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The universe is slowing down. It's not so much that
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matter can't be destroyed.
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It can.
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It can be converted into energy, right? Matter and energy
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are two sides of the same coin. That famous equation,
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energy equals mass times the speed of light squared. Good
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old Albert Einstein. So you can destroy matter. You can
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make it into energy and you can make energy into matter.
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And so eventually the universe, all of the photons that
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were high energy, they're going to lose energy over time.
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So it's a misnomer to call it a heat death
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if it's actually a cold death.
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It gets cooler and cooler. Yeah.
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It's the heat that's just like, go on without me.
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Just go on without me. This is StarTalk. Neil deGrasse Tyson,
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your personal astrophysicist. Got with me Chuck Nice. How you doing, man?
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What's up, Neil?
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All right. We're doing cosmic queries today. Yes, we are.
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With an old friend and colleague, Michelle Thaller. Michelle, welcome
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to StarTalk.
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It is wonderful to be here. Great to be talking
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to you guys.
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Yeah, so you're not only a fellow astrophysicist, you're a
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fellow science communicator. And we love that species of scientist
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out there. You were recently of NASA Goddard Space Flight Center.
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But the last time you weren't recently of it, you
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were of it. So how recently have you no longer
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been part of them?
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Yeah, I retired in October. I think it was October 2024.
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Okay.
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Yeah, so I've been retired for a couple of years.
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I've been doing speaking. I've been doing a lot of
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lecturing with Smithsonian Journeys. That's been a lot of fun.
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I know them, yes.
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Yeah, just having fun being a freelance astrophysicist. There you go.
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Nice.
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Whoa, astrophysicist at large.
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We got a personal astrophysicist and a freelance astrophysicist.
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We can talk about whatever you want. I'm not working
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for anybody, so total honesty here.
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I'm not working for anybody. No, that's right. I like that.
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Let me just finish up with your CV here. You
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were a research scientist with the Spitzer Space Telescope, one
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of the one of the big, what do they call them?
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The grand- The great observatories, yes. Great observatories. And that
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one was a band of the spectrum that Hubble did
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not cover. So that was infrared, right? The Spitzer telescope?
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That's right, yeah.
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Could you straighten us out here? Locally, we have the
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Goddard Institute for Space Studies, who lost their lease with
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Columbia as it was removed by the White House. Yes.
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But that has the word Goddard in it. And then
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we have the Goddard Space Flight Center in Maryland- They're
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both NASA. Could you just help us distinguish the two? Well, yes.
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So the Goddard Institute for Space Studies has for a long,
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long time been the center for NASA, basically earth science,
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climate science.
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Yes.
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And so that was the thing. So they had a
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very close link to Columbia University. Columbia University leased this
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building to them. Famously, it's the building that if you
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remember Seinfeld, you know, the sitcom Seinfeld, it's the cafe.
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The diner.
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It's that building.
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Yeah, that's right.
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The diner's in that building.
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It just says restaurant on the front.
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Yeah, absolutely.
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It's the greatest name for any eatery ever.
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It's a restaurant.
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Restaurant. Yeah, yeah.
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So, I mean, absolute heroes of mine work there. I mean,
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these are the people that are doing, you know, they're
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in the middle of Antarctica ground truthing measurements from satellites.
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They're making sure we understand what's going on with, you know,
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the atmosphere and the oceans and all of that.
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You could say it, Michelle. You could say they're doing
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God's work. You could say that.
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Goddard's work.
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Goddard's work.
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Goddard's work. Goddard's work.
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Goddard's work.
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Absolutely.
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No, two heroes of mine. And yeah, it's been rough.
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It's been a rough couple of years for them.
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Yeah.
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In fact, at the museum, we have a few refugees
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that have taken pitch tent within our facility because we're
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just down the street a couple of miles from GISS,
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Goddard Institute for Space Studies. But they're homeless at this point.
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They're still all paid as scientists, but they're homeless. But
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it has the name Goddard in it, yet so did
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the Space Flight Center. So now we go to Maryland
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and what happens there? Well, yeah.
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So Maryland, right. So this is this giant base. At
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the moment, it's still NASA's largest base in terms of
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people that go there. I think they're down a little bit.
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But when I was there, there were about 10,000 people
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that worked there every day. And that's pretty incredible. I mean,
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one statistic they had is that if Goddard were to
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leave NASA, then Goddard would become the world's second largest
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space program. I mean, Goddard itself is bigger than the
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other space programs around the world.
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And again, I mean, just- So Goddard builds satellites or
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telescopes that get launched. Well, yeah.
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So, I mean, the Hubble Space Telescope was built largely
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at Goddard. The observatory part of the James Webb Space Telescope.
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We build the GOES satellites, the weather satellites. I mean, yeah.
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I mean, there's four huge science divisions. You've got earth science,
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which is the biggest one. And then heliophysics, study of
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the sun, the Space Weather Action Center. You know, all
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the stuff the sun's thrown at us. And then you've
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got the planetary stuff and the astrophysics stuff. It's
the
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world's largest science space that we know of.
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Yeah, for now.
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Please keep it that way.
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Yes.
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We'll get there, Chuck. Yeah.
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Yeah.
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Michelle, tell me what are the consequences of the budget
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cuts we've read about to NASA overall and to Goddard
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specifically where you once worked?
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It's been a couple years of, I mean, I really
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feel for all of these people, all my former friends,
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and so many of them have left. I mean, I've
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seen some of our absolute best scientists, and not only that,
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our best engineers. One of my best friends, who's just
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an incredible kick-ass systems engineer, she got scooped up by Switzerland.
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And I mean, the scientists are going overseas. With NASA
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and Goddard in general, it's been this real seesaw. Is
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there going to be a huge cut? Or, well, then
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Congress kind of restores the funding, so maybe not. Oh, no, no,
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we're going to do the huge cut. Oh, well, well,
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maybe not. So, I mean, it's this time of terrible uncertainty.
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And aside from programs being on the canceling block and
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losing scientists, the other big thing I've been seeing that's
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been heartbreaking is the best young people, the best scientists. So,
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NASA was required to get rid of all of their,
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you know, all the people that were hired in the
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last three years, right? All the people that were still
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on probation, you know, I mean, this may be the
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person you wanted to get the leader, you know, right
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out of graduate school, they're going to be the leader
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for the future. If they were there less than three years,
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you can still legally fire them. And so those people
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are gone. And, and you have a lot of the
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best scientists now going, well, why should I work for NASA?
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Why should I work for any kind of government agency?
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because they can just up and cancel my job at
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a moment's notice.
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And just to be clear, when you use the word probation,
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you don't mean they did something bad and they're under observation.
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This is just the starter period of time over which
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you could be removed for no cause at all, just
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because you're not vested in the government system yet. Is
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that a fair way to characterize that?
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That's right. I mean, everybody sort of has a trial
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period when you're hired as a government scientist, you know,
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Equivalent to sort of like getting tenure at a university.
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You're there sort of for a while where it's legally
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easy to say, oh, well, that wasn't the right fit.
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Maybe you should go somewhere else. But then when they
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make you permanent, that's harder to do. And so, yeah,
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by probationary, that doesn't mean that anybody– nothing was wrong.
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These are the best people in the world.
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If you do something wrong, they put you on double
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secret probation. Yes, that's right.
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So, Michelle, this sounds like when we– I think I
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might be a little older than you, but same sort
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of generation– Where we're in graduate school and we, as
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a nation, are the beneficiaries of the smartest people in
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other countries coming to the United States for opportunity to
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express their talents and their brilliance. And bad for their
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home country, good for America.
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Yeah.
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And now I have colleagues, as do you, who are
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getting the phone call from Europe. We got a lab
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for you in Germany. We got a lab for you
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in Paris. And here's money, and it's funded, and it's stable.
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Come on down. And so now the world is cherry-picking us.
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They weren't sending us their best, their brightest. They weren't. Yeah,
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but now we're sending our best and brightest out.
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Yeah, yeah. So where does this land, do you think?
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Are we going to recover from this?
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Well, I mean, one of the physics journals I remember
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had a full-page ad from the country of Denmark saying,
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you know, come to a place where facts still.
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Matter, right?
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Damn. Oh, damn.
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Yeah, no, other countries are on it.
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Oh, that's a burn.
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Yeah, I mean, Europe is a beneficiary, Canada, and China.
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I mean, China as well. I have a lot of
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colleagues that got offers. It's like, well, bring your whole
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lab over, all your graduate students, like you said, funding.
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It's so unnecessary. I mean, the thing that has been
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so tragic about this is that science research in the
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United States is a low budget item. Oh, my God.
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You know, we do not spend a lot of money
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on this already. I mean, the thing that I was
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so proud of, I mean, you know, I worked for
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sort of the science part of NASA, doing all the
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Earth science, the Mars rovers, you know, the Webb telescopes.
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About 110 active missions at any given time. Each of
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those missions employs thousands of people. In some cases, tens
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of thousands of people across the country, across the world.
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They do it all for under $ 6 billion a year.
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That's a nothing burger when it comes to a budget.
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We get so much innovation. You can demonstrate. We've had
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economists do studies that you get two, three times more
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the economic advancement of money put into science research.
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Just to be clear, that's the $ 6 billion out of
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the $ 30 billion that is NASA's annual budget, and you're
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referring to just the science, which is not put people
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in orbit. That's not the space station. That is not
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launching astronauts. That is science.
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But putting people in orbit, of course, has to be
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more expensive because you need to be a lot more
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careful when there are human lives on stake.
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Yeah, they want to come back usually. They want to
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come back.
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Oh, yeah.
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The rovers don't need to come back. People, you got
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to bring them back, you know.
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What you can do for the cheap. I mean, some
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of the missions that blow me away, you know, I mean,
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basic physics, how to neutron stars work nicer. That's actually
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on the space station, but it's a small thing, just
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a couple hundred million dollars. I mean, these little budget items.
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James Webb, of course, is a bigger one, but that
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was over 20 years and employed, again, tens of thousands
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of people. These are tremendously great value for the money.
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Did you say it was $ 30 billion? That's all we spend?
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$ 30 billion?
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The total. Yeah, it's around there, plus or minus for
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NASA in a year. $ 30 billion is less than four-tenths
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of 1% of your tax dollar. I do the experiment.
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You take a full dollar and just cut into it,
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just a single dollar bill, cut into it, four tenths
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of 1% of its width, and it doesn't even reach
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the paint, the ink of the bill. Okay, you can
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remove that and the bill is still there. A. B,
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what I wanted is to create a new budgeting system
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where agencies get the money people think they're getting. Because
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the visibility of NASA is so huge. compared to their
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actual budget, no one would guess off the top that
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they're getting 4 tenths of 1%. They would say 5%.
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I've heard some people say 10%. And I say, that's
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the budget we should give them.
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I like that.
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Give them their visibility budget. Yeah. Yeah.
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And by the way, everybody loves NASA still. It's one
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of the few government agencies where people believe in the
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institution of the agency, and they also trust it. And
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it's respected around the world. It's respected around the world.
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That and what was formerly the NIH, which is now
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the SAD, as in just sad.
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Yeah.
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That doesn't even stand for anything. It's just sad.
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I mean, NIH is a whole other story. I mean, honestly,
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that's even more worth saving than NASA. I mean, as
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much as I'm a huge NASA and space fan, I mean,
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do not mess with the NIH.
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Good Lord.
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I mean, we need to keep that research going, the
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cancer research, the Alzheimer's research. I mean, again, Center for
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Disease Control, things like that. Oh my God, do we
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need those?
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So, so yeah.
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And remember, I mean, for 30 billion, you're still talking
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about the whole budget of NASA and the human space
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program is the big chunk of that. All the earth science,
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all the climate science, all the weather satellites, you know,
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all the monitoring the sun, all the exploring the universe.
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And all the space telescopes are in the science.
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All the space telescopes.
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Yeah.
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So, I mean, it's, it's nothing. I mean, I don't
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know if this is true, but I remember one economist
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saying that, that they'd shown that the Pentagon, the military
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cross all over the world, had spent more money on
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air conditioning in a year than that budget.
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Oh, my God.
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So I'm not absolutely sure that's true. But, you know,
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it's on that level. I mean, we're not even a
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fighter jet, basically.
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Looks like America has stepped in a pile of doge crap.
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Yeah, doge doo doo.
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Space has a way of humbling us. Every observation, every mission,
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every new data set reminds us that the universe is
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far more complex than our first assumptions. That's a perspective
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Michelle Thaler has spent her career sharing, helping bridge the
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gap between cutting-edge astrophysics and public understanding. But when science
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enters the news cycle, that clarity can get distorted. Some
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headlines push bold claims, while others take a more measured approach,
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focusing on data and
uncertainty. That's why we've been partnered
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with Ground News since 2024. Their app and website give
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us a data-driven approach to reading the news... by pulling
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articles from over 50,000 sources worldwide in one place. You
300
00:14:07.009 --> 00:14:09.970
can easily compare how different sources cover the same story
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and get a visual breakdown on the bias, reliability of
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a source, and who owns it. Take this recent story
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about NASA's race to save the Swift Observatory before the
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aging spacecraft falls back to Earth. Over 200 sources reported
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on this story, and when you look at the headlines,
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they're all reporting on the same NASA mission. yet they
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leave you with very different impressions. Some focus on the
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engineering and science behind the rescue, while others emphasize the
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danger with phrases like high risk or burning up. The
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facts haven't changed, but the framing has. That's exactly what
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Ground News helps you uncover, making it easy to compare
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how different outlets tell the same story before you draw
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your own conclusions. We've been partnered with Ground News since
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2024 for their transparency, and because they're fully subscriber-funded, so
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there aren't corporate interests deciding what you can and can't see.
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If that's the kind of world you want to live in,
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you can get the same unlimited Vantage plan we use
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for 40% off at ground.news.com or by scanning the QR code.
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On the screen.
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So let's pivot now to our questions. So Michelle, we've
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solicited questions from our fan base, well, from our Patreon supporters,
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and they know who you are, they know your expertise.
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And these are targeted for you. And to the extent
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that we overlap in expertise, I'm happy to put in
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my two cents. But we're really here to see what
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you've got to say in response to these questions. Chuck
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has them all. I haven't seen any of them. And so, Chuck,
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what do you have for us?
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All right. So, inquiring minds want to know. This is
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Ross Graves, who says, Hello, I admire and I respect
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you all, Dr. Tyson, Dr. Thaller. Lord Nice, this is
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Ross from California. When a photon is absorbed and re-emitted
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or reflected, is the journey through space-time physically continuous, or
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does that interaction create an entirely new quantum history for
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the outgoing light in the sense that the light experiences
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no time of its own if reflected? Did it hit
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a surface and restart its existence? experience as a reflection? Dude,
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that's a matrix like crap. He just came up with that.
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That is an amazing question.
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I love it. I love it. Did it take on
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a new identity as a reflected photon? That's what that
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comes down to. So Michelle, what do you have to
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say about that? Okay. All right.
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All right.
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So I'm going to say, I'm going to start out
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saying this is something that is a question of mind. So,
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I mean, well done, because I mean, this is actually
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something that I wish I understood better. I only recently
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came to a better understanding because of some great podcasts, actually.
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It was the podcast Veritasium that Derek Muller does, that
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finally I could understand like why the speed of light
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is different speeds. When you go through the vacuum of space,
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it's the fastest anything can go, the speed of light,
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when it passes through air or water or glass. You
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see that classic bend, right? When you look through water,
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you see light bend, and that's because the speed changes.
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And it was only his podcast that finally got me
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to understand light is an electromagnetic field. And when it's
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in the presence of other electromagnetic fields, when you're not
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in a vacuum, there's other atoms and molecules around. the
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electromagnetic field basically becomes a combination of those two fields.
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And he did this great podcast about that. The question
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about whether a photon is
reflected becomes a different photon
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is fascinating. So let's break it up. Let's go back
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to the beginning. I mean, this is one of the
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craziest and it's true. You know, the idea that when
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you're traveling at the speed of light, I mean, photons
368
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obviously don't have any consciousness. They're not able to observe this.
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But a photon has no idea that space and time exist.
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When you're traveling at the speed of light, time goes
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to a zero. You don't experience the passage of time. And,
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you know, when you think about you're frozen in a
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moment of time, you can go any distance in the
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universe instantaneously to your perspective.
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So a photon.
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doesn't really experience the universe as ever having expanded. You know,
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we're still a point, a thing, you know, almost a
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singularity to a photon. It does not experience space and time.
379
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What the hell does that mean? I mean, how do
380
00:18:35.079 --> 00:18:38.000
you wrap your head around that? When, I mean, the
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00:18:38.200 --> 00:18:40.579
light that's, you know, bouncing off my lamp from my
382
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face right now doesn't agree with me that space and
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time exist. Now, I mean, help me unpack this, Neil,
384
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because I don't have a great answer. I would like
385
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a better answer.
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00:18:50.390 --> 00:18:53.150
Let me restate what you said, but I don't have
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00:18:53.190 --> 00:18:56.700
a deeper understanding just for having restated it. It's the
388
00:18:56.759 --> 00:19:02.519
photon has to know that the universe expands because it
389
00:19:03.319 --> 00:19:07.799
gets redshifted, right? So the photon you detect has a
390
00:19:07.980 --> 00:19:13.049
different energy than the photon that was emitted. So even
391
00:19:13.089 --> 00:19:17.650
though the photon does not experience space-time, we measure a
392
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different photon. a different energy for that photon. Some of
393
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that energy got shared with the expansion of the universe.
394
00:19:26.410 --> 00:19:29.910
So that's something I can't claim to fully understand, how
395
00:19:30.210 --> 00:19:34.430
it doesn't exist in time at all, yet it changed
396
00:19:34.470 --> 00:19:38.819
its wavelength before it arrived on location with you. Now,
397
00:19:38.859 --> 00:19:41.099
let me ask you, I didn't see that episode with veritasium,
398
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but it was also a recent understanding of mine as well,
399
00:19:46.180 --> 00:19:50.230
that when photon moves through a medium, It is. is
400
00:19:50.309 --> 00:19:54.119
moving at the speed of light between atoms of the
401
00:19:54.150 --> 00:20:00.779
transparent medium, but it interacts with each atom and continues
402
00:20:00.859 --> 00:20:05.750
forward and that interaction creates a time delay. So the
403
00:20:05.809 --> 00:20:09.279
photon is never actually ever going slower than the speed
404
00:20:09.319 --> 00:20:15.279
of light. It just got waylaid en route through the
405
00:20:15.319 --> 00:20:18.640
transparent medium. Now, is that consistent with what you got
406
00:20:18.740 --> 00:20:20.220
out of the Veritasium episode?
407
00:20:20.240 --> 00:20:25.349
So wait, Neil, let me just, because, well, Jesus. So.
408
00:20:28.759 --> 00:20:29.900
I'm trying to, I'm trying to.
409
00:20:29.900 --> 00:20:32.200
Take a cleansing breath, Chuck. Yes. Take a cleansing breath.
410
00:20:32.440 --> 00:20:37.640
Okay. I'm trying to get this as a metaphor because
411
00:20:37.660 --> 00:20:40.259
that's how I see and understand things. So in the
412
00:20:40.299 --> 00:20:43.200
vacuum of space, that would be like taking a pool
413
00:20:43.269 --> 00:20:46.309
ball and shooting it straight across the table into the pocket.
414
00:20:46.910 --> 00:20:49.519
And it's going at that speed. But then when you
415
00:20:49.539 --> 00:20:52.140
put it through a medium, that would be like having
416
00:20:52.180 --> 00:20:55.539
the same speed but banking it off of three banks
417
00:20:55.660 --> 00:20:59.029
and then going into the pocket. So your speed doesn't change,
418
00:20:59.269 --> 00:21:00.890
but the fact that you had to bank it three
419
00:21:00.950 --> 00:21:04.410
times is what slowed you down.
420
00:21:04.809 --> 00:21:08.240
However, what you're describing does happen to light, but that's
421
00:21:08.259 --> 00:21:10.619
when light scatters. Okay.
422
00:21:11.000 --> 00:21:12.200
Oh, so that's a different phenomenon.
423
00:21:12.220 --> 00:21:14.480
Because a transparent medium, it keeps in the same direction
424
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at all times.
425
00:21:16.119 --> 00:21:17.779
Ah, gotcha, gotcha, gotcha, gotcha, gotcha.
426
00:21:17.819 --> 00:21:21.170
That's the difference between a transparent medium, a translucent medium,
427
00:21:21.470 --> 00:21:25.630
and just something that completely scatters the light. So, Michelle,
428
00:21:25.890 --> 00:21:28.309
are we in agreement that we're talking about a new
429
00:21:28.369 --> 00:21:32.410
photon as it goes through, a newly shaped photon after
430
00:21:32.450 --> 00:21:34.769
it interacted with these other fields? Is that a fair
431
00:21:34.789 --> 00:21:35.589
way to think about it?
432
00:21:36.799 --> 00:21:38.509
The way the podcast did it, and this was the
433
00:21:38.690 --> 00:21:40.710
first time I ever sort of
thought, oh, okay, I
434
00:21:40.730 --> 00:21:43.670
get this. You know, we were sort of talking about
435
00:21:43.710 --> 00:21:46.539
photons as particles here, as like little billiard balls and stuff.
436
00:21:46.579 --> 00:21:51.000
But of course, remember, famously, they're electromagnetic waves, right? I mean,
437
00:21:51.019 --> 00:21:54.890
they're not just little balls. And so what the podcast
438
00:21:54.930 --> 00:21:57.369
did is it showed that there's electromagnetic wave, there's a
439
00:21:57.390 --> 00:22:02.170
photon going in, and there's other atoms around. And basically
440
00:22:02.230 --> 00:22:06.119
the electromagnetic wave starts those other atoms kind of vibrating
441
00:22:06.160 --> 00:22:09.880
along with it. But there's a delay, there's a lag
442
00:22:09.900 --> 00:22:12.420
to kind of get those other fields, those other electric
443
00:22:12.480 --> 00:22:15.920
fields vibrating as the photon goes by. And the resulting
444
00:22:16.059 --> 00:22:19.960
speed is actually a combination. It's actually a way of
445
00:22:20.019 --> 00:22:23.279
resolving those two different vibrational modes.
446
00:22:23.779 --> 00:22:28.779
So the photon is like to the other, you know, Adams, like, bro,
447
00:22:29.599 --> 00:22:30.420
you're bringing me down.
448
00:22:31.799 --> 00:22:33.309
Yeah.
449
00:22:33.809 --> 00:22:36.289
You're dragging me, man. I can't, I got it. Come on.
450
00:22:36.589 --> 00:22:38.970
I'm serious. Like get off me. And then let me
451
00:22:38.990 --> 00:22:40.089
get the hell out of this medium.
452
00:22:40.470 --> 00:22:42.450
Yeah. Cause once he exits the medium, it's back at
453
00:22:42.490 --> 00:22:43.049
the speed of light.
454
00:22:43.700 --> 00:22:45.559
The speed of the wave that we measure is a
455
00:22:45.599 --> 00:22:48.140
combination of the speed of the photon in a vacuum,
456
00:22:48.509 --> 00:22:52.009
but then also the speed of the variations of basically
457
00:22:52.049 --> 00:22:56.529
the oscillations of everything around it. Those two combine into
458
00:22:56.569 --> 00:22:59.569
the measured speed of the photon that we see. That's fascinating.
459
00:22:59.869 --> 00:23:02.410
So the question about, I mean, it's the same thing, Neil.
460
00:23:02.769 --> 00:23:03.210
Absolutely.
461
00:23:03.230 --> 00:23:05.890
When you talk about how a photon changes, even as
462
00:23:05.930 --> 00:23:09.140
it goes through a vacuum, it loses energy. It's a
463
00:23:09.200 --> 00:23:12.440
very similar question that if a photon is reflected, Is
464
00:23:12.509 --> 00:23:15.130
it a different photon? I mean, it can certainly be
465
00:23:15.150 --> 00:23:18.529
a different energy, right? I mean, when a photon is reflected,
466
00:23:18.569 --> 00:23:21.970
you usually lose some energy in the reflection. So, I mean,
467
00:23:22.009 --> 00:23:25.440
there's all sorts of things. Photons absolutely can change.
468
00:23:26.240 --> 00:23:28.180
Just to be clear, Chuck, if a photon hits a
469
00:23:28.200 --> 00:23:31.839
surface and reflects, some of its energy is imparted as
470
00:23:31.900 --> 00:23:34.859
momentum to that surface. And that's why solar sails work
471
00:23:34.880 --> 00:23:35.140
at all.
472
00:23:35.529 --> 00:23:36.180
Has to be.
473
00:23:36.240 --> 00:23:39.509
Yeah, yeah. Yeah. So, yeah, there's an energy change there.
474
00:23:40.029 --> 00:23:44.789
So I'm voting for a completely different photon here. What
475
00:23:44.809 --> 00:23:45.869
do you think, Michelle?
476
00:23:46.829 --> 00:23:49.839
Yeah, like I said, Ross Graves is a name that's
477
00:23:49.859 --> 00:23:53.579
familiar to me. So yes, thank you for this fabulous question.
478
00:23:53.940 --> 00:23:56.859
And I have to say, I do not have an
479
00:23:56.880 --> 00:24:00.630
extremely clear answer. I'm not ashamed of that. This is
480
00:24:00.789 --> 00:24:02.309
one I've wondered myself.
481
00:24:02.769 --> 00:24:06.049
Okay. So let's, let's vote. That's right.
482
00:24:06.089 --> 00:24:06.450
Yeah.
483
00:24:06.549 --> 00:24:07.089
Yeah.
484
00:24:07.329 --> 00:24:10.089
I'm voting that the photon that came out, it's a
485
00:24:10.150 --> 00:24:15.779
new quantum state that is carrying the mission forward after
486
00:24:15.839 --> 00:24:19.059
it had its delay from the medium through which it
487
00:24:19.259 --> 00:24:22.359
passed or the medium off of which it reflected. I'm
488
00:24:22.380 --> 00:24:22.920
going with that.
489
00:24:24.660 --> 00:24:28.420
I wish I had the same properties and there was
490
00:24:28.640 --> 00:24:33.160
a reflection Chuck and real Chuck and I could tell
491
00:24:33.700 --> 00:24:36.009
all the people I owe money, you need to go
492
00:24:36.049 --> 00:24:37.400
talk to reflection Chuck.
493
00:24:38.940 --> 00:24:39.869
That's not me anymore.
494
00:24:39.930 --> 00:24:40.650
That's not me.
495
00:24:40.569 --> 00:24:46.950
Anymore, buddy. That's a great question. Okay. What else do
496
00:24:46.970 --> 00:24:47.960
you have, Chuck? All right.
497
00:24:48.000 --> 00:24:52.119
Here we go. This is Jao Costa. Jao Costa says,
498
00:24:52.680 --> 00:24:57.380
good tidings, Dr. Tyson, Dr. Thaler, Lord, nice deep breath now, Chuck.
499
00:24:57.680 --> 00:25:00.829
Jao Costa here. Greetings from Portugal.
500
00:25:01.509 --> 00:25:02.509
All right.
501
00:25:02.970 --> 00:25:07.250
Yes. He says, if matter isn't being created, only transformed-
502
00:25:07.650 --> 00:25:10.710
Will there come a day when the universe runs out
503
00:25:10.829 --> 00:25:14.960
of matter to create new astral bodies? If so, how
504
00:25:15.039 --> 00:25:18.240
will we be able to notice such a situation developing?
505
00:25:18.500 --> 00:25:22.799
Will the creation start to become rarer, smaller, or deficient,
506
00:25:23.079 --> 00:25:27.099
as in less frequent, less energetic, or less stable? Thank you,
507
00:25:27.519 --> 00:25:32.680
and please keep making our necks hurt. Oh, I like it.
508
00:25:32.930 --> 00:25:34.069
Look up. making that hurt.
509
00:25:34.450 --> 00:25:37.150
Oh, no. I see. I see what he did there. Okay.
510
00:25:37.410 --> 00:25:39.009
You got him looking up so much. You gave him
511
00:25:39.049 --> 00:25:39.869
a neck ache, Neil.
512
00:25:42.109 --> 00:25:43.769
Okay. You can lay down and look up and then
513
00:25:43.789 --> 00:25:49.579
you're just looking straight ahead. The geometry. Yeah.
514
00:25:51.220 --> 00:25:51.599
Yeah.
515
00:25:52.519 --> 00:25:54.680
Well, it sounds to me like somebody is just describing
516
00:25:54.740 --> 00:25:56.259
what's called the heat death of the universe. And the
517
00:25:56.299 --> 00:25:59.039
answer is yes. The answer is that the, the, the
518
00:25:59.119 --> 00:26:04.140
universe is slowing down in the sense that, um, It's
519
00:26:04.200 --> 00:26:06.019
not so much that matter can't be destroyed.
520
00:26:06.079 --> 00:26:06.380
It can.
521
00:26:06.420 --> 00:26:08.829
It can be converted into energy. Matter and energy are
522
00:26:09.150 --> 00:26:12.250
two sides of the same coin. That famous equation, hopefully
523
00:26:12.269 --> 00:26:13.609
the only one you ever have to deal with in life,
524
00:26:14.069 --> 00:26:16.609
unless you want to be a scientist, is energy equals
525
00:26:16.710 --> 00:26:19.250
mass times the speed of light squared. Good old Albert Einstein.
526
00:26:19.589 --> 00:26:20.490
E equals MC squared.
527
00:26:20.509 --> 00:26:23.299
That's most people's first equation they learn in elementary school,
528
00:26:23.319 --> 00:26:24.559
even before you know what it means.
529
00:26:24.579 --> 00:26:25.779
It's your elementary school equation.
530
00:26:26.059 --> 00:26:26.200
Yeah.
531
00:26:27.480 --> 00:26:29.920
So you can destroy matter. You can make it into energy.
532
00:26:30.039 --> 00:26:32.180
And you can make energy into matter. That's what we
533
00:26:32.220 --> 00:26:35.680
do in particle accelerators. We get things going with such
534
00:26:35.759 --> 00:26:38.609
high energy. When things collide, there's so much energy around,
535
00:26:38.640 --> 00:26:41.609
it actually creates new matter. That's how you find new
536
00:26:41.650 --> 00:26:46.950
types of particles. So energy and matter are equivalent. But
537
00:26:47.930 --> 00:26:50.849
absolutely what's happening is that in the early universe, there
538
00:26:50.869 --> 00:26:54.710
were things that were much higher temperature, much higher energy. Stars,
539
00:26:54.769 --> 00:26:57.329
for example, are an example of something that's a very
540
00:26:57.490 --> 00:27:05.160
low entropy. Stars create very high energy radiation. And over time, yes,
541
00:27:05.380 --> 00:27:10.660
I mean, every time you basically generate heat, I mean,
542
00:27:10.680 --> 00:27:13.680
if sunlight comes down, it's a high energy photon, hits
543
00:27:13.720 --> 00:27:17.079
the earth, warms things up. What's released, the heat is
544
00:27:17.119 --> 00:27:20.079
a lower energy type of light. You've lost energy. You've
545
00:27:20.099 --> 00:27:22.180
made from a high energy particle of light. Now it's
546
00:27:22.200 --> 00:27:25.920
a lower energy type of light. And so eventually the universe,
547
00:27:26.059 --> 00:27:28.380
all of the photons that were high energy are going
548
00:27:28.400 --> 00:27:31.410
to hit things, get absorbed by things, make things warm,
549
00:27:31.430 --> 00:27:34.690
get re-emitted, and they're going to lose energy over time.
550
00:27:35.549 --> 00:27:38.650
And so yes, the universe is running down. And eventually
551
00:27:38.670 --> 00:27:41.710
we're going to get to a point where there's nothing left,
552
00:27:41.750 --> 00:27:44.559
but very low energy photons, you know, photons that are
553
00:27:44.599 --> 00:27:47.779
so low energy, they're probably not even detectable. And then
554
00:27:47.819 --> 00:27:51.710
it's sort of anybody's guess as to, you know, does
555
00:27:51.769 --> 00:27:55.279
time and space exist anymore when there's really, everything is
556
00:27:55.319 --> 00:27:58.000
just the same temperature. A very, very low temperature is
557
00:27:58.039 --> 00:27:59.380
the only thing that the universe has.
558
00:28:00.019 --> 00:28:02.359
So it's a misnomer to call it a heat death
559
00:28:02.819 --> 00:28:05.559
if it's actually a cold death.
560
00:28:05.579 --> 00:28:06.640
It gets cooler and cooler.
561
00:28:06.660 --> 00:28:07.039
Yeah.
562
00:28:07.180 --> 00:28:10.059
Yeah. I mean, it's the heat that's dying.
563
00:28:10.640 --> 00:28:11.500
Yeah.
564
00:28:12.309 --> 00:28:17.460
It's the heat that's just like, oh, go away out there. Yeah.
565
00:28:17.700 --> 00:28:23.450
Just go on without me. Plus the expanding universe also drops,
566
00:28:23.490 --> 00:28:24.619
dropping the temperature with it.
567
00:28:24.750 --> 00:28:24.930
Right.
568
00:28:25.390 --> 00:28:25.789
Absolutely.
569
00:28:25.809 --> 00:28:28.210
You got a photon going through expanding space and think about,
570
00:28:28.269 --> 00:28:30.809
you know, draw a squiggly line on a piece of
571
00:28:30.849 --> 00:28:33.559
elastic and pull the elastic. And then that, that wavelength
572
00:28:33.579 --> 00:28:36.140
drops down, you lose energy. You know, I mean, it's, it's,
573
00:28:36.299 --> 00:28:37.539
it's really kind of as simple as that.
574
00:28:37.660 --> 00:28:39.920
Wait, wait, just to be precise, the wavelength gets longer.
575
00:28:40.599 --> 00:28:41.519
The wavelength gets longer.
576
00:28:41.599 --> 00:28:42.220
That's right. Yes.
577
00:28:42.259 --> 00:28:43.720
And that's a lower energy wavelength.
578
00:28:43.789 --> 00:28:44.329
Lower energy.
579
00:28:44.420 --> 00:28:44.990
So it drops down.
580
00:28:45.009 --> 00:28:46.769
The wavelength gets longer, the frequency drops.
581
00:28:47.109 --> 00:28:47.349
Right.
582
00:28:47.690 --> 00:28:51.349
And if I may, what Michelle just described is exactly
583
00:28:51.490 --> 00:28:55.769
how
the warming of the planet happens. High energy comes in,
584
00:28:55.890 --> 00:29:00.819
pierces our atmosphere, becomes lower energy and a longer wavelength,
585
00:29:01.200 --> 00:29:05.539
which is trapped by greenhouse gases. And that's how we
586
00:29:05.599 --> 00:29:08.799
heat up. Because as everybody has learned from Neil- The
587
00:29:08.980 --> 00:29:13.519
atmosphere isn't hot. The ground gets hot and radiates heat
588
00:29:13.779 --> 00:29:16.660
back into the atmosphere. And that is the cycle that
589
00:29:16.700 --> 00:29:18.779
creates a warming of the planet. Just so that you
590
00:29:18.819 --> 00:29:20.380
guys know that it's real.
591
00:29:21.549 --> 00:29:25.789
Okay? It's real. And send $ 5 to Chuck's tenant campaign.
592
00:29:25.809 --> 00:29:29.990
By the way, just to be precise, there is a
593
00:29:30.029 --> 00:29:33.150
layer of the atmosphere that does absorb light directly from
594
00:29:33.190 --> 00:29:38.279
the sun. And that's the thermosphere where the ultraviolet gets
595
00:29:38.319 --> 00:29:42.539
absorbed and by the ozone. And so that there is
596
00:29:42.579 --> 00:29:45.480
a layer that is hotter, but we're not experiencing that
597
00:29:45.609 --> 00:29:46.869
right down here. Right.
598
00:29:47.049 --> 00:29:47.930
Oh yeah. That's cool.
599
00:29:47.970 --> 00:29:50.210
Yeah. The hottest part of the troposphere is right above
600
00:29:50.250 --> 00:29:52.569
earth's surface. Right above earth's surface. Okay.
601
00:29:52.990 --> 00:29:53.509
Nice.
602
00:29:53.789 --> 00:29:54.430
Yeah.
603
00:29:54.450 --> 00:29:58.420
Yeah. Right. And what's the part, see now, now, This
604
00:29:58.480 --> 00:30:01.009
is where the explainers are all swirling in my head.
605
00:30:01.680 --> 00:30:07.309
What is the part where the excitation of the molecules
606
00:30:07.809 --> 00:30:11.349
is such that it's, we say it's cold, but it's
607
00:30:11.609 --> 00:30:13.049
actually hotter?
608
00:30:13.769 --> 00:30:16.579
Chuck, could it be that there's a layer, upper layers
609
00:30:16.619 --> 00:30:22.619
of the atmosphere where the particles themselves are high energy,
610
00:30:22.940 --> 00:30:25.440
but there isn't many of them so that you don't
611
00:30:25.740 --> 00:30:29.190
feel that temperature? that you otherwise would.
612
00:30:29.210 --> 00:30:29.990
That's what I'm saying.
613
00:30:30.009 --> 00:30:33.250
So the concept of temperature kind of loses practical meaning.
614
00:30:32.990 --> 00:30:36.150
There, right? Okay, I said it like a- It could
615
00:30:36.170 --> 00:30:38.839
be what you're thinking about. Yeah, that's exactly what I
616
00:30:38.859 --> 00:30:41.119
was thinking about, but I said it like a dumb two-year-old.
617
00:30:41.759 --> 00:30:42.440
No, no.
618
00:30:42.460 --> 00:30:48.920
Michelle, if I flew you through the sun's corona, which
619
00:30:49.059 --> 00:30:52.450
is 5 million degrees, would you feel that given how
620
00:30:52.569 --> 00:30:56.049
low density the particles are that have such high temperature?
621
00:30:56.710 --> 00:30:58.789
We are really, really lucky the answer is no, because
622
00:30:58.829 --> 00:31:01.109
I mean, the corona is one thing, but also let's remember,
623
00:31:01.190 --> 00:31:03.609
I mean, we actually, our whole solar system is in
624
00:31:03.650 --> 00:31:06.170
this hot bubble of gas in the Milky Way galaxy.
625
00:31:07.329 --> 00:31:09.470
Maybe there was a star that exploded here billions of
626
00:31:09.509 --> 00:31:12.410
years ago, but the temperature of the gas we're going
627
00:31:12.430 --> 00:31:14.779
through is in the millions of degrees in our galaxy.
628
00:31:15.130 --> 00:31:19.119
The thing is, the gas between the stars is so thin.
629
00:31:19.759 --> 00:31:21.779
It's like, OK, there goes there goes a proton. You know,
630
00:31:21.799 --> 00:31:24.539
there goes an electron. You know, I mean, there's so
631
00:31:24.599 --> 00:31:27.440
few particles that it doesn't really impart any heat to you.
632
00:31:27.789 --> 00:31:30.410
I mean, yes, the average speed of these high energy
633
00:31:30.450 --> 00:31:34.009
particles is equivalent to being, you know, millions of degree gas.
634
00:31:34.430 --> 00:31:37.630
And just like Neil said, so the sun's corona is
635
00:31:37.650 --> 00:31:42.309
this extended atmosphere of very hot gas. We have a spacecraft.
636
00:31:42.349 --> 00:31:44.809
NASA has a spacecraft called the Parker Solar Probe. that
637
00:31:44.849 --> 00:31:48.559
is orbiting well within the solar corona right now. You
638
00:31:48.599 --> 00:31:51.240
better believe it would not be a live returning data
639
00:31:51.400 --> 00:31:56.809
if it really felt like 500 degrees. So the analogy
640
00:31:56.869 --> 00:31:59.549
we used to use is when you think about everybody
641
00:31:59.589 --> 00:32:01.400
who's done some baking, you get your oven up to
642
00:32:01.400 --> 00:32:01.660
500 degrees.
643
00:32:02.619 --> 00:32:05.000
That's some serious baking if you're baking at 500 degrees.
644
00:32:05.859 --> 00:32:06.759
Pizza.
645
00:32:06.779 --> 00:32:07.869
We're going for pizza ovens here.
646
00:32:07.920 --> 00:32:11.630
Yeah, yeah. You're a pizza shop on the corner of
647
00:32:11.670 --> 00:32:13.569
Lenox Avenue, 125th Street.
648
00:32:13.589 --> 00:32:13.930
Yeah.
649
00:32:13.950 --> 00:32:16.089
If you have a 500 degree oven. Okay.
650
00:32:16.109 --> 00:32:17.450
So if you open the oven and you just stick
651
00:32:17.470 --> 00:32:21.380
your hand in, your hand is not actually feeling like
652
00:32:21.420 --> 00:32:23.119
it's 500 degrees all of a sudden. If you were
653
00:32:23.140 --> 00:32:25.359
to touch like a metal part of the oven, if
654
00:32:25.380 --> 00:32:28.319
you were to touch the rack, then you'd burn your hand. Because,
655
00:32:28.339 --> 00:32:29.640
I mean, all of a sudden now you have a
656
00:32:29.740 --> 00:32:31.289
denser object. You've got the metal.
657
00:32:31.609
--> 00:32:31.789
Yeah.
658
00:32:32.079 --> 00:32:33.759
A little bit of a thing about the Parker Solar Probe.
659
00:32:33.819 --> 00:32:37.829
It's another incredible person, Eugene Parker. And he was the
660
00:32:37.849 --> 00:32:40.369
person that discovered this wind of high energy particles from
661
00:32:40.410 --> 00:32:41.390
the sun, the solar wind.
662
00:32:41.650 --> 00:32:42.650
The solar wind.
663
00:32:43.029 --> 00:32:45.769
Yeah, a fabulous launch. I'm glad somebody told me that
664
00:32:45.789 --> 00:32:48.180
a Delta Heavy looks like it explodes on the pad
665
00:32:48.240 --> 00:32:50.000
before the rocket comes up. I was at that launch.
666
00:32:50.019 --> 00:32:54.119
It was amazing. The whole idea, the surface of the
667
00:32:54.160 --> 00:32:58.119
sun is only about, say, roughly like 10,000 degrees Fahrenheit.
668
00:32:58.559 --> 00:33:00.130
But as soon as you get off the surface, the
669
00:33:00.150 --> 00:33:03.650
gas becomes millions of degrees hot. I mean, this was
670
00:33:03.670 --> 00:33:07.660
a Big mystery. And how does the sun do that?
671
00:33:07.700 --> 00:33:10.599
I mean, normally, if you've got a hot campfire, the
672
00:33:10.619 --> 00:33:13.210
farther away you walk, the cooler it seems. Why does
673
00:33:13.230 --> 00:33:15.569
the temperature go up? And the Parker Solar Probe has
674
00:33:15.609 --> 00:33:20.190
really helped answer that. There's all of these complicated accelerations
675
00:33:20.210 --> 00:33:22.759
due to magnetic fields around the sun. The particles pick
676
00:33:22.799 --> 00:33:25.700
up speed. There are shocks in there. So, I mean,
677
00:33:26.119 --> 00:33:28.960
we're figuring out how the sun works. It's not something
678
00:33:29.000 --> 00:33:32.380
we know until we go there near the sun, fly
679
00:33:32.420 --> 00:33:34.569
around in this corona, and see what's going on.
680
00:33:34.910 --> 00:33:37.069
And look at that. You're getting all of that for
681
00:33:37.109 --> 00:33:38.869
a lousy $ 6 billion.
682
00:33:39.230 --> 00:33:39.710
Okay.
683
00:33:39.869 --> 00:33:42.549
What the hell is wrong with you people?
684
00:33:44.430 --> 00:33:46.700
Okay, Chuck, that's his daily, I got to blow a
685
00:33:46.720 --> 00:33:49.460
gasket once a day reaction.
686
00:33:49.519 --> 00:33:51.599
It's worth it. It's worth blowing a gasket over.
687
00:33:51.980 --> 00:33:55.140
If memory serves, the Parker Solar Probe set a speed record.
688
00:33:55.599 --> 00:33:56.099
Oh, yeah.
689
00:33:56.299 --> 00:33:58.380
It goes over 400,000 miles an hour.
690
00:33:59.140 --> 00:34:00.259
Yeah.
691
00:34:00.380 --> 00:34:00.920
Wow.
692
00:34:01.859 --> 00:34:02.079
Yeah.
693
00:34:02.279 --> 00:34:03.769
I keep having to look that up because I don't
694
00:34:03.809 --> 00:34:05.069
believe it. And then I look it up again.
695
00:34:05.089 --> 00:34:06.829
You don't believe it. Because it gets pulled in by
696
00:34:06.849 --> 00:34:10.570
the sun's gravity. That's right. And there it is, 400,000
697
00:34:10.570 --> 00:34:11.090
miles an hour.
698
00:34:11.469 --> 00:34:13.750
Wow. Amazing.
699
00:34:14.630 --> 00:34:15.010
All right.
700
00:34:15.070 --> 00:34:16.130
Well, let's move on.
701
00:34:16.150 --> 00:34:18.190
I have a few more questions. Let's try to fit
702
00:34:18.230 --> 00:34:21.429
in a bunch more. So let's tighten up the answers
703
00:34:21.469 --> 00:34:22.559
and see how many we can fit in.
704
00:34:22.570 --> 00:34:25.250
Let's just do the questions, and then we just have
705
00:34:25.269 --> 00:34:28.639
to have Michelle back to ask more. That's all. I'm
706
00:34:28.679 --> 00:34:31.440
always here. That's right. Yeah, we're not going anywhere. I mean,
707
00:34:31.480 --> 00:34:33.519
why are these people just like, you didn't get to
708
00:34:33.539 --> 00:34:35.000
my question?
709
00:34:35.019 --> 00:34:35.559
What? What?
710
00:34:35.679 --> 00:34:37.820
You got information we don't? We're getting canceled?
711
00:34:37.920 --> 00:34:38.900
What do you know?
712
00:34:39.039 --> 00:34:41.360
What do you know that we don't know? You know,
713
00:34:41.519 --> 00:34:42.380
we could do this again.
714
00:34:42.619 --> 00:34:43.800
I'm always up for questions.
715
00:34:44.139 --> 00:34:48.619
All right, here we go. This is Tristan Breaker, who says,
716
00:34:49.059 --> 00:34:52.960
Good evening, Dr. Tyson, Dr. Thaler, Lord Nice. Tristan here
717
00:34:53.099 --> 00:34:59.159
from Utah. Considering gravity is caused by the curvature of space-time, hypothetically,
718
00:34:59.480 --> 00:35:03.500
could gravitational waves from two separate sources intersect, forming a
719
00:35:03.539 --> 00:35:10.960
constructive interference pattern combining their amplitudes? If so... Could this
720
00:35:11.079 --> 00:35:14.550
create regions in space where the curvature of spacetime is
721
00:35:14.659 --> 00:35:18.150
great enough to produce a gravitational field as though a
722
00:35:18.210 --> 00:35:21.849
celestial body were present even though nothing is there? Additionally,
723
00:35:22.210 --> 00:35:26.550
wouldn't the crest of the waves create an inverse gravitational field?
724
00:35:26.829 --> 00:35:31.449
Could spacetime curve in the opposite direction, imagining the common
725
00:35:31.610 --> 00:35:37.030
fabric of gravity of demonstration, for instance, producing a repulsive
726
00:35:37.170 --> 00:35:41.989
field rather than an attractive one. My heartfelt thanks to
727
00:35:42.050 --> 00:35:46.679
you for bringing awareness to the wonders of the universe. Well, Christian,
728
00:35:47.300 --> 00:35:49.679
all I can say is, first of all, I need
729
00:35:49.699 --> 00:35:55.199
some of that weed you smoking. Because, man, that is
730
00:35:55.239 --> 00:35:56.579
some serious stuff.
731
00:35:58.179 --> 00:36:02.300
Maybe check with our producers. Maybe for questions like that,
732
00:36:02.719 --> 00:36:05.219
we should create a little certificate that we send back
733
00:36:05.300 --> 00:36:07.980
out to them for questions that are above and beyond
734
00:36:08.019 --> 00:36:08.719
the call of duty.
735
00:36:10.679 --> 00:36:12.480
We've had two so far in this show.
736
00:36:12.500 --> 00:36:16.820
It's a deep thought question, right? That's a deep thought question. Michelle,
737
00:36:17.199 --> 00:36:19.599
are you up on gravitational waves? What's the latest there?
738
00:36:19.679 --> 00:36:21.559
Oh, I love gravitational waves. Are you kidding? I was
739
00:36:21.579 --> 00:36:24.949
a postdoc at Caltech. I better love gravitational waves. So,
740
00:36:25.610 --> 00:36:28.469
oh my God, let me just say how impressed I
741
00:36:28.670 --> 00:36:31.809
am with gravitational wave detection, because this is something when
742
00:36:31.829 --> 00:36:34.250
I was a postdoc at Caltech, it was a big deal.
743
00:36:34.269 --> 00:36:39.090
The LIGO project, the Laser Interferometric Gravitational Wave Observatory was
744
00:36:39.130 --> 00:36:43.070
something that Caltech was involved in. And I honestly, I
745
00:36:43.230 --> 00:36:46.329
talk about my skeptical nature. I was like, they're never
746
00:36:46.369 --> 00:36:50.349
gonna detect these bastards. I mean, this is really, so
747
00:36:50.409 --> 00:36:53.510
LIGO at the time, there were two facilities. There are
748
00:36:53.550 --> 00:36:56.619
now more. You've got a you've got a laser that's
749
00:36:56.679 --> 00:37:00.210
about about two miles long and another one going out
750
00:37:00.230 --> 00:37:03.829
in a 90 degree angle. There we go. In a corner.
751
00:37:04.230 --> 00:37:08.639
So two miles each direction. And those lasers, you know,
752
00:37:08.719 --> 00:37:10.980
are supposed to be exactly the same length. Imagine trying
753
00:37:11.000 --> 00:37:13.440
to calibrate that, you know, and so the lasers are
754
00:37:13.460 --> 00:37:15.929
going back and forth, bouncing around. And then if a
755
00:37:15.969 --> 00:37:19.760
gravitational wave comes by, a gravitational wave is literally a
756
00:37:19.800 --> 00:37:22.460
wave in space and time. And so space contracts in
757
00:37:22.559 --> 00:37:24.619
one direction. And all of a sudden, the two lasers
758
00:37:24.659 --> 00:37:28.579
are no longer the same length. They're different because space contracted.
759
00:37:29.239 --> 00:37:32.110
And so the person with the question is absolutely right.
760
00:37:32.119 --> 00:37:35.309
That's what gravitational waves do. The thing that makes it
761
00:37:35.510 --> 00:37:40.090
mind blowing that we detected these things is they're tiny.
762
00:37:40.869 --> 00:37:46.250
Luckily for us. I mean, they're a thousand times smaller
763
00:37:46.610 --> 00:37:49.610
than a proton. And to give you a sense of that,
764
00:37:49.630 --> 00:37:51.949
I mean, not that the human brain can even get that,
765
00:37:52.010 --> 00:37:53.329
and the human brain's not going to get the next
766
00:37:53.429 --> 00:37:56.389
one either, but it's the equivalent of measuring from us
767
00:37:56.409 --> 00:37:59.489
to the nearest star, Alpha Centauri, about four light years.
768
00:37:59.800 --> 00:38:03.119
A light year is about six trillion miles. Damn. You're
769
00:38:03.139 --> 00:38:07.219
going on 24 trillion miles. That would be the equivalent
770
00:38:07.239 --> 00:38:09.420
of the distance between us and the nearest star varying
771
00:38:09.460 --> 00:38:10.659
by the thickness of a human hair.
772
00:38:12.079 --> 00:38:12.280
Wow.
773
00:38:12.840 --> 00:38:14.690
They're trying to measure that.
774
00:38:15.869 --> 00:38:16.449
Holy.
775
00:38:17.469 --> 00:38:18.969
Are you allowed to swear on this podcast?
776
00:38:19.170 --> 00:38:20.710
I'll do it for you.
777
00:38:20.750 --> 00:38:22.409
Holy shit.
778
00:38:24.699 --> 00:38:25.900
I could go more than that probably.
779
00:38:25.920 --> 00:38:27.880
I could swear all day.
780
00:38:28.860 --> 00:38:31.360
You know, I did not think they'd be able to
781
00:38:31.400 --> 00:38:31.739
do this.
782
00:38:32.739 --> 00:38:35.519
And in fact, Michelle, I would, you know, the Nobel prize,
783
00:38:35.579 --> 00:38:39.829
which was ultimately given to the project. For me, I
784
00:38:39.869 --> 00:38:43.340
view that as not only, a prize for the scientific result,
785
00:38:43.699 --> 00:38:48.579
but for the engineering that enabled it. Oh my gosh. Yeah.
786
00:38:48.980 --> 00:38:54.110
With that measurement being so infinitesimally small, how do they
787
00:38:54.269 --> 00:38:56.489
know that somebody didn't just bump the table?
788
00:38:57.150 --> 00:38:59.849
Absolutely. So, I mean, so this is the thing, right?
789
00:38:59.909 --> 00:39:03.429
I mean, somebody bumped a table in the next state, right?
790
00:39:03.489 --> 00:39:04.690
In Australia.
791
00:39:12.090 --> 00:39:14.389
So there's, I mean, there's all of these, you know,
792
00:39:14.409 --> 00:39:16.800
there's all this noise in the detector, right? The detector,
793
00:39:16.880 --> 00:39:19.000
like you said, there's all kinds of noise going on
794
00:39:19.019 --> 00:39:21.179
in the detector. And then this, I was just making
795
00:39:21.219 --> 00:39:23.719
sure I had my dates and everything. So this would
796
00:39:23.739 --> 00:39:25.969
have been in September of 2015.
797
00:39:25.969 --> 00:39:30.050
And just to clarify, when a scientist uses the word noise...
798
00:39:30.679 --> 00:39:34.730
they're not necessarily and almost hardly ever are talking about sound.
799
00:39:35.119 --> 00:39:41.760
Yeah, they're not in the lab going, shut your ass.
800
00:39:41.949 --> 00:39:42.550
Up. Who knows?
801
00:39:42.789 --> 00:39:43.869
Maybe that's what the detector was saying.
802
00:39:43.889 --> 00:39:44.829
Cut down the noise.
803
00:39:47.340 --> 00:39:49.900
No, we're talking about sources of interference to the signal
804
00:39:49.920 --> 00:39:52.800
you're trying to measure, no matter what those sources are. Right.
805
00:39:52.820 -->
00:39:53.880
So go on, Michelle.
806
00:39:53.900 --> 00:39:57.260
There's all kinds of little variations. I mean, the lasers
807
00:39:57.300 --> 00:39:59.650
are under vacuum, but there's all kinds of things happening.
808
00:40:00.110 --> 00:40:06.130
So in September of 2015, there's all kinds of noise.
809
00:40:06.150 --> 00:40:08.090
There's all kinds of variation. But then all of a sudden,
810
00:40:08.150 --> 00:40:13.000
one of the detectors goes, boom, just like that. And
811
00:40:13.019 --> 00:40:16.099
then at the speed of light between one detector, which
812
00:40:16.139 --> 00:40:17.780
was in Louisiana, and the other one was in Oregon,
813
00:40:18.219 --> 00:40:21.989
The same pattern, wumba, wumba, wumba, boom, goes off. And
814
00:40:22.050 --> 00:40:25.610
it was absolutely unquestionable. It was the same pattern, the
815
00:40:25.650 --> 00:40:28.909
same frequency at the speed of light. Gravitational waves travel
816
00:40:28.929 --> 00:40:31.309
at the speed of light from one detector. And people
817
00:40:31.329 --> 00:40:32.260
were like, Nobel Prize.
818
00:40:32.340 --> 00:40:33.400
Yeah, that's fantastic.
819
00:40:33.639 --> 00:40:37.360
Oh, my God. But, I mean, let me just say,
820
00:40:37.380 --> 00:40:40.780
because I want to say what that event was. There
821
00:40:40.820 --> 00:40:46.039
were two black holes there. 1.4 billion light years away.
822
00:40:46.340 --> 00:40:49.940
This event happened 1.4 billion years ago. The black holes
823
00:40:49.980 --> 00:40:50.760
were both on the order.
824
00:40:50.780 --> 00:40:52.800
In another galaxy. In another galaxy.
825
00:40:52.929 --> 00:40:54.510
Yeah, it was way out of our galaxy.
826
00:40:54.530 --> 00:40:55.489
Far, far away, by the way.
827
00:40:56.369 --> 00:40:58.869
Yeah, far, far away. Yes.
828
00:40:58.909 --> 00:40:59.409
Thank you, Chuck.
829
00:41:00.989 --> 00:41:01.869
Those two black.
830
00:41:01.670 --> 00:41:03.369
Holes were both about- It's far, far away.
831
00:41:03.389 --> 00:41:06.530
It's far away. Yeah, yeah. 1.4 billion light years. Don't
832
00:41:06.550 --> 00:41:09.150
need to worry about it. Yeah, yeah. That's right. You know,
833
00:41:09.309 --> 00:41:11.280
there were two black holes that were roughly 30 times
834
00:41:11.320 --> 00:41:13.949
the mass of the sun apiece. We caught them in
835
00:41:14.030 --> 00:41:18.170
only the last two seconds, 0.2, two-tenths of a second
836
00:41:18.449 --> 00:41:20.909
of them spiraling together and merging into a bigger black hole.
837
00:41:21.719 --> 00:41:26.659
And in that 0.2 seconds, they accelerated from 30% the
838
00:41:26.699 --> 00:41:29.760
speed of light to 60% the speed of light. Black
839
00:41:29.780 --> 00:41:33.559
holes 30 times the mass of the sun. And about
840
00:41:33.699 --> 00:41:36.000
two times the mass of the sun was converted into
841
00:41:36.039 --> 00:41:42.159
pure energy. In 0.2 seconds. This is an unbelievable thing.
842
00:41:42.199 --> 00:41:45.280
It's real. That is a monster proportions that the human
843
00:41:45.320 --> 00:41:48.679
brain can't go any, I have no idea what that is.
844
00:41:49.300 --> 00:41:50.599
And it happened and we measured it.
845
00:41:51.099 --> 00:41:54.639
Michelle, wasn't that the most energetic event in the universe
846
00:41:54.739 --> 00:41:56.889
in that moment? I think it had to be.
847
00:41:56.929 --> 00:42:00.190
It was more energy than every star in every galaxy
848
00:42:00.250 --> 00:42:01.369
in the observable universe.
849
00:42:01.530 --> 00:42:01.909
Wow.
850
00:42:02.070 --> 00:42:04.489
Yeah. In that 0.2 seconds, right? In that 0.2 seconds.
851
00:42:06.949 --> 00:42:08.269
Jeez Louise.
852
00:42:08.670 --> 00:42:12.949
Okay, so tell us about, so if this happens with
853
00:42:13.010 --> 00:42:17.659
some frequency, no pun intended there, then two waves that
854
00:42:17.800 --> 00:42:21.219
do intersect, what can we say about them? Do they
855
00:42:22.159 --> 00:42:28.219
magnify any kind of gravitational disturbance in the space-time? What
856
00:42:28.260 --> 00:42:31.769
can we say about what is happening? Because when you
857
00:42:31.789 --> 00:42:35.469
drop two pebbles in a pond- you see interference patterns
858
00:42:35.530 --> 00:42:37.590
with the peak gets higher and the valleys get lower.
859
00:42:37.789 --> 00:42:42.329
So it exaggerates what's there. Presumably, we can expect just
860
00:42:42.389 --> 00:42:43.670
that same thing, can't we?
861
00:42:44.170 --> 00:42:45.449
Yeah, I think the answer is yes, but it's at
862
00:42:45.489 --> 00:42:50.250
a tiny, tiny, tiny scale. And also, I mean, this
863
00:42:50.269 --> 00:42:53.869
was a fantastic energetic event that the gravitational wave detector
864
00:42:53.889 --> 00:42:56.110
was able to detect this event. But there's also a
865
00:42:56.170 --> 00:42:59.929
background of gravitational waves, binary stars going around each other,
866
00:43:00.389 --> 00:43:02.889
all kinds of things. I'm actually making tiny little gravitational
867
00:43:02.929 --> 00:43:07.550
waves right now So, you know, again, we come to
868
00:43:07.610 --> 00:43:08.730
this idea of noise.
869
00:43:09.369 --> 00:43:11.869
Wait, you were making gravitational waves because you were lifting
870
00:43:11.889 --> 00:43:12.630
your hands up and down.
871
00:43:12.650 --> 00:43:15.849
A mass is moving. There's something moving. There's mass moving around.
872
00:43:15.869 --> 00:43:17.650
That's right. It's really, really small.
873
00:43:18.010 --> 00:43:20.429
It's not that you have special powers. You're just moving
874
00:43:20.449 --> 00:43:21.949
your body, just to be clear.
875
00:43:22.010 --> 00:43:23.679
Yeah.
876
00:43:23.699 --> 00:43:26.159
That'd be a great superpower, you know, making gravitational waves.
877
00:43:26.179 --> 00:43:28.579
But anyway, yeah. So the answer, I think, is yes.
878
00:43:29.000 --> 00:43:32.300
But I don't think there's going to be any organized
879
00:43:33.320 --> 00:43:36.489
effect of that. Because there's just, I mean, think about
880
00:43:37.289 --> 00:43:40.269
waves on a giant lake, a giant ocean. There's ripples
881
00:43:40.309 --> 00:43:43.969
going every which way. And yes, they are interfering when
882
00:43:44.170 --> 00:43:48.269
they add together or they can, I think all that's happening.
883
00:43:49.110 --> 00:43:51.380
But I don't think that has any measurable effect on
884
00:43:51.420 --> 00:43:53.960
what's going on in the universe. It's tiny.
885
00:43:54.039 --> 00:43:57.659
So in Tristan's question, it was, would it be able
886
00:43:57.760 --> 00:44:00.780
to perhaps give the appearance of a celestial body being
887
00:44:00.820 --> 00:44:03.110
there when none is there because of the, Curbature of
888
00:44:03.190 --> 00:44:06.760
space-time itself and you're saying that that's not gonna happen.
889
00:44:07.030 --> 00:44:10.719
Okay, cool The energetics are too small. So just to
890
00:44:10.760 --> 00:44:15.219
be clear it gave off more energy Than all stars
891
00:44:15.280 --> 00:44:18.139
combined in the universe over those point two seconds, but
892
00:44:18.159 --> 00:44:21.719
then that energy in the form of gravitational waves moved
893
00:44:23.380 --> 00:44:24.980
How many billions of miles to reach.
894
00:44:24.900 --> 00:44:26.880
Us 1.4 billion light 1.4 billion much so.
895
00:44:26.780 --> 00:44:32.769
It's been diluted over that distance and to the low
896
00:44:32.889 --> 00:44:37.260
energies that were ultimately detected in LIGO, right? I mean,
897
00:44:37.280 --> 00:44:41.619
just think of the volume. Because anybody at this distance
898
00:44:41.920 --> 00:44:45.170
in any direction from those colliding black holes could make
899
00:44:45.210 --> 00:44:49.650
this measure. So that energy is expanding through the entire
900
00:44:49.730 --> 00:44:52.099
universe and we're just catching our one little piece of it.
901
00:44:52.630 --> 00:44:55.019
What was that event like? I mean, because if you're
902
00:44:55.059 --> 00:44:58.730
close to that event, I mean, that must have ripped
903
00:44:58.789 --> 00:45:03.190
apart any matter within quite a large distance. I mean,
904
00:45:03.210 --> 00:45:06.250
I'm sure we could have somebody do the math on that. So,
905
00:45:06.610 --> 00:45:10.150
I mean, I don't think there would be, it can't
906
00:45:10.349 --> 00:45:11.989
make it seem like there's a star there. This is
907
00:45:12.030 --> 00:45:13.289
not a solution for dark matter.
908
00:45:13.329 --> 00:45:13.670
Sorry.
909
00:45:14.090 --> 00:45:15.690
It's not a good thing. Nope, that's.
910
00:45:17.489 --> 00:45:17.809
Lame.
911
00:45:20.929 --> 00:45:21.230
Ready?
912
00:45:21.750 --> 00:45:26.949
Do you harbor questions about the universe? Some long-held Bit
913
00:45:26.989 --> 00:45:32.420
of cosmic curiosity lingering within you or questions about anything
914
00:45:33.440 --> 00:45:38.019
at all. You can become a Patreon
supporter of StarTalk.
915
00:45:38.719 --> 00:45:41.659
You have access to our exclusive question line on our website.
916
00:45:42.500 --> 00:45:45.420
Those are where we draw our questions for our cosmic.
917
00:45:45.949 --> 00:45:49.869
Some of the most extreme objects in the universe. StarTalk
918
00:45:49.929 --> 00:45:54.289
is a work in progress where we... Every month, come
919
00:45:54.329 --> 00:45:57.130
up with some new way, some new idea, some new
920
00:45:57.250 --> 00:46:00.699
understanding of how to bring the universe down to earth.
921
00:46:01.400 --> 00:46:03.579
We could not do that without your support.
922
00:46:04.460 --> 00:46:07.260
Thank you. And as always, keep looking up.
923
00:46:08.670 --> 00:46:12.190
This is Rachel Ambrose who says, Rachel here from Texas.
924
00:46:12.650 --> 00:46:16.199
I loved Michelle's Big Think interview. It was the first
925
00:46:16.260 --> 00:46:19.840
time I heard someone articulate the profound weirdness of reality
926
00:46:20.179 --> 00:46:24.500
in a way that completely resonated with how I have
927
00:46:24.679 --> 00:46:28.559
always felt but could never adequately explain. And I just
928
00:46:28.800 --> 00:46:33.030
appreciated that so much. Thank you, Michelle. My question is
929
00:46:33.090 --> 00:46:38.010
about neutron stars. I am confused why the high-energy fast
930
00:46:38.070 --> 00:46:42.150
radio bursts, the FRBs, come to us in the form
931
00:46:42.230 --> 00:46:47.909
of low-energy radio frequencies rather than X-rays or gamma rays.
932
00:46:48.349 --> 00:46:53.769
What mechanism causes such a high-energy event to manifest as
933
00:46:53.949 --> 00:46:55.130
radio light?
934
00:46:55.389 --> 00:46:56.789
Ooh.
935
00:46:56.849 --> 00:46:59.570
So this has built in the knowledge that radio waves
936
00:46:59.650 --> 00:47:00.829
are lower-energy light.
937
00:47:00.909 --> 00:47:01.150
Energy.
938
00:47:01.480 --> 00:47:04.530
Then X-rays or gamma rays. And if it's a high
939
00:47:04.590 --> 00:47:08.550
energy phenomenon, why is it wasting itself with radio waves?
940
00:47:08.670 --> 00:47:14.969
So Michelle, you answer that one, Michelle. Yeah, right.
941
00:47:15.550 --> 00:47:16.010
Okay.
942
00:47:16.090 --> 00:47:18.369
So yeah, I at least know a little bit about that.
943
00:47:18.389 --> 00:47:19.829
I mean, as I said, I mean, one of the
944
00:47:19.869 --> 00:47:23.610
missions I absolutely adore is called NICER, the Neutron Star
945
00:47:23.650 --> 00:47:26.199
Interior Composition Explorer. It's on the space station. It's a
946
00:47:26.219 --> 00:47:30.510
Goddard-run mission. Fantastic. It's about the size of a washing machine. Again,
947
00:47:30.590 --> 00:47:35.050
not an expensive mission. And it's able to actually get
948
00:47:35.429 --> 00:47:38.250
X-rays in this case, X-rays from neutron stars. And it
949
00:47:38.329 --> 00:47:41.510
times the arrival of the X-rays so precisely, we can
950
00:47:41.530 --> 00:47:43.489
make a map of what the surface of a neutron
951
00:47:43.530 --> 00:47:46.550
star is like. They're tiny. Neutron stars are only about
952
00:47:46.550 --> 00:47:50.030
20 miles across. They usually have about twice the mass
953
00:47:50.070 --> 00:47:55.119
of the sun. packed into 20 miles. These are extreme things,
954
00:47:55.179 --> 00:47:57.280
and they're real. I mean, we studied many of these.
955
00:47:58.099 --> 00:48:01.199
And they're so incredible. When you do a map of these,
956
00:48:01.260 --> 00:48:04.530
and they often are rotating very fast, you actually get
957
00:48:04.550 --> 00:48:08.369
this strange effect on the side of the map because
958
00:48:08.530 --> 00:48:12.070
light is bending around. There's so much mass. The curvature
959
00:48:12.090 --> 00:48:15.590
of space and time is so extreme. Two solar masses
960
00:48:15.650 --> 00:48:18.750
packed into 20 miles. that you actually can see behind
961
00:48:18.829 --> 00:48:20.710
a neutron star as well as in front, the light
962
00:48:20.769 --> 00:48:25.369
curves around it. And so, I mean, what an incredible
963
00:48:25.710 --> 00:48:27.030
real monster.
964
00:48:27.610 --> 00:48:29.949
So what you're saying is it has many properties that
965
00:48:29.989 --> 00:48:32.730
we would find with black holes in its distortion of
966
00:48:32.750 --> 00:48:35.510
the fabric of space and time. in their vicinity.
967
00:48:35.550 --> 00:48:37.610
In fact, the neutron star group at Goddard said that
968
00:48:37.650 --> 00:48:40.030
neutron stars are far more interesting than black holes because
969
00:48:40.070 --> 00:48:42.610
with black holes, you have this dark event horizon that
970
00:48:42.690 --> 00:48:44.590
nothing ever comes out of. You don't know what's going
971
00:48:44.650 --> 00:48:46.699
on in there. With neutron stars, you got the fricking
972
00:48:46.739 --> 00:48:47.659
thing right in front of you.
973
00:48:47.960 --> 00:48:48.400
It's very bright.
974
00:48:48.420 --> 00:48:50.679
It's still here with us.
975
00:48:50.860 --> 00:48:55.340
And you can study something that has such extreme conditions
976
00:48:55.719 --> 00:48:58.179
that there's no laboratory on earth we can even study
977
00:48:58.219 --> 00:49:00.650
what matter is like under these conditions. It's amazing.
978
00:49:00.949 --> 00:49:01.210
Wow.
979
00:49:02.010 --> 00:49:03.889
But yeah, OK, so going back to why it's radio waves,
980
00:49:04.389 --> 00:49:08.110
neutron stars definitely do emit high energy radiation. They're actually
981
00:49:08.130 --> 00:49:10.489
the source of what we think are gamma ray bursts,
982
00:49:10.650 --> 00:49:14.289
dangerous blasts of high energy radiation. We're using an X-ray
983
00:49:14.309 --> 00:49:17.329
telescope to observe these things. The surface of a neutron
984
00:49:17.349 --> 00:49:20.820
star is very hot. It definitely does. generate these high
985
00:49:20.840 --> 00:49:24.739
energy things. The way you get radio waves is something, Neil,
986
00:49:24.760 --> 00:49:26.320
I'm sure it's a favorite of yours too. It's a
987
00:49:26.360 --> 00:49:31.639
lovely thing called synchrotron radiation. And would you like to
988
00:49:31.659 --> 00:49:33.340
go ahead and talk about synchrotron radiation?
989
00:49:33.579 --> 00:49:36.909
Oh, as I understood it. No, as I understand it,
990
00:49:38.239 --> 00:49:40.940
The neutron star has to be magnetic, has to have
991
00:49:40.980 --> 00:49:42.039
a magnetic field.
992
00:49:42.059 --> 00:49:42.500
That's right.
993
00:49:42.900 --> 00:49:47.780
And as it rotates, it can accelerate electrons that are
994
00:49:48.280 --> 00:49:52.820
ambient in the environment. And you can accelerate electrons off
995
00:49:52.840 --> 00:49:57.809
of a magnetic field that will radiate radio waves. Yes.
996
00:49:57.829 --> 00:50:00.650
We call it synchrotron radiation. I think I accounted for
997
00:50:00.670 --> 00:50:01.630
that correctly. Is that correct?
998
00:50:02.250 --> 00:50:05.050
Yeah, I mean, the one thing that's perhaps something to
999
00:50:05.230 --> 00:50:07.369
mention about synchrotron radiation, I mean, so you've got a
1000
00:50:07.389 --> 00:50:09.510
couple of things going on. I mean, you also have,
1001
00:50:10.269 --> 00:50:12.949
you know, electrons are charged particles. They respond to a
1002
00:50:12.969 --> 00:50:16.630
magnetic field. They can actually be accelerated. Neutron stars have jets.
1003
00:50:17.750 --> 00:50:21.909
We see those as well. Also, when you get synchrotron
1004
00:50:21.969 --> 00:50:25.429
radiation happens largely when electrons spirals around a magnetic field.
1005
00:50:26.750 --> 00:50:28.889
Just by the act of spinning around, that's a form
1006
00:50:28.909 --> 00:50:29.250
of acceleration.
1007
00:50:29.269 --> 00:50:33.480
That's what it was. It creates its own frequency, spiral
1008
00:50:33.539 --> 00:50:36.960
frequency that is the radio wave. So what's fun about
1009
00:50:37.219 --> 00:50:42.000
the neutron star, just to summarize that, is different processes
1010
00:50:42.079 --> 00:50:45.260
within the environment of a neutron star give you different
1011
00:50:45.719 --> 00:50:49.019
bands of light that our different telescopes can participate in,
1012
00:50:49.449 --> 00:50:51.289
which is kind of fun. And then you can compare notes.
1013
00:50:51.940 --> 00:50:53.159
across different wavelengths of light.
1014
00:50:53.199 --> 00:50:55.380
And this is why astronomers just aren't greedy. It's like, oh,
1015
00:50:55.400 --> 00:50:58.000
we need a radio telescope and an infrared telescope and
1016
00:50:58.019 --> 00:51:01.489
an X-ray telescope and a visible light telescope. But you're
1017
00:51:01.570 --> 00:51:05.809
absolutely true. You see totally different things in these different
1018
00:51:05.829 --> 00:51:08.869
wavelengths of light. And so as high energy and dramatic
1019
00:51:09.010 --> 00:51:12.139
objects neutron stars are, you better believe they are. There
1020
00:51:12.159 --> 00:51:17.420
was one in, God, was it 2007? There was an
1021
00:51:17.460 --> 00:51:20.260
event that actually blew off a measurable amount of our atmosphere.
1022
00:51:20.909 --> 00:51:23.710
And the whole magnetic field of the Earth was ringing
1023
00:51:23.730 --> 00:51:24.610
like a bell for a while.
1024
00:51:24.929 --> 00:51:26.949
Now you're telling us this?
1025
00:51:27.469 --> 00:51:31.369
Look this up. This is all real. And we traced
1026
00:51:31.409 --> 00:51:33.090
it back to a neutron star that we think is
1027
00:51:33.130 --> 00:51:35.530
about 50,000 light years away. The neutron star had a
1028
00:51:35.539 --> 00:51:37.820
little bit of a bad day. The crust, we think,
1029
00:51:37.840 --> 00:51:41.199
shifted by about a centimeter. And that gave off so
1030
00:51:41.239 --> 00:51:44.679
much energy that 50,000 light years away, it blew off
1031
00:51:44.699 --> 00:51:45.639
a bunch of our atmosphere.
1032
00:51:45.860 --> 00:51:46.199
Oh, my.
1033
00:51:46.880 --> 00:51:48.559
These are intense things.
1034
00:51:49.000 --> 00:51:51.980
Michelle, I'm going to be honest. I could have lived
1035
00:51:52.019 --> 00:51:53.199
without that information.
1036
00:51:53.219 --> 00:51:55.739
Yeah, I know. It keeps you up at night, doesn't it?
1037
00:51:55.920 --> 00:51:58.969
It's great. I mean, who cares about asteroids, right?
1038
00:51:59.030 --> 00:52:02.969
I mean, killer asteroids. No, I mean, these blasts of
1039
00:52:03.030 --> 00:52:06.309
high-energy radiation from neutron stars, some people think that may
1040
00:52:06.369 --> 00:52:08.909
limit the age of civilizations in the galaxy. Eventually, we
1041
00:52:08.929 --> 00:52:09.610
all get hit by one.
1042
00:52:09.969 --> 00:52:13.840
Wow. Another great question. Thank you, Rachel. All right. This
1043
00:52:13.889 --> 00:52:17.460
is Brett. And Brett says, hi, Dr. Tyson, Dr. Thaler,
1044
00:52:17.500 --> 00:52:23.889
Lord Nice. Tuning in from Denver. Dublin, Ireland, my question is,
1045
00:52:24.949 --> 00:52:33.260
what unlikely possibility or possibilities do you hope are true?
1046
00:52:33.280 --> 00:52:33.349
Ooh.
1047
00:52:37.559 --> 00:52:44.260
That's father for good thought. It is. An unlikely possibility
1048
00:52:44.949 --> 00:52:47.610
that you're like, oh, man, that'd be so great if
1049
00:52:47.670 --> 00:52:48.449
that were true.
1050
00:52:50.119 --> 00:52:50.639
Yeah.
1051
00:52:50.920 --> 00:52:54.000
So, boy, that can go in so many different directions.
1052
00:52:54.039 --> 00:52:55.980
Because, I mean, I've got, I mean, one of the
1053
00:52:56.000 --> 00:52:58.139
things I- What a great question, Brett. Look at you.
1054
00:52:58.159 --> 00:53:00.650
I can lead off. I got one for you, Michelle. Okay.
1055
00:53:00.690 --> 00:53:01.190
I got one too.
1056
00:53:01.230 --> 00:53:01.570
You go ahead.
1057
00:53:01.630 --> 00:53:02.389
I think I got it.
1058
00:53:02.409 --> 00:53:02.570
Yeah.
1059
00:53:02.849 -->
00:53:06.750
I think it's unlikely that we'll find anything other than
1060
00:53:06.849 --> 00:53:10.309
microbial life on Mars if we find life at all.
1061
00:53:11.230 --> 00:53:14.190
But it would be really cool if we found sort
1062
00:53:14.210 --> 00:53:19.019
of macroscopic crawly things. living in the subsurface of Mars.
1063
00:53:19.239 --> 00:53:22.179
I think that's unlikely, but that would be really cool
1064
00:53:22.780 --> 00:53:24.980
if creatures crawled out from home.
1065
00:53:25.400 --> 00:53:28.179
Would you still be satisfied if those macroscopic crawly things
1066
00:53:28.300 --> 00:53:31.179
were fossilized in some way, but they're no longer there?
1067
00:53:31.239 --> 00:53:34.079
No, no, no. We're talking about unlikely things that we
1068
00:53:34.099 --> 00:53:37.619
want to happen. Let the thing crawl out and, and
1069
00:53:37.800 --> 00:53:41.500
ride one of the rovers like a, like a, like a, you.
1070
00:53:40.949 --> 00:53:42.909
Know, like, like what do you call those horses?
1071
00:53:43.469 --> 00:53:48.500
Those, Buck and Bronco.
1072
00:53:48.619 --> 00:53:51.780
Yeah, Buck and Bronco. I want to come out and
1073
00:53:51.820 --> 00:53:57.719
ride one of our rovers. Unlikely, but it'd be really
1074
00:53:57.739 --> 00:54:00.400
cool if it was true. So now your turn, Michelle.
1075
00:54:01.039 --> 00:54:02.679
So just riffing on that, do you think it might
1076
00:54:02.699 --> 00:54:04.789
be more likely to find macroscopic life on the moons
1077
00:54:04.829 --> 00:54:07.849
of Jupiter and Saturn in the oceans? You know, Europa
1078
00:54:07.889 --> 00:54:08.610
and Saladus?
1079
00:54:08.690 --> 00:54:11.969
We're talking about unlikely things that we want to happen. Oh,
1080
00:54:11.989 --> 00:54:13.050
you think that's a likely thing?
1081
00:54:13.110 --> 00:54:13.980
Okay, all right, got it.
1082
00:54:14.010 --> 00:54:14.630
Yeah, yeah.
1083
00:54:14.789 --> 00:54:15.670
Unlikely things.
1084
00:54:16.199 --> 00:54:18.079
Yeah, there could be like little brine shrimp and stuff.
1085
00:54:19.280 --> 00:54:20.340
Yeah.
1086
00:54:20.360 --> 00:54:23.699
One of my big excitements right now with the Webb
1087
00:54:23.719 --> 00:54:26.980
telescope is it's looking so far away that we're looking
1088
00:54:27.019 --> 00:54:30.579
back to a time roughly, like, let's say about 300
1089
00:54:30.579 --> 00:54:33.000
million years after the Big Bang. And we're actually seeing
1090
00:54:33.019 --> 00:54:39.860
the very first stars form. And they're absolutely different. I mean,
1091
00:54:39.900 --> 00:54:42.000
we haven't actually found, you know, one of these first
1092
00:54:42.019 --> 00:54:46.489
stars yet. I really want to find... first generation star.
1093
00:54:46.670 --> 00:54:48.409
We're going to be looking back to a time, just
1094
00:54:48.429 --> 00:54:49.889
like I said, a couple hundred million years after the
1095
00:54:49.909 --> 00:54:52.849
Big Bang when stars started to form. Webb can now
1096
00:54:53.369 --> 00:54:56.050
see that far back. We have that power. And we're
1097
00:54:56.070 --> 00:54:59.750
starting to see these pseudo stars that are formed around
1098
00:54:59.809 --> 00:55:02.070
black holes. They're about a million times the mass of
1099
00:55:02.090 --> 00:55:06.500
the sun, relatively small. I mean, these things may become
1100
00:55:06.539 --> 00:55:08.559
the seeds of the big black holes that are in
1101
00:55:08.579 --> 00:55:11.360
the centers of all galaxies. We're starting to see that
1102
00:55:11.460 --> 00:55:14.380
forming now. And my question, I mean, I was a
1103
00:55:14.440 --> 00:55:17.280
stellar astrophysicist. I was a stellar astrophysicist.
1104
00:55:17.320 --> 00:55:18.219
I studied stars.
1105
00:55:18.260 --> 00:55:18.900
That was my thing.
1106
00:55:19.440 --> 00:55:21.519
Outstanding in your field.
1107
00:55:21.760 --> 00:55:24.659
Not outstanding, but that's what I studied. And I would
1108
00:55:24.719 --> 00:55:26.679
love to see what one of the first generation stars
1109
00:55:26.719 --> 00:55:29.530
looks like. Because my guess is it's going to look
1110
00:55:29.590 --> 00:55:33.289
totally different. That the universe was more dense back then.
1111
00:55:33.329 --> 00:55:36.789
There was more dark matter prevalent. I mean, dark matter
1112
00:55:36.809 --> 00:55:38.969
has gravity. That's going to get sucked into the formation
1113
00:55:38.989 --> 00:55:42.110
of a star just from gravity too. What was that
1114
00:55:42.269 --> 00:55:44.690
first generation of stars like? My guess is they're going
1115
00:55:44.710 --> 00:55:48.579
to be huge, many, many times the mass of the sun, many,
1116
00:55:48.619 --> 00:55:51.360
many times bigger than the most massive stars we have today.
1117
00:55:52.219 --> 00:55:54.300
And I'm wondering if they're going to work really differently
1118
00:55:54.320 --> 00:55:55.719
because there's more dark matter.
1119
00:55:57.860 --> 00:55:58.179
In them.
1120
00:55:58.260 --> 00:55:58.519
Okay.
1121
00:55:58.590 --> 00:56:01.590
Interesting. I want to see that first generation of stars.
1122
00:56:02.110 --> 00:56:06.730
And just to be clear, James Webb was specifically designed
1123
00:56:06.769 --> 00:56:11.329
and tuned for that exercise. to see the beginnings of
1124
00:56:12.090 --> 00:56:14.949
the formation of matter in the early universe. So you're
1125
00:56:14.969 --> 00:56:16.670
betting on the right horse there, I think.
1126
00:56:17.349 --> 00:56:19.349
Yeah, we're doing it. I mean, these things, I mean,
1127
00:56:19.369 --> 00:56:21.590
never let astronomers name anything. These things are called little
1128
00:56:21.650 --> 00:56:26.619
red dots. Ha ha, yeah. They're massive pseudo stars around
1129
00:56:26.639 --> 00:56:28.780
a giant black hole at the beginning of the universe
1130
00:56:28.800 --> 00:56:30.099
that we're calling little red dots.
1131
00:56:30.440 --> 00:56:33.380
Because they look like little
red dots. Little red dots, yeah.
1132
00:56:33.400 --> 00:56:36.900
But they're so far away. Yeah, that's one of my favorites.
1133
00:56:37.400 --> 00:56:38.800
Chuck, time for like two more questions.
1134
00:56:39.429 --> 00:56:40.409
All right, here we go.
1135
00:56:40.429 --> 00:56:44.590
But only if Michelle is efficient in her answers.
1136
00:56:46.170 --> 00:56:46.969
I promise to be efficient.
1137
00:56:48.329 --> 00:56:49.530
You're unnoticed.
1138
00:56:49.650 --> 00:56:52.159
You don't have to promise anything, Michelle. It's going to
1139
00:56:52.179 --> 00:56:57.400
do what you want. This is Alyssa Feldhaus who says, hello,
1140
00:56:57.659 --> 00:57:05.039
Fowler the Great. This is Alyssa Feldhaus tuning in from Hendersonville, Tennessee.
1141
00:57:06.159 --> 00:57:09.280
As such a prominent female figure in the science world,
1142
00:57:09.840 --> 00:57:13.519
what message can you give all the little girls out
1143
00:57:13.599 --> 00:57:18.260
there that will one day stand on our shoulders? Me
1144
00:57:18.320 --> 00:57:22.090
and my girls love how the universe works. And thank
1145
00:57:22.130 --> 00:57:25.230
you for keeping science cool.
1146
00:57:28.050 --> 00:57:29.670
Oh, I always think of myself as so nerdy. I
1147
00:57:29.949 --> 00:57:33.349
never think about cool. Okay, so a message I always have.
1148
00:57:33.369 --> 00:57:35.150
The nerdy is the new cool. Nerdy is the new cool.
1149
00:57:35.170 --> 00:57:37.590
Nerdy is the new cool, absolutely, yeah. I guess a
1150
00:57:37.639 --> 00:57:41.059
message I already have is you're already the right type
1151
00:57:41.079 --> 00:57:43.460
of person to be a scientist. Math and physics did
1152
00:57:43.500 --> 00:57:45.880
not come quickly to me. I didn't get particularly good
1153
00:57:45.920 --> 00:57:47.980
grades in school in math and physics. It took me
1154
00:57:48.019 --> 00:57:52.199
some time. I just loved it so much. You know,
1155
00:57:52.219 --> 00:57:55.409
paying attention to your own curiosity and not being discouraged
1156
00:57:55.449 --> 00:57:58.230
when maybe you don't get something very, very quickly. You're
1157
00:57:58.289 --> 00:58:01.579
already enough. You're already there. For so long, I wondered,
1158
00:58:01.599 --> 00:58:03.139
you know, do I have what it takes to be
1159
00:58:03.159 --> 00:58:05.820
an astrophysicist? I love this, but maybe I just don't
1160
00:58:05.960 --> 00:58:10.349
have the magic thing, the right stuff. And science doesn't
1161
00:58:10.449 --> 00:58:12.889
work that way. If you want to study it, you
1162
00:58:12.909 --> 00:58:15.170
can study it. It's like learning a language. You know,
1163
00:58:15.190 --> 00:58:18.630
it takes a while to become fluent in a different language.
1164
00:58:19.210 --> 00:58:20.909
You don't really go up to a young person and say,
1165
00:58:20.969 --> 00:58:24.800
you could never learn Spanish, even if you tried. You know, no, no.
1166
00:58:25.079 --> 00:58:27.960
I
mean, science is a beautiful thing to study. It
1167
00:58:28.019 --> 00:58:31.389
takes time. And anyone can learn it if they're interested
1168
00:58:31.409 --> 00:58:34.989
in it and have that passion more than any innate
1169
00:58:35.369 --> 00:58:39.090
ability and talent to get all of this very quickly. So,
1170
00:58:39.250 --> 00:58:41.349
you know, I spent way too much time thinking maybe
1171
00:58:41.389 --> 00:58:45.269
I'm not the right personality. I'm not smart enough. And
1172
00:58:45.630 --> 00:58:50.699
it's a cultural, you know, bullshit that science requires a
1173
00:58:50.880 --> 00:58:56.619
certain type of brilliant, different person. So, you know, you're enough. And,
1174
00:58:56.639 --> 00:58:59.889
you know, you're going to be the best scientist from
1175
00:59:00.050 --> 00:59:03.010
your perspective, right? I mean, we're all people have different
1176
00:59:03.050 --> 00:59:05.489
science talents. Some people are better at the math. Some
1177
00:59:05.510 --> 00:59:07.969
people see the larger concepts. Some people are really good
1178
00:59:07.989 --> 00:59:10.639
at communicating it. These are all really important. steps and
1179
00:59:10.659 --> 00:59:13.820
you can find that part that you fit into. So
1180
00:59:14.039 --> 00:59:16.179
you don't have to be anything other than just the
1181
00:59:16.199 --> 00:59:16.760
way you are.
1182
00:59:17.239 --> 00:59:17.579
Wow.
1183
00:59:17.639 --> 00:59:19.500
I love it. I love it.
1184
00:59:19.719 --> 00:59:23.760
And if I can add, not having ever been female,
1185
00:59:24.159 --> 00:59:27.500
but being a black man in the world, there are
1186
00:59:27.579 --> 00:59:32.679
resonant challenges that we face entering a world that role
1187
00:59:32.719 --> 00:59:37.670
models are not there. So I would just add that
1188
00:59:37.829 --> 00:59:40.250
there are always people who will learn something faster than
1189
00:59:40.289 --> 00:59:43.889
you will. And the school system tends to reward that
1190
00:59:44.469 --> 00:59:47.090
and call those people smart and they might get a
1191
00:59:47.130 --> 00:59:51.510
higher grade. But in the end, that's not what matters.
1192
00:59:51.550 --> 00:59:55.150
What matters is your motivation to ultimately learn what you
1193
00:59:55.170 --> 00:59:57.349
need to learn. If it takes you longer to learn it,
1194
00:59:58.469 --> 01:00:00.900
longer than the time before you're tested on it. It
1195
01:00:01.119 --> 01:00:03.179
takes you a little longer. So what? It took you
1196
01:00:03.219 --> 01:00:05.719
a little longer. If you get there and your ambition
1197
01:00:05.739 --> 01:00:09.820
takes you and your interest, then ultimately that's what will
1198
01:00:09.860 --> 01:00:12.980
dominate who and what you are as a participant on
1199
01:00:13.019 --> 01:00:17.110
the research frontier, not how quickly you learn a problem
1200
01:00:17.150 --> 01:00:20.389
set on an exam in high school or in college.
1201
01:00:21.010 --> 01:00:25.050
So ambition is something that tests hardly ever test for.
1202
01:00:26.050 --> 01:00:27.789
And that's what you need. And that's what you need
1203
01:00:27.829 --> 01:00:29.190
confidence in. Yeah.
1204
01:00:29.610 --> 01:00:31.099
And just being able to stick to something.
1205
01:00:31.760 --> 01:00:32.039
Yeah.
1206
01:00:32.239 --> 01:00:34.380
And just having the grit. I mean, when I got
1207
01:00:34.420 --> 01:00:36.860
to college, I got placed in remedial math. I mean,
1208
01:00:36.920 --> 01:00:38.780
I came from a public school system that didn't have
1209
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a whole lot of math. And I knew I could
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not get space out of my head. I was so
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fascinated by it. And I am so glad I stuck
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in when I was thinking, geez, I just don't have
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the talent for this.
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And that became the driver, your source of energy to
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pursue it. And I like your language analogy because no
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one will ever say, oh, you're not smart enough to
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learn Spanish. No one will ever say that. They just say,
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are you committed enough to learn Spanish? And you learn
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a little bit today and a little bit next week
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and next month. And eventually you wake up and you're
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just talking fluent Spanish, you know, and everyone can learn it.
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And I think that's also true with math. As a
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language of the universe. Yes.
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01:01:25.340 --> 01:01:28.849
Well, let me add, Alyssa, that as a product of
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Philadelphia public schools, there's always comedy.
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01:01:42.489 --> 01:01:47.170
All right. So, Chuck, we only actually had time for
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that one last question, but that was a really good
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one to end this episode on. So, Michelle, thank you
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for being a guest on StarTalk.
1230
01:01:56.000 --> 01:01:57.679
Hey, I'm always here.
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Where are you based right now?
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Right now I'm in Milwaukee, Wisconsin.
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01:02:02.510 --> 01:02:03.789
Whoa, is that where you're based?
1234
01:02:04.389 --> 01:02:05.050
Yes, yes.
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Cool, cool. Okay. Well, we will make sure to find
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you again because you're a delight to share in our
1237
01:02:12.659 --> 01:02:15.780
answers here and to get your perspectives on the state
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of science in America and in the universe.
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All right.
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Chuck, always good to have you, man.
1241
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Always a pleasure.
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These are fan favorites, these Cosmic Queries. And we delight
1243
01:02:28.500 --> 01:02:32.559
in the questions that we receive. And keep them coming.
1244
01:02:33.000 --> 01:02:36.019
But you have to be a member of the Patreon
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01:02:36.059 --> 01:02:36.980
community first.
1246
01:02:37.980 --> 01:02:42.630
Yes, but it's only $ 5. That's it. $ 5 a month.
1247
01:02:43.329 --> 01:02:46.809
And I got to tell you, that's less than what
1248
01:02:47.510 --> 01:02:49.650
the budget of NASA is. Yes.
1249
01:02:55.780 --> 01:03:00.590
All right. I'm Neil deGrasse Tyson, your personal astrophysicist. As always,
1250
01:03:00.610 --> 01:03:02.630
I bid you to keep looking up.