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Alex Filippenko: Supernovae, Dark Energy, Aliens & the Expanding Universe | Lex Fridman Podcast #137


small model | large model

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The following is a conversation with Alex Filipenko, an astrophysicist and professor
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of astronomy from Berkeley.
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He was a member of both the Supernova Cosmology Project and the HiZ Supernova Search Team
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which used observations of the extragalactic supernova to discover that the universe is
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accelerating and that this implies the existence of dark energy.
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This discovery resulted in the 2011 NOVA Prize for Physics.
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Outside of his groundbreaking research, he is a great science communicator and is one
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of the most widely admired educators in the world.
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I really enjoyed this conversation and am sure Alex will be back again in the future.
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Quick mention of each sponsor, followed by some thoughts related to the episode.
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Neuro, the maker of functional, sugar free gum and mints that I used to give my brain
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a quick caffeine boost.
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BetterHelp, an online therapy with a licensed professional, Masterclass, online courses
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that I enjoy from some of the most amazing humans in history, and CashApp, the app I
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use to send money to friends.
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Please check out these sponsors in the description to get a discount and to support this podcast.
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As a side note, let me say that as we talk about in this conversation, the objects that
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populate the universe are both awe inspiring and terrifying in their capacity to create
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and to destroy us.
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Solar flares and asteroids lurking in the darkness of space threaten our humble, fragile
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existence here on Earth.
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In the chaos, tension, conflict, and social division of 2020, it's easy to forget just
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how lucky we humans are to be here, and with a bit of hard work, maybe one day, we'll
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venture out towards the stars.
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If you enjoy this thing, subscribe on YouTube, review it with Five Stars on Apple Podcast,
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follow on Spotify, support on Patreon, or connect with me on Twitter at Lex Friedman.
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And now, here's my conversation with Alex Filipenko.
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Let's start by talking about the biggest possible thing, the universe.
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Will the universe expand forever or collapse on itself?
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Well, you know, that's a great question.
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It's one of the big questions of cosmology, and of course, we have evidence that the matter
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density is sufficiently low that the universe will expand forever.
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But not only that, there's this weird repulsive effect, we call it dark energy for want of
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a better term, and it appears to be accelerating the expansion of the universe.
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So if that continues, the universe will expand forever, but it need not necessarily continue.
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It could reverse sign, in which case the universe could, in principle, collapse at some point
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in the far, far future.
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So in terms of investment advice, if you were to give me and then to bet all my money on
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one or the other, where does your intuition currently lie?
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Well, right now, I would say that it would expand forever because I think that the dark
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energy is likely to be just quantum fluctuations of the vacuum.
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The vacuum zero energy state is not a state of zero energy.
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That is, the ground state is a state of some elevated energy which has a repulsive effect
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to it.
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And that will never go away because it's not something that changes with time.
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So if the universe is accelerating now, it will forever continue to do so.
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And yet, I mean, you so effortlessly mentioned dark energy.
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Do we have any understanding of what the heck that thing is?
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Well, not really.
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But we're getting progressively better observational constraints.
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So different theories of what it might be predict different sorts of behavior for the
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evolution of the universe.
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And we've been measuring the evolution of the universe now.
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And the data appear to agree with the predictions of a constant density vacuum energy, a zero
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point energy.
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But one can't prove that that's what it is because one would have to show that the measured
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numbers agree with the predictions to an arbitrary number of decimal places.
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And of course, even if you've got 8, 9, 10, 12 decimal places, what if in the 13th one,
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the measurements significantly differ from the prediction?
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Then the dark energy isn't this vacuum state, ground state energy of the vacuum.
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And so then it could be some sort of a field, some sort of a new energy, a little bit like
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light, like electromagnetism, but very different from light, that fills space.
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And that type of energy could in principle change in the distant future.
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It could become gravitationally attractive for all we know.
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There is a historical precedent to that, and that is that the inflation with which the
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universe began when the universe was just a tiny blink of an eye old, a trillionth of
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a trillionth of a trillionth of a second, the universe went whoosh, it exponentially
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expanded.
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That dark energy like substance, we call it the inflaton, that which inflated the universe,
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later decayed into more or less normal gravitationally attractive matter.
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So the exponential early expansion of the universe did transition to a deceleration,
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which then dominated the universe for about nine billion years.
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And now this small amount of dark energy started causing an acceleration about five billion
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years ago.
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And whether that will continue or not is something that we'd like to answer, but I don't know
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that we will anytime soon.
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So there could be this interesting field that we don't yet understand that's morphing over
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time, that's changing the way the universe is expanding.
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I mean, it's funny that you were thinking through this rigorously like an experimentalist.
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But what about like the fundamental physics of dark energy?
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Is there any understanding of what the heck it is, or is this the kind of the god of the
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gaps or the field of the gaps?
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So like there must be something there because of what we're observing.
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I'm very much a person who believes that there's always a cause, you know, there are no miracles
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of a supernatural nature, okay?
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So I mean, there are two broad categories, either it's the vacuum zero point energy,
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or it's some sort of a new energy field that pervades the universe.
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The latter could change with time, the former, the vacuum energy cannot.
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So if it turns out that it's one of these new fields, and there are many, many possibilities,
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they go by the name of quintessence and things like that, but there are many categories of
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those sorts of fields, we try with data to rule them out by comparing the actual measurements
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with the predictions.
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And some have been ruled out, but many, many others remain to be tested.
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And the data just have to become a lot better before we can rule out most of them and become
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reasonably convinced that this is a vacuum energy.
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So there is hypotheses for different fields, like with names and stuff like that?
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Yeah, you know, generically quintessence, like the Aristotelian fifth essence, but there
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are many, many versions of quintessence.
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There's K essence, there's even ideas that, you know, this isn't something from within
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this dark energy, but rather, there are a bunch of, say, bubble universes surrounding
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our universe, and this whole idea of the multiverse is not some crazy madman type idea anymore.
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It's, you know, real card carrying physicists are seriously considering this possibility
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of a multiverse.
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And some types of multiverses could have, you know, a bunch of bubbles on the outside,
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which gravitationally act outward on our bubble because gravity or gravitons, the quantum
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particle that is thought to carry gravity, is thought to traverse the bulk, the space
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between these different little bubble membranes and stuff.
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And so it's conceivable that these other universes are pulling outward on us.
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That's not a favored explanation right now, but really, nothing has been ruled out.
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No class of models has been ruled out completely.
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Certain examples within classes of models have been ruled out.
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But in general, I think we still have really a lot to learn about what's causing this
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observed acceleration of the expansion of the universe, be it dark energy or some forces
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from the outside, or perhaps, you know, I guess it's conceivable that, and sometimes
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I wake up in the middle of the night screaming, that dark energy, that which causes the acceleration,
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and dark matter, that which causes galaxies and clusters of galaxies to be bound gravitationally
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even though there's not enough visible matter to do so.
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Maybe these are our 20th and 21st century Ptolemaic epicycles.
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So Ptolemy had a geocentric and Aristotelian view of the world.
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Everything goes around Earth.
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But in order to explain the backward motion of planets among the stars that happens every
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year or two, or sometimes several times a year for Mercury and Venus, you needed the
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planets to go around in little circles called epicycles, which themselves then went around
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Earth.
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And in this part of the epicycle where the planet is going in the direction opposite
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to the direction of the overall epicycle, it can appear in projection to be going backward
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among the stars, so called retrograde motion.
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And it was a brilliant mathematical scheme.
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In fact, he could have added epicycles on top of epicycles and reproduced the observed
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positions of planets to arbitrary accuracy.
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And this is really the beginning of what we now call Fourier analysis, right?
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Any periodic function can be represented by a sum of sines and cosines of different periods,
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amplitudes, and phases.
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So it could have worked arbitrarily well.
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But other data show that, in fact, Earth is going around the sun.
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So our dark energy and dark matter, just these band aids that we now have to try to explain
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the data, but they're just completely wrong.
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That's a possibility as well.
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And as a scientist, I have to be open to that possibility as an open minded scientist.
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How do you put yourself in the mindset of somebody that, or majority of the scientific
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community or majority of people believe that the Earth, everything rotates around Earth?
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How do you put yourself in that mindset and then take a leap to propose a model that the
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sun is, in fact, at the center of the solar system?
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Sure.
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I mean, so that puts us back in the shoes of Copernicus, right, 500 years ago, where
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he had this philosophical preference for the sun being the dominant body in what we now
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call the solar system.
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The observational evidence in terms of the measured positions of planets was not better
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explained by the heliocentric, sun centered system.
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It's just that Copernicus saw that the sun is the source of all our light and heat, and
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he knew from other studies that it's far away.
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So the fact that it appears as big as the moon means it's actually way, way bigger because
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even at that time, it was known that the sun is much farther away than the moon.
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So he just felt, wow, it's big, it's bright.
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What if it's the central thing?
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But the observed positions of planets at the time in the early to mid 16th century under
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the heliocentric system was not a better match, at least not a significantly better match
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than Ptolemy's system, which was quite accurate and lasted 1500 years.
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Yeah.
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That's so fascinating to think that the philosophical predispositions that you bring to the table
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are essential.
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So like you have to have a young person come along that has a weird infatuation with the
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sun.
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Yeah.
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That like almost philosophically is like however their upbringing is, they're more ready for
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whatever the more the simpler answer is.
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Right.
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Oh, that's kind of sad.
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It's a sad from an individual descendant of eight perspective because then that means
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like me, you as a scientist, you're stuck with whatever the heck philosophies you brought
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to the table and you might be almost completely unable to think outside this particular box
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you've built.
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Right.
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This is why I'm saying that, you know, as an objective scientist, one needs to have
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an open mind to crazy sounding new ideas.
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And even Copernicus was very much a man of his time and dedicated his work to the Pope.
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He still used circular orbits.
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The sun was a little bit off center, it turns out, and a slightly off center circle looks
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like a slightly eccentric elliptical orbit.
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So then when Kepler, in fact, showed that the orbits are actually in general ellipses,
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not circles, the reason that he needed Tuco Brahe's really great data to show that distinction
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was that a slightly off center circle is not much different from a slightly eccentric ellipse.
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And so there wasn't much difference between Kepler's view and Copernicus's view and Kepler
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needed the better data, Tuco Brahe's data.
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And so that's, again, a great example of science and observations and experiments working together
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with hypotheses and they kind of bounce off each other.
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They play off of each other and you continually need more observations.
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And it wasn't until Galileo's work around 1610 that actual evidence for the heliocentric
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hypothesis emerged.
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It came in the form of Venus, the planet Venus, going through all of the possible phases from
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new to crescent to quarter to gibbous to full to waning gibbous, third quarter waning crescent,
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and then new again.
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It turns out in the Ptolemaic system with Venus between Earth and the sun, but always
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roughly in the direction of the sun, you could only get the new and crescent phases of Venus.
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But the observations showed a full set of phases.
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And moreover, when Venus was gibbous or full, that meant it was on the far side of the sun.
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That meant it was farther from Earth than when it's crescent, so it should appear smaller
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and indeed it did.
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So that was the nail in the coffin in a sense.
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And then Galileo's other great observation was that Jupiter has moons going around it,
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the four Galilean satellites.
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And even though Jupiter moves through space, so too do the moons go with it.
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So first of all, Earth is not the only thing that has other things going around it.
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And secondly, Earth could be moving as Jupiter does and things would move with it.
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We wouldn't fly off the surface and our moon wouldn't be left behind and all this kind
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of stuff.
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So that was a big breakthrough as well, but it wasn't as definitive in my opinion as
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the phases of Venus.
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Sometimes I'm revealing my ignorance, but I didn't realize how much data they were working
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with.
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So it wasn't Einstein or Freud thinking in theories.
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It was a lot of data and you're playing with it and seeing how to make sense of it.
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So it isn't just coming up with completely abstract thought experiments.
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It's looking at the data.
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Sure.
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And you look at Newton's great work, right?
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The Principia, it was based in part on Galileo's observations of balls rolling down inclined
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planes, supposedly falling off the Leaning Tower of Pisa, but that's probably apocryphal.
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In any case, the Roman Catholic Church did history a favor, not that I'm condoning them,
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but they placed Galileo under house arrest and that gave Galileo time to publish, to
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assemble and publish the results of his experiments that he had done decades earlier.
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It's not clear he would have had time to do that, had he not been under house arrest.
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And so Newton, of course, very much used Galileo's observations.
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Let me ask the old Russian overly philosophical question about death.
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So we're talking about the expanding universe.
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Sure.
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How do you think human civilization will come to an end if we avoid the near term issues
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we're having?
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Will it be our sun burning out?
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Will it be comets?
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Oh, okay.
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Will it be, what is it?
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Do you think we have a shot at reaching the heat death of the universe?
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Yeah.
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So we're going to leave out the anthropogenic causes of our potential destruction, which
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I actually think are greater than the celestial causes.
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So if we get lucky and intelligent, I don't know.
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So no way will we as humans reach the heat death of the universe.
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It's conceivable that machines, which I think will be our evolutionary descendants, might
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reach that, although even they will have less and less energy with which to work as time
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progresses because eventually even the lowest mass stars burn out, although it takes them
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trillions of years to do so.
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So the point is that certainly on Earth, there are other celestial threats, existential threats,
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comets, exploding stars, the sun burning out.
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So we will definitely need to move away from our solar system to other solar systems.
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And then the question is, can they keep on propagating to other planetary systems sufficiently
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long?
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In our own solar system, the sun burning out is not the immediate existential threat.
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That'll happen in about five billion years when it becomes a red giant, although I should
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hasten to add that within the next one or two billion years, the sun will have brightened
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enough that unless there are compensatory atmospheric changes, the oceans will evaporate
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away.
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They're going to need much less carbon dioxide for the temperatures to be maintained roughly
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at their present temperature, and plants wouldn't like that very much.
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So you can't lower the carbon dioxide content too much.
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So within one or two billion years, probably the oceans will evaporate away.
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But on a sooner time scale than that, I would say an asteroid collision leading to a potential
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mass extinction, or at least an extinction of complex beings such as ourselves that require
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quite special conditions unlike cockroaches and amoebas to survive, one of these civilization
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changing asteroids is only one kilometer or so in diameter and bigger, and a true mass
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extinction event is 10 kilometers or larger.
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Now it's true that we can find and track the orbits of asteroids that might be headed toward
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Earth, and if we find them 50 or 100 years before they impact us, then clever applied
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physicists and engineers can figure out ways to deflect them.
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But at some point, some comet will come in from the deep freeze of the solar system,
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and there we have very little warning, months to a year.
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What's the deep freeze, sorry to interrupt.
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The deep freeze is sort of out beyond Neptune.
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There's this thing called the Kuiper Belt, and it consists of a bunch of dirty ice balls
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or icy dirt balls.
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It's the source of the comets that occasionally come close to the Sun.
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And then there's an even bigger area called the Scattered Disk, which is sort of a big
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doughnut surrounding the solar system way out there from which other comets come.
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And then there's the Oort Cloud, W O O R T after Jan Oort, a Dutch astrophysicist, and
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it's the better part of a light year away from the Sun, so a good fraction of the distance
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to the nearest star, but that's like a trillion or 10 trillion comet like objects that occasionally
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get disturbed by a passing star or whatever, and most of them go flying out of the solar
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system, but some go toward the Sun, and they come in with little warning.
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00:21:46.960
By the time we can see them, they're only a year or two away from us.
link |
00:21:53.240
And moreover, not only is it hard to determine their trajectories sufficiently accurately
link |
00:21:59.080
to know whether they'll hit a tiny thing like Earth, but outgassing from the comet of gases
link |
00:22:07.040
when the ices sublimate, that outgassing can change the trajectory just because of conservation
link |
00:22:13.600
of momentum, right?
link |
00:22:14.600
It's the rocket effect.
link |
00:22:15.920
Gases go out in one direction, the object moves in the other direction.
link |
00:22:19.100
And so since we can't predict how much outgassing there will be and in exactly what direction
link |
00:22:25.000
because these things are tumbling and rotating and stuff, it's hard to predict the trajectory
link |
00:22:30.400
with sufficient accuracy to know that it will hit.
link |
00:22:33.280
And you certainly don't want to deflect a comet that would have missed but you thought
link |
00:22:38.760
it was going to hit and end up having it hit.
link |
00:22:41.980
That would be like the ultimate Charlie Brown goat instead of trying to be the hero, right?
link |
00:22:47.200
He ended up being the goat.
link |
00:22:50.960
What would you do if it seemed like in a matter of months that there is some nonzero probability,
link |
00:22:58.960
maybe a high probability that there will be a collision?
link |
00:23:02.480
So from a scientific perspective, from an engineering perspective, I imagine you would
link |
00:23:06.680
actually be in the room of people deciding what to do.
link |
00:23:10.520
What uh, philosophically too.
link |
00:23:12.680
It's a tough one, right?
link |
00:23:13.720
Because if you only have a few months, that's not much time in which to deflect it.
link |
00:23:19.680
Early detection and early action are key because when it's far away, you only have to deflect
link |
00:23:27.920
it by a tiny little angle.
link |
00:23:30.320
And then by the time it reaches us, the perpendicular motion is big enough to miss Earth.
link |
00:23:37.160
All you need is one radius or one diameter of the Earth, right?
link |
00:23:41.520
That actually means that all you would need to do is slow it down so it arrives four minutes
link |
00:23:47.540
later or speed it up so it arrives four minutes earlier and Earth will have moved through
link |
00:23:54.320
one radius in that time.
link |
00:23:56.400
So it doesn't take much.
link |
00:23:57.400
But you can imagine if a thing is about to hit you, you have to deflect it 90 degrees
link |
00:24:02.600
or more, right?
link |
00:24:03.600
You know, and you don't have much time to do so and you have to slow it down or speed
link |
00:24:07.160
it up a lot if that's what you're trying to do to it.
link |
00:24:09.280
And so decades is sufficient time, but months is not sufficient time.
link |
00:24:14.680
So at that point, I would think the name of the game would be to try to predict where
link |
00:24:20.200
it would hit.
link |
00:24:22.560
And if it's in a heavily populated region, try to start an orderly evacuation perhaps.
link |
00:24:33.440
But you know, that might cause just so much panic that I'm, how would you do with New
link |
00:24:37.720
York City or Los Angeles or something like that, right?
link |
00:24:41.400
I might have a different opinion a year ago, I'm a bit disheartened by, you know, in the
link |
00:24:48.360
movies, there's always extreme competence from the government.
link |
00:24:54.760
Competence, yeah.
link |
00:24:55.760
Competence, yeah.
link |
00:24:56.760
But we expect extreme incompetence, if anything, right?
link |
00:24:59.720
Yes, no.
link |
00:25:00.720
So I'm quite disappointed.
link |
00:25:02.240
But sort of from a medical perspective, I think you're saying there, and a scientific
link |
00:25:07.000
one, it's almost better to get better and better, maybe telescopes and data collection
link |
00:25:13.080
to be able to predict the movement of these things, or like come up with totally new technologies
link |
00:25:17.920
that you can imagine actually sending out, like probes out there to be able to sort of
link |
00:25:24.240
almost have little finger sensors throughout our solar system to be able to detect stuff.
link |
00:25:29.680
Well, that's right.
link |
00:25:30.680
Yeah, monitoring the asteroid belt is very important and 99% of the so called near earth
link |
00:25:35.640
objects ultimately come from the asteroid belt.
link |
00:25:39.200
And so there we can track the trajectories and even if there's a close encounter between
link |
00:25:43.640
two asteroids which deflects one of them toward earth, it's unlikely to be on a collision
link |
00:25:48.640
course with earth in the immediate future, it's more like tens of years, so that gives
link |
00:25:53.720
us time.
link |
00:25:54.860
But we would need to improve our ability to detect the objects that come in from a great
link |
00:26:00.840
distance.
link |
00:26:01.840
And those are much rarer, the comets come in, 1% of the collisions perhaps are with
link |
00:26:09.720
comets that come in without any warning hardly.
link |
00:26:16.380
So that might be more like a billion or two billion years before one of those hits us.
link |
00:26:23.280
So maybe we have to worry about the sun getting brighter on that time scale.
link |
00:26:28.240
I mean, there's the possibility that a star will explode near us in the next couple of
link |
00:26:34.760
billion years.
link |
00:26:35.760
But over the course of the history of life on earth, the estimates are that maybe only
link |
00:26:46.680
one of the mass extinctions was caused by a star blowing up in particular, a special
link |
00:26:54.520
kind called a gamma ray burst, and I think it's the Ordovician–Silurian extinction
link |
00:27:03.080
420 or so, 440 million years ago that is speculated to have come from one of these particular
link |
00:27:09.240
types of exploding stars called gamma ray bursts.
link |
00:27:12.240
But even there, the evidence is circumstantial.
link |
00:27:15.680
So those kinds of existential threats are reasonably rare.
link |
00:27:20.800
The greater danger I think is civilization changing events where it's a much smaller
link |
00:27:28.040
asteroid, which those are harder to detect, or a giant solar flare that shorts out the
link |
00:27:37.200
grid in all of North America, let's say.
link |
00:27:40.880
Now, astronomers are monitoring the sun 24 seven with various satellites and we can tell
link |
00:27:46.560
when there's a flare or a coronal mass ejection and we can tell that in a day or two, a giant
link |
00:27:52.840
bundle of energetic particles will arrive and twang the magnetic field of earth and
link |
00:27:58.080
send all kinds of currents through long distance power lines and that's what shorts out the
link |
00:28:03.120
transformers and transformers are expensive and hard to replace and hard to transport
link |
00:28:09.800
and all that kind of stuff.
link |
00:28:10.800
So if we can warn the power companies and they can shut down the grid before the big
link |
00:28:18.640
bundle of particle hits, then we will have mitigated much of this.
link |
00:28:21.360
Now for a big enough bundle of particles, you can get short circuits even over small
link |
00:28:27.080
distance scales, so not everything will be saved, but at least the whole grid might not
link |
00:28:32.680
go out.
link |
00:28:33.680
So again, astronomers, I like to say, support your local astronomer, they may help someday
link |
00:28:40.400
save humanity by telling the power companies to shut down the grid, finding the asteroid
link |
00:28:46.160
50 or 100 years before it hits, then having clever physicists and engineers deflect it.
link |
00:28:52.260
So many of these cosmic threats, cosmic existential threats, we can actually predict and do something
link |
00:29:00.960
about or observe before they hit and do something about.
link |
00:29:05.360
So it's terrifying to think that people would listen to this conversation.
link |
00:29:10.920
It's like when you listen to Bill Gates talk about pandemics in his Ted talk a few years
link |
00:29:14.600
ago and realizing we should have supported our local astronomer more.
link |
00:29:19.480
Well, I don't know whether it's more because as I said, I actually think human induced
link |
00:29:24.520
threats or things that occur naturally on earth, either a natural pandemic or perhaps
link |
00:29:29.440
a bioengineering type pandemic or something like a super volcano.
link |
00:29:36.120
There was one event towed by I think it was 70 plus thousand years ago that caused a gigantic
link |
00:29:44.080
decrease in temperatures on earth because it sent up so much soot that it blocked the
link |
00:29:50.640
sun.
link |
00:29:51.640
It's the nuclear winter type disaster scenario that some people including Carl Sagan talked
link |
00:29:55.420
about decades ago.
link |
00:29:57.440
What we can see in the history of volcanic eruptions even more recently in the 19th century,
link |
00:30:02.280
Tambora and other ones, you look at the record and you see rather large dips in temperature
link |
00:30:08.840
associated with massive volcanic eruptions.
link |
00:30:12.120
Well these super volcanoes, one of which by the way exists under Yellowstone in the central
link |
00:30:18.000
US, it's not just one or two states, it's a gigantic region and there's controversy
link |
00:30:25.400
as to whether it's likely to blow anytime in the next 100,000 years or so.
link |
00:30:30.880
But that would be perhaps not a mass extinction or perhaps not a complete existential threat
link |
00:30:37.080
because you have to get rid of the very last humans for that, but at least getting rid
link |
00:30:43.220
of killing off so many humans, truly billions and billions of humans.
link |
00:30:49.460
There have been ones tens of thousands of years ago including this one, Toba I think
link |
00:30:55.880
it's called, where it's estimated that the human population was down to 10,000 or 5,000
link |
00:31:02.880
individuals, something like that.
link |
00:31:05.040
If you have a 15 degree drop in temperature over quite a short time, it's not clear that
link |
00:31:11.320
even with today's advanced technology, we would be able to adequately respond at least
link |
00:31:15.960
for the vast majority of people.
link |
00:31:18.260
Maybe some would be in these underground caves where you'd keep the president and a bunch
link |
00:31:21.840
of other important people, but the typical person is not going to be protected when all
link |
00:31:28.080
of agriculture is cut off.
link |
00:31:32.120
It could be hundreds of millions or billions of people starving to death.
link |
00:31:36.960
Exactly.
link |
00:31:37.960
That's right.
link |
00:31:38.960
They don't all die immediately, but they use up their supplies or again, this electrical
link |
00:31:44.080
grid.
link |
00:31:45.080
First of toilet paper.
link |
00:31:46.080
Dash that toilet paper or the electrical grid.
link |
00:31:50.840
Imagine North America without power for a year.
link |
00:31:55.240
We've become so dependent, we're no longer the cave people.
link |
00:31:58.420
They would do just fine.
link |
00:32:00.160
What do they care about the electrical grid?
link |
00:32:02.480
What do they care about agriculture, their hunters and gatherers?
link |
00:32:06.040
But we now have become so used to our way of life that the only real survivors would
link |
00:32:12.240
be those rugged individualists who live somewhere out in the forest or in a cave somewhere,
link |
00:32:17.520
completely independent of anyone else.
link |
00:32:20.160
Yeah.
link |
00:32:21.160
Recently I recommended, it's totally new to me, this kind of survivalist folks, but there's
link |
00:32:26.080
a few shows.
link |
00:32:27.500
There's a lot of shows of those, but I saw one on Netflix and I started watching them
link |
00:32:32.720
and they make a lot of sense.
link |
00:32:37.040
They reveal to you how dependent we are on all aspects of this beautiful systems we human
link |
00:32:43.260
have built and how fragile they are.
link |
00:32:47.200
Incredibly fragile.
link |
00:32:48.380
And this whole conversation is making me realize how lucky we are.
link |
00:32:53.040
Oh, we're incredibly lucky, but we've set ourselves up to be very, very fragile and
link |
00:32:59.240
we are intrinsically complex biological creatures that except for the fact that we have brains
link |
00:33:05.720
and minds with which we can try to prevent some of these things or respond to them.
link |
00:33:11.800
We as a living organism require quite a narrow set of conditions in order to survive.
link |
00:33:18.700
We're not cockroaches.
link |
00:33:20.240
We're not going to survive a nuclear war.
link |
00:33:23.120
So we're kind of this beautiful dance between, we've been talking about astronomy, that astronomy,
link |
00:33:31.360
the stars like inspires everybody and at the same time, there's this pragmatic aspect that
link |
00:33:37.840
we're talking about.
link |
00:33:39.140
And so I see space exploration as the same kind of way that it's reaching out to other
link |
00:33:44.880
planets, reaching out to the stars, this really beautiful idea.
link |
00:33:48.760
But if you listen to somebody like Elon Musk, he talks about space exploration as very pragmatic.
link |
00:33:56.800
Like we have to be, he has this ridiculous way of sounding like an engineer about it,
link |
00:34:03.880
which is like, it's obvious we need to become a multi planetary species if we were to survive
link |
00:34:09.440
long term.
link |
00:34:10.540
So maybe both philosophically in terms of beauty and in terms of practical, what's your
link |
00:34:18.080
thoughts on space exploration, on the challenges of it, on how much we should be investing
link |
00:34:24.260
in it and on a personal level, like how excited you are by the possibility of going to Mars,
link |
00:34:30.760
colonizing Mars and maybe going outside the solar system.
link |
00:34:34.600
Yeah.
link |
00:34:35.600
You know, great question.
link |
00:34:37.920
There's a lot to unpack there of course.
link |
00:34:41.280
Humans are by their very nature explorers, pioneers.
link |
00:34:44.460
They want to go out, climb the next mountain, see what's behind it, explore the option depths,
link |
00:34:51.440
explore space.
link |
00:34:52.460
This is our destiny to go out there.
link |
00:34:55.360
And of course, from a pragmatic perspective, yes, we need to plant our seeds elsewhere
link |
00:35:02.420
really because things could go wrong here on Earth.
link |
00:35:05.480
Now some people say that's an excuse to not take care of our planet.
link |
00:35:11.080
Well, we say we're elsewhere and so we don't have to take good care of our planet.
link |
00:35:14.280
No, we should take the best possible care of our planet.
link |
00:35:18.160
We should be cognizant of the potential impact of what we're doing.
link |
00:35:22.120
Nevertheless, it's prudent to have us be elsewhere as well.
link |
00:35:26.880
So in that regard, I actually agree with Elon.
link |
00:35:31.200
It'd be good to be on Mars.
link |
00:35:32.420
That would be yet another place for us from which to explore further.
link |
00:35:38.240
Would that be a good next step?
link |
00:35:39.640
Well, it's a good next step.
link |
00:35:42.160
I happen to disagree with him as to how quickly it will happen.
link |
00:35:46.360
I think he's very optimistic.
link |
00:35:48.120
Now you need visionary people like Elon to get people going and to inspire them.
link |
00:35:52.760
I mean, look at the success he's had with multiple companies.
link |
00:35:57.120
So maybe he gives this very optimistic timeline in order to be inspirational to those who
link |
00:36:03.480
are going out there.
link |
00:36:04.480
And certainly his success with the rocket that is reusable because it landed upright
link |
00:36:10.000
and all that.
link |
00:36:11.000
I mean, that's a game changer.
link |
00:36:12.400
It's sort of like every time you flew from San Francisco to Los Angeles, you discard
link |
00:36:16.880
the airplane, right?
link |
00:36:17.880
I mean, that's crazy, right?
link |
00:36:20.240
So that's a game changer.
link |
00:36:21.840
But nevertheless, the timescale over which he thinks that there could be a real thriving
link |
00:36:27.080
colony on Mars, I think is far too optimistic.
link |
00:36:30.680
What's the biggest challenges to you?
link |
00:36:33.480
One is just getting rockets, not rockets, but people out there and two is the colonization.
link |
00:36:40.360
Do you have thoughts about this, the challenges of this kind of prospect?
link |
00:36:44.360
Yeah, I haven't thought about it in great detail other than recognizing that Mars is
link |
00:36:50.040
a harsh environment.
link |
00:36:51.040
Yeah.
link |
00:36:52.040
You don't have much of an atmosphere there.
link |
00:36:53.360
You've got less than a percent of Earth's atmosphere.
link |
00:36:57.000
So you'd need to build some sort of a dome right away, right?
link |
00:37:00.320
And that would take time.
link |
00:37:02.280
You need to melt the water that's in the permafrost or have canals dug from which you transport
link |
00:37:09.280
it from the polar ice caps.
link |
00:37:11.840
You know, I was reading recently in terms of like, what's the most efficient source
link |
00:37:17.240
of nutrition for humans that were to live on Mars?
link |
00:37:20.440
And people should look into this, but it turns out to be insects.
link |
00:37:23.480
Insects.
link |
00:37:24.480
Yeah.
link |
00:37:25.480
So you want, you want to build giant colonies of insects and just be eating them.
link |
00:37:29.680
Yeah, insects have a lot of protein.
link |
00:37:30.680
Yeah, a lot of protein.
link |
00:37:32.000
And they're easy to grow.
link |
00:37:34.280
Like you can think of them as farming.
link |
00:37:36.200
Right.
link |
00:37:37.200
But it's not going to be as easy as growing a whole plot of potatoes like in the movie
link |
00:37:41.960
The Martian, you know, or something, right?
link |
00:37:44.240
It's not going to be that easy.
link |
00:37:45.880
But you know, so there's this thin atmosphere.
link |
00:37:48.420
It's got the wrong composition.
link |
00:37:49.620
It's mostly carbon dioxide.
link |
00:37:51.820
There are these violent dust storms.
link |
00:37:54.900
The temperatures are generally cold.
link |
00:37:57.800
You know, you'd need to do a lot of things.
link |
00:37:59.360
You need to terraform it basically in order to make it nicely livable without some dome
link |
00:38:04.840
surrounding you.
link |
00:38:05.840
And if you, and if you insist on a dome, well, that's not going to house that many people,
link |
00:38:10.880
right?
link |
00:38:11.880
You know, so let's look, let's look briefly then, you know, we're looking for a new apartment
link |
00:38:17.480
to move into.
link |
00:38:18.480
Right.
link |
00:38:19.480
So let's look outside the solar system.
link |
00:38:20.480
Do you think you've, you've spoken about exoplanets as well?
link |
00:38:25.440
Do you think there's possible homes out there for us outside of our solar system?
link |
00:38:31.840
There are lots and lots of homes.
link |
00:38:33.960
Possible homes.
link |
00:38:34.960
There are, there's a planetary system around nearly every star you see in the sky.
link |
00:38:40.480
And one in five of those is thought to have a roughly Earth like planet.
link |
00:38:45.920
And that's a relatively new discovery.
link |
00:38:46.920
Yeah.
link |
00:38:47.920
It's a new discovery.
link |
00:38:48.920
I mean, the Kepler satellite, which was flying around above Earth's atmosphere was able to
link |
00:38:53.320
monitor the brightness of stars with exquisite detail.
link |
00:38:57.180
And they could detect planets crossing the line of sight between us and the star, thereby
link |
00:39:03.880
dimming its light for a short time ever so slightly.
link |
00:39:08.080
And it's amazing.
link |
00:39:09.240
So there are now thousands and thousands of these exoplanet candidates of which something
link |
00:39:14.120
like 90% are probably genuine exoplanets.
link |
00:39:17.380
And you have to remember that only about 1% of stars have their planetary system oriented
link |
00:39:25.100
edge on to your line of sight, which is what you need for this transit method to work,
link |
00:39:30.960
right?
link |
00:39:31.960
Your planetary angle won't work and certainly perpendicular to your line of sight.
link |
00:39:36.200
That is in the plane of the sky won't work because the planet is orbiting the star and
link |
00:39:40.920
never crossing your line of sight.
link |
00:39:43.680
So the fact that they found planets orbiting about 1% of the stars that they looked at
link |
00:39:51.240
in this field of 150 plus thousand stars, they found planets around 1%.
link |
00:39:57.720
You then multiply by the inverse of 1%, which is 1% is about what the fraction of the stars
link |
00:40:06.820
that have their planetary system oriented the right way.
link |
00:40:10.720
And that already back of the envelope calculation tells you that of order 50 to 100% of all
link |
00:40:16.840
stars have planets.
link |
00:40:18.280
And then they've been finding these Earth like planets, et cetera, et cetera.
link |
00:40:21.780
So there are many potential homes.
link |
00:40:23.840
The problem is getting there.
link |
00:40:26.680
So then a typical bright star, Sirius, the brightest star in the sky, maybe not a typical
link |
00:40:32.720
bright star, but it's 8.7 light years away.
link |
00:40:37.600
So that means the light took 8.7 years to reach us.
link |
00:40:43.440
We're seeing it as it was about nine years ago.
link |
00:40:47.460
So then you ask how long would a rocket take to get there at Earth's escape speed, which
link |
00:40:54.560
is 11 kilometers per second.
link |
00:40:57.000
And it turns out it's about a quarter of a million years.
link |
00:41:01.540
Now that's 10,000 generations.
link |
00:41:04.120
Let's say a generation of humans is 25 years.
link |
00:41:07.360
So you'd need this colony of people that is able to sustain itself, all their food, all
link |
00:41:14.760
their waste disposal, all their water, all the recycling of everything.
link |
00:41:18.660
For 10,000 generations, they have to commit themselves to living on this vehicle.
link |
00:41:26.800
I just don't see it happening.
link |
00:41:28.920
What I see potentially happening, if we avoid self destruction, intentional or unintentional
link |
00:41:34.520
here on Earth, is that machines will do it, robots that can essentially hibernate.
link |
00:41:40.960
They don't need to do much of anything for a long, long time as they're traveling.
link |
00:41:44.640
And moreover, if some energetic charged particle, some cosmic ray, hits the circuitry, it fixes
link |
00:41:50.720
itself.
link |
00:41:51.720
Machines can do this.
link |
00:41:55.800
It's a form of artificial intelligence.
link |
00:41:57.940
You just tell the thing, fix yourself basically.
link |
00:42:00.100
And then when you land on the planet, start producing copies of yourself, initially from
link |
00:42:05.920
materials that were perhaps sent, or you just have a bunch of copies there.
link |
00:42:10.280
And then they set up factories with which to do this.
link |
00:42:13.740
This is very, very futuristic, but it's much more feasible, I think, than sending flesh
link |
00:42:20.800
and blood over interstellar distances, a quarter of a million years to even the nearest stars.
link |
00:42:28.480
You're subject to all kinds of charged particles and radiation.
link |
00:42:32.180
You have to shield yourself really well.
link |
00:42:34.440
That's by the way, one of the problems of going to Mars is that it's not a three day
link |
00:42:38.080
journey like going to the moon.
link |
00:42:40.040
You're out there for the better part of a year or two, and you're exposed to lots of
link |
00:42:45.460
radiation, which typically doesn't do well with living tissue, or living tissue doesn't
link |
00:42:52.560
do well with the radiation.
link |
00:42:54.800
And the hope is that the robots, the AI systems might be able to carry the fire of consciousness,
link |
00:43:05.400
whatever makes us humans, like a little drop of whatever makes us humans so special, not
link |
00:43:11.120
to be too poetic about it.
link |
00:43:12.720
No, but I like being poetic about it because it's an amazing question.
link |
00:43:17.480
Is there something beyond just the bits, the ones and zeros to us?
link |
00:43:22.400
It's an interesting question.
link |
00:43:24.760
I like to think that there isn't anything, and that how beautiful it is that our thoughts,
link |
00:43:29.520
our emotions, our feelings, our compassion all come from these ones and zeros, right?
link |
00:43:35.880
That to me actually is a beautiful thought.
link |
00:43:38.800
And the idea that machines, silicon based life effectively, could be our natural evolutionary
link |
00:43:45.520
descendants, not from a DNA perspective, but they are our creations and they then carry
link |
00:43:51.360
on.
link |
00:43:52.360
That to me is a beautiful thought in some ways, but others find it to be a horrific
link |
00:43:55.880
thought.
link |
00:43:56.880
So that's exciting to you.
link |
00:43:58.480
It is exciting to me as well because to me, from a purely an engineering perspective,
link |
00:44:05.240
I believe it's impossible to create, like whatever systems we create that take over
link |
00:44:11.280
the world, it's impossible for me to imagine that those systems will not carry some aspect
link |
00:44:17.540
of what makes humans beautiful.
link |
00:44:19.840
So like a lot of people have these kind of paperclip ideas that we'll build machines
link |
00:44:26.000
that are cold inside or philosophers call them zombies.
link |
00:44:31.240
That naturally the systems that will out compete us on this earth will be cold and non conscious,
link |
00:44:41.660
not capable of all the human emotions and empathy and compassion and love and hate,
link |
00:44:48.720
the beautiful mix of what makes us human.
link |
00:44:53.160
But to me, intelligence requires all of that.
link |
00:44:56.520
So in order to out compete humans, you better be good at the full picture.
link |
00:45:01.680
Right.
link |
00:45:02.680
So artificial general intelligence, in my view, encompasses a lot of these attributes
link |
00:45:08.280
that you just talked about, curiosity, inquisitiveness, you know, right?
link |
00:45:13.540
It might look very different than us humans, but it will have some of the magic.
link |
00:45:17.160
But it'll also be much more able to survive the onslaught of existential threats that
link |
00:45:24.120
either we bring upon ourselves or don't anticipate here on earth, or that occasionally come from
link |
00:45:30.040
beyond and there's nothing much we can do about a supernova explosion that just suddenly
link |
00:45:34.400
goes off.
link |
00:45:36.200
And really, if we want to move to other planets outside our solar system, I think realistically
link |
00:45:42.640
that's a much better option than thinking that humans will actually make these gigantic
link |
00:45:48.200
journeys.
link |
00:45:49.200
And, you know, then I do this calculation for my class, you know, Einstein's special
link |
00:45:53.280
theory of relativity says that you can do it in a short amount of time in your own frame
link |
00:45:57.360
of reference if you go close to the speed of light.
link |
00:46:00.520
But then you bring in E equals MC squared and you figure out how much energy it takes
link |
00:46:05.680
to get you accelerated to close enough to the speed of light to make the time scales
link |
00:46:10.880
short in your own frame of reference.
link |
00:46:13.880
And the amount of energy is just unfathomable, right?
link |
00:46:17.380
We can do it at the Large Hadron Collider with protons, you know, we can accelerate
link |
00:46:22.120
them to 99.9999% of the speed of light, but that's just a proton.
link |
00:46:27.560
We're gazillions of protons, okay?
link |
00:46:29.800
And that doesn't even count the rocket that would carry us, the payload.
link |
00:46:34.040
And you would need to either store the fuel in the rocket, which then requires even more
link |
00:46:39.900
mass for the rocket or collect fuel along the way, which, you know, is difficult.
link |
00:46:44.920
And so getting close to the speed of light, I think, is not an option either other than
link |
00:46:49.880
for a little tiny thing like, you know, Yuri Milner and others are thinking about this,
link |
00:46:54.840
the Starshot project where they'll send a little tiny camera to Alpha Centauri 4.2 light
link |
00:47:00.040
years away.
link |
00:47:01.040
They'll zip past it, take a picture of the exoplanets that we know, orbit that three
link |
00:47:06.080
or more star system and say hello real quick.
link |
00:47:09.320
Say hello real quickly and then send the images back to us, okay?
link |
00:47:12.760
So that's a tiny little thing, right?
link |
00:47:15.060
Maybe you can accelerate that to, they're hoping, 20% of the speed of light with a whole
link |
00:47:19.960
bunch of high powered lasers aimed at it.
link |
00:47:22.680
It's not clear that other countries will allow us to do that, by the way, but that's a very
link |
00:47:26.480
forward looking thought.
link |
00:47:27.480
I mean, I very much support the idea, but there's a big difference between sending a
link |
00:47:31.600
little tiny camera and sending a payload of people with equipment that could then mine
link |
00:47:38.920
the resources on the exoplanet that they reach and then go forth and multiply, right?
link |
00:47:46.400
Well, let's talk about the big galactic things and how we might be able to leverage them
link |
00:47:51.920
to travel fast.
link |
00:47:52.920
I know this is a little bit science fiction, but, you know, ideas of wormholes and ideas
link |
00:48:03.200
at the edge of black holes that reveal to us that this fabric of space time could be
link |
00:48:10.680
messed with, perhaps.
link |
00:48:13.240
Is that at all an interesting thing for you?
link |
00:48:16.680
I mean, in looking out at the universe and studying it as you have, is that also a possible,
link |
00:48:24.840
like a dream for you that we might be able to find clues how we can actually use it to
link |
00:48:29.720
improve our transportation?
link |
00:48:31.600
It's an interesting thought.
link |
00:48:32.600
I'm certainly excited by the potential physics that suggests this kind of faster than light
link |
00:48:40.400
travel effectively or, you know, cutting the distance to make it very, very short through
link |
00:48:45.320
a wormhole or something like that.
link |
00:48:47.280
Possible?
link |
00:48:48.280
No?
link |
00:48:49.280
Well, you know, call me not very imaginative, but based on today's knowledge of physics,
link |
00:48:54.000
which I realize, you know, people have gone down that rabbit hole and, you know, a century
link |
00:48:58.600
ago, Lord Kelvin, one of the greatest physicists of all time, said that all of fundamental
link |
00:49:03.440
physics is done, the rest is just engineering, and guess what?
link |
00:49:07.280
Then came special relativity, quantum physics, general relativity, how wrong he was.
link |
00:49:12.340
So let me not be another Lord Kelvin.
link |
00:49:15.120
On the other hand, I think we know a lot more now about what we know and what we don't know
link |
00:49:20.360
and what the physical limitations are.
link |
00:49:23.340
And to me, most of these schemes, if not all of them, seem very farfetched, if not impossible.
link |
00:49:30.300
So travel through wormholes, for example, you know, it appears that for a non rotating
link |
00:49:36.820
black hole, that's just a complete no go because the singularity is a point like singularity
link |
00:49:42.480
and you have to reach it to traverse the wormhole and you get squished by the singularity, okay?
link |
00:49:49.640
Now for a rotating black hole, it turns out there is a way to pass through the event horizon,
link |
00:49:55.000
the boundary of the black hole, and avoid the singularity and go out the other side
link |
00:49:59.940
or even traverse the donut hole like singularity.
link |
00:50:04.220
In the case of a rotating black hole, it's a ring singularity.
link |
00:50:06.880
So there's actually two theoretical ways you could get through a rotating black hole or
link |
00:50:11.400
a charged black hole, not that we expect charged black holes to exist in nature because they
link |
00:50:16.320
would quickly bring in the opposite charge so as to neutralize themselves.
link |
00:50:21.040
But rotating black holes, definitely a reality.
link |
00:50:23.640
We now have good evidence for them.
link |
00:50:25.720
Do they have traversable wormholes?
link |
00:50:29.240
Probably not because it's still the case that when you go in, you go in with so much energy
link |
00:50:34.760
that it either squeezes the wormhole shut or you encounter a whole bunch of incoming
link |
00:50:42.280
and outgoing energy that vaporizes you.
link |
00:50:46.080
It's called the mass inflation instability, and it just sort of vaporizes you.
link |
00:50:50.600
Nevertheless, you could imagine, well, you're in some vapor form, but if you make it through,
link |
00:50:55.060
maybe you could reform or something.
link |
00:50:58.200
So it's still information.
link |
00:50:59.200
Yeah, it's still information.
link |
00:51:00.200
It's scrambled information, but there's a way maybe of bringing it back, right?
link |
00:51:04.480
But then the thing that really bothers me is that as soon as you have this possibility
link |
00:51:11.680
of traversal of a wormhole, you have to come to grips with a fundamental problem, and that
link |
00:51:16.760
is that you could come back to your universe at a time prior to your leaving, and you could
link |
00:51:24.400
essentially prevent your grandparents from ever meeting.
link |
00:51:27.480
This is called the grandfather paradox, right?
link |
00:51:29.580
And if they never met, and if your parents were never born, and if you were never born,
link |
00:51:33.880
how would you have made the journey to prevent the history from allowing you to exist, right?
link |
00:51:44.880
It's a violation of causality, of cause and effect.
link |
00:51:48.560
Now physicists such as myself take causality violation very, very seriously.
link |
00:51:54.720
We've never seen it.
link |
00:51:55.720
You took a stand.
link |
00:51:56.720
Yeah, I mean, it's one of these back to the future type movies, right?
link |
00:52:01.600
And you have to work things out in such a way that you don't mess things up, right?
link |
00:52:06.640
Some people say that, well, you come back to the universe, but you come back in such
link |
00:52:10.500
a way that you cannot affect your journey.
link |
00:52:14.960
But then that seems kind of contrived to me.
link |
00:52:19.360
Or some say that you end up in a different universe, and this also goes into the many
link |
00:52:24.640
different types of the multiverse hypothesis and the many worlds interpretation and all
link |
00:52:28.880
that.
link |
00:52:29.880
And then it's not the universe from which you left, right?
link |
00:52:34.000
And you don't come back to the universe from which you left.
link |
00:52:37.000
And so you're not really going back in time to the same universe, and you're not even
link |
00:52:42.700
going forward in time necessarily then to the same universe, right?
link |
00:52:46.720
You're ending up in some other universe.
link |
00:52:50.200
So what have you achieved, right?
link |
00:52:53.680
You've traveled.
link |
00:52:56.600
You ended up in a different place than you started in more ways than one.
link |
00:53:00.720
Yeah.
link |
00:53:01.720
And then there's this idea, the Alcubierre drive, where you warp space time in front
link |
00:53:07.320
of you so as to greatly reduce the distance, and you can expand the space time behind you.
link |
00:53:12.480
So you're sort of riding a wave through space time.
link |
00:53:16.120
But the problem I see with that, beyond the practical difficulties and the energy requirements,
link |
00:53:20.440
and by the way, how do you get out of this bubble through which you're riding this wave
link |
00:53:25.740
of space time?
link |
00:53:26.740
And Miguel Alcubierre acknowledged all these things.
link |
00:53:29.160
He said this is purely theoretical, fanciful, and all that.
link |
00:53:31.880
But a fundamental problem I see is that you'd have to get to those places in front of you
link |
00:53:38.280
so as to change the shape of space time so as to make the journey quickly.
link |
00:53:44.080
But to get there, you got there in the normal way at a speed considerably less than that
link |
00:53:49.320
of light.
link |
00:53:50.740
So in a sense, you haven't saved any time, right?
link |
00:53:53.640
You might as well have just taken that journey and gotten to where you were going, right?
link |
00:54:00.680
What have you done?
link |
00:54:01.680
It's not like you snap your fingers and say, okay, let that space there be compressed,
link |
00:54:06.480
and then I'll make it over to Alpha Centauri in the next month.
link |
00:54:10.040
You can't snap your fingers and do that.
link |
00:54:12.240
Yeah.
link |
00:54:13.240
But yeah, we're sort of assuming that we can fix all the biological stuff that requires
link |
00:54:18.260
for humans to persist through that whole process, because ultimately, it might go down to just
link |
00:54:24.560
extending the life of the human in some form, whether it's through the robot, through the
link |
00:54:29.360
digital form, or actually just figuring out genetically how to live forever, because that
link |
00:54:35.240
journey that you mentioned, the long journey, might be different if somehow our understanding
link |
00:54:41.800
of genetics, of our understanding of our own biology, all that kind of stuff, that's another
link |
00:54:47.280
trajectory that possibly...
link |
00:54:48.280
Well, right.
link |
00:54:49.280
If you could put us into some sort of suspended animation, hibernation or something, and greatly
link |
00:54:54.080
increase the lifetime, and so these 10,000 generations I talked about, what do they care?
link |
00:54:58.580
It's just one generation, and they're asleep, okay?
link |
00:55:00.960
It's a long nap.
link |
00:55:02.280
So then you can do it.
link |
00:55:04.500
It's still not easy, right?
link |
00:55:05.500
Because you've got some big old huge colony, and that just through E equals MC squared,
link |
00:55:09.320
right?
link |
00:55:10.320
That's a lot of mass.
link |
00:55:11.320
That's a lot of stuff to accelerate.
link |
00:55:13.480
The Newtonian kinetic energy is gigantic, right?
link |
00:55:18.200
So you're still not home free, but at least you're not trying to do it in a short amount
link |
00:55:23.480
of clock time, right?
link |
00:55:26.240
Which if you look at E equals MC squared, requires truly unfathomable amounts of energy,
link |
00:55:32.520
because the energy is your rest mass, M naught C squared, divided by the square root of one
link |
00:55:39.800
minus V squared over C squared.
link |
00:55:42.200
And if your listeners want to just sort of stick into their pocket calculator, as V over
link |
00:55:46.440
C approaches one, that one over the square root of one minus V squared over C squared
link |
00:55:52.100
approaches infinity.
link |
00:55:54.160
So if you wanted to do it in zero time, you'd need an infinite amount of energy.
link |
00:55:58.520
That's basically why you can't reach, let alone exceed the speed of light, for a particle
link |
00:56:04.680
moving through a preexisting space.
link |
00:56:07.960
It's that it takes an infinite amount of energy to do so.
link |
00:56:11.640
So that's talking about us going somewhere.
link |
00:56:15.080
What about, one of the things that inspires a lot of folks, including myself, is the possibility
link |
00:56:22.040
that there's other, that this conversation is happening on another planet in different
link |
00:56:27.920
forms with intelligent life forms.
link |
00:56:35.360
So first we could start, as a cosmologist, what's your intuition about whether there
link |
00:56:41.840
is or isn't intelligent life out there?
link |
00:56:45.400
Outside of our own?
link |
00:56:46.400
Yeah, I would say I'm one of the pessimists in that I don't necessarily think that we're
link |
00:56:51.280
the only ones in the observable universe, which goes out, you know, roughly 14 billion
link |
00:56:57.880
years in light travel time and more like, you know, 46 billion years when you take into
link |
00:57:02.640
account the expansion of space.
link |
00:57:04.280
So the diameter of our observable universe is something like, you know, 90, 92 billion
link |
00:57:08.480
light years.
link |
00:57:09.700
That encompasses, you know, a hundred billion to a trillion galaxies with, you know, a hundred
link |
00:57:16.040
billion stars each.
link |
00:57:17.280
So now you're talking about something like 10 to the 22nd, 10 to the 23rd power stars
link |
00:57:22.400
and roughly an equal number of Earth like planets and so on.
link |
00:57:27.880
So there may well be other intelligent life.
link |
00:57:32.000
But your sense is our galaxy is not teeming with life.
link |
00:57:35.120
Yeah, our galaxy, our Milky Way galaxy with several hundred billion stars and potentially
link |
00:57:41.080
habitable planets is not teeming with intelligent life.
link |
00:57:44.080
Intelligent.
link |
00:57:45.080
Yeah, I wouldn't, well, I'll get to the primitive life, the bacteria in a moment, but, you know,
link |
00:57:51.520
we may well be the only ones in our Milky Way galaxy, at most a handful, I'd say, but
link |
00:57:56.920
I'd probably side with the school of thought that suggests we're the only ones in our own
link |
00:58:03.200
galaxy, just because I don't see human intelligence as being a natural evolutionary path for life.
link |
00:58:13.520
I mean, there's a number of arguments.
link |
00:58:16.000
First of all, there's been more than 10 billion species of life on Earth in its history.
link |
00:58:22.000
Everything has approached our level of intelligence and mechanical ability and curiosity.
link |
00:58:27.400
You know, whales and dolphins appear to be reasonably intelligent, but there's no evidence
link |
00:58:31.600
that they can think abstract thoughts that they're curious about the world.
link |
00:58:35.360
They certainly can't build machines with which to study the world.
link |
00:58:39.720
So that's one argument.
link |
00:58:41.520
Secondly, we came about as early hominids only four or five million years ago and as
link |
00:58:47.560
homo sapiens only about a quarter of a million years ago.
link |
00:58:52.100
So for the vast majority of the history of life on Earth, an intelligent alien zipping
link |
00:58:56.920
by Earth would have said there's nothing particularly intelligent or mechanically able on Earth.
link |
00:59:02.640
Okay.
link |
00:59:03.640
Thirdly, it's not clear that our intelligence is a long term evolutionary advantage.
link |
00:59:10.760
Now it's clear that in the last 100 years, 200 years, we've improved the lives of hundreds
link |
00:59:15.680
of millions of people, but at the risk of potentially destroying ourselves either intentionally
link |
00:59:21.800
or unintentionally or through neglect, as we discussed before.
link |
00:59:26.200
That's a really interesting point, which is it's possible that they're a huge amount of
link |
00:59:32.120
intelligent civilizations have been born even through our galaxy, but they live very briefly
link |
00:59:38.200
and they die.
link |
00:59:39.200
Flash bulbs in the night.
link |
00:59:42.200
That brings me to the fourth issue and that is the Fermi paradox.
link |
00:59:47.960
If they're common, where the hell are they?
link |
00:59:52.440
Notwithstanding the various UFO reports in Roswell and all that, they just don't meet
link |
00:59:56.480
the bar.
link |
00:59:57.700
They don't clear the bar of scientific evidence in my opinion.
link |
01:00:02.680
So there's no clear evidence that they've ever visited us on Earth here.
link |
01:00:08.240
And SETI has been now, the search for extraterrestrial intelligence has been scanning the skies and
link |
01:00:13.440
true, we've only looked a couple of hundred light years out and that's a tiny fraction
link |
01:00:17.320
of the whole galaxy, a tiny fraction of these hundred billion plus stars.
link |
01:00:22.560
Nevertheless, if the galaxy were teaming with life, especially intelligent life, you'd expect
link |
01:00:30.540
some of it to have been far more advanced than ours.
link |
01:00:34.800
There's nothing special about when the industrial revolution started on Earth.
link |
01:00:39.880
The chemical evolution of our galaxy was such that billions of years ago, nuclear processing
link |
01:00:45.420
and stars had built up clouds of gas after their explosion that were rich enough in heavy
link |
01:00:51.280
elements to have formed Earth like planets, even billions of years ago.
link |
01:00:54.680
So there could be civilizations that are billions of years ahead of ours.
link |
01:00:58.960
And if you look at the exponential growth of technology among Homo sapiens in the last
link |
01:01:03.680
couple of hundred years and you just project that forward, I mean, there's no telling what
link |
01:01:07.400
they could have achieved even in 1000 or 10,000 years, let alone a million or 10 million or
link |
01:01:13.360
a billion years.
link |
01:01:15.300
And if they reach this capability of interstellar travel and colonization, then you can show
link |
01:01:21.120
that within 10 million years or certainly a hundred million years, you can populate
link |
01:01:25.860
the whole galaxy.
link |
01:01:28.960
So then you don't have to have tried to detect them beyond a hundred or a thousand light
link |
01:01:33.680
years.
link |
01:01:34.680
They would already be here.
link |
01:01:35.680
Do you think as a thought experiment, do you think it's possible that they are already
link |
01:01:41.360
here, but we humans are so human centric that we're just not like our conception of what
link |
01:01:47.720
intelligent life looks like is, we don't want to acknowledge it.
link |
01:01:53.720
Like what if trees?
link |
01:01:54.720
Right.
link |
01:01:55.720
Right.
link |
01:01:56.720
Right.
link |
01:01:57.720
Okay, I guess the, in the form of a question, do you think we'll actually detect intelligent
link |
01:02:02.640
life if it came to visit us?
link |
01:02:04.480
Yeah.
link |
01:02:05.480
I mean, it's like, you know, you're an ant crawling around on a sidewalk somewhere and
link |
01:02:08.240
do you notice the humans wandering around and the empire state building and you know,
link |
01:02:13.160
rocket ships flying to the moon and all that kind of stuff, right?
link |
01:02:16.760
It's conceivable that we haven't detected it and that we're so primitive compared to
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01:02:21.340
them that we're just not able to do so.
link |
01:02:23.240
Like if you look at dark energy, maybe we call it as a field.
link |
01:02:27.540
It's just that my own feeling is that in science now through observations and experiments,
link |
01:02:33.800
we've measured so many things and basically we understand a lot of stuff.
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01:02:40.000
Okay.
link |
01:02:41.000
Fabric of reality.
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01:02:42.000
Yeah.
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01:02:43.000
The fabric of reality, we understand quite well.
link |
01:02:44.000
And there are a few little things like dark matter and dark energy that may be some sign
link |
01:02:47.480
of some super intelligence, but I doubt it.
link |
01:02:50.240
Okay.
link |
01:02:51.240
You know, why would some super intelligence be holding clusters of galaxies together?
link |
01:02:54.480
Why would they be responsible for accelerating the expansion of the universe?
link |
01:02:58.280
So the point is, is that through science and applied science and engineering, we understand
link |
01:03:04.440
so much now that I'm not saying we know everything, but we know a hell of a lot.
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01:03:09.920
Okay.
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01:03:10.920
And so there's, it's not like there are lots of mysteries flying around there that are
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01:03:14.820
completely outside our level of exploration or understanding.
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01:03:23.560
Yeah.
link |
01:03:24.920
From a, I would say from, from a mystery perspective, it seems like the mystery of our own like
link |
01:03:32.760
cognition and consciousness is much grander than like the degrees of freedom of possible
link |
01:03:38.760
explanations for what the heck is going on is much greater there than in the, in the
link |
01:03:42.840
physics of the observed.
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01:03:44.440
How the brain works.
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01:03:46.000
How did life arise?
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01:03:47.560
Yeah.
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01:03:48.560
That's big, big questions.
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01:03:50.500
But they, to me, don't indicate the existence of, of, of an alien or something.
link |
01:03:57.000
I mean, unless we are the aliens, you know, we could have been contamination from some
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01:04:00.760
rocket ship that, that hit here a long, long time ago and all evidence of it has been destroyed.
link |
01:04:06.120
But again, that alien would have started out somewhere.
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01:04:09.740
They're not, they're not here watching us right now, right?
link |
01:04:14.260
They're not among us.
link |
01:04:16.060
And so though there are expert potential explanations for the Fermi paradox, and one of them that
link |
01:04:22.480
I kind of like is that the truly intelligent creatures are those that decided not to colonize
link |
01:04:29.120
the whole galaxy because they'd quickly run out of room there because it's exponential,
link |
01:04:33.280
right?
link |
01:04:34.280
You send a probe to a planet, it makes two copies, they go out, they make two copies
link |
01:04:39.480
each and it's an exponential, right?
link |
01:04:41.480
They quickly colonize the whole galaxy.
link |
01:04:43.200
But then the distance to the next galaxy, the next big one like Andromeda, that's two
link |
01:04:47.620
and a half million light years.
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01:04:50.080
That's a much grander scale now, right?
link |
01:04:52.480
And so it also could be that the reason they survived this long is that they got over this
link |
01:04:59.080
tendency that may well exist among sufficiently intelligent creatures, this tendency for aggression
link |
01:05:06.720
and self destruction, right?
link |
01:05:09.280
If they bypass that, and that may be one of the great filters if there are more than one,
link |
01:05:14.480
right?
link |
01:05:15.480
Then they may not be a type of creature that feels the need to go and say, oh, there's
link |
01:05:21.800
a nice looking planet and there's a bunch of ants on it, let's go squish them and colonize
link |
01:05:28.640
it.
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01:05:29.640
No, it could even be the kind of Star Trek like prime directive where you go and explore
link |
01:05:34.120
worlds, but you don't interfere in any way, right?
link |
01:05:38.340
And also we call it exploration is beautiful and everything, but there is underlying this
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01:05:44.080
desire to explore is a desire to conquer.
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01:05:47.240
Yeah.
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01:05:48.240
I mean, if we're just being really honest right now for us, it is right.
link |
01:05:52.720
And you're saying it's possible to separate, but I would venture to say that you wouldn't
link |
01:05:58.960
that those are coupled.
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01:06:00.280
So I could, I could imagine a civilization that lives on for billions of years that just
link |
01:06:06.160
stays on, it's like figures out the minimal effort way of just peacefully existing.
link |
01:06:12.440
It's like a monastery.
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01:06:13.440
Yeah.
link |
01:06:14.440
And it limits itself.
link |
01:06:15.440
Yeah.
link |
01:06:16.440
It limits itself.
link |
01:06:17.440
You know, it's, it's planted its seeds in a number of places.
link |
01:06:19.560
So it's not vulnerable to a single point failure, right?
link |
01:06:24.280
Supernova going off near one of these stars or something, or an asteroid or a comet coming
link |
01:06:28.760
in from the Oort cloud equivalent of that planetary system and without warning, you
link |
01:06:33.320
know, thrashing them to bits.
link |
01:06:35.240
So they've got their seeds in a bunch of places, but they chose not to colonize, colonize the
link |
01:06:40.480
galaxy.
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01:06:41.480
And they also choose not to interfere with this incredibly prevalent, primitive organism
link |
01:06:47.960
homo sapiens, right?
link |
01:06:51.360
Or they, uh, this is like a, they enjoy, this is like a TV show for them.
link |
01:06:57.320
Yeah.
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01:06:58.320
It could be like a TV show.
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01:06:59.320
Right.
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01:07:00.320
So they just tuned in.
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01:07:01.800
Right.
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01:07:02.800
There are no other possible explanations yet.
link |
01:07:05.400
I think that to me, the most likely explanation for the peri me paradox is that they really
link |
01:07:10.640
are very, very rare.
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01:07:12.600
And you know, Carl Sagan estimated a hundred thousand of them.
link |
01:07:16.080
If there's that many, some of them would have been way ahead of us and, and I think we would
link |
01:07:20.120
have seen them by now.
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01:07:22.080
If there are a handful, maybe they're there.
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01:07:24.360
But at that point, you're right on this dividing line between being a pessimist and an optimist.
link |
01:07:29.720
Yeah.
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01:07:30.720
And what are the odds for that?
link |
01:07:31.720
Right.
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01:07:32.720
What are the things that had to go right for us?
link |
01:07:35.080
Yeah.
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01:07:36.080
And then, you know, getting back to something you said earlier, let's discuss, you know,
link |
01:07:39.600
primitive life.
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01:07:40.600
Yeah.
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01:07:41.600
That could be the thing that's difficult to achieve.
link |
01:07:44.520
Just getting the random molecules together to a point where they start self replicating
link |
01:07:50.200
and evolving and becoming better and all that.
link |
01:07:53.960
That's an inordinately difficult thing, I think, though I'm not, you know, some molecular
link |
01:07:58.120
or cell biologist, but just it's, it's, it's the usual argument.
link |
01:08:01.960
You know, you're wandering around in the Sahara desert and you stumble across a watch.
link |
01:08:06.660
Is your, is your initial response, oh, you know, a bunch of sand grains just came together
link |
01:08:12.760
randomly and formed this watch.
link |
01:08:14.560
No, you, you think that something formed it or it came from some simpler structure that
link |
01:08:21.200
then became, you know, more complex.
link |
01:08:23.360
All right.
link |
01:08:24.360
It didn't just form.
link |
01:08:26.000
Well, even the simplest life is, is a very, very complex structure.
link |
01:08:32.040
Even the, even the simplest prokaryotic cells, not to mention eukaryotic cells, although
link |
01:08:36.640
that transition may have been the so called great filter as well.
link |
01:08:40.580
Maybe the cells without a nucleus are relatively easy to form.
link |
01:08:45.180
And then the big next step is where you have a nucleus, which then provides a lot of energy,
link |
01:08:50.240
which allows the cell to become much, much more complex and so on.
link |
01:08:54.440
Interestingly, going from eukaryotic cells, single cells to multicellular organisms does
link |
01:09:01.480
not appear to be, at least on earth, one of these great filters because there's evidence
link |
01:09:05.640
that it happened dozens of times independently on earth.
link |
01:09:08.980
So by, by a really great filter, something that happens very, very rarely, I mean that
link |
01:09:14.640
we had to get through an obstacle that is just incredibly rare to get through.
link |
01:09:25.320
And one of the really exciting scientific things is that that particular point is something
link |
01:09:32.120
that we might be able to discover, even in our lifetimes that find life elsewhere like
link |
01:09:37.020
Europa or be able to see that would be bad news, right?
link |
01:09:42.840
Because if we find lots of pretty advanced life, yeah, that would suggest, and especially
link |
01:09:49.640
if we found some, you know, defunct, you know, fossilized civilization or something somewhere
link |
01:09:53.520
else that would be bacteria, you mean, defunct civilization of like, oh, I'm sorry, I switched
link |
01:10:00.660
gears there.
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01:10:01.660
If we, if we found some intelligent or even trilobites right and stuff, you know, elsewhere,
link |
01:10:06.840
that would be bad news for us because that would mean that the great filter is ahead
link |
01:10:09.840
of us, you know, right, because it would mean that lots of, lots of things have gotten roughly
link |
01:10:16.400
to our level.
link |
01:10:17.400
Yeah.
link |
01:10:18.400
But, but given the Fermi paradox, if you accept that the Fermi paradox means that there's
link |
01:10:23.400
no one else out there, you don't necessarily have to accept that, but if you accept that
link |
01:10:27.800
it means that no one else is out there and yet there are lots of things we found that
link |
01:10:31.980
are at or roughly at our level, that means that the great filter is ahead of us and that
link |
01:10:36.940
bodes poorly for our longterm future, you know, it's funny you said, uh, you started by saying
link |
01:10:45.700
you're a little bit on the pessimistic side, but it's funny because we're doing this kind
link |
01:10:51.040
of dance between pessimism and optimism because I'm not sure if us being alone in the observable
link |
01:10:56.600
universe as intelligent beings is pessimistic, well, it's good news in a sense for us because
link |
01:11:03.080
it means that we made it through, see, if we're the only ones and there are such great
link |
01:11:10.880
filters, maybe more than one formation of life might be one of them formation of eukaryotic
link |
01:11:16.400
that is with the nucleus cells being another development of human like intelligence might
link |
01:11:22.000
be another, right?
link |
01:11:23.040
There might be several such filters and we were the lucky ones.
link |
01:11:27.720
And you know, then people say, well then that means you're putting yourself into a special
link |
01:11:31.640
perspective and every time we've done that we've been wrong and yeah, yeah, I know all
link |
01:11:35.520
those arguments, but it still could be the case that there's one of us at least per galaxy
link |
01:11:41.400
or pretend or a hundred or a thousand galaxies and we're sitting here having this conversation
link |
01:11:47.260
because we exist.
link |
01:11:49.000
And so there's a, there's an observational selection effect there, right?
link |
01:11:53.180
Just because we're special doesn't mean that we shouldn't have these conversations about
link |
01:11:57.000
whether or not we're special, right?
link |
01:11:59.920
Yeah, so that's, that's so exciting.
link |
01:12:02.120
That's optimistic.
link |
01:12:03.360
So that's the, that's the optimistic part that if we don't find other intelligent life
link |
01:12:08.400
there, it might mean that we're the ones that made it.
link |
01:12:13.120
And in general, outside the great filter and so on, you know, it's not obvious that the
link |
01:12:19.160
Stephen Hawking thing, which is, it's not obvious that life out there is going to be kind to
link |
01:12:23.760
us.
link |
01:12:24.760
Oh yeah.
link |
01:12:25.760
So, you know, I knew Hawking and I greatly respect his, his scientific work and in particular
link |
01:12:33.040
the early work on the unification of general theory of relativity and quantum physics to
link |
01:12:38.320
two great pillars in modern physics, you know, Hawking radiation and all that fantastic work.
link |
01:12:42.760
You know, if you were alive, you should have been a recipient of this year's physics Nobel
link |
01:12:47.240
prize, which was for the discovery of black holes and also by Roger Penrose for the theoretical
link |
01:12:53.260
work showing that given a star that's massive enough, you basically can't avoid having a
link |
01:13:00.120
black hole.
link |
01:13:01.120
Anyway, Hawking, fantastic.
link |
01:13:02.120
I, I tip my hat to him.
link |
01:13:04.420
May he rest in peace.
link |
01:13:05.420
That would have been a heck of a Nobel prize, black holes, heck of a good group.
link |
01:13:10.400
But, but, but going back to what he said that we shouldn't be broadcasting our presence
link |
01:13:14.820
to others there, I actually disagree with him respectfully because first of all, we've
link |
01:13:21.160
been unintentionally broadcasting our presence for a hundred years since the development
link |
01:13:25.360
of radio and TV.
link |
01:13:27.200
Okay.
link |
01:13:28.200
Secondly, any alien that has the capability of coming here and squashing us either already
link |
01:13:35.600
knows about us and you know, doesn't care because we're just like little ants.
link |
01:13:39.880
And when there are ants in your kitchen, you tend to squash them.
link |
01:13:42.920
But if there are ants on the sidewalk and you're walking by, do you feel some great
link |
01:13:47.400
conviction that you have to squash any of them?
link |
01:13:49.720
No, you generally don't, right?
link |
01:13:51.440
We're irrelevant to them.
link |
01:13:53.040
All they need to do is keep an eye on us to see whether we're approaching the kind of
link |
01:13:57.800
technological capability and know about them and have intentions of attacking them.
link |
01:14:04.800
And then they can squash us, right?
link |
01:14:06.960
Um, you know, they, they could have done it long ago.
link |
01:14:10.800
Yeah.
link |
01:14:11.800
They'll, they'll do it if they want to, whether we advertise our presence or not is, is irrelevant.
link |
01:14:17.160
So I really think that that's not a huge existential threat.
link |
01:14:21.720
So this is a good place to bring up a difficult topic.
link |
01:14:25.020
You mentioned, um, they might, they would be paying attention to us to see if we come
link |
01:14:31.160
up with any crazy technology.
link |
01:14:34.120
There's folks who have reported UFO sightings.
link |
01:14:37.840
There's actually, I've recently found out there's a websites that track this, the data,
link |
01:14:42.520
the data of these reportings, and there's millions of them in the past, uh, several
link |
01:14:48.680
decades.
link |
01:14:49.680
So seven decades and so on that they've been recorded and the ufologist community, as they
link |
01:14:58.760
refer to themselves, you know, one of the ideas that I find compelling from an alien
link |
01:15:05.040
perspective that they kind of started showing up ever since we figured out how to build
link |
01:15:11.560
nuclear weapons that we should, uh, so I mean, you know, if I was an LA and I would start
link |
01:15:19.760
showing up then as well, just, well, why not just observe us from afar?
link |
01:15:23.240
No, I know.
link |
01:15:24.240
Right.
link |
01:15:25.240
I would figure out, but that's why I'm always, uh, keeping a distance and staying blurry,
link |
01:15:30.160
but very pixelated, very pixelated, you know, that there is a something in the human condition
link |
01:15:37.320
that a cognition that wants to see, wants to believe beautiful things and, uh, some
link |
01:15:43.320
are terrifying, some are exciting, uh, goats, Bigfoot is a big fascination for folks.
link |
01:15:51.040
Yeah.
link |
01:15:52.040
And, uh, UFO sightings, I think falls into that.
link |
01:15:54.000
There's people that look at lights in the night sky and I mean, there's, it's kind of
link |
01:16:02.320
a downer to think in a skeptical sense, to think that that's just a light.
link |
01:16:07.840
Yeah.
link |
01:16:08.840
You want to feel like there's something magical there.
link |
01:16:11.280
Sure.
link |
01:16:12.280
Uh, I mean, I felt that first when my dad, my dad's a physicist, when he first told me
link |
01:16:16.600
about ball lightning when I was like a little kid, very weird, very like weird physical
link |
01:16:22.080
phenomenon.
link |
01:16:23.080
And he said, his intuition was telling me this as a little kid, uh, like, I really like
link |
01:16:29.880
math.
link |
01:16:30.880
His intuition was whoever figures out ball lightning, we'll get a Nobel prize.
link |
01:16:34.680
Like he, I think that was a side comment he gave me and I decided there when I was like
link |
01:16:40.040
five years old or whatever, I'm going to win a Nobel prize for figuring out ball lightning.
link |
01:16:44.840
That was like one of the first sort of sparks of the scientific mindset.
link |
01:16:49.040
Those mysteries, they capture your imagination.
link |
01:16:51.560
I think when I speak to people that report UFOs, that's that fire.
link |
01:16:56.880
That's what I see.
link |
01:16:57.880
That excitement.
link |
01:16:58.880
And I understand that.
link |
01:16:59.880
But what, what do we do with that?
link |
01:17:02.960
Because there's hundreds of thousands, if not millions, and then the scientific community,
link |
01:17:08.120
you're like the perfect person.
link |
01:17:09.120
You have an awesome Einstein shirt.
link |
01:17:13.120
What, what do we do with those reports?
link |
01:17:17.120
It's a, most of the scientific community kind of rolls their eyes and dismisses it.
link |
01:17:21.840
Is it possible that a tiny percent of those folks saw something that's worth deeply investigating?
link |
01:17:30.520
Sure.
link |
01:17:31.520
We should investigate it.
link |
01:17:32.600
It's just one of these things where, you know, they've not brought us a hunk of kryptonite
link |
01:17:37.000
or something like that, right?
link |
01:17:38.340
They haven't brought us actual tangible physical evidence with which experiments can be done
link |
01:17:44.320
in laboratories.
link |
01:17:45.320
Right.
link |
01:17:46.320
It's, it's anecdotal evidence.
link |
01:17:48.120
The photographs are, in some cases, in most cases, I would say quite ambiguous.
link |
01:17:54.360
I don't know what to think about.
link |
01:17:55.560
So David Faber is the first person.
link |
01:17:58.000
He's a Navy pilot, commander, and there's a bunch of them, but he's sort of one of the
link |
01:18:02.960
most legit pilots and people I've ever met.
link |
01:18:08.900
The fact that he saw something weird, he doesn't know what the heck it is, but he saw something
link |
01:18:14.160
weird.
link |
01:18:15.160
I mean, I don't know what to do with that.
link |
01:18:16.920
And one on the psychological side, so I'm pretty confident he saw what he says he saw,
link |
01:18:24.040
which he's not, he's saying it's something weird.
link |
01:18:29.240
One of the interesting psychological things that worries me is that everybody in the Navy,
link |
01:18:36.560
everybody in the US government, everybody in the scientific community, just kind of
link |
01:18:40.960
like pretended that nothing happened.
link |
01:18:45.800
That kind of instinct.
link |
01:18:47.200
That's what makes me believe if aliens show up, we would all like just ignore their presence.
link |
01:18:53.260
That's what bothered me that you don't, you don't investigate it more carefully and use
link |
01:19:00.000
this opportunity to inspire the world.
link |
01:19:03.520
So in terms of kryptonite, I think the conspiracy theory folks say that whenever there is some
link |
01:19:12.120
good hard evidence that scientists would be excited about, there's this kind of conspiracy
link |
01:19:17.480
that I don't like because it's ultimately negative that the US government will somehow
link |
01:19:21.360
hide the good evidence to protect it.
link |
01:19:26.080
Of course, there's some legitimacy to it because you want to protect military secrets, all
link |
01:19:32.200
that kind of stuff.
link |
01:19:33.200
But I don't know what to do with this beautiful mess because I think millions of people are
link |
01:19:41.680
inspired by UFOs and it feels like an opportunity to inspire people about science.
link |
01:19:47.760
So I would say, as Carl Sagan used to say, extraordinary claims require extraordinary
link |
01:19:53.200
evidence.
link |
01:19:54.200
I've quoted him a number of times.
link |
01:19:59.240
We would welcome such evidence.
link |
01:20:03.000
On the other hand, a lot of the things that are seen or perhaps even hidden from us, you
link |
01:20:08.960
could imagine for military purposes, surveillance purposes, the US government doesn't want us
link |
01:20:15.560
to know.
link |
01:20:16.560
Or maybe some of these pilots saw Soviet or Israeli or whatever satellites or some of
link |
01:20:24.120
the crashes that have occurred were later found to be weather balloons or whatever.
link |
01:20:31.040
When there are more conventional explanations, science tends to stay away from the sensational
link |
01:20:40.720
ones.
link |
01:20:41.960
And so it may be that someone else's calling in life is to investigate these phenomena.
link |
01:20:49.000
And I welcome that as a scientist.
link |
01:20:51.640
I don't categorically actually deny the possibility that ships of some sort could have visited
link |
01:20:58.360
us because, as I said earlier, at slow speeds, there's no problem in reaching other stars.
link |
01:21:04.240
In fact, our Voyager and Pioneer spacecraft in a few million years are going to be in
link |
01:21:08.920
the vicinity of different stars.
link |
01:21:10.920
We can even calculate which ones they're going to be in the vicinity of, right?
link |
01:21:15.200
So there's nothing that breaks any laws of physics if you do it slowly.
link |
01:21:19.280
But that's different, just having Voyager or Pioneer fly by some star, that's different
link |
01:21:24.480
from having active aliens altering the trajectory of their vehicle in real time, spying on us,
link |
01:21:31.680
and then either zipping back to their home planet or sending signals that tell them about
link |
01:21:38.200
us because they are likely many light years away, and they're not going to have broken
link |
01:21:44.760
that barrier as well, okay?
link |
01:21:48.800
So I just, you know, go ahead, study them.
link |
01:21:54.080
For some young kid who wants to do it, it might be their calling, and that's how they
link |
01:22:00.400
might find meaning in their lives, is to be the scientist who really explores these things.
link |
01:22:05.960
I chose not to because at a very young age, I found the evidence, to the degree that I
link |
01:22:11.520
investigated it, to be really quite unconvincing, and I had other things that I wanted to do.
link |
01:22:18.320
But I don't categorically deny the possibility, and I think it should be investigated.
link |
01:22:23.040
Yeah, I mean, this is one of those phenomena that 99.9% of people are almost definitely,
link |
01:22:31.840
there's conventional explanations, and then there's like mysterious things that probably
link |
01:22:38.300
have explanations that are a little bit more complicated, but there's not enough to work
link |
01:22:45.400
with.
link |
01:22:46.400
I tend to believe that if aliens showed up, there will be plenty of evidence for scientists
link |
01:22:52.440
to study.
link |
01:22:53.440
Yeah.
link |
01:22:54.440
And exactly as you said, avoid your type of spacecraft that could see sort of some kind
link |
01:23:03.760
of, kind of a dumb thing, almost like a sensor that's like probing, like statistically speaking.
link |
01:23:09.240
Flying by.
link |
01:23:10.240
Flying by, maybe lands, maybe there's some kind of robot type of thingies that just like
link |
01:23:13.920
move around and so on, like in ways that we don't understand.
link |
01:23:17.920
But I feel like, well, I feel like there'll be plenty of hard, hard to dismiss evidence.
link |
01:23:27.320
And I also, especially this year, believe that the US government is not sufficiently
link |
01:23:33.900
competent given the huge amount of evidence that will be revealed from this kind of thing
link |
01:23:39.460
to conceal all of it.
link |
01:23:41.400
Right.
link |
01:23:42.400
At least in modern times, you can say maybe decades ago, but in modern times.
link |
01:23:46.720
Right, you know, the people I speak to and the reason I bring it up is because so many
link |
01:23:51.200
people write to me, they're inspired by it.
link |
01:23:53.600
By the way, I wanted to comment on something you said earlier on, yeah, I had said that
link |
01:23:57.160
I'm sort of a pessimist in that I think there are very few other intelligent, mechanically
link |
01:24:03.640
able creatures out there.
link |
01:24:06.160
But then I said, yes, in a sense, I'm an optimist, as you pointed out, because it means
link |
01:24:10.360
that we made it through the great filter.
link |
01:24:13.240
Right.
link |
01:24:14.240
I meant originally that I'm a pessimist in that I'm pessimistic about the possibility
link |
01:24:19.440
that there are many, many of us out there, you know, mathematically speaking in the Drake
link |
01:24:23.920
equation.
link |
01:24:24.920
Exactly.
link |
01:24:25.920
Right.
link |
01:24:26.920
Right.
link |
01:24:27.920
But it may mean a good thing for our ultimate survival.
link |
01:24:28.920
Right.
link |
01:24:29.920
So I'm glad you caught me on that.
link |
01:24:30.920
Yeah, I definitely agree with you.
link |
01:24:32.440
It is ultimately an optimistic statement.
link |
01:24:34.000
But anyway, I think, you know, UFO research is interesting.
link |
01:24:38.140
And I guess one of the reasons I've not been terribly convinced is that I think there are
link |
01:24:43.280
some scientists who are investigating this and they've not found any clear evidence.
link |
01:24:49.080
Now, I must admit, I have not looked through the literature to convince myself that there
link |
01:24:53.880
are many scientists doing systematic studies of these various reports.
link |
01:24:58.000
I can't say for sure that there's a critical mass of them, but it's just that you never
link |
01:25:03.620
get these reports from hardcore scientists.
link |
01:25:06.580
That's another thing.
link |
01:25:07.580
And astronomers, you know, what do we do?
link |
01:25:08.680
We spend our time studying the heavens and you'd think we'd be the ones that are most
link |
01:25:12.760
likely aside from pilots, perhaps, at seeing weird things in the sky.
link |
01:25:17.480
And we just never do of the unexplained UFO type nature.
link |
01:25:22.240
Yeah, I definitely, I try to keep an open mind, but for people who listen, it's actually
link |
01:25:28.720
really difficult for scientists.
link |
01:25:30.680
Like I get probably like this year, I've probably gotten over probably maybe over a thousand
link |
01:25:38.160
emails on the topic of AGI.
link |
01:25:42.740
It's very difficult to, you know, people write to me, it's like, how can you ignore this
link |
01:25:48.760
in AGI side?
link |
01:25:49.880
Like this model, this is obviously the model that's going to achieve general intelligence.
link |
01:25:53.880
How can you ignore it?
link |
01:25:54.880
I'm giving you the answer.
link |
01:25:55.880
Here's my document.
link |
01:25:56.880
And they're always just these large write ups.
link |
01:26:00.600
The problem is it's very difficult to weed through a bunch of BS.
link |
01:26:07.920
It's very possible that you had actually saw the UFO, but you have to acknowledge that
link |
01:26:15.040
by UFO, I mean, an extraterrestrial life, you have to acknowledge the hundreds of thousands
link |
01:26:20.460
of people who are a little bit, if not a lot full of BS.
link |
01:26:26.600
And from a scientist perspective, it's really hard work and it's when there's amazing stuff
link |
01:26:33.560
out there, it's like, why invest in Bigfoot when evolution in all of its richness is beautiful?
link |
01:26:40.240
Who cares about a monkey that walks on two feet or eight or whatever?
link |
01:26:43.360
Like there's a zillion decoys at observatories.
link |
01:26:47.940
True fact.
link |
01:26:48.940
We get lots and lots of phone calls when Venus, the evening star, but just really a bright
link |
01:26:55.280
planet happens to be close to the crescent moon because it's such a striking pair.
link |
01:27:00.360
This happens once in a while.
link |
01:27:01.360
And we get these phone calls, oh, there's a UFO next to the moon.
link |
01:27:04.720
And no, it's Venus.
link |
01:27:06.280
And so they're just and I'm not saying the best UFO reports are of that nature.
link |
01:27:12.520
No, there are some much more convincing cases.
link |
01:27:14.400
And I've seen some of the footage and blah, blah, blah.
link |
01:27:17.240
But it's just there's so many decoys, right?
link |
01:27:19.520
So much so much noise that you have to filter out.
link |
01:27:22.660
And there's only so many scientists.
link |
01:27:23.920
So it's hard.
link |
01:27:24.920
There's only so much.
link |
01:27:25.920
There's only so much time as well.
link |
01:27:27.240
And you have to choose what problems you work on.
link |
01:27:30.000
You know, this might be a fun question to ask to kind of explore the idea of the expanding
link |
01:27:37.720
universe.
link |
01:27:38.720
Yeah.
link |
01:27:39.720
So the the radius of the observable universe is 45.7 billion light years.
link |
01:27:46.800
Yeah.
link |
01:27:47.800
And the age of the universe is 13.7 billion years.
link |
01:27:56.240
That's less than the radius of the universe.
link |
01:28:00.880
How's that possible?
link |
01:28:01.880
So that's a great question.
link |
01:28:03.560
So I meant to bring a little a little prop I have with ping pong balls on a rubber hose,
link |
01:28:08.720
a rubber band.
link |
01:28:09.720
I use it in many of the lectures that one can find of me online.
link |
01:28:14.080
But you have in an expanding universe, the space itself between galaxies or more correctly,
link |
01:28:20.120
clusters of galaxies expanding.
link |
01:28:23.040
So imagine light going from one cluster to another.
link |
01:28:27.080
It traverses some distance and then while it's traversing the rest, that part that it
link |
01:28:33.640
already traveled through continues to expand.
link |
01:28:38.440
Now 13.7 billion years might have gone by since the light that we are seeing from the
link |
01:28:47.160
early stages, the so called cosmic microwave background radiation, which is the afterglow
link |
01:28:52.280
of the Big Bang or the echo of the Big Bang.
link |
01:28:54.760
Yeah, 13.7 billion years have gone by.
link |
01:28:57.400
That's how long it's taken that light to reach us.
link |
01:29:00.840
But while it's been traveling that distance, the parts that it already traveled continue
link |
01:29:06.080
to expand.
link |
01:29:08.000
So it's like you're walking on at an airport, you know, on one of these walkways and you're
link |
01:29:13.280
walking along because you're trying to get to your terminal.
link |
01:29:16.200
But the walkway is continuing as well.
link |
01:29:19.240
You end up traveling a greater distance or the same distance faster is another way of
link |
01:29:24.160
putting it, right?
link |
01:29:25.280
That's why you get on one of these traveling walkways.
link |
01:29:28.360
So you get roughly a factor of pi, you know, but it's more like 3.2, I think.
link |
01:29:33.560
But when you work it all out, you multiply the number of years the universe has been
link |
01:29:38.640
in existence by, you know, three and a quarter or so.
link |
01:29:42.520
And that's how you get this 46 billion light year radius.
link |
01:29:48.920
But how is that, let me ask some nice dumb questions, how is that not traveling faster
link |
01:29:56.000
than the speed of light?
link |
01:29:57.000
Yeah, it's not traveling faster than the speed of light because locally at any point, if
link |
01:30:01.160
you were to measure the light, the photons zipping past, it would not be exceeding the
link |
01:30:06.640
speed of light.
link |
01:30:08.000
The speed of light is a locally measured quantity.
link |
01:30:11.320
After light has traversed some distance, if the rubber band keeps on stretching, then
link |
01:30:16.280
yes, it looks like the light traveled a greater distance than it would have had the space
link |
01:30:23.680
not been expanding.
link |
01:30:25.240
But locally, it never was exceeding the speed of light.
link |
01:30:28.180
It's just that the distance through which it already traveled then went off and expanded
link |
01:30:32.600
on its own some more.
link |
01:30:35.360
And if you give the light credit, so to speak, for having traversed that distance, well,
link |
01:30:40.960
then it looks like it's going faster than the speed of light.
link |
01:30:43.680
But that's not how speed works.
link |
01:30:47.480
And in relativity, also, the other thing that is interesting is that if you take two ping
link |
01:30:54.720
pong balls that are sufficiently far apart, especially in an accelerating universe, you
link |
01:30:59.280
can easily have them moving apart from one another faster than the speed of light.
link |
01:31:03.400
So take two ping pong balls that were originally 400,000 kilometers from each other and let
link |
01:31:09.680
every centimeter in your rubber band expand to two in one second.
link |
01:31:14.280
Then suddenly, this 400,000 kilometer distance is 800,000 kilometers.
link |
01:31:20.720
It went out by 400,000 kilometers in one second.
link |
01:31:24.480
That exceeds the 300,000 kilometer per second speed of light.
link |
01:31:29.620
But that light limit, that particle limit in special relativity, applies to objects
link |
01:31:36.240
moving through a preexisting space.
link |
01:31:39.640
There's nothing in either special or general relativity that prevents space itself from
link |
01:31:46.160
expanding faster than the speed of light.
link |
01:31:48.680
That's no problem.
link |
01:31:49.680
Einstein wouldn't have had a problem with a universe as observed now by cosmologists.
link |
01:31:55.760
Yeah, I'm not sure I'm yet ready to deal emotionally with expanding space.
link |
01:32:04.240
That to me is one of the most awe inspiring things, starting from the Big Bang.
link |
01:32:09.560
It's definitely abstract.
link |
01:32:11.480
Space itself is expanding.
link |
01:32:13.320
Right.
link |
01:32:14.320
Could you, can we talk about the Big Bang a little bit?
link |
01:32:18.600
Sure.
link |
01:32:19.600
Yeah, yeah.
link |
01:32:20.600
What, so like the entirety of it, the universe, was very small.
link |
01:32:27.360
Right.
link |
01:32:28.360
But it was not a point.
link |
01:32:29.360
It was not a point.
link |
01:32:31.160
Because if we live in what's called a closed universe now, a sphere or the three dimensional
link |
01:32:36.080
version of that would be a hypersphere, then regardless of how far back in time you go,
link |
01:32:43.120
it was always that topological shape.
link |
01:32:45.880
You can't turn a point suddenly into a shell, okay?
link |
01:32:49.320
It always had to be a shell.
link |
01:32:52.020
So when people say, well, the universe started out as a point, that's being kind of flippant,
link |
01:32:57.040
kind of glib.
link |
01:32:58.160
It didn't really.
link |
01:32:59.160
It just started out at a very high density.
link |
01:33:02.480
And we don't know actually whether it was finite or infinite, I think personally that
link |
01:33:06.880
it was finite at the time, but it expanded very, very quickly.
link |
01:33:10.400
Indeed, if it exponentiated and continued in some places to exponentiate, then it could
link |
01:33:16.300
in fact be infinite right now.
link |
01:33:18.140
And most cosmologists think that it is infinite.
link |
01:33:20.480
Wait, wait, wait.
link |
01:33:21.480
Yeah, sorry.
link |
01:33:22.480
What infinite, which dimension, mass, size?
link |
01:33:25.040
Infinite in space.
link |
01:33:26.440
Infinite in space.
link |
01:33:27.440
And by that I mean that if you were trying to measure.
link |
01:33:29.560
There's no boundary.
link |
01:33:30.560
There's no light to measure its size.
link |
01:33:33.280
You'd never be able to measure its size because it would always be bigger than the distance
link |
01:33:37.400
light can travel.
link |
01:33:39.260
That's what you get in a universe that's accelerating in its expansion.
link |
01:33:42.760
Okay.
link |
01:33:43.760
But if a thing was a hypersphere, it's very small, not a point, how can that thing be
link |
01:33:50.280
infinite?
link |
01:33:51.280
Well, it expands exponentially.
link |
01:33:54.040
That's what the inflation theory is all about.
link |
01:33:56.200
Indeed, at your home institution, Alan Guth is one of the originators of the whole inflationary
link |
01:34:01.400
universe idea, along with Andre Linde at Stanford University here in the Bay Area.
link |
01:34:07.280
And others, Alexei Starobinsky and others had similar sorts of ideas.
link |
01:34:11.240
But in an exponentially expanding universe, if you actually try to make this measurement,
link |
01:34:17.400
you send light out to try to see it curve back around and hit you in the back of the
link |
01:34:22.720
head.
link |
01:34:23.720
But in an exponentially expanding universe, the amount of space remaining to be traversed
link |
01:34:29.360
is always a bigger and bigger quantity.
link |
01:34:32.400
So you'll never get there from here.
link |
01:34:34.520
You'll never reach the back of your head.
link |
01:34:35.920
So observationally or operationally, it can be thought of as being infinite.
link |
01:34:41.160
That's one of the best definitions of infinity, by the way.
link |
01:34:43.680
What's that?
link |
01:34:44.680
That's one of the best sort of physical manifestations of infinity.
link |
01:34:49.520
Yeah, yeah.
link |
01:34:50.640
Because you have to ask, how would you actually measure it?
link |
01:34:53.200
Now, I sometimes say to my cosmology theoretical friends, well, if I were God and I were outside
link |
01:34:58.920
this whole thing and I took a godlike slice in time, wouldn't it be finite no matter how
link |
01:35:05.140
big it is?
link |
01:35:06.140
And they object and they say, Alex, you can't be outside and take a godlike slice of time,
link |
01:35:13.000
you know?
link |
01:35:14.000
Because there's nothing outside.
link |
01:35:15.000
Well, I'm not, you know, or also, you know, what slice of time you're taking depends on
link |
01:35:22.000
your motion.
link |
01:35:23.000
And that's true even in special relativity that slices of time get tilted, in a sense,
link |
01:35:28.680
if you're moving quickly, the axes, x and t actually become tilted, not perpendicular
link |
01:35:36.100
to one another.
link |
01:35:37.920
And you can look at Brian Greene's books and lectures and other things where he imagines
link |
01:35:43.320
taking a loaf of bread and slicing it in units of time as you progress forward.
link |
01:35:50.120
But then if you're zipping along relative to that loaf of bread, the slices of time
link |
01:35:55.160
actually become tilted.
link |
01:35:57.400
And so it's not even clear what slices of time mean.
link |
01:36:00.700
But I'm an observational astronomer, I know which end of the telescope to look through.
link |
01:36:05.040
And the way I understand the infinity is, as I just told you, that operationally or
link |
01:36:09.480
observationally, there'd be no way of seeing that it's a finite universe, of measuring
link |
01:36:16.340
a finite universe.
link |
01:36:17.340
And so in that sense, it's infinite, even if it started out as a finite little dot.
link |
01:36:25.600
Not a dot, I'm sorry, a finite little hypersphere.
link |
01:36:29.720
But it didn't really start out there because what happened before that?
link |
01:36:37.800
Well, we don't know.
link |
01:36:38.800
So this is where it gets into a lot of speculation.
link |
01:36:41.480
Let's go, I mean...
link |
01:36:42.480
Let's go there.
link |
01:36:43.480
Okay, sure.
link |
01:36:44.480
So, you know...
link |
01:36:45.480
The idea of what happened before t equals zero and whether there are other universes
link |
01:36:50.440
out there, I like to say that these are sort of on the boundaries of science.
link |
01:36:55.160
They're not just ideas that we wake up at three in the morning to go to the bathroom
link |
01:36:58.820
and say, oh, well, let's think about what happened before the Big Bang or let there
link |
01:37:02.160
be a multiplicity of universes.
link |
01:37:04.880
In other words, we have real testable physics that we can use to draw certain conclusions
link |
01:37:12.280
that are plausibility arguments based on what we know.
link |
01:37:16.400
Now, admittedly, there are not really direct tests of these hypotheses.
link |
01:37:24.160
That's why I call them hypotheses.
link |
01:37:26.040
They're not really elevated to a theory because a theory in science is really something that
link |
01:37:30.980
has a lot of experimental or observational support behind it.
link |
01:37:34.960
So they're hypotheses, but they're not unreasonable hypotheses based on what we know about general
link |
01:37:41.400
relativity and quantum physics.
link |
01:37:44.240
And they may have indirect tests in that if you adopt this hypothesis, then there might
link |
01:37:49.720
be a bunch of things you expect of the universe, and lo and behold, that's what we measure.
link |
01:37:54.560
But we're not actually measuring anything at t less than zero, or we're not actually
link |
01:38:00.620
measuring the presence of another universe in this multiverse, and yet there are these
link |
01:38:05.780
indirect ideas that stem forth.
link |
01:38:09.180
So it's hard to prove uniqueness, and it's hard to completely convince oneself that a
link |
01:38:15.560
certain hypothesis must be true.
link |
01:38:19.540
But the more and more tests you have that it satisfies, let's say there are 50 predictions
link |
01:38:24.420
it makes, and 49 of them are things that you can measure.
link |
01:38:30.360
And then the 50th one is the one where you want to measure the actual existence of that
link |
01:38:35.640
other universe, or what happened before t equals zero, and you can't do that.
link |
01:38:41.840
But you've satisfied 49 of the other testable predictions, and so that's science, right?
link |
01:38:49.000
Now a conventional condensed matter physicist or someone who deals with real data in the
link |
01:38:53.680
laboratory might say, oh, you cosmologists, that's not really science because it's not
link |
01:38:58.040
directly testable, but I would say it's sort of testable.
link |
01:39:02.480
But it's not completely testable, and so it's at the boundary, but it's not like we're coming
link |
01:39:06.040
up with these crazy ideas, among them quantum fluctuations out of nothing, and then inflating
link |
01:39:11.980
into a universe with, you might say, well, you created a giant amount of energy.
link |
01:39:16.720
But in fact, this quantum fluctuation out of nothing in a quantum way violates the conservation
link |
01:39:22.800
of energy.
link |
01:39:23.800
But who cares?
link |
01:39:24.800
That was a classical law anyway.
link |
01:39:26.600
And then an inflating universe maintains whatever energy it had, be it zero or some infinitesimal
link |
01:39:32.760
amount.
link |
01:39:33.760
In a sense, the stuff of the universe has a positive energy, but there's a negative
link |
01:39:38.800
gravitational energy associated with it.
link |
01:39:41.280
It's like I drop an apple.
link |
01:39:43.000
I got kinetic energy, energy of motion out of that, but I did work on it to bring it
link |
01:39:47.880
to that height.
link |
01:39:49.800
So by going down and gaining energy of motion, positive one, two, three, four, five units
link |
01:39:55.880
of kinetic energy, it's also gaining or losing, depending on how you want to think of it,
link |
01:40:01.160
negative one, two, three, four, five units of potential energy, so the total energy remains
link |
01:40:06.200
the same.
link |
01:40:07.240
An inflating universe can do that, or other physicists say that energy isn't conserved
link |
01:40:12.260
in general relativity.
link |
01:40:13.840
That's another way out of creating a universe out of nothing.
link |
01:40:17.520
But the point is that this is all based on reasonably well tested physics, and although
link |
01:40:22.920
these extrapolations seem kind of outrageous at first, they're not completely outrageous.
link |
01:40:30.080
They're within the realm of what we call science already.
link |
01:40:33.600
And maybe some young whippersnapper will be able to figure out a way to directly test
link |
01:40:39.080
what happened before T equals zero or to test for the presence of these other universes,
link |
01:40:44.060
but right now we don't have a way of doing that.
link |
01:40:46.460
So speaking of young whippersnappers, Roger Penrose.
link |
01:40:52.040
So he kind of has a, you know, idea that we, there may be some information that travels
link |
01:40:58.240
from whatever the heck happened before the Big Bang.
link |
01:41:00.760
Yeah, maybe.
link |
01:41:01.760
I kind of doubt it.
link |
01:41:03.320
So do you think it's possible to detect something, like actually experimentally be able to detect
link |
01:41:09.480
some, I don't know what it is, radiation, some sort of...
link |
01:41:13.640
Yeah, and the cosmic microwave background radiation, there may be ways of doing that.
link |
01:41:18.240
But is it, is it philosophically or practically possible to detect signs that this was before
link |
01:41:25.480
the Big Bang or is it, or is it what you said, which is like everything we observe will,
link |
01:41:32.000
as we currently understand, will have to be a creation of this particular observable universe?
link |
01:41:36.200
Yeah.
link |
01:41:37.200
I mean, you know, if you, it's very difficult to answer right now because we don't have
link |
01:41:40.480
a single verified, fully self consistent, experimentally tested quantum theory of gravity.
link |
01:41:48.360
Right.
link |
01:41:49.360
And of course the beginning of the universe is a large amount of stuff in a very small
link |
01:41:53.600
space.
link |
01:41:54.600
Yeah.
link |
01:41:55.600
So you need both quantum mechanics and general relativity.
link |
01:41:57.120
Same thing if our universe re collapses and then bounces back to another Big Bang.
link |
01:42:01.400
You know, there's also ideas there that some of the information leaks through or survives.
link |
01:42:06.320
I don't know that we can answer that question right now because we don't have a quantum
link |
01:42:11.560
theory of gravity that most physicists believe in.
link |
01:42:15.360
And belief is perhaps the wrong word that most physicists trust because the experimental
link |
01:42:20.600
evidence favors it.
link |
01:42:22.480
Yeah.
link |
01:42:23.480
Right?
link |
01:42:24.480
Yeah.
link |
01:42:25.480
There are various forms of string theory.
link |
01:42:26.480
There's quantum loop gravity.
link |
01:42:27.480
There are various ideas, but which, if any, will be the one that survives the test of
link |
01:42:33.240
time and more importantly, within that, the test of experiment and observation.
link |
01:42:38.840
Yeah.
link |
01:42:39.840
So my own feeling is probably these things don't survive.
link |
01:42:43.280
I don't think we've seen any evidence in the cosmic microwave background radiation
link |
01:42:47.400
of information leaking through.
link |
01:42:50.520
Similarly, the one way or one of the few ways in which we might test for the presence of
link |
01:42:55.880
other universes is if they were to collide with ours, that would leave a pattern, a temperature
link |
01:43:02.200
signature in the cosmic microwave background radiation.
link |
01:43:05.920
Some astrophysicists claim to have found it, but in my opinion, it's not statistically
link |
01:43:10.200
significant to the level that would be necessary to have such an amazing claim, right?
link |
01:43:17.280
It's just a 5% chance that the microwave background had that distribution just by chance.
link |
01:43:22.960
5% isn't very long odds if you're claiming that instead that you're finding evidence
link |
01:43:32.680
from another universe.
link |
01:43:33.680
I mean, it's like if the Large Hadron Collider people had claimed after gathering enough
link |
01:43:39.760
data to show the Higgs particle when there was a 5% chance it could be just a statistical
link |
01:43:47.780
fluctuation in their data.
link |
01:43:50.040
No, they required 5 sigma, 5 standard deviations, which is roughly one chance in 2 million that
link |
01:43:57.640
this is a statistical fluctuation of no physical greater significance.
link |
01:44:04.280
Extraordinary claims require extraordinary evidence.
link |
01:44:05.560
There you go.
link |
01:44:06.560
It all boils down to that.
link |
01:44:07.560
And the greater your claim, the greater is the evidence that is needed and the more evidence
link |
01:44:12.420
you need from independent ways of measuring or of coming to that deduction.
link |
01:44:20.640
A good example was the accelerating universe.
link |
01:44:23.560
When we found evidence for it in 1998 with supernovae with exploding stars, it was great
link |
01:44:29.840
that there were two teams that lent some credibility to the discovery.
link |
01:44:34.240
But it was not until other astrophysicists used not only that technique, but more importantly,
link |
01:44:41.200
other independent techniques that had their own potential sources of systematic error
link |
01:44:46.760
or whatever.
link |
01:44:47.940
But they all came to the same conclusion and that started giving a much more complete picture
link |
01:44:52.760
of what was going on and a picture in which most astrophysicists quickly gained confidence.
link |
01:44:59.220
That's why that idea caught on so quickly is that there were other physicists and astronomers
link |
01:45:06.200
doing observations completely independent of supernovae that seemed to indicate the
link |
01:45:11.640
same thing.
link |
01:45:12.640
Yeah.
link |
01:45:13.640
That period of your life that work with an incredible team of people that won the Nobel
link |
01:45:22.480
Prize is just fascinating work.
link |
01:45:25.880
Oh gosh.
link |
01:45:26.880
Never in my wildest dreams as a kid did I think that I would be involved, much less
link |
01:45:33.280
so heavily involved, in a discovery that's so revolutionary.
link |
01:45:37.880
As a kid, as a scientist, if you're realistic, once you learn a little bit more about how
link |
01:45:41.760
science is done and you're not going to win a Nobel Prize and be the next Newton or Einstein
link |
01:45:45.840
or whatever, you just hope that you'll contribute something to humankind's understanding of
link |
01:45:51.020
how nature works and you'll be satisfied with that.
link |
01:45:55.040
But here I was in the right place at the right time, a lot of luck, a lot of hard work, and
link |
01:46:01.040
there it was.
link |
01:46:02.180
We discovered something that was really amazing and that was the greatest thrill, right?
link |
01:46:08.400
I couldn't have asked for anything more than being involved in that discovery.
link |
01:46:14.060
So the couple of teams, the Supernova Cosmology Project and the HiZ Supernova Search Team,
link |
01:46:20.200
what was the Nobel Prize given for?
link |
01:46:21.960
It was given for the discovery of the accelerating expansion of the universe, not for the elucidation
link |
01:46:27.280
of what dark energy is or what causes that expansion, that acceleration, be it universes
link |
01:46:33.040
on the outside or whatever, it was only for the observational fact.
link |
01:46:36.840
So first of all, what is the accelerating universe?
link |
01:46:39.200
So the accelerating universe is simply that if we look at the galaxies moving away from
link |
01:46:45.640
us right now, we would expect them to be moving away more slowly than they were billions of
link |
01:46:52.120
years ago.
link |
01:46:53.120
That's because galaxies have visible matter, which is gravitationally attractive, and dark
link |
01:46:58.080
matter of an unknown sort that holds galaxies together and holds clusters of galaxies together.
link |
01:47:04.600
And of course, they then pull on one another and they would tend to retard the expansion
link |
01:47:09.400
of the universe.
link |
01:47:10.400
Just as when I toss an apple up, even ignoring air resistance, the mutual gravitational attraction
link |
01:47:17.280
between Earth and the apple slows the apple down.
link |
01:47:20.640
If that attraction is great enough, then the apple will someday stop and even come back.
link |
01:47:24.800
The Big Crunch, you could call it, or the Gnab Gibb, which is Big Bang backwards, right?
link |
01:47:29.080
That's what could have happened to the universe.
link |
01:47:30.520
But even if the universe's original expansion energy was so great that it avoids the Big
link |
01:47:36.860
Crunch, that's like an apple thrown at Earth's escape speed.
link |
01:47:39.800
It's like the rockets that go to Mars someday, right, with people.
link |
01:47:47.040
Even then, you'd expect the universe to be slowing down with time.
link |
01:47:50.800
But we looked back through the history of the universe by looking at progressively more
link |
01:47:55.600
distant galaxies and by seeing that the evolution of this expansion rate is that in the first
link |
01:48:06.000
nine billion years, yeah, it was slowing down.
link |
01:48:09.340
But in the last five billion years, it's been speeding up.
link |
01:48:13.720
So who asked for that, right, you know?
link |
01:48:17.320
I think it's interesting to talk about a little bit of the human story of the Nobel Prize,
link |
01:48:22.080
which is, I mean, it's fascinating.
link |
01:48:24.920
It's a really, first of all, the prize itself.
link |
01:48:27.960
It's kind of fascinating on the psychological level that prizes, I know we kind of think
link |
01:48:34.040
that prizes don't matter, but somehow they kind of focus the mind about some of the most
link |
01:48:38.720
special things we've accomplished.
link |
01:48:39.720
They do.
link |
01:48:40.720
It's the recognition, the funding, you know.
link |
01:48:43.200
And also inspiration for, like I said, when I was a little kid, thinking about the Nobel
link |
01:48:47.580
Prize, like I didn't, you know, it inspires millions of young scientists.
link |
01:48:53.600
At the same time, there's a sadness to it a little bit that, especially in the field,
link |
01:48:59.200
like depending on the field, but experimental fields that involve teams of, I don't know,
link |
01:49:04.400
sometimes hundreds of brilliant people, the Nobel Prize is only given to just a handful.
link |
01:49:12.200
That's right.
link |
01:49:13.200
Is it maxed at three?
link |
01:49:14.760
Yeah.
link |
01:49:15.760
Yeah.
link |
01:49:16.760
And it's not even written in Alfred Nobel's will, it turns out.
link |
01:49:18.920
One of our teammates looked into it in a museum in Stockholm when we went there for Nobel
link |
01:49:23.960
Week in 2011.
link |
01:49:25.840
The leaders who got the prize formally knew that without the rest of us working hard in
link |
01:49:30.560
the trenches, the result would not have been discovered.
link |
01:49:35.080
So they invited us to participate in Nobel Week.
link |
01:49:37.560
And so one of the team members looked in the will and it's not there.
link |
01:49:41.320
It's just tradition.
link |
01:49:42.320
That's interesting.
link |
01:49:43.320
But it's archaic, you know, that's the way science used to be done.
link |
01:49:47.080
It's not the way a lot of science is done now.
link |
01:49:49.320
And you look at gravitational wave discovery, which was, you know, recognized with the Nobel
link |
01:49:54.700
Prize in 2017, Ray Weiss at MIT got it and Kip Thorne and Barry Barish at Caltech.
link |
01:50:03.720
And Ron Drever, one of the masterminds, had passed away earlier in the year.
link |
01:50:07.560
So again, one of the rules of Nobel is that it's not given posthumously, or at least the
link |
01:50:13.840
one exception might be if they've made their decision and they're busy making their press
link |
01:50:17.960
releases right before October, the first week in October or whatever, and then the person
link |
01:50:23.460
passes away.
link |
01:50:24.460
I think they don't change their minds then.
link |
01:50:25.920
But yeah, you know, it doesn't square with today's reality that a lot of science is done
link |
01:50:32.460
by big teams, in that case, a team of a thousand people.
link |
01:50:35.800
In our case, it was two teams consisting of about 50 people.
link |
01:50:40.160
And we used techniques that were arguably developed in part by people who, astrophysicists
link |
01:50:46.120
who weren't even on those two papers, I mean, some of them were, but other papers were written
link |
01:50:51.320
by other people, you know, and so it's like we're standing on the shoulders of giants.
link |
01:50:56.560
And none of those people was officially recognized.
link |
01:50:59.520
And to me, it was okay.
link |
01:51:01.800
You know, again, it was the thrill of doing the work and ultimately the work, the discovery
link |
01:51:06.560
was recognized with the prize.
link |
01:51:08.760
And you know, we got to participate in Nobel week and, you know, it's okay with me.
link |
01:51:14.360
I've known other physicists whose lives were ruined because they did not get the Nobel
link |
01:51:20.500
prize and they felt strongly that they should have.
link |
01:51:23.840
Ralph Alpher of the Alpher beta gamma paper predicting the microwave background radiation,
link |
01:51:31.560
we should have gotten it.
link |
01:51:33.400
His advisor Gamoff was dead by that point.
link |
01:51:36.600
But you know, Penzias and Wilson got it for the discovery and an Alpher, apparently from
link |
01:51:42.560
colleagues who knew him well, I've talked to them.
link |
01:51:45.120
His life was ruined by this.
link |
01:51:46.760
He just, it just not at his innards so much.
link |
01:51:50.840
It's very possible that in a small handful of people, even three, that you would be one
link |
01:51:56.040
of the Nobel, one of the winners of the Nobel prize.
link |
01:51:59.440
That doesn't weigh heavy on you.
link |
01:52:00.920
Well, you know, there were the two team leaders, Saul Perlmutter and Brian Schmidt.
link |
01:52:05.080
And usually there's the team leaders that are recognized.
link |
01:52:07.600
And then Adam Rees was my postdoc.
link |
01:52:10.520
First author, I guess.
link |
01:52:11.520
Yeah.
link |
01:52:12.520
First author.
link |
01:52:13.520
I was second author of that paper.
link |
01:52:14.520
Yeah.
link |
01:52:15.520
So I was his direct mentor at the time.
link |
01:52:16.520
Although he was, you know, one of these people who just, you know, runs with things.
link |
01:52:19.920
He was an MIT undergraduate by the way, Harvard graduate student, and then a postdoc as a
link |
01:52:26.200
so called Miller fellow for basic research and science at Berkeley, something that I
link |
01:52:30.840
was back in 84 to 86.
link |
01:52:33.240
But you're, you know, you're largely a free agent, but he worked quite closely with me
link |
01:52:37.680
and he came to Berkeley to work with me and on Schmidt's team, he was charged with analyzing
link |
01:52:43.000
the data and he measured the brightnesses of these distant supernovae showing that they're
link |
01:52:48.440
fainter and thus more distant than anticipated.
link |
01:52:51.480
And that led to this conclusion that the universe had to have accelerated in order to push them
link |
01:52:56.420
out to such great distances.
link |
01:52:58.520
And I was shocked when he showed me the data, the results of his calculations and measurements.
link |
01:53:04.800
But it's very, you know, so he deserved it.
link |
01:53:07.000
And on Sol's team, Gerson Goldhaber deserved it.
link |
01:53:10.440
But he died, I think a year earlier in 2010, but that would have been four.
link |
01:53:14.840
And so, and me, well, I was on both teams, but, you know, was I number four, five, six,
link |
01:53:21.720
seven?
link |
01:53:22.720
I don't know.
link |
01:53:23.720
It's also very, so if I were to, it's possible that you're, I mean, I can make a very good
link |
01:53:28.800
case for urine in the three.
link |
01:53:31.400
And does that, is that psychologically, I mean, listen, it weighs on me a little bit
link |
01:53:38.440
because I don't know what to do with that.
link |
01:53:44.560
Perhaps it should motivate the rethinking, like Time magazine started doing like, you
link |
01:53:51.120
know, person of the year and like they would start doing like concepts and almost like
link |
01:53:56.120
the black hole gets the Nobel prize or the universe gets the Nobel prize and here's the
link |
01:54:02.380
list of people.
link |
01:54:03.800
So like, or like the Oscar that you could say, because it's a team effort now and it
link |
01:54:11.160
should be redone.
link |
01:54:12.160
And the breakthrough prize in fundamental physics, which was started by Yuri Milner
link |
01:54:16.360
and Zuckerberg is involved in others as well, you know, uh, they recognize the larger team.
link |
01:54:22.080
Yeah, they, they recognize teams.
link |
01:54:24.440
And so in fact, both teams in the accelerating universe were recognized with the breakthrough
link |
01:54:28.840
prize in 2015.
link |
01:54:31.480
Nevertheless, the same three people, Reese Perlmutter and Schmidt got the red carpet
link |
01:54:37.720
rolled out for them and were at the big ceremony and shared half of the prize money.
link |
01:54:43.480
And the rest of us, roughly 50 shared the other half and didn't get to go to the ceremony.
link |
01:54:48.240
So, but I, I feel for them, I mean, for the gravitational waves, it was a thousand people.
link |
01:54:52.880
What are they going to do?
link |
01:54:53.880
Invite everyone for the Higgs particle.
link |
01:54:55.980
It was six to 8,000 physicists and engineers.
link |
01:54:58.760
In fact, because of the whole issue of who gets it experimentally, that discovery still
link |
01:55:04.500
has not been recognized, right?
link |
01:55:06.620
The theoretical work by Peter Higgs and, uh, Anglaire got recognized, but there was a troika
link |
01:55:13.240
of other people who perhaps wrote the most complete paper and they were, they were left
link |
01:55:18.240
out and, um, another guy died, you know, and
link |
01:55:22.360
it's hard.
link |
01:55:23.360
It's all of his heartbreak.
link |
01:55:24.360
And some people argue that the Nobel prize has been diluted too, because if you look
link |
01:55:28.400
at Roger Penrose, you can make an argument that he should get the prize by himself.
link |
01:55:33.600
Like it's just separate those, like he could have and should have, perhaps he should have
link |
01:55:37.720
perhaps gotten it with Hawking before Hawking's death, right?
link |
01:55:41.720
The problem was Hawking radiation had not been detected, but you could argue that Hawking
link |
01:55:46.320
made enough other fundamental contributions to the theoretical study of black holes and
link |
01:55:52.240
the observed data were already good enough at the time of before Hawking's death.
link |
01:55:57.920
Okay.
link |
01:55:58.920
I mean, the latest results by Reinhard Genzel's group is that they see the time dilation effect
link |
01:56:03.280
of a star that's passing very close to the black hole in the middle of our galaxy.
link |
01:56:07.680
That's cool, but, and it adds additional evidence, but hardly anyone doubted the existence of
link |
01:56:13.240
the supermassive black hole and Andrea Gaz's group, I believe hadn't yet shown that relativistic
link |
01:56:18.880
effect and yet she got part of the prize as well.
link |
01:56:21.060
So clearly it was given for the, the original evidence that was really good.
link |
01:56:25.560
And that evidence is at least a decade old, you know, so one could make the case for,
link |
01:56:30.320
for Hawking, one could make the case that in 2016, when Mayor and Caloz won the Nobel
link |
01:56:37.460
Prize for the discovery of the first exoplanet, 51B Pegasi, well, there was a fellow at Penn
link |
01:56:45.560
State, Alex Wolszczan, who in 1992, three years preceding 1995, found a planet orbiting
link |
01:56:55.000
a pulsar, a very weird kind of star, a neutron star, and that wouldn't have been a normal
link |
01:56:59.920
planet.
link |
01:57:00.920
Sure.
link |
01:57:01.920
And so the Nobel committee, you know, they gave it for the discovery of planets around
link |
01:57:05.840
normal sun like stars, but, but hell, you know, Wolszczan found a planet so they could
link |
01:57:11.160
have given it to him as the third person instead of to Jim Peebles for the development of what's
link |
01:57:16.520
called physical cosmology.
link |
01:57:18.360
He's at Princeton, he deserved it, but they could have given Nobel for the development
link |
01:57:22.860
of physical cosmology to Peebles and I would claim some other people were pretty important
link |
01:57:27.920
in that development as well.
link |
01:57:29.000
You know, and they could have given it some other year.
link |
01:57:32.600
So there's, there's a lot of controversy.
link |
01:57:35.040
I try not to dwell on it.
link |
01:57:36.600
Was I number three?
link |
01:57:37.760
Probably not.
link |
01:57:38.760
You know, Adam Riess did the work.
link |
01:57:40.680
You know, I helped bounce ideas off of him, but we wouldn't have had the result without
link |
01:57:46.040
him.
link |
01:57:47.040
Yeah.
link |
01:57:48.040
And I was on both teams for reasons, I mean, you know, I, the style of the first team,
link |
01:57:53.360
the supernova cosmology project didn't match mine.
link |
01:57:56.320
They came largely from experimental high energy particle physics, physics where there's these
link |
01:58:00.520
hierarchical teams and stuff and it's hard for the little guy to have a say, at least
link |
01:58:05.440
that's what I kind of thought.
link |
01:58:06.960
Whereas the team of astronomers led by Brian Schmidt was first of all, a bunch of my friends
link |
01:58:12.200
and they grew up as astronomers making contributions on little teams and we decided to band together,
link |
01:58:18.320
but all of us had our voices heard.
link |
01:58:20.440
So it was sort of a culture, a style that I preferred really.
link |
01:58:25.480
But let me tell you a story at the Nobel banquet, okay?
link |
01:58:30.240
I'm sitting there between two physicists who are members of the committee of the Swedish
link |
01:58:35.020
National Academy of Sciences, you know, and I strategically kept, you know, offering them
link |
01:58:39.920
wine and stuff during this long drawn out Nobel ceremony, right?
link |
01:58:45.080
And I got them to be pretty talkative and then in a polite diplomatic way, I started
link |
01:58:50.080
asking them pointed questions and basically they admitted that if there are four or more
link |
01:58:55.840
people equally deserving, they wait for one of them to die or they just don't give the
link |
01:59:01.600
prize at all when it's unclear who the three are, at least unclear to them.
link |
01:59:07.040
But unclear to them, they're not even right part of the time.
link |
01:59:12.400
I mean, Jocelyn Bell discovered pulsars with a radio antenna, a set of radio antennas that
link |
01:59:20.920
her advisor Anthony Hewish conceived and built, so he deserves some credit, but he didn't
link |
01:59:28.800
discover the pulsar.
link |
01:59:30.520
She did.
link |
01:59:31.520
And his initial reaction to the data that she showed him was a condescending rubbish,
link |
01:59:38.400
my dear.
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01:59:39.400
Yeah, I'm not kidding.
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01:59:41.400
Now, I know Jocelyn Bell and she did not let this destroy her life.
link |
01:59:46.960
She won every other prize under the sun, okay?
link |
01:59:51.080
Vera Rubin, arguably one of the discoverers of dark matter, although there, if you look
link |
01:59:57.320
at the history, there were a number of people and that was the issue, I think there were
link |
02:00:00.520
a number of people, four or more who had similar data and similar ideas at about the same time.
link |
02:00:06.480
Rubin won every prize under the sun, the new big large scale survey telescope being built
link |
02:00:12.440
in Chile is being renamed the Vera Rubin Telescope because she passed away in December of 2015,
link |
02:00:19.080
I think.
link |
02:00:21.880
You know, it'll conduct this survey, large scale survey with the Rubin Telescope.
link |
02:00:26.620
So she's been recognized, but never with the Nobel Prize.
link |
02:00:30.120
And I would say that to her credit, she did not let that consume her life either.
link |
02:00:36.000
And perhaps it was a bit easier because there had been no Nobel given for the discovery
link |
02:00:41.200
of dark matter, whereas in the case of pulsars and Jocelyn Bell, there was a prize given
link |
02:00:46.840
for the discovery of the freaking pulsars and she didn't get it.
link |
02:00:50.560
Well, I mean, what a travesty of justice.
link |
02:00:53.080
So I also think as a fan of fiction, as a fan of stories that the travesty and the tragedy
link |
02:01:01.840
and the unfairness and the tension of it is what makes the prize and similar prizes beautiful.
link |
02:01:11.240
The decisions of other humans that result in dreams being broken and, you know, like
link |
02:01:19.200
that's why we love the Olympics as so many, you know, people, athletes give their whole
link |
02:01:24.600
life for this particular moment and then there's referee decisions and like little slips of
link |
02:01:31.280
here and there, like the little misfortunes that destroy entire dreams.
link |
02:01:36.400
And that's, it's, it's weird to say, but it feels like that makes the entirety of it even
link |
02:01:42.360
more special.
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02:01:43.360
Yeah.
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02:01:44.360
If it was perfect, it wouldn't be interesting.
link |
02:01:46.720
Humans like competition and they like heroes and unfortunately it gives the impression
link |
02:01:51.160
to youngsters today that science is still done by white men with gray beards wearing
link |
02:01:57.720
white lab coats.
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02:01:59.200
And I'm very pleased to see that this year, you know, Andrea Ghez, the fourth woman in
link |
02:02:04.080
the history of the physics prize to have received it.
link |
02:02:07.520
And then two women, one at Berkeley, one elsewhere won the Nobel prize in chemistry without any
link |
02:02:14.000
male co recipient.
link |
02:02:16.040
And so that's sending a message I think to girls that they can do science and they have
link |
02:02:21.400
role models.
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02:02:23.600
I think the breakthrough prize and other such prizes show that teams get recognized as well.
link |
02:02:31.240
And if you pay attention to the newspapers, you know, most of the good authors like, you
link |
02:02:37.120
know, Dennis Overby of the New York Times and others said that these were teams of people
link |
02:02:41.520
and they, they emphasize that and, you know, they all played a role.
link |
02:02:46.040
And you know, maybe if some grad student hadn't soldered some circuit, maybe the whole thing
link |
02:02:49.920
wouldn't have worked, you know.
link |
02:02:52.220
But still, you know, Ray Weiss and Kip Thorne was the theoretical, you know, impetus for
link |
02:02:59.800
the whole search for gravitational waves, Barry Barish brought the MIT and Caltech teams
link |
02:03:05.860
together to get them to cooperate at a time when the project was nearly dead from what
link |
02:03:11.080
I understand and contributed greatly to the experimental setup as well.
link |
02:03:16.120
He's a great experimental physicist, but he was really good at bringing these two teams
link |
02:03:20.280
together instead of having them duke it out in blows and leaving both of them bleeding
link |
02:03:24.280
and dying.
link |
02:03:25.280
You know, the National Science Foundation was going to cut the funding from what I understand,
link |
02:03:29.680
you know.
link |
02:03:30.680
So, so there's human drama involved in this whole thing.
link |
02:03:33.880
And the Olympics, yeah, you know, a runner, a swimmer, a runner, runner, you know, they
link |
02:03:38.960
slip just at the moment that they were taking off from the first thing and that costs them
link |
02:03:43.720
some fraction of a second and that's it.
link |
02:03:46.400
They didn't win, you know.
link |
02:03:47.560
And in that case, I mean, the coaches, the families, which I met a lot of Olympic athletes
link |
02:03:53.920
and the coaches and the families of the athletes are really the winners of the medals.
link |
02:04:01.280
But they don't get the medal and it's, you know, credit assignment is a fascinating thing.
link |
02:04:06.240
I mean, that's the full human story we have.
link |
02:04:10.040
And outside of prizes, it's fascinating.
link |
02:04:13.520
I mean, just to be in the middle of it for artificial intelligence, there's a field of
link |
02:04:18.080
deep learning.
link |
02:04:19.080
That's really exciting.
link |
02:04:20.080
And people have been, there's yet another award, the touring awards given for deep learning
link |
02:04:26.320
to three folks who are very much responsible for the field, but so are a lot of others.
link |
02:04:32.560
Yeah, that's right.
link |
02:04:33.960
And there's a few, there's a, there's a fellow by the name of Schmidt Huber who sort of symbolizes
link |
02:04:43.480
the, the forgotten folks in the deep learning community.
link |
02:04:48.880
But you know, that's, that's the unfortunate sad thing where you remember, remember Isaac
link |
02:04:55.040
Newton or remember these, these, these special figures and the ones that flew close to them,
link |
02:05:04.080
we forget.
link |
02:05:05.080
Well, that's right.
link |
02:05:06.080
And you know, often the breakthroughs are made based on the body of knowledge that had
link |
02:05:10.220
been assimilated prior to that.
link |
02:05:13.320
But you know, again, people like to worship heroes.
link |
02:05:15.840
You mentioned the Oscars earlier and you know, you look at the direct, I mean, well, I mean,
link |
02:05:21.800
okay, directors and stuff sometimes get awards and stuff, but you know, you look at even
link |
02:05:26.520
something like, I don't know, songwriters, musicians, Elton John or something, right?
link |
02:05:30.320
Bernie Taupin, right?
link |
02:05:32.240
Wrote many of the words or he's not as well known or the Beatles or something like that.
link |
02:05:39.800
I was heartbroken to learn that Elvis didn't write most of the songs.
link |
02:05:43.400
Yeah, Elvis.
link |
02:05:44.400
That's right.
link |
02:05:45.400
There you go.
link |
02:05:46.400
But he was the king, right?
link |
02:05:47.400
And he had such a personality and it was such a performer, right?
link |
02:05:50.840
But it's the unsung heroes in many cases.
link |
02:05:53.880
Yeah.
link |
02:05:54.880
So maybe taking a step back, we talked about the Nobel prize of the accelerating universe,
link |
02:06:00.480
but your work and the ideas around supernova were important in detecting this accelerating
link |
02:06:11.040
universe.
link |
02:06:12.040
Can we go to the very basics of what is this beautiful, mysterious object of a supernova?
link |
02:06:17.480
Right.
link |
02:06:18.480
So a supernova is an exploding star.
link |
02:06:21.160
Most stars die a relatively quiet death, our own sun, well, despite the fact that it'll
link |
02:06:25.660
become a red giant and incinerate earth, it'll do that reasonably slowly.
link |
02:06:30.360
But there's a small minority of stars that end their lives in a Titanic explosion.
link |
02:06:35.860
And that's not only exciting to watch from afar, but it's critical to our existence because
link |
02:06:40.880
it is in these explosions that the heavy elements synthesize through nuclear reactions during
link |
02:06:46.960
the normal course of the star's evolution and during the explosion itself, get injected
link |
02:06:52.640
into the cosmos, making them available as raw material for new stars, planets, and ultimately
link |
02:06:59.560
life.
link |
02:07:00.560
And that's just a great story, the best in some ways.
link |
02:07:04.880
So we like to study these things and our origins, but it turns out these are incredibly useful
link |
02:07:11.040
beacons as well, because if you know how powerful an exploding star really is by measuring the
link |
02:07:19.640
apparent brightness at its peak in galaxies whose distances we already know through having
link |
02:07:25.680
made other measurements, and you can thus calibrate how powerful the thing really is,
link |
02:07:32.040
and then you find ones that are much more distant, then you can use their observed brightness
link |
02:07:38.360
compared with their true intrinsic power or luminosity to judge their distance and hence
link |
02:07:43.780
the distance of the galaxy in which they're located.
link |
02:07:49.160
Let me just give this one analogy.
link |
02:07:51.980
You judge the distance of an oncoming car at night by looking at how bright its headlights
link |
02:07:57.160
appear to be, and you've calibrated how bright the headlights are of a car that's two or
link |
02:08:02.600
three meters away of known distance, and you go, oh, that's a faint headlight, and so that's
link |
02:08:07.760
pretty far away.
link |
02:08:09.120
You also use the apparent angular separation between the two headlights as a consistency
link |
02:08:14.120
check in your brain, but that's what your brain is doing.
link |
02:08:16.720
So we can do that for cars, we can do that for stars.
link |
02:08:19.760
Nice, I like that.
link |
02:08:21.720
But you know, with cars, the headlights are all, there's some variation, but they're somewhat
link |
02:08:28.480
similar so you can make those kinds of conclusions.
link |
02:08:32.480
How much variation is there between supernova that you can detect them?
link |
02:08:38.880
Right, so first of all, there are several different ways that stars can explode, and
link |
02:08:42.800
it depends on their mass and whether they're in a binary system and things like that.
link |
02:08:47.540
And the ones that we used for these cosmological purposes, studying the expansion of the history
link |
02:08:52.840
of the universe, are the so called type Roman numeral I, lowercase a, type Ia supernovae.
link |
02:09:00.560
They come from a weird type of a star called a white dwarf.
link |
02:09:04.340
Our own sun will turn into a white dwarf in about seven billion years.
link |
02:09:09.080
It'll have about half its present mass compressed into a volume just the size of Earth.
link |
02:09:14.920
So that's an inordinate density, okay?
link |
02:09:17.120
It's incredibly dense.
link |
02:09:18.880
And the matter is what's called by quantum physicists degenerate matter, not because
link |
02:09:23.400
it's morally reprehensible or anything like that, but this is just the name that quantum
link |
02:09:28.400
physicists give to electrons that are squeezed into a very tight space.
link |
02:09:33.000
The electrons take on a motion due to Heisenberg's uncertainty principle, and also due to the
link |
02:09:39.240
Pauli exclusion principle that electrons don't like to be in the same place, they like to
link |
02:09:43.860
avoid each other.
link |
02:09:44.860
And those two things mean that a lot of electrons are moving very rapidly, which gives the star
link |
02:09:50.280
an extra pressure far above the thermal pressure associated with just the random motions of
link |
02:09:56.040
particles inside the star.
link |
02:09:57.920
So it's a weird type of star, but normally it wouldn't explode and our sun won't explode,
link |
02:10:04.680
except that if such a white dwarf is in a pair with another more or less normal star,
link |
02:10:10.240
it can steal material from that normal star until it gets to an unstable limit, roughly
link |
02:10:18.760
one and a half times the mass of our sun, 1.4 or so.
link |
02:10:22.460
This is known as the Chandrasekhar limit after Subramanian Chandrasekhar, an Indian astrophysicist
link |
02:10:29.200
who figured this out when he was about 20 years old on a voyage from India to England
link |
02:10:34.960
where he was to be educated.
link |
02:10:37.000
And then he did this and then 50 years later he won the Nobel Prize in physics in 1984
link |
02:10:42.520
largely for this work that he did as a youngster who was on his way to be educated.
link |
02:10:48.600
And his advisor, the great Arthur Eddington in England, who had done a lot of great things
link |
02:10:54.440
and was a great astrophysicist, nevertheless, he too was human and had his faults.
link |
02:10:59.640
He ridiculed Chandra's scientific work at a conference in England and most of us, if
link |
02:11:07.400
we had been Chandra, would have just given up astrophysics at that time when the great
link |
02:11:12.760
Arthur Eddington ridicules our work.
link |
02:11:16.880
That's another inspirational story for the youngster.
link |
02:11:19.960
Just keep going.
link |
02:11:20.960
But anyway, no matter what your advisor says or don't always pay attention to your advisor.
link |
02:11:28.960
Don't lose hope if you really think you're onto something.
link |
02:11:32.520
That doesn't mean never listen to your advisor.
link |
02:11:34.360
They may have sage advice as well.
link |
02:11:36.720
But anyway, when a white dwarf grows to a certain mass, it becomes unstable.
link |
02:11:43.540
And one of the ways it can end its life is to go through a thermonuclear runaway.
link |
02:11:48.960
So basically, the carbon nuclei inside the white dwarf start fusing together to form
link |
02:11:54.960
heavier nuclei.
link |
02:11:56.880
And the energy that those fusion reactions emit doesn't go into being dissipated out
link |
02:12:06.800
of the star or expanding it the way if you take a blowtorch to the middle of the Sun,
link |
02:12:14.120
you heat up its gases, the gases would expand and cool.
link |
02:12:17.640
But this degenerate star can't expand and cool.
link |
02:12:21.240
And so the energy pumped in through these fusion reactions goes into making the nuclei
link |
02:12:27.200
move faster.
link |
02:12:28.560
And that gets more of them sufficiently close together that they can undergo nuclear fusion,
link |
02:12:33.880
thereby releasing more energy that goes into speeding up more nuclei.
link |
02:12:38.880
And thus you have a runaway, a bomb, an uncontrolled fusion reactor instead of the controlled fusion,
link |
02:12:46.440
which is what our Sun does.
link |
02:12:48.360
Our Sun is a marvelous controlled fusion reactor.
link |
02:12:51.420
This is what we need here on Earth, fusion energy to solve our energy crisis, right?
link |
02:12:56.280
But the Sun holds the stuff in through gravity and you need a big mass to do that.
link |
02:13:01.100
So this uncontrolled fusion reaction blows up a star that's pretty much the same in
link |
02:13:07.600
all cases.
link |
02:13:09.640
And you measure it to be almost the same in all cases.
link |
02:13:13.000
But the devil is in the details, and in fact, we observe them to not be all the same.
link |
02:13:18.940
And theoretically, they might not be all the same because the rate of the fusion reactions
link |
02:13:23.360
might depend on the amount of trace heavier elements in the white dwarf.
link |
02:13:28.600
And that could depend on how old it is, whether it was born billions of years ago when there
link |
02:13:33.440
weren't many heavier elements or whether it's a relatively young white dwarf and all
link |
02:13:38.300
kinds of other things.
link |
02:13:40.080
And part of my work was to show that indeed, not all the Type Ia's are the same.
link |
02:13:44.940
You have to be careful when you use them.
link |
02:13:47.520
You have to calibrate them.
link |
02:13:49.160
They're not standard candles the way it just, if all headlights or all candles were the
link |
02:13:55.460
same lumens or whatever, you'd say they're standard and then it would be relative.
link |
02:13:59.900
Standard candles is an awesome term, okay.
link |
02:14:01.940
Standard candles is what astronomers like to say, but I don't like that term because
link |
02:14:05.700
there aren't any standard candles, but there are standardizable candles.
link |
02:14:10.240
And by looking at these type Ia's, you look at enough of them in nearby galaxies whose
link |
02:14:17.800
distances you know independently.
link |
02:14:20.640
And what you can tell is that, you know, this is something that a colleague of mine, Mark
link |
02:14:25.220
Phillips did who was on Schmidt's team and arguably was one of the people who deserved
link |
02:14:30.560
the Nobel Prize.
link |
02:14:31.560
He showed that the intrinsically more powerful Type Ia's decline in brightness, and it turns
link |
02:14:39.720
out rise in brightness as well, more slowly than the less luminous Ia's.
link |
02:14:45.080
And so if you calibrate this by measuring a whole bunch of nearby ones and then you
link |
02:14:50.260
look at a distant one, instead of saying, well, it's a 100 watt Type Ia supernova, they're
link |
02:14:56.120
much more powerful than that by the way, plus or minus 50, you can say, no, it's a hundred
link |
02:15:01.440
and 12 plus or minus 15, or it's 84 plus or minus 17.
link |
02:15:08.940
It tells you where it is in the power scale and it greatly decreases the uncertainties.
link |
02:15:15.240
And that's what makes these things cosmologically useful.
link |
02:15:18.720
I showed that if you spread the light out into a spectrum, you can tell spectroscopically
link |
02:15:24.080
that these things are different as well.
link |
02:15:26.560
And in 1991, I happened to study two of the extreme peculiar ones, the low luminosity
link |
02:15:33.580
ones and the high luminosity ones, 1991BG and 1991T.
link |
02:15:40.560
This showed that not all the Ia's are the same.
link |
02:15:43.520
And indeed, at the time of 1991, I was a little bit skeptical that we could use Type Ia's
link |
02:15:50.520
because of this diversity that I was observing.
link |
02:15:53.120
But in 1993, Mark Phillips wrote a paper that showed this correlation between the light
link |
02:16:00.080
curve, the brightness versus time and the peak luminosity.
link |
02:16:03.760
Which gives you enough information to calibrate.
link |
02:16:05.920
Then they become calibratable and that was a game changer.
link |
02:16:08.280
How many Type Ia's are out there to use for data?
link |
02:16:12.320
Now there are thousands of them, but at the time, the high Z team had 16 and the supernova
link |
02:16:19.840
cosmology project had 40.
link |
02:16:22.640
But the 16 were better measured than the 40.
link |
02:16:25.840
And so our statistical uncertainties were comparable if you look at the two papers that
link |
02:16:31.080
were published.
link |
02:16:32.080
How does that make you feel that there's these gigantic explosions just sprinkled out there?
link |
02:16:38.760
Well, I certainly don't want one to be very nearby and it would have to be within something
link |
02:16:43.380
like 10 light years to be an existential threat.
link |
02:16:46.400
So they can happen in our galaxy?
link |
02:16:48.960
Oh yeah, yeah.
link |
02:16:49.960
So they would be okay?
link |
02:16:52.480
In most cases we'd be okay because our galaxy is 100,000 light years across.
link |
02:16:57.160
And you'd need one of these things to be within about 10 light years to be an existential
link |
02:17:01.360
threat.
link |
02:17:02.360
And it gives birth to a bunch of other stars, I guess?
link |
02:17:07.040
Yeah, it gives birth to expanding gases that are chemically enriched and those expanding
link |
02:17:11.060
gases mixed with other chemically enriched expanding gases or primordial clouds of hydrogen
link |
02:17:17.520
and helium.
link |
02:17:18.520
I mean, this is in a sense the greatest story ever told, right?
link |
02:17:24.800
I teach this introductory astronomy course at Berkeley and I tell them there's only five
link |
02:17:29.840
or six things that I want them to really understand and remember and I'm going to come to their
link |
02:17:34.660
deathbed and I'm going to ask them about this and if they get it wrong, I will retroactively
link |
02:17:39.020
fail and their whole career will have been shot.
link |
02:17:42.240
That's a student's worst nightmare.
link |
02:17:43.240
If they don't know and observe a total solar eclipse and yet they had the opportunity to
link |
02:17:46.680
do so, I will retroactively fail them.
link |
02:17:49.080
But one of them is, where did we come from?
link |
02:17:51.800
Where did the elements in our DNA come from?
link |
02:17:54.560
The carbon in our cells, the oxygen that we breathe, the calcium in our bones, the iron
link |
02:17:59.480
in our red blood cells.
link |
02:18:01.780
Those elements, the phosphorus in our DNA, they all came from stars, from nuclear reactions
link |
02:18:07.680
in stars and they were ejected into the cosmos and in some cases, like iron, made during
link |
02:18:15.280
the explosions and those gases drifted out, mixed with other clouds, made a new star or
link |
02:18:22.200
a star cluster, some of whose members then evolved and exploded, thus enriching the gases
link |
02:18:30.240
in the galaxy progressively more with time until finally, four and a half billion years
link |
02:18:35.120
ago from one of these chemically enriched clouds, our solar system formed with a rocky
link |
02:18:41.560
earthlike planet and somewhere, somehow, these self replicating, evolving molecules, bacteria
link |
02:18:49.440
formed and evolved through paramecia and amoebas and slugs and apes and us.
link |
02:18:58.940
And here we are, sentient beings that can ask these questions about our very origins
link |
02:19:05.040
and with our intellect and with the machines we make, come to a reasonable understanding
link |
02:19:12.540
of our origins.
link |
02:19:15.080
What a beautiful story.
link |
02:19:16.640
I mean, if that does not put you at least in awe, if not in love with science and its
link |
02:19:24.280
power of deduction, I don't know what will, right?
link |
02:19:30.100
It's one of the greatest stories, if not the greatest story.
link |
02:19:33.040
Obviously, that's personality dependent and all that, it's a subjective opinion, but it's
link |
02:19:38.040
perhaps the greatest story ever told.
link |
02:19:41.280
I mean, you could link it to the Big Bang and go even farther, right, to make an even
link |
02:19:45.040
more complete story, but as a subset, that's even in some ways a greater story than even
link |
02:19:51.600
the existence of the universe in some ways, because you could just imagine some really
link |
02:19:56.280
boring universe that never leads to sentient creatures such as ourselves.
link |
02:20:01.300
And is a supernova usually the introduction to that story?
link |
02:20:06.880
So are they usually the thing that launches the, is there other engines of creation?
link |
02:20:12.200
Well, the supernova is the one, I mean, I touch upon the subject earlier in my course,
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02:20:18.360
in fact, right about now in my lectures, because I talk about how our sun right now is fusing
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02:20:22.880
hydrogen to form helium nuclei and later it'll form carbon and oxygen nuclei, but that's
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02:20:29.440
where the process will stop for our sun, it's not massive enough, some stars that are more
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massive can go somewhat beyond that.
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02:20:37.060
So that's the beginning of this idea of the birth of the heavy elements, since they couldn't
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02:20:42.760
have been born at the time of the Big Bang, conditions of temperature and pressure weren't
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sufficient to make any significant quantities of the heavier elements.
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02:20:51.960
And so that's the beginning, but then you need some of these stars to explode, right?
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02:20:57.480
Because if those heavy elements remained forever trapped in the cores of stars, then they would
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not be available for the production of new stars, planets, and ultimately life.
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02:21:08.920
So indeed the supernova, my main area of interest, plays a leading role in this whole story.
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02:21:17.400
I saw that you got a chance to call Richard Feynman a mentor of yours when you were at
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Caltech.
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02:21:23.520
Yeah.
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02:21:24.520
Do you have any fond memories of Feynman, any lessons that stick with you?
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02:21:28.880
Oh yeah, he was quite a character and one of the deepest thinkers of all time probably,
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02:21:36.040
and at least in my life, the physicist who had the single most intuitive understanding
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02:21:42.840
of how nature works of anyone I've met.
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02:21:48.960
I learned a number of things from him, he was not my thesis advisor, I worked with Wallace
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02:21:53.240
Sargent at Caltech on what are called active galaxies, big black holes in the centers of
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02:21:58.140
galaxies that are accreting or swallowing material, a little bit like the stuff of this
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02:22:03.180
year's Nobel Prize in Physics 2020.
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02:22:06.860
But Feynman I had for two courses, one was general theory of relativity at the graduate
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level and one was applications of quantum physics to all kinds of interesting things.
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02:22:18.100
And he had this very intuitive way of looking at things that he tried to bring to his students
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02:22:28.880
and he felt that if you can't explain something in a reasonably simple way to a non scientist
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02:22:38.200
or at least someone who is versed a little bit with science but is not a professional
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02:22:43.680
scientist then you probably don't understand it very well yourself very thoroughly.
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02:22:49.420
So that in me made a desire to be able to explain science to the general public and
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02:22:58.400
I've often found that in explaining things, yeah, there's a certain part that I didn't
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02:23:02.580
really understand myself, that's one reason I like to teach the introductory courses to
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02:23:06.760
the lay public is that I sometimes find that my explanations are lacking in my own mind.
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02:23:12.700
So he did that for me.
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02:23:14.180
Is there a, if I could just pause for a second, you said he had one of the most intuitive
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02:23:18.220
understanding of nature.
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02:23:20.820
What if you could break apart what intuitive means, like is that on the philosophical level?
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02:23:26.940
No, sort of physical.
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02:23:28.580
How do you draw a mental picture or a picture on paper of what's going on?
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02:23:33.660
And he's perhaps most famous in this regard for his Feynman diagrams, which in what's
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02:23:39.000
called quantum electrodynamics, a quantum field theory of electricity and magnetism.
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02:23:44.140
What you have are actually an exchange of photons between charged particles and they
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02:23:48.800
might even be virtual photons if the particles are at rest relative to one another.
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02:23:55.500
And there are ways of doing calculations that are brute force that take pages on pages and
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02:24:00.140
pages of calculations.
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02:24:02.340
And Julian Schwinger developed some of the mathematics for that and won the Nobel prize
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02:24:06.780
for it.
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02:24:07.780
But Feynman had these diagrams that he made and he had a set of rules of what to do at
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02:24:12.500
the vertex.
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02:24:13.500
You'd have two particles coming together and then a particle going out and then two particles
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02:24:17.020
coming out again.
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02:24:18.020
And he'd have these rules associated when there were vertices and when there were particles
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02:24:22.100
splitting off from one another and all that.
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02:24:24.380
And it looked a little bit like a bunch of a hodgepodge at first.
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02:24:27.920
But to those who learned the rules and understood them, they saw that you could do these complex
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02:24:34.220
calculations in a much simpler way.
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02:24:37.340
And indeed, in some ways, Freeman Dyson had an even better knack for explaining really
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02:24:42.700
what quantum electrodynamics actually was.
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02:24:46.180
But I didn't know Freeman Dyson.
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02:24:48.300
I knew Feynman.
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02:24:49.300
Maybe he did have a more intuitive view of the world than Feynman did.
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02:24:52.920
But of the people I knew, Feynman was the most intuitive, most sort of, is there a picture?
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02:24:58.860
Is there a simple way you can understand this?
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02:25:01.980
In the path that a particle follows even, you can get the classical path, at least for
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02:25:10.580
a baseball or something like that, by using quantum physics if you want.
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02:25:14.700
But in a sense, the baseball sniffs out all possible paths.
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02:25:19.740
It goes out to the Andromeda galaxy and then goes to the batter.
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02:25:23.060
But the probability of doing that is very, very small because tiny little paths next
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02:25:28.420
door to any given path cancel out that path.
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02:25:32.500
And the ones that all add together, they're the ones that are more likely to be followed.
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02:25:38.940
And this actually ties in with Fermat's principle of least action and there are ideas in optics
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02:25:45.740
that go into this as well and just sort of beautifully brings everything together.
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02:25:50.620
But the particle sniffs out all possible paths.
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02:25:54.060
What a crazy idea.
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02:25:55.060
But if you do the mathematics associated with that, it ends up being actually useful, a
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02:26:00.980
useful way of looking at the world.
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02:26:02.540
So you're also, I mean, you're widely acknowledged as, I mean, outside of your science work as
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02:26:07.780
being one of the greatest educators in the world.
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02:26:12.500
And Feynman is famous for being that.
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02:26:16.140
Is there something about being a teacher that you...
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02:26:19.220
Well, it's very, very rewarding when you have students who are really into it.
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02:26:23.260
You know, going back to Feynman, at Caltech, I was taking these graduate courses and there
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02:26:29.220
were two of us, myself and Jeff Richmond, who's now a professor of physics at University
link |
02:26:34.140
of California, Santa Barbara, who asked lots of questions.
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02:26:38.100
And a lot of the Caltech students are nervous about asking questions.
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02:26:42.780
They want to save face.
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02:26:43.980
They seem to think that if they ask a question, their peers might think it's a stupid question.
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02:26:49.100
Well, I didn't really care what people thought and Jeff Richmond didn't either.
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02:26:52.620
We asked all these questions and in fact, in many cases, they were quite good questions
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02:26:57.300
and Feynman said, well, the rest of you should be having questions like this.
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02:27:00.660
And I remember one time in particular when he said to the rest of the class, why is it
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02:27:07.260
always these two?
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02:27:09.620
Aren't the rest of you curious about what I'm saying?
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02:27:12.020
Do you really understand it all that well?
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02:27:14.580
If so, why aren't you asking the next most logical question?
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02:27:17.980
No, you guys are too scared to ask these questions that these two are asking.
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02:27:23.300
So he actually invited us to lunch a couple of times where just the three of us sat and
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02:27:28.420
had lunch with one of the greatest thinkers of 20th century physics.
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02:27:33.540
And so, yeah, he rubbed off on me and, you know, you encourage questions as well, encourage
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02:27:38.220
questions, you know, and yeah, you know, definitely, I mean, you know, I encourage questions.
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02:27:45.140
I like it when students ask questions.
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02:27:46.980
I tell them that they shouldn't feel shy about asking a question.
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02:27:51.340
Probably half the students in the class would have that same question if they even understood
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02:27:55.580
the material enough to ask that question.
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02:27:58.460
Yeah.
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02:27:59.460
Curiosity is the first step of seeing the beauty of something.
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02:28:04.580
So yeah, and the question is the ultimate form of curiosity.
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02:28:10.180
Let me ask, what is the meaning of life?
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02:28:14.220
The meaning of life, you know, from a cosmologist's perspective or from a human perspective, personal,
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02:28:19.900
you know, life is what you make of it, really, right?
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02:28:23.300
It's each of us has to have our own meaning and it doesn't have to be.
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02:28:31.100
Well, I think that in many cases, meaning is to some degree associated with goals.
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02:28:36.220
You set some goals or expectations for yourself, things you want to accomplish, things you
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02:28:41.380
want to do, things you want to experience, and to the degree that you experience those
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02:28:47.100
and do those things, it can give you meaning.
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02:28:50.740
You don't have to change the world the way Newton or Michelangelo or da Vinci did.
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02:28:56.540
I mean, people often say, you changed the world, but look, come on, there's seven and
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02:29:00.180
a half, close to eight billion of us now.
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02:29:02.780
Most of us are not going to change the world and does that mean that most of us are leading
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02:29:06.300
meaningful lives?
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02:29:07.900
No, it just has to be something that gives you meaning, that gives you satisfaction,
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02:29:15.220
that gives you a good feeling about what you did.
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02:29:17.860
And often, based on human nature, which can be very good and also very bad, but often
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02:29:24.480
it's the things that help others that give us meaning and a feeling of satisfaction.
link |
02:29:31.800
You taught someone to read, you cared for someone who was terminally ill, you brought
link |
02:29:37.100
up a nice family, you brought up your kids, you did a good job, you put your heart and
link |
02:29:43.220
soul into it, you read a lot of books if that's what you wanted to do, had a lot of perspectives
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02:29:49.780
on life, you traveled the world if that's what you wanted to do.
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02:29:54.840
But if some of these things are not within reach, you're in a socioeconomic position
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02:30:00.260
where you can't travel the world or whatever, you find other forms of meaning.
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02:30:06.500
It doesn't have to be some profound, I'm going to change the world, I'm going to be
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02:30:13.660
the one who everyone remembers type thing, right?
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02:30:17.900
In the context of the greatest story ever told, like the fact that we came from stars
link |
02:30:26.100
and now we're two apes asking about the meaning of life, how does that fit together?
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02:30:31.500
How does that make any sense?
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02:30:34.780
It does, it does, and this is sort of what I was referring to, that it's a beautiful
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02:30:39.700
universe that allows us to come into creation, right?
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02:30:46.820
It's a way that the universe found of knowing, of understanding itself, because I don't
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02:30:52.780
think that inanimate rocks and stars and black holes and things have any real capability
link |
02:31:00.420
of abstract thoughts and of learning about the rest of the universe or even their origins.
link |
02:31:08.260
I mean, they're just a pile of atoms that has no conscience, has no ability to think,
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02:31:16.060
has no ability to explore, and we do.
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02:31:20.620
And I'm not saying we're the epitome of all life forever, but at least for life on Earth
link |
02:31:27.940
so far the evidence suggests that we are the epitome in terms of the richness of our thoughts,
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02:31:36.060
the degree to which we can explore the universe, do experiments, build machines, understand
link |
02:31:42.180
our origins.
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02:31:43.180
And I just hope that we use science for good, not evil, and that we don't end up destroying
link |
02:31:50.300
ourselves.
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02:31:51.300
I mean, the whales and dolphins are plenty intelligent.
link |
02:31:54.320
They don't ask abstract questions, they don't read books, but on the other hand, they're
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02:31:59.180
not in any danger of destroying themselves and everything else as well.
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02:32:03.360
And so maybe that's a better form of intelligence, but at least in terms of our ability to explore
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02:32:10.100
and make use of our minds, I mean, to me, it's this.
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02:32:16.300
It's this that gives me the potential for meaning, right?
link |
02:32:21.740
The fact that I can understand and explore.
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02:32:24.520
It's kind of fascinating to think that the universe created us and eventually we've built
link |
02:32:31.560
telescopes to look back at it, to look back at its origins and to wonder how the heck
link |
02:32:38.500
the thing works.
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02:32:39.500
It's magnificent.
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02:32:40.500
It needn't have been that way, right?
link |
02:32:44.260
And this is one of the, you know, the multiverse sort of things.
link |
02:32:48.480
You know, you can alter the laws of physics or even the constants of nature, seemingly
link |
02:32:53.460
inconsequential things like the mass ratio of the proton and the neutron, you know, wake
link |
02:32:58.020
me up when it's over, right?
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02:32:59.720
What could be more boring?
link |
02:33:00.720
But it turns out you play with things a little bit like the ratio of the mass of the neutron
link |
02:33:04.900
to the proton and you generally get boring universes, only hydrogen or only helium or
link |
02:33:11.700
only iron.
link |
02:33:12.700
You can't even get the rich periodic table, let alone bacteria, paramecia, slugs and humans,
link |
02:33:19.020
okay?
link |
02:33:20.020
I'm not even anthropocentrizing this to the degree that I could.
link |
02:33:25.440
Even a rich periodic table wouldn't be possible if certain constants weren't this way, but
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02:33:33.060
they are.
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02:33:34.060
And that to me leads to the idea of a multiverse that, you know, the dice were thrown many,
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02:33:39.420
many times and there's this cosmic archipelago where most of the universes are boring and
link |
02:33:44.020
some might be more interesting.
link |
02:33:45.700
But we are in the rare breed that's really quite darn interesting.
link |
02:33:51.700
And if there were only one and maybe there is only one, well then that's truly amazing.
link |
02:33:57.060
We're lucky.
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02:33:58.060
We're lucky.
link |
02:33:59.060
But I actually think there are lots and lots, just like there are lots of planets.
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02:34:03.020
Earth isn't special for any particular reason.
link |
02:34:05.860
There are lots of planets in our solar system and especially around other stars.
link |
02:34:09.820
And occasionally there are going to be ones that are conducive to the development of complexity
link |
02:34:14.660
culminating in life as we know it.
link |
02:34:17.100
And that's a beautiful story.
link |
02:34:18.820
I don't think there's a better way to end it.
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02:34:21.660
Alex, it's a huge honor.
link |
02:34:23.100
One of my favorite conversations I've had in this podcast.
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02:34:25.300
Well, thank you so much for talking to us.
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02:34:27.580
For the honor of having been asked to do this.
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02:34:31.900
Thanks for listening to this conversation with Alex Filipenko, and thank you to our
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02:34:36.420
sponsors.
link |
02:34:37.420
Neuro, the maker of functional sugar free gum and mints that I use to give my brain
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02:34:41.940
a quick caffeine boost.
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02:34:44.040
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02:34:47.580
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02:34:58.460
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02:35:03.180
If you enjoy this thing, subscribe on YouTube, review it with 5 Stars and Apple Podcast,
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02:35:09.100
follow on Spotify, support on Patreon, or connect with me on Twitter at Lex Friedman.
link |
02:35:15.540
And now, let me leave you with some words from Carl Sagan.
link |
02:35:19.580
The nitrogen in our DNA, the calcium in our teeth, the iron in our blood, the carbon in
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02:35:26.880
our apple pies, were made in the interiors of collapsing stars.
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02:35:32.340
We are made of star stuff.
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02:35:36.060
Thank you for listening, and hope to see you next time.