katie feel about

1317
01:09:53.520 --> 01:09:57.520
<v Speaker 2>the detection of gravitational waves. This was the Lego project

1318
01:09:57.560 --> 01:09:59.319
<v Speaker 2>you may have heard about in twenty sixteen.

1319
01:09:59.439 --> 01:10:05.399
<v Speaker 1>The detection gravitational waves by the Ligo instrument was probably

1320
01:10:05.439 --> 01:10:08.319
<v Speaker 1>the biggest discovery in physics in my lifetime.

1321
01:10:09.039 --> 01:10:09.439
<v Speaker 4>Damn.

1322
01:10:09.920 --> 01:10:12.600
<v Speaker 1>Yeah, that's a big deal. It's a super big deal.

1323
01:10:13.319 --> 01:10:16.840
<v Speaker 1>I win the announcement. So the first the first detection

1324
01:10:17.159 --> 01:10:20.199
<v Speaker 1>was last year sometime. Well, the detection was the end

1325
01:10:20.239 --> 01:10:22.960
<v Speaker 1>of twenty fifteen and it was announced I guess during

1326
01:10:23.000 --> 01:10:28.880
<v Speaker 1>twenty sixteen. The announcement was in I don't remember what

1327
01:10:28.920 --> 01:10:30.800
<v Speaker 1>times when it was or whatever, but it was such

1328
01:10:30.840 --> 01:10:33.039
<v Speaker 1>that it was going to be two am local time

1329
01:10:33.079 --> 01:10:37.680
<v Speaker 1>in Melbourne, And so a bunch of us got together

1330
01:10:38.119 --> 01:10:42.800
<v Speaker 1>and like had a party in a university department. Like

1331
01:10:42.840 --> 01:10:45.840
<v Speaker 1>we brought food and booze and like we watched videos

1332
01:10:45.920 --> 01:10:48.720
<v Speaker 1>and like we took like we took selfies. It was

1333
01:10:48.840 --> 01:10:52.319
<v Speaker 1>really late, but we were just like we got to

1334
01:10:52.359 --> 01:10:55.079
<v Speaker 1>see this live, you know. And and there were there

1335
01:10:55.079 --> 01:10:57.119
<v Speaker 1>were two people in the room who were part of

1336
01:10:57.159 --> 01:11:00.520
<v Speaker 1>the collaboration, so they they already knew what was going

1337
01:11:00.600 --> 01:11:03.079
<v Speaker 1>to be done, but the rest of us, like we'd

1338
01:11:03.079 --> 01:11:04.880
<v Speaker 1>heard rumors, but we didn't know for sure what was

1339
01:11:04.960 --> 01:11:07.880
<v Speaker 1>what that was going to be announced. And yeah, it was.

1340
01:11:07.920 --> 01:11:10.119
<v Speaker 1>It was just a huge party and it was a

1341
01:11:10.199 --> 01:11:14.399
<v Speaker 1>we were really excited and like we just everybody was

1342
01:11:14.479 --> 01:11:17.520
<v Speaker 1>like clapping and stuff when it happened, and I mean

1343
01:11:17.600 --> 01:11:18.640
<v Speaker 1>it was it was a huge deal.

1344
01:11:18.680 --> 01:11:22.479
<v Speaker 2>Of the way that it was announced was like a

1345
01:11:22.720 --> 01:11:26.319
<v Speaker 2>press conference from like an awesome eighties movie. Yeah, ladies

1346
01:11:26.319 --> 01:11:33.000
<v Speaker 2>and gentlemen, we have detected gravitational waves.

1347
01:11:33.199 --> 01:11:33.960
<v Speaker 1>We did it.

1348
01:11:37.319 --> 01:11:39.840
<v Speaker 2>I mean, how cute is that. So that was Dave Rightzi.

1349
01:11:40.000 --> 01:11:42.760
<v Speaker 2>He's a laser physicist and he's director of the Lego lab,

1350
01:11:43.000 --> 01:11:47.079
<v Speaker 2>and I love that audio so much. It's just like

1351
01:11:47.319 --> 01:11:53.439
<v Speaker 2>pure triumph, like the last scene of a Schwarzenegger movie

1352
01:11:53.479 --> 01:11:59.880
<v Speaker 2>or something. We have detected gravitational waves. It was like

1353
01:12:00.279 --> 01:12:00.720
<v Speaker 2>the beast.

1354
01:12:00.920 --> 01:12:02.760
<v Speaker 1>Yeah, yeah, no, I remember that very clearly.

1355
01:12:03.119 --> 01:12:06.000
<v Speaker 2>So explain to me why the detection of gravitational waves

1356
01:12:06.079 --> 01:12:07.039
<v Speaker 2>is such a big deal.

1357
01:12:07.399 --> 01:12:12.279
<v Speaker 1>Okay, So, first, gravitational waves are ripples in this fabric

1358
01:12:12.279 --> 01:12:14.800
<v Speaker 1>of space time. So you know, space can be bent

1359
01:12:14.840 --> 01:12:19.000
<v Speaker 1>around massive objects. And when massive objects are moving through space,

1360
01:12:19.119 --> 01:12:21.640
<v Speaker 1>if they're moving in an accelerated way, which could be

1361
01:12:21.720 --> 01:12:24.199
<v Speaker 1>in an orbit in orbit as a kind of accelerated motion,

1362
01:12:25.640 --> 01:12:29.800
<v Speaker 1>that creates ripples in this sort of space time fabric,

1363
01:12:30.199 --> 01:12:32.319
<v Speaker 1>which is kind of hard to visualize and explain, but

1364
01:12:32.479 --> 01:12:36.239
<v Speaker 1>it ripples through space. And so like when you have

1365
01:12:36.920 --> 01:12:41.359
<v Speaker 1>really massive objects moving really quickly, that can make large

1366
01:12:41.399 --> 01:12:44.119
<v Speaker 1>disturbances relative to other things. I mean, if I wave

1367
01:12:44.199 --> 01:12:47.560
<v Speaker 1>my hands, I'm making gravitational waves, but like that's not detectable.

1368
01:12:48.439 --> 01:12:53.279
<v Speaker 1>So two black holes orbiting each other make really big

1369
01:12:53.399 --> 01:12:57.079
<v Speaker 1>detectable gravitational waves, especially when they get so close that

1370
01:12:57.079 --> 01:13:00.399
<v Speaker 1>they're about to merge into one thing. So you can

1371
01:13:00.439 --> 01:13:03.239
<v Speaker 1>have two black holes in a binary orbit orbiting each other,

1372
01:13:03.279 --> 01:13:05.720
<v Speaker 1>and then as they get closer and closer, the signal

1373
01:13:05.760 --> 01:13:08.800
<v Speaker 1>gets stronger and stronger, you know, the waves get stronger

1374
01:13:08.840 --> 01:13:10.680
<v Speaker 1>and stronger, and then they merge and that makes this

1375
01:13:10.720 --> 01:13:16.039
<v Speaker 1>big sort of burst of gravitational waves. And the way

1376
01:13:16.079 --> 01:13:20.760
<v Speaker 1>that gravitational waves work, they're not like ripples on a pond.

1377
01:13:20.840 --> 01:13:23.920
<v Speaker 1>Usually when you see a visualization, it's like ripples on

1378
01:13:23.960 --> 01:13:28.840
<v Speaker 1>a pond, but that's that two dimensional analog, you know again,

1379
01:13:30.520 --> 01:13:34.840
<v Speaker 1>And they're not like if you're standing there, the gravitational

1380
01:13:34.880 --> 01:13:39.039
<v Speaker 1>wave like moves your space that you're in, but it

1381
01:13:39.039 --> 01:13:40.840
<v Speaker 1>doesn't just like move you up and down. What it

1382
01:13:40.880 --> 01:13:44.880
<v Speaker 1>does is it stretches and squeezes the space that you're in.

1383
01:13:46.079 --> 01:13:48.359
<v Speaker 1>So let's say that you're standing there and a gravitational

1384
01:13:48.359 --> 01:13:50.920
<v Speaker 1>wave comes, it hits you in the face. What that

1385
01:13:51.079 --> 01:13:54.000
<v Speaker 1>does to you is it stretches your space a little bit,

1386
01:13:54.039 --> 01:13:56.119
<v Speaker 1>so you get a little bit taller and at the

1387
01:13:56.119 --> 01:13:57.800
<v Speaker 1>same time a little skinnier, and then a little bit

1388
01:13:57.800 --> 01:14:00.520
<v Speaker 1>shorter and a little wider, and like it all oscillates

1389
01:14:00.560 --> 01:14:03.000
<v Speaker 1>back and forth. So as the waves are coming at you,

1390
01:14:03.560 --> 01:14:06.560
<v Speaker 1>each wave is giving you that that stretch and squeeze

1391
01:14:06.560 --> 01:14:11.119
<v Speaker 1>stretch and squeeze. What and so it's actually distorting your shape.

1392
01:14:11.279 --> 01:14:12.840
<v Speaker 1>Oh my god, what is happening?

1393
01:14:12.920 --> 01:14:15.439
<v Speaker 2>This is like a big boy are yowing? And it's

1394
01:14:15.479 --> 01:14:20.399
<v Speaker 2>it keep like for everything that creates gravitational waves?

1395
01:14:20.439 --> 01:14:24.800
<v Speaker 1>Is this doing this to all the time? Micro micro basis? Yeah? Yeah.

1396
01:14:24.840 --> 01:14:29.640
<v Speaker 1>So the Lego experiment is built to detect these things.

1397
01:14:29.640 --> 01:14:32.000
<v Speaker 1>So they have two detectors, and each detector is like

1398
01:14:32.720 --> 01:14:37.359
<v Speaker 1>it's an L shaped thing. Each arm is four kilometers long.

1399
01:14:37.479 --> 01:14:40.000
<v Speaker 2>Now, if you've seen photos of this, you might think

1400
01:14:40.279 --> 01:14:42.560
<v Speaker 2>from a distance, is some shit that we built like

1401
01:14:42.600 --> 01:14:47.560
<v Speaker 2>on Mars, because there's just this treeless, ocre landscape in

1402
01:14:47.600 --> 01:14:50.720
<v Speaker 2>the desert. It seems to look lonely in every direction.

1403
01:14:51.039 --> 01:14:52.880
<v Speaker 2>But no, it's just Washington State.

1404
01:14:52.960 --> 01:14:56.199
<v Speaker 1>And they shoot lasers back and forth along these two

1405
01:14:56.279 --> 01:14:59.279
<v Speaker 1>arms there. They meet at the center and and they're measuring.

1406
01:14:59.359 --> 01:15:01.479
<v Speaker 1>The lasers are just there to measure the length of

1407
01:15:01.520 --> 01:15:06.039
<v Speaker 1>those arms, basically, and when a gravitational wave comes and

1408
01:15:06.119 --> 01:15:09.600
<v Speaker 1>hits that detector, it makes one of the arms a

1409
01:15:09.640 --> 01:15:11.600
<v Speaker 1>little longer while the other one gets a little shorter,

1410
01:15:11.680 --> 01:15:14.880
<v Speaker 1>and vice versa, depending on the direction and the you know,

1411
01:15:15.039 --> 01:15:18.800
<v Speaker 1>phase and everything. So if it does that, then the

1412
01:15:18.840 --> 01:15:21.960
<v Speaker 1>detector can detect that the length of the arms has changed,

1413
01:15:23.399 --> 01:15:26.600
<v Speaker 1>and then that's the signal, is the changing of the

1414
01:15:26.680 --> 01:15:30.479
<v Speaker 1>length of the arms and the level on which that happens.

1415
01:15:30.479 --> 01:15:32.600
<v Speaker 1>So this is four kilometers right, Yeah.

1416
01:15:32.399 --> 01:15:35.319
<v Speaker 2>That's about two and a half miles America.

1417
01:15:35.399 --> 01:15:39.640
<v Speaker 1>The first detection, when it was detected, the length of

1418
01:15:39.760 --> 01:15:43.640
<v Speaker 1>that four kilometer arm changed in length by a thousandth

1419
01:15:43.800 --> 01:15:44.880
<v Speaker 1>the width of a proton.

1420
01:15:45.159 --> 01:15:46.359
<v Speaker 2>Oh my god.

1421
01:15:46.680 --> 01:15:49.680
<v Speaker 1>Yeah that's a teensy tiny that's really small.

1422
01:15:49.880 --> 01:15:53.079
<v Speaker 2>And this was a huge collision.

1423
01:15:53.199 --> 01:15:55.640
<v Speaker 1>Yeah, yeah, this was like it was one point three

1424
01:15:55.680 --> 01:15:58.520
<v Speaker 1>billion light years away, so it's very far. But it

1425
01:15:58.600 --> 01:16:01.359
<v Speaker 1>was like the black holes around thirty times as massive

1426
01:16:01.399 --> 01:16:05.079
<v Speaker 1>as the Sun, and they collided, and so it was

1427
01:16:05.119 --> 01:16:08.920
<v Speaker 1>a pretty strong signal, Like it was a surprisingly strong signal,

1428
01:16:08.960 --> 01:16:11.520
<v Speaker 1>Like if you actually looked at the data, raw data,

1429
01:16:11.560 --> 01:16:13.560
<v Speaker 1>like you could see it, which is not usually the

1430
01:16:13.600 --> 01:16:16.399
<v Speaker 1>case in this kind of field, usually, like you have

1431
01:16:16.439 --> 01:16:18.600
<v Speaker 1>to do lots of processing, but like you can see

1432
01:16:18.800 --> 01:16:23.479
<v Speaker 1>the signal is very strong. But yeah, thousands the width

1433
01:16:23.520 --> 01:16:26.359
<v Speaker 1>of a proton, so that you know, your own height

1434
01:16:26.439 --> 01:16:28.760
<v Speaker 1>is changing much less than that, right, because you're not

1435
01:16:28.800 --> 01:16:29.720
<v Speaker 1>four kilometers long.

1436
01:16:30.079 --> 01:16:32.880
<v Speaker 2>Sure, so I'm getting a little bit not quite as

1437
01:16:33.000 --> 01:16:34.720
<v Speaker 2>tall and not quite as skinny and not kind of

1438
01:16:34.800 --> 01:16:37.720
<v Speaker 2>quite as short as fat as it's not noticeable in

1439
01:16:37.760 --> 01:16:38.359
<v Speaker 2>a photograph.

1440
01:16:38.439 --> 01:16:41.720
<v Speaker 1>Say, yes, yeah, yeah, it's really it's a really subtle effect.

1441
01:16:42.399 --> 01:16:46.359
<v Speaker 1>But but yeah, so that's the gravitational wave. It's the

1442
01:16:46.399 --> 01:16:51.039
<v Speaker 1>detection of that change in length, that sort of stretching

1443
01:16:51.039 --> 01:16:54.039
<v Speaker 1>and squeezing of space time. And each time the black holes,

1444
01:16:54.600 --> 01:16:58.239
<v Speaker 1>you know, black holes or something collide, you get this

1445
01:16:58.399 --> 01:17:01.760
<v Speaker 1>kind of like the the wiggles will come faster and

1446
01:17:01.760 --> 01:17:04.920
<v Speaker 1>closer together. And so the frequency of this changing of

1447
01:17:05.159 --> 01:17:07.760
<v Speaker 1>shape is going up and the amplitude is going up,

1448
01:17:07.800 --> 01:17:09.880
<v Speaker 1>and so it makes this kind of rising sound if

1449
01:17:09.920 --> 01:17:12.359
<v Speaker 1>you transmit it, if you change it into sound, it's

1450
01:17:12.399 --> 01:17:16.079
<v Speaker 1>like a sort of like and the like end part

1451
01:17:16.119 --> 01:17:19.600
<v Speaker 1>is when they collide. And the reason people change it

1452
01:17:19.600 --> 01:17:22.680
<v Speaker 1>to sound a lot is because the frequency of these

1453
01:17:22.680 --> 01:17:26.399
<v Speaker 1>waves coming, like how how quickly the stretching and squeezing happens,

1454
01:17:26.720 --> 01:17:30.000
<v Speaker 1>is about the same frequency as like sound waves. Okay,

1455
01:17:30.119 --> 01:17:32.399
<v Speaker 1>so it is kind of audible, Like if you change

1456
01:17:32.439 --> 01:17:33.680
<v Speaker 1>it to sound, it's kind of audible.

1457
01:17:34.119 --> 01:17:37.479
<v Speaker 2>And that was like the the boop heard around the world, right.

1458
01:17:37.359 --> 01:17:39.960
<v Speaker 1>Yeah, yeah, it's called a chirp, a chirp, Yes.

1459
01:17:42.720 --> 01:17:46.159
<v Speaker 2>Okay, you ready for this? This is the sound of history.

1460
01:17:48.039 --> 01:17:52.920
<v Speaker 2>So what does that mean going forward for astrophysicists? And like,

1461
01:17:53.119 --> 01:17:54.960
<v Speaker 2>how many more have we heard since then?

1462
01:17:55.800 --> 01:17:58.039
<v Speaker 1>So there have been oh gosh, I didn't even know

1463
01:17:58.079 --> 01:18:03.119
<v Speaker 1>the number, like something like five seen now and the

1464
01:18:03.119 --> 01:18:06.159
<v Speaker 1>most recent, most recent one was two black holes. But

1465
01:18:06.199 --> 01:18:08.319
<v Speaker 1>the one before that was a neutrons. There was two

1466
01:18:08.359 --> 01:18:11.760
<v Speaker 1>neutron stars, and those were a big deal because those

1467
01:18:11.840 --> 01:18:14.640
<v Speaker 1>when they collided, also created a gamma.

1468
01:18:14.399 --> 01:18:19.079
<v Speaker 2>Ray burst, a gamma ray burst super energetic explosion, so

1469
01:18:19.199 --> 01:18:21.760
<v Speaker 2>we can't see gamma rays, but they pack of punch

1470
01:18:21.800 --> 01:18:22.800
<v Speaker 2>and a burst.

1471
01:18:22.600 --> 01:18:25.279
<v Speaker 1>And so we were able to see the collision from

1472
01:18:25.359 --> 01:18:29.000
<v Speaker 1>the gravitational waves but also from light. And that was

1473
01:18:29.000 --> 01:18:31.520
<v Speaker 1>a huge deal. And I can talk about that for hours,

1474
01:18:32.720 --> 01:18:35.760
<v Speaker 1>but it's it's a big deal. The whole thing is

1475
01:18:35.800 --> 01:18:37.560
<v Speaker 1>a big deal for a bunch of reasons. One is

1476
01:18:37.600 --> 01:18:42.199
<v Speaker 1>that this, like the existence of gravitational waves, was kind

1477
01:18:42.239 --> 01:18:46.399
<v Speaker 1>of known indirectly because we'd seen systems where like you

1478
01:18:46.439 --> 01:18:49.760
<v Speaker 1>had two pulsars orbiting each other. So pulsar is a

1479
01:18:49.840 --> 01:18:52.000
<v Speaker 1>kind of neutron star. A neutron star is like the

1480
01:18:52.000 --> 01:18:57.279
<v Speaker 1>core of a dead star. It's so we'd seen things

1481
01:18:57.359 --> 01:19:00.199
<v Speaker 1>orbiting each other where the changing of the orbit it

1482
01:19:00.680 --> 01:19:04.279
<v Speaker 1>could only really be easily explained by gravitational waves kind

1483
01:19:04.279 --> 01:19:06.920
<v Speaker 1>of radiating energy away from the orbit, and so the

1484
01:19:07.000 --> 01:19:10.000
<v Speaker 1>orbit got smaller because gravitational waves were pulling energy away

1485
01:19:11.000 --> 01:19:16.279
<v Speaker 1>and sort of shrinking that orbit. So we had indirect

1486
01:19:16.279 --> 01:19:19.319
<v Speaker 1>evidence that gravitational waves existed, but we'd never seen them directly.

1487
01:19:19.960 --> 01:19:24.760
<v Speaker 1>And seeing like directly, like detecting, like feeling the gravitational

1488
01:19:24.800 --> 01:19:28.680
<v Speaker 1>wave is a huge deal, right, And the gravitational waves

1489
01:19:28.720 --> 01:19:32.319
<v Speaker 1>were like the last, the last prediction of Einstein's relativity

1490
01:19:32.399 --> 01:19:33.119
<v Speaker 1>to be confirmed.

1491
01:19:33.239 --> 01:19:37.039
<v Speaker 2>Einstein's theory of relativity. Remember, our perception of the force

1492
01:19:37.039 --> 01:19:41.920
<v Speaker 2>of gravity is a bendy spacetime thing. I'm very paraphrasing

1493
01:19:42.239 --> 01:19:42.640
<v Speaker 2>a lot.

1494
01:19:43.199 --> 01:19:47.000
<v Speaker 1>So he predicted them one hundred years, about one hundred

1495
01:19:47.079 --> 01:19:50.640
<v Speaker 1>years before the first detection was made, so it was

1496
01:19:50.720 --> 01:19:53.560
<v Speaker 1>it took a long time to see these things, but

1497
01:19:53.800 --> 01:19:57.359
<v Speaker 1>so it was confirmed that And it's just this incredible

1498
01:19:57.439 --> 01:20:03.800
<v Speaker 1>laboratory for relativity for physics because by detecting the gravitational

1499
01:20:03.840 --> 01:20:06.359
<v Speaker 1>ways and looking at the signal, we were able to

1500
01:20:06.399 --> 01:20:08.960
<v Speaker 1>determine that gravitational waves travel at the speed of light.

1501
01:20:09.520 --> 01:20:11.680
<v Speaker 1>We didn't know for sure before that was part of

1502
01:20:11.680 --> 01:20:13.640
<v Speaker 1>the theory, but we didn't know for sure, so we

1503
01:20:14.039 --> 01:20:17.880
<v Speaker 1>figured that out. It told us stuff about how black

1504
01:20:17.880 --> 01:20:20.199
<v Speaker 1>holes are made, like what black holes are made of,

1505
01:20:20.239 --> 01:20:23.359
<v Speaker 1>sort of like the properties of black holes, by examining

1506
01:20:23.439 --> 01:20:27.319
<v Speaker 1>very closely how they come together and merge, how much

1507
01:20:27.439 --> 01:20:32.680
<v Speaker 1>energy the gravitational wave burst creates, you know a lot

1508
01:20:32.680 --> 01:20:35.439
<v Speaker 1>of stuff about about that. And then because now we

1509
01:20:35.600 --> 01:20:41.119
<v Speaker 1>can we can watch black holes colliding in the distant universe,

1510
01:20:41.199 --> 01:20:44.039
<v Speaker 1>we can learn about how black holes grow, you know,

1511
01:20:44.239 --> 01:20:46.439
<v Speaker 1>by when they collide with each other, and that tells

1512
01:20:46.479 --> 01:20:49.079
<v Speaker 1>us something about how black holes grow. It tells us

1513
01:20:49.119 --> 01:20:52.000
<v Speaker 1>something about how galaxies grow. It tells us something about

1514
01:20:52.000 --> 01:20:55.239
<v Speaker 1>how stars form, because black holes are the end results

1515
01:20:55.239 --> 01:20:55.680
<v Speaker 1>of stars.

1516
01:20:55.720 --> 01:20:57.439
<v Speaker 2>When you were a kid, were you ever hoping that

1517
01:20:57.479 --> 01:21:00.000
<v Speaker 2>this that we would be able to detect gravitational waves

1518
01:21:01.119 --> 01:21:03.600
<v Speaker 2>where Like, I've been waiting since I was a little.

1519
01:21:03.359 --> 01:21:08.479
<v Speaker 1>Girl, So I didn't know a whole lot about gravitational

1520
01:21:08.479 --> 01:21:10.000
<v Speaker 1>ways when I was a little kid. But there was

1521
01:21:10.039 --> 01:21:14.680
<v Speaker 1>there was a really beautiful moment during one of the

1522
01:21:15.079 --> 01:21:17.880
<v Speaker 1>detection of the neutron star collisions when one of the

1523
01:21:17.920 --> 01:21:22.279
<v Speaker 1>scientists was he was he was talking about the neutron

1524
01:21:22.319 --> 01:21:24.680
<v Speaker 1>star collision and the neutron stars when they collide, they

1525
01:21:24.720 --> 01:21:26.960
<v Speaker 1>make a slightly different kind of like chirp sound.

1526
01:21:27.119 --> 01:21:31.039
<v Speaker 2>Okay, here's the sound of the neutron stars booping themselves together.

1527
01:21:37.159 --> 01:21:39.159
<v Speaker 1>So the black hole one is actually a lot quicker

1528
01:21:39.239 --> 01:21:41.159
<v Speaker 1>than what I said, But the neutron star one goes

1529
01:21:41.199 --> 01:21:44.000
<v Speaker 1>like oo, it takes it. It takes a while, and it

1530
01:21:44.039 --> 01:21:48.560
<v Speaker 1>does it. So and there'd been simulations of this for years.

1531
01:21:48.560 --> 01:21:50.840
<v Speaker 1>I mean, the scientist who was talking about the discovery

1532
01:21:50.960 --> 01:21:54.079
<v Speaker 1>said that he'd been waiting to hear that sound from

1533
01:21:54.159 --> 01:21:58.479
<v Speaker 1>nature for twenty years and he just did and it

1534
01:21:58.520 --> 01:22:00.920
<v Speaker 1>was really touching. I mean. So for me, I knew

1535
01:22:00.960 --> 01:22:05.960
<v Speaker 1>about LOGO because it was it was partly headed by

1536
01:22:05.960 --> 01:22:07.640
<v Speaker 1>people at cal Tech, and I was an undergrad at

1537
01:22:07.640 --> 01:22:09.920
<v Speaker 1>cal Tech, and so when I was an undergrad there,

1538
01:22:10.640 --> 01:22:12.800
<v Speaker 1>people were talking about it a lot, and there was

1539
01:22:13.479 --> 01:22:17.000
<v Speaker 1>there was a famous bet between like Kip Thorn and

1540
01:22:17.119 --> 01:22:18.319
<v Speaker 1>Stephen Hawking or something.

1541
01:22:18.439 --> 01:22:21.800
<v Speaker 2>Kip Thorn, by the way, is a theoretical physicist, the

1542
01:22:22.039 --> 01:22:24.760
<v Speaker 2>twenty seventeen Nobel Laureate.

1543
01:22:24.840 --> 01:22:27.199
<v Speaker 1>About whether or not gravitational waves would be detected by

1544
01:22:27.199 --> 01:22:30.880
<v Speaker 1>the year two thousand. I started cal Tech in ninety nine,

1545
01:22:31.680 --> 01:22:34.520
<v Speaker 1>so they were not detected by the year two thousand,

1546
01:22:34.560 --> 01:22:38.000
<v Speaker 1>so that bet was lost. But it was a funny

1547
01:22:38.000 --> 01:22:40.039
<v Speaker 1>thing because when I first got to cal Tech, they

1548
01:22:40.039 --> 01:22:42.479
<v Speaker 1>were building LOGO and it was this big deal and

1549
01:22:42.520 --> 01:22:44.640
<v Speaker 1>everybody's like, we're going to detect gravitational waves. It's going

1550
01:22:44.680 --> 01:22:47.920
<v Speaker 1>to be amazing. And then you know, and LIGO is

1551
01:22:47.960 --> 01:22:49.840
<v Speaker 1>being built, and I was like, oh, it's any minute now.

1552
01:22:50.159 --> 01:22:52.640
<v Speaker 1>And then I left cal Tech and I went to

1553
01:22:52.680 --> 01:22:54.680
<v Speaker 1>grad school, and then after a while, I was like,

1554
01:22:55.439 --> 01:22:57.359
<v Speaker 1>I haven't heard anything about this for a while, you know,

1555
01:22:57.399 --> 01:23:00.760
<v Speaker 1>And I realized that like they'd kind of like they'd

1556
01:23:00.800 --> 01:23:02.560
<v Speaker 1>been like, yeah, we're gonna detect your reputation wise, and

1557
01:23:02.560 --> 01:23:04.319
<v Speaker 1>then they kind of got quiet for a while, and

1558
01:23:04.359 --> 01:23:06.399
<v Speaker 1>I found out later on asked about it, and they

1559
01:23:06.399 --> 01:23:08.319
<v Speaker 1>were like, oh no, it's advanced.

1560
01:23:07.880 --> 01:23:10.319
<v Speaker 2>LEGO was so there are some upgrades over the years

1561
01:23:10.479 --> 01:23:16.399
<v Speaker 2>from initial LAGO to Enhanced LAGO to advanced LEGO. It's

1562
01:23:16.479 --> 01:23:21.960
<v Speaker 2>kind of like the Tall Grande and Venti gravitational wave detectors.

1563
01:23:22.600 --> 01:23:24.239
<v Speaker 2>Just then maybe you need a little more to get

1564
01:23:24.239 --> 01:23:25.079
<v Speaker 2>the job done.

1565
01:23:25.000 --> 01:23:27.680
<v Speaker 1>Really gonna do the detection. The initial LEGO was like

1566
01:23:27.720 --> 01:23:29.760
<v Speaker 1>maybe it would get lucky, but advanced lago will really

1567
01:23:29.760 --> 01:23:33.880
<v Speaker 1>see something. I'm like really, so like for a while,

1568
01:23:33.920 --> 01:23:35.680
<v Speaker 1>I was like, I don't know what I feel like,

1569
01:23:35.880 --> 01:23:37.439
<v Speaker 1>I don't know if I believe that this is really

1570
01:23:37.439 --> 01:23:39.720
<v Speaker 1>going to happen. But then you know, as soon as

1571
01:23:39.760 --> 01:23:43.680
<v Speaker 1>they turned advanced Lago on, like within like a week

1572
01:23:43.840 --> 01:23:47.319
<v Speaker 1>or something, they saw this thing. So that's like they

1573
01:23:47.399 --> 01:23:49.520
<v Speaker 1>really they really did it. And it's the most like

1574
01:23:49.720 --> 01:23:53.479
<v Speaker 1>it's the most precise instrument ever built by humans. I

1575
01:23:53.479 --> 01:23:57.279
<v Speaker 1>think I read that somewhere. It's like the I mean,

1576
01:23:57.359 --> 01:24:02.239
<v Speaker 1>you're measuring something so tiny. It's crazy, It's it's impossible.

1577
01:24:02.239 --> 01:24:07.159
<v Speaker 1>I use, it's incredible. How like what went into it

1578
01:24:07.239 --> 01:24:10.239
<v Speaker 1>in terms of the engineering and you know, just the

1579
01:24:10.640 --> 01:24:13.319
<v Speaker 1>physics and like they had to they had to correct

1580
01:24:13.319 --> 01:24:16.840
<v Speaker 1>for things like the like how much the photons hitting

1581
01:24:16.840 --> 01:24:18.279
<v Speaker 1>the mirrors would move them.

1582
01:24:18.560 --> 01:24:20.520
<v Speaker 2>Oh my god, Oh my god.

1583
01:24:21.000 --> 01:24:23.960
<v Speaker 1>That's a big part of the noise in the signal

1584
01:24:24.760 --> 01:24:27.239
<v Speaker 1>that's called the photon shot noise. They have to deal

1585
01:24:27.279 --> 01:24:30.079
<v Speaker 1>with that. Yeah, so stuff like that. I mean, it's

1586
01:24:30.119 --> 01:24:31.920
<v Speaker 1>it's incredible that they were able to do this.

1587
01:24:32.079 --> 01:24:34.560
<v Speaker 2>So can you get the chirp as a ring tone?

1588
01:24:34.720 --> 01:24:36.920
<v Speaker 1>I believe you can. You can I believe? So, yeah,

1589
01:24:37.000 --> 01:24:37.319
<v Speaker 1>would you.

1590
01:24:37.319 --> 01:24:40.359
<v Speaker 3>Get the neutron whoop? Or would you get the the

1591
01:24:40.359 --> 01:24:42.960
<v Speaker 3>black hole one? The black hole one, you have to

1592
01:24:43.000 --> 01:24:45.520
<v Speaker 3>speed it up to make it sound cool, so you

1593
01:24:45.560 --> 01:24:48.720
<v Speaker 3>can still hear it, but it's more like a like so,

1594
01:24:48.800 --> 01:24:51.800
<v Speaker 3>so in the actual data it's like that, that's kind

1595
01:24:51.800 --> 01:24:54.199
<v Speaker 3>of what it sounds like. But then when you when you.

1596
01:24:54.199 --> 01:24:56.760
<v Speaker 1>Speed it up, it goes whoop whoop, but it's very quick,

1597
01:24:56.760 --> 01:24:59.439
<v Speaker 1>whereas the neutron star one it's like ooop.

1598
01:25:00.239 --> 01:25:02.119
<v Speaker 2>I feel like, yeah, I feel like that's the way

1599
01:25:02.159 --> 01:25:02.399
<v Speaker 2>to go.

1600
01:25:02.800 --> 01:25:03.159
<v Speaker 1>Yeah.

1601
01:25:03.279 --> 01:25:06.800
<v Speaker 2>Let's say someone is interesting cosmology but doesn't know a

1602
01:25:06.800 --> 01:25:08.840
<v Speaker 2>lot about it and is intimidated by it. What is

1603
01:25:08.880 --> 01:25:11.800
<v Speaker 2>the best book to pick up? I actually, and this

1604
01:25:11.840 --> 01:25:13.119
<v Speaker 2>is I don't know if you've ever read this, but

1605
01:25:13.159 --> 01:25:15.800
<v Speaker 2>I was. I was in Thailand and I was staying

1606
01:25:15.800 --> 01:25:17.399
<v Speaker 2>in a hut and there was some there was a

1607
01:25:17.399 --> 01:25:19.960
<v Speaker 2>free book pile, and I picked up a book called

1608
01:25:20.039 --> 01:25:22.760
<v Speaker 2>Quantum Mechanics Can't Hurt You. This book was actually called

1609
01:25:22.800 --> 01:25:27.159
<v Speaker 2>Quantum Theory Cannot Hurt You. It's by Marcus Choone and

1610
01:25:27.279 --> 01:25:30.720
<v Speaker 2>it's delightful. I found my copy. It's still moldy from

1611
01:25:30.720 --> 01:25:31.359
<v Speaker 2>a monsoon.

1612
01:25:31.520 --> 01:25:31.960
<v Speaker 1>It was good.

1613
01:25:32.079 --> 01:25:35.680
<v Speaker 2>It was very it was very layperson's terms, but I

1614
01:25:35.880 --> 01:25:38.920
<v Speaker 2>clearly don't didn't retain any of it. But is there

1615
01:25:39.039 --> 01:25:41.920
<v Speaker 2>a book or a documentary or something that's just a

1616
01:25:41.920 --> 01:25:45.880
<v Speaker 2>good primer because like in this episode, there's no way

1617
01:25:45.960 --> 01:25:48.840
<v Speaker 2>to describe everything, But like, what's a good go to,

1618
01:25:49.239 --> 01:25:53.399
<v Speaker 2>like astrophysics for dummies? What are we talking here? Is

1619
01:25:53.399 --> 01:25:54.560
<v Speaker 2>there a pamphlet?

1620
01:25:55.199 --> 01:25:58.279
<v Speaker 1>Uh? So I wish I had a really good answer

1621
01:25:58.279 --> 01:25:58.479
<v Speaker 1>for this.

1622
01:26:00.000 --> 01:26:03.399
<v Speaker 2>I fel like, you don't You're winter.

1623
01:26:04.159 --> 01:26:07.399
<v Speaker 1>So the thing is like, I don't. I don't read

1624
01:26:07.720 --> 01:26:12.479
<v Speaker 1>a lot of popular level stuff. And there's a couple

1625
01:26:12.560 --> 01:26:13.239
<v Speaker 1>of reasons for that.

1626
01:26:13.600 --> 01:26:16.199
<v Speaker 2>So number one, she doesn't have much time to read

1627
01:26:16.520 --> 01:26:19.199
<v Speaker 2>non papers because there's like a billion papers, and when

1628
01:26:19.199 --> 01:26:22.680
<v Speaker 2>she does, she likes to read about spaceships. Okay too,

1629
01:26:22.880 --> 01:26:26.720
<v Speaker 2>when something is written for the general public, astro physicists

1630
01:26:27.199 --> 01:26:30.439
<v Speaker 2>have to take that lay information and kind of back

1631
01:26:30.560 --> 01:26:33.880
<v Speaker 2>translate it to a more technical version in their head.

1632
01:26:34.239 --> 01:26:37.119
<v Speaker 2>So it's like if you're a bartender and someone writes

1633
01:26:37.319 --> 01:26:41.760
<v Speaker 2>she drank a whiskey, but you're distracted wondering a whiskey? Well,

1634
01:26:42.159 --> 01:26:44.760
<v Speaker 2>is it like a bourbon? Is this a single malt scotch?

1635
01:26:44.880 --> 01:26:47.840
<v Speaker 2>Was it a Rye, Tennessee whiskey is this on the rocks?

1636
01:26:48.039 --> 01:26:50.279
<v Speaker 2>Was in a cocktail? There's so much detail omitted.

1637
01:26:50.479 --> 01:26:53.640
<v Speaker 1>I mean, Sean Carroll's written several books that are really good,

1638
01:26:54.600 --> 01:26:58.760
<v Speaker 1>so take a look at those. There's a physicist Katie

1639
01:26:58.760 --> 01:27:03.560
<v Speaker 1>Freeze Catherine, who's a dark matter theorist like me. Oh,

1640
01:27:04.079 --> 01:27:06.439
<v Speaker 1>she's a dark matter cosmologist and she's written a book

1641
01:27:06.520 --> 01:27:11.560
<v Speaker 1>called Cosmic Cocktail and it's all about about dark matter

1642
01:27:11.800 --> 01:27:14.760
<v Speaker 1>and also like some aati biographical stuff. It's really cool.

1643
01:27:17.520 --> 01:27:20.720
<v Speaker 2>About What about movies? Do you have a favorite or

1644
01:27:20.760 --> 01:27:23.680
<v Speaker 2>a least favorite movie about space or cosmology?

1645
01:27:23.800 --> 01:27:25.880
<v Speaker 1>You're like, could I not answer some of these?

1646
01:27:26.000 --> 01:27:26.279
<v Speaker 2>Yes?

1647
01:27:26.399 --> 01:27:32.920
<v Speaker 1>Yes, yes, okay, so so favorite yes. So there aren't

1648
01:27:32.960 --> 01:27:35.840
<v Speaker 1>a lot of movies where I feel like the cosmology,

1649
01:27:35.960 --> 01:27:39.000
<v Speaker 1>Like cosmology is hard to have as a topic of

1650
01:27:39.000 --> 01:27:41.199
<v Speaker 1>a movie because it's just too big a topic, and

1651
01:27:41.279 --> 01:27:44.399
<v Speaker 1>like stuff happens on cosmological time scales, which is like

1652
01:27:45.159 --> 01:27:50.520
<v Speaker 1>incredibly long times, and so having something happen within a

1653
01:27:50.560 --> 01:27:55.680
<v Speaker 1>movie time frame is really hard. But there's a movie

1654
01:27:55.720 --> 01:27:59.000
<v Speaker 1>that I really liked for how it portrayed the scientists

1655
01:27:59.000 --> 01:28:02.600
<v Speaker 1>and it had some some cosmology ish stuff in it,

1656
01:28:04.680 --> 01:28:08.039
<v Speaker 1>so that was sunshine, okay, which the science is wrong,

1657
01:28:08.760 --> 01:28:11.439
<v Speaker 1>just putting that out there. It's it's about the sun

1658
01:28:11.640 --> 01:28:14.079
<v Speaker 1>has like burned out or is burning out and they

1659
01:28:14.119 --> 01:28:16.319
<v Speaker 1>have to fix it and none of that can happen.

1660
01:28:16.439 --> 01:28:19.199
<v Speaker 1>All of that's false, All that's fake. But it's done

1661
01:28:19.199 --> 01:28:21.520
<v Speaker 1>really well in terms of like they have physicists who

1662
01:28:22.079 --> 01:28:24.560
<v Speaker 1>acts like a physicist, and like they have people who

1663
01:28:24.560 --> 01:28:27.439
<v Speaker 1>talk like scientists. And I kind of just enjoyed it. Okay,

1664
01:28:27.880 --> 01:28:29.960
<v Speaker 1>so I thought that, and then there's like a monster thing,

1665
01:28:30.039 --> 01:28:32.560
<v Speaker 1>so anyway, but I thought that was done really well.

1666
01:28:33.880 --> 01:28:37.600
<v Speaker 1>I really enjoyed gravity. There's also bad physics in gravity

1667
01:28:37.680 --> 01:28:39.800
<v Speaker 1>in some places, but I thought it was a beautiful

1668
01:28:39.800 --> 01:28:43.319
<v Speaker 1>movie and it portrayed space very well.

1669
01:28:43.399 --> 01:28:44.640
<v Speaker 2>How do you feel about space balls?

1670
01:28:44.720 --> 01:28:47.119
<v Speaker 1>I think it was funny. It's been a long time.

1671
01:28:47.800 --> 01:28:49.000
<v Speaker 2>Oh hell yes, that was good.

1672
01:28:49.239 --> 01:28:52.760
<v Speaker 1>Yeah. Other space movies like The Martian was fun. Interstellar

1673
01:28:52.800 --> 01:28:54.279
<v Speaker 1>had a very pretty black hole in it.

1674
01:28:54.520 --> 01:28:59.920
<v Speaker 2>Okay, that you are being very complimentary, and that is due.

1675
01:29:00.079 --> 01:29:03.359
<v Speaker 2>We noted you are being a very nice person.

1676
01:29:05.079 --> 01:29:07.520
<v Speaker 1>The black hole and the wormhole and Interstellar were very

1677
01:29:07.560 --> 01:29:13.119
<v Speaker 1>beautifully done and done with with proper relativistic equations. It

1678
01:29:13.199 --> 01:29:15.479
<v Speaker 1>was very clever because what they did is they they

1679
01:29:15.720 --> 01:29:18.399
<v Speaker 1>they had these simulations that are very very difficult and

1680
01:29:18.399 --> 01:29:21.880
<v Speaker 1>take a very long time on supercomputers, and they gave

1681
01:29:21.920 --> 01:29:25.359
<v Speaker 1>them to the the the people who do movie graphics,

1682
01:29:25.359 --> 01:29:29.159
<v Speaker 1>who have really powerful supercomputers, and they're like, no, we

1683
01:29:29.199 --> 01:29:32.279
<v Speaker 1>need to do this black hole properly. So they calculated

1684
01:29:32.319 --> 01:29:34.119
<v Speaker 1>it and now they got some like papers out of

1685
01:29:34.159 --> 01:29:38.359
<v Speaker 1>it because the result was such such a good calculation

1686
01:29:38.640 --> 01:29:41.119
<v Speaker 1>that they were able to get actual science out of

1687
01:29:41.159 --> 01:29:44.720
<v Speaker 1>the calculation done for the graphics in the movie.

1688
01:29:44.840 --> 01:29:46.279
<v Speaker 2>Because movies are better funded.

1689
01:29:46.359 --> 01:29:49.840
<v Speaker 1>Then yeah, yeah, so it was it was a very

1690
01:29:49.840 --> 01:29:52.800
<v Speaker 1>good move. But but you should you should know that

1691
01:29:52.800 --> 01:29:56.119
<v Speaker 1>that the black hole in Interstellar, although there are some

1692
01:29:56.159 --> 01:29:58.960
<v Speaker 1>aspects that are done very faithfully, they did have they

1693
01:29:58.960 --> 01:30:02.840
<v Speaker 1>did tweak something so it actually would look pretty different

1694
01:30:03.560 --> 01:30:05.720
<v Speaker 1>if we saw an actual black hole in real life.

1695
01:30:05.720 --> 01:30:07.279
<v Speaker 1>So there are a couple of things that were tweaked

1696
01:30:07.279 --> 01:30:08.239
<v Speaker 1>that were a bit different.

1697
01:30:08.359 --> 01:30:11.039
<v Speaker 2>So, speaking of movies, Katie and I were supposed to

1698
01:30:11.119 --> 01:30:13.680
<v Speaker 2>go to one after this interview, and we did, but

1699
01:30:13.800 --> 01:30:17.239
<v Speaker 2>we barely made it. Because this is all really great information.

1700
01:30:17.720 --> 01:30:20.199
<v Speaker 2>We hadn't even gotten to the wrapid fire around of

1701
01:30:20.239 --> 01:30:23.760
<v Speaker 2>all of your questions, so I asked your questions. We

1702
01:30:24.039 --> 01:30:26.640
<v Speaker 2>raced to the showing and this poor woman had to

1703
01:30:26.680 --> 01:30:29.800
<v Speaker 2>smuggle a burrito and eat it in the theater. I'm

1704
01:30:29.880 --> 01:30:31.840
<v Speaker 2>so sorry. By the way, we saw murder on the

1705
01:30:31.920 --> 01:30:36.279
<v Speaker 2>Oran Express. It features a very bizarre mustache. I will

1706
01:30:36.279 --> 01:30:39.560
<v Speaker 2>give it that, So stay tuned the first two parter

1707
01:30:39.600 --> 01:30:43.600
<v Speaker 2>Anology's history when we resume with your questions, so you

1708
01:30:43.680 --> 01:30:46.359
<v Speaker 2>now have a solid base, Tune in next week to

1709
01:30:46.399 --> 01:30:51.399
<v Speaker 2>hear Astro Katie address your questions, including is there a

1710
01:30:51.479 --> 01:30:54.880
<v Speaker 2>name for the disorientation and panic one feels when considering

1711
01:30:54.880 --> 01:30:58.119
<v Speaker 2>the vastness of the universe? There is are any of

1712
01:30:58.119 --> 01:31:00.159
<v Speaker 2>the sci fi movie methods to save the place in

1713
01:31:00.199 --> 01:31:03.720
<v Speaker 2>it plausible? Or are we basically doomed if an asteroid

1714
01:31:04.079 --> 01:31:07.640
<v Speaker 2>uses us as a target? Will the universe expand forever?

1715
01:31:08.199 --> 01:31:13.119
<v Speaker 2>What's the deal with MultiVersus? Are there aliens? And speaking

1716
01:31:13.119 --> 01:31:15.359
<v Speaker 2>of your submissions, I wanted to let you know I

1717
01:31:15.439 --> 01:31:18.000
<v Speaker 2>totally see the reviews you write on iTunes and it's

1718
01:31:18.039 --> 01:31:22.600
<v Speaker 2>so appreciated. Rating and reviewing and subscribing is free. It

1719
01:31:22.640 --> 01:31:26.239
<v Speaker 2>takes very little time, and it helps ologies stay up

1720
01:31:26.279 --> 01:31:29.199
<v Speaker 2>there in the science charts, so more folks know about it,

1721
01:31:29.319 --> 01:31:33.000
<v Speaker 2>so thank you so much. Katie is at astro Katie

1722
01:31:33.039 --> 01:31:37.039
<v Speaker 2>on Twitter, where she has approximately one billion trillion followers,

1723
01:31:37.560 --> 01:31:41.399
<v Speaker 2>and she is academic Nomad on Instagram. So thank you

1724
01:31:41.479 --> 01:31:44.359
<v Speaker 2>to all you ologites for tweeting and gramming and meming

1725
01:31:44.359 --> 01:31:46.880
<v Speaker 2>at us, and to all the folks on Patreon who

1726
01:31:46.880 --> 01:31:51.199
<v Speaker 2>make the show possible. It is currently four am on

1727
01:31:51.239 --> 01:31:53.680
<v Speaker 2>a Friday night, and I'm recording this to send it

1728
01:31:53.720 --> 01:31:56.680
<v Speaker 2>off to Stephen Ray Morris. He's going to help edit it,

1729
01:31:56.920 --> 01:32:00.760
<v Speaker 2>and your funding is making this dream project possible and

1730
01:32:00.960 --> 01:32:04.079
<v Speaker 2>putting a lot of facts in a lot of human minds.

1731
01:32:04.800 --> 01:32:06.720
<v Speaker 2>You can also keep the show going by stopping at

1732
01:32:06.720 --> 01:32:10.079
<v Speaker 2>ologiesmerch dot com. I also want you to know that, yes,

1733
01:32:10.119 --> 01:32:14.039
<v Speaker 2>it's super late at night and I'm recording this partly

1734
01:32:14.079 --> 01:32:19.479
<v Speaker 2>because the mass of porridge that occupies the space where

1735
01:32:19.479 --> 01:32:21.520
<v Speaker 2>a brain would be. I had to spend a little

1736
01:32:21.560 --> 01:32:24.840
<v Speaker 2>longer trying to understand and explain these concepts that I thought.

1737
01:32:25.319 --> 01:32:28.840
<v Speaker 2>And right now, as I record this middle of the night,

1738
01:32:29.199 --> 01:32:33.359
<v Speaker 2>my neighbors had been blasting techno Christmas pop songs for

1739
01:32:33.479 --> 01:32:37.520
<v Speaker 2>four hours while I was learning about wormholes. The world

1740
01:32:37.560 --> 01:32:41.920
<v Speaker 2>feels very surreal. Also, congratulations to anyone who made it

1741
01:32:41.920 --> 01:32:44.640
<v Speaker 2>to the end of this episode. Man, you stuck it out.

1742
01:32:44.920 --> 01:32:48.039
<v Speaker 2>I appreciate that. As a special thanks, I'm going to

1743
01:32:48.079 --> 01:32:50.159
<v Speaker 2>tell you a secret that no one in the world knows.

1744
01:32:50.520 --> 01:32:53.199
<v Speaker 2>Earlier tonight, I ate cereal. I bought from a gas

1745
01:32:53.239 --> 01:32:56.039
<v Speaker 2>station and I loved it. So if you listen to

1746
01:32:56.079 --> 01:32:58.199
<v Speaker 2>the end of this episode, feel free to holler at

1747
01:32:58.199 --> 01:33:01.079
<v Speaker 2>Ologies or Ali Ward. I'm sure I'll have a new

1748
01:33:01.119 --> 01:33:03.479
<v Speaker 2>secret for you next week at the very end, when

1749
01:33:03.520 --> 01:33:06.600
<v Speaker 2>we are back with Katie, max Q and A. So

1750
01:33:06.880 --> 01:33:09.600
<v Speaker 2>until then, ask smart people dumb questions because they love

1751
01:33:09.640 --> 01:33:12.720
<v Speaker 2>it and we're just tiny meat blobs on a dust

1752
01:33:13.359 --> 01:33:19.359
<v Speaker 2>spec So let's just live. Can we live? Okay? Byebye pacadermatology,

1753
01:33:19.439 --> 01:33:31.479
<v Speaker 2>hobbiology or do zoology, lithology, technology, meteorology, pology, anthology, zeriology, elinology,
