WEBVTT - Is there a pattern to asteroid impacts on Earth?

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<v Speaker 1>Ay, Katie, what's the weather going to be like tomorrow?

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<v Speaker 1>And you're part of Italy, let me check. It says

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<v Speaker 1>it's going to be sunny with a chance of meatballs,

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<v Speaker 1>and you believe in that, or the weather prediction is

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<v Speaker 1>pretty reliable over there, not really. We're kind of near

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<v Speaker 1>the Alps and that seems to scramble whatever weather radar

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<v Speaker 1>that they use, So sometimes you plan a picnic and

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<v Speaker 1>sometimes you get meat balled on. It's sure would be

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<v Speaker 1>nice if the weather was more reliable, like it was

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<v Speaker 1>just a pattern and it repeated, like you could sort

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<v Speaker 1>of schedule the rain at like two pm and then

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<v Speaker 1>at three o'clock you get some snow. That would be awesome.

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<v Speaker 1>Or you know, you could also just try my strategy.

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<v Speaker 1>What's that? Just moved to a place where there isn't

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<v Speaker 1>any weather. It's just sunny every day. So essentially you're

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<v Speaker 1>going to move to the moon. Sometimes southern California does

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<v Speaker 1>feel like the moon? Is it because of all the

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<v Speaker 1>people just as alien? It's because of all the people

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<v Speaker 1>acting like aliens. Hi, I'm Daniel. I'm a particle physicist

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<v Speaker 1>and a professor at UC Irvine in Southern California, and

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<v Speaker 1>I definitely do appreciate the sunshine. My name is Katie.

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<v Speaker 1>I'm the host of Creature Feature and Animals podcast. I

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<v Speaker 1>live in northern Italy and I do appreciate that our

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<v Speaker 1>weather is mainly like pasta and pesto based. And I

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<v Speaker 1>know we're joking around, but is there an expression in

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<v Speaker 1>Italian that's something like a cloudy with a chance of meatballs?

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<v Speaker 1>Or is that a purely American thing? I think that's

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<v Speaker 1>pretty American. In fact, meatballs are not so much of

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<v Speaker 1>a thing in Italy. It's as much of the iconic

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<v Speaker 1>Italian food as it seems in the US that is

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<v Speaker 1>more kind of an Americanized version of Italy. So it's

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<v Speaker 1>neither on our plates nor in our weather. So there's

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<v Speaker 1>no like strange weather event that would make Italians say

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<v Speaker 1>it's raining meatballs, huge pieces of hail or something not

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<v Speaker 1>that I know of. Now, well, welcome to the podcast.

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<v Speaker 1>Daniel and Jorge explain the Universe, in which we examine

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<v Speaker 1>all of the crazy and amazing and surprising things that

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<v Speaker 1>the universe does. We dig into whether it all makes

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<v Speaker 1>sense and whether it can be predicted, whether we can

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<v Speaker 1>find simple scientific, mathematical stories that explain all of the

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<v Speaker 1>amazing things that the universe does, from compressing matter the

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<v Speaker 1>hearts of black holes, to whizzing corks and gluons together

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<v Speaker 1>inside neutron stars, to causing all of the weather patterns

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<v Speaker 1>on Earth, to maybe even wiping out huge parts of

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<v Speaker 1>life on the planet. This sounds fun. We try to

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<v Speaker 1>be an uplifting podcast as usual, though we don't shy

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<v Speaker 1>away from facing the truth and from accepting our ignorance

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<v Speaker 1>of it. My friend and usual co host Orge can't

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<v Speaker 1>be here today, but I'm very glad to be joined

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<v Speaker 1>by one of our regular co host Katie. Katie, thanks

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<v Speaker 1>again for joining us. Yeah. Absolutely. I noticed Jorge is

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<v Speaker 1>suspiciously absent the day we're talking about asteroid impacts, and

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<v Speaker 1>I gotta ask, does he got a secret space ship?

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<v Speaker 1>Maybe he's the one causing the asteroid impacts, you know,

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<v Speaker 1>he's the one dropping these things on the planet. Has

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<v Speaker 1>Jorge ever been in the same room with you as

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<v Speaker 1>the asteroid. No, but it does seem like sometimes he

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<v Speaker 1>does want to wipe everything out. But I love thinking

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<v Speaker 1>about the long history of life on Earth. You know,

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<v Speaker 1>we are curious beings. We look around ourselves here on

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<v Speaker 1>the planet. We wonder how do we get here? How

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<v Speaker 1>did the Earth end up to be this way and

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<v Speaker 1>not some other way? And one of the more fascinating

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<v Speaker 1>things about the history of life on Earth is how

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<v Speaker 1>much it hinges on certain tipping points, specific moments in history,

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<v Speaker 1>which if they had gone another way, we might not

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<v Speaker 1>be here, or we might look totally different, or we

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<v Speaker 1>might have to there's or three heads. It's fun to

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<v Speaker 1>imagine alternative earths. If you had run this experimental universe

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<v Speaker 1>many times and had different earths, what would life on

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<v Speaker 1>Earth look like at this point? Would there still be dinosaurs?

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<v Speaker 1>Would we all be huge intelligent ladybugs. It's fun to

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<v Speaker 1>imagine all the different varieties and what chance there was

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<v Speaker 1>for us to actually get here. I love the idea

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<v Speaker 1>of being huge intelligent ladybugs. I think we'd need a

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<v Speaker 1>lot more oxygen for that, But I think we would

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<v Speaker 1>also look much more fashionable. Do you think ladybugs, if

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<v Speaker 1>they developed intelligence and technology, would also develop clothing. I mean,

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<v Speaker 1>because they already look good naked. They already looked pretty fantastic.

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<v Speaker 1>But I can't imagine some sort of fashion revolution of

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<v Speaker 1>a ladybug who dares to wear stripes instead of thoughts

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<v Speaker 1>the Ladybug Fashion Podcast. Pretty controversial stuff, but it is

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<v Speaker 1>part of our job here, not just to understand what

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<v Speaker 1>are the basic rules of the universe. How do the

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<v Speaker 1>tiny particles come together and we've our reality out of

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<v Speaker 1>little corks and gluons and electrons or whatever other particles

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<v Speaker 1>might be out there. How does the dark matter shape

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<v Speaker 1>the formation of the universe. We also like to think

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<v Speaker 1>about the formation of life here on Earth and what

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<v Speaker 1>happened to create this story, What exactly led to us

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<v Speaker 1>being here having a podcast that isn't hosted by two ladybugs.

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<v Speaker 1>I mean, in a way, we are feasting on the

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<v Speaker 1>bones of dinosaurs because by their mass death came the

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<v Speaker 1>rise of mammals, and we are mammals, So we can

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<v Speaker 1>thank a dead dinosaur for being here, I think, in

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<v Speaker 1>my opinion, do you think that's like the best example

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<v Speaker 1>of inherited privilege ever? You know, It's like, we're not

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<v Speaker 1>responsible for the dinosaur's extinction directly, but we're definitely benefiting

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<v Speaker 1>from the fact that they were wiped out. Are you

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<v Speaker 1>saying that some kind of very early prehistoric shrew was

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<v Speaker 1>colluding with the asteroid and saying make it look like

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<v Speaker 1>an accident It certainly does seem convenient, right, you know,

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<v Speaker 1>when we benefit from the kinds of things. Well, hopefully

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<v Speaker 1>the dinosaurs of today, that is, birds will not sue us.

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<v Speaker 1>Statute of limitations is long, long, long expired. And one

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<v Speaker 1>fascinating thing about the history of life on Earth is

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<v Speaker 1>that it is punctuated with these mass extinctions. It's not

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<v Speaker 1>just the asteroid that hit the Earth that probably wiped

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<v Speaker 1>out the dinosaurs that created a new flowering of mammals.

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<v Speaker 1>There many times in the history of life on Earth

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<v Speaker 1>when there were these wipeout events where a huge fraction

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<v Speaker 1>of life on Earth was killed, making room for new developments,

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<v Speaker 1>new explorations of the evolutionary tree by the remaining life.

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<v Speaker 1>And it's interesting to think about how each of these

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<v Speaker 1>contribute to us being here today. Right, If all of

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<v Speaker 1>those hadn't gone exactly the way that they went, we

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<v Speaker 1>wouldn't be here talking about it. Maybe we wouldn't even

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<v Speaker 1>be any intelligent life on Earth. It would just be

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<v Speaker 1>a bunch of dumb dinosaurs ting on each other and

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<v Speaker 1>nibbling on plants, right, I mean, it's just hard to

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<v Speaker 1>know where things would have been. I mean, as you said,

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<v Speaker 1>like when there is a die off of animals, there

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<v Speaker 1>is an opportunity as long as the earth is still

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<v Speaker 1>habitable for a new kind of group, a resurgence of

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<v Speaker 1>species who otherwise would not be able to really thrive

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<v Speaker 1>because they'd be out competed by the animals that went extinct.

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<v Speaker 1>So it's hard to imagine, you know, if dinosaurs hadn't

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<v Speaker 1>died off, you know, maybe there would not have been

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<v Speaker 1>evolutionary pressure for any one species to become as intelligent

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<v Speaker 1>as humans. Maybe it would have been too dangerous a

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<v Speaker 1>life for primates to have been able to come to power.

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<v Speaker 1>It's just it's so hard to know. Of course, you know,

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<v Speaker 1>we could have also just been like two dinosaurs now

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<v Speaker 1>talking about stuff on the podcast, talking about like what

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<v Speaker 1>if we had gone extinct because of an asteroid? Would

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<v Speaker 1>some of those little shrews turned into weird pink things? Yea, exactly.

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<v Speaker 1>And I think there's something really interesting that you brought

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<v Speaker 1>up there that's not widely enough appreciated, which is the

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<v Speaker 1>importance of randomness and opportunity in evolution. You know, some

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<v Speaker 1>people feel like evolution is this transformation where species develop

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<v Speaker 1>into more and more advanced versions of themselves. But you know,

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<v Speaker 1>there's really a randomness there, Like how does the species

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<v Speaker 1>change from generation to generation. It's from like changes in

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<v Speaker 1>the genetic code, which comes from transcription errors or cosmic rays.

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<v Speaker 1>There's no design here. It's really just like a random

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<v Speaker 1>walk through genetic space. Right, It's like throwing a bunch

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<v Speaker 1>of dice to see what your kids are going to be. Like, yeah,

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<v Speaker 1>I mean, so evolution doesn't have a game plan. I

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<v Speaker 1>think that's one of the most important things to understand

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<v Speaker 1>is evolution is not this like efficient force perfecting things

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<v Speaker 1>into their most like quote unquote perfect forms. It's just

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<v Speaker 1>a very simple rule. If something survives and passes on

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<v Speaker 1>its genetic information, hooray, it's survived and passed on its

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<v Speaker 1>genetic information to the next that's it. That is absolutely it.

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<v Speaker 1>And for that extremely simple rule, you get incredibly marvelous complexity.

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<v Speaker 1>So there are a lot of things that can happen.

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<v Speaker 1>It's not just the random mutation of DNA. It's the

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<v Speaker 1>reshuffling of DNA. Right, you have like mate choice, what

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<v Speaker 1>happens there, And then it's the environment, like what happens

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<v Speaker 1>with your environment. There can be random changes in the

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<v Speaker 1>environment that leads to selective pressures, to extinction events, two

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<v Speaker 1>changes in related species that then causes the other species

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<v Speaker 1>to have to evolve. So there's so many factors that

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<v Speaker 1>go into evolution that from this incredibly simple rule just

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<v Speaker 1>like if you can pass on your DNA, yeah you

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<v Speaker 1>did it. You passed on your DNA, and then the

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<v Speaker 1>next generation gets a shot at that. That has turned

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<v Speaker 1>into just this incredibly immensely complex and convoluted situation with

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<v Speaker 1>life on Earth, where sometimes an animal will have weird

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<v Speaker 1>features that we try to look at, we think, what

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<v Speaker 1>is this, what is the thing? Why did they evolve it?

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<v Speaker 1>And it just turns out it's this weird artifact of

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<v Speaker 1>earlier evolution or something like you know, we have this

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<v Speaker 1>appendix and it's kind of mysterious. What does it do.

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<v Speaker 1>We're not really sure if it has much of a

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<v Speaker 1>purpose for us. But it's not like evolution has that

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<v Speaker 1>foresight of like, well, I better take this appendix out

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<v Speaker 1>because they're not really going to need it that much

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<v Speaker 1>as modern humans. So like, it's not an intelligent designer.

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<v Speaker 1>It's kind of just improv all the time. I think

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<v Speaker 1>that's a really fascinating aspect of it, not just that

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<v Speaker 1>there's a randomness there, but that it's so tightly linked

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<v Speaker 1>to the environment in which this exploration is happening. Right,

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<v Speaker 1>It's really a reflection. It's like a mirroring of the

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<v Speaker 1>situation that doing the selection because one animal might survive

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<v Speaker 1>very well in one context and just die off rapidly

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<v Speaker 1>in another, and so the animals, the life we have

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<v Speaker 1>here on Earth is a reflection of the selection pressure

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<v Speaker 1>which comes from the environment in which we live, of course, right,

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<v Speaker 1>But that goes also backwards in time. As you say,

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<v Speaker 1>it's like it's telling story of the selection pressure over time.

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<v Speaker 1>Every species that survives has survived through changing environments. Right,

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<v Speaker 1>Things were colder and then they were hotter, and in in

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<v Speaker 1>order to get here, you have to manage all of

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<v Speaker 1>those changes somehow. It's your population grows and evolves and

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<v Speaker 1>gains hair and lose his hair and all that kind

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<v Speaker 1>of stuff. So I think it's really fascinating that not

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<v Speaker 1>only does the earth itself tell the histories you like,

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<v Speaker 1>dig down through the layers and see layers of rock

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<v Speaker 1>and events that have happened through the history, but life

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<v Speaker 1>on Earth also carries with it the history of its evolution. Right,

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<v Speaker 1>As you say, why do you have this vestigial bid. Oh, well,

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<v Speaker 1>we needed that millions of years ago, and we're still

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<v Speaker 1>getting rid of it due to the new pressure. So

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<v Speaker 1>I think that's super fascinating to look at the history

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<v Speaker 1>of life on Earth, And to me, that's one of

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<v Speaker 1>the most important things about science is answering this question,

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<v Speaker 1>like how did we get here? What is the story

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<v Speaker 1>of us? It tells us sort of how to live

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<v Speaker 1>our lives and who we are, and in some sense,

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<v Speaker 1>you know, as much as science can, it tells us

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<v Speaker 1>why we're here at least what happened before we got here. Yeah,

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<v Speaker 1>And I think it's so interesting because our life spans

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<v Speaker 1>are relatively short compared to the universe, even compared to

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<v Speaker 1>our own Earth. So our perception of what is stable, right,

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<v Speaker 1>like what stable species are existence is warped by our

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<v Speaker 1>you know, relatively short lifespans, and so we have this

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<v Speaker 1>sense of things are as they are. Giraffes have always existed,

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<v Speaker 1>We've always existed, but that's really not the case. And

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<v Speaker 1>you know, when we look at some of these animals

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<v Speaker 1>that have gone extinct and we think, like, wow, how

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<v Speaker 1>could something that's strange have existed? Well, maybe hopefully if

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<v Speaker 1>we're still alive, and like a thousand years. Potentially some

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<v Speaker 1>species like the panda that's highly specialized to eat massive

0:12:48.720 --> 0:12:52.040
<v Speaker 1>quantities of bamboo, which makes it very vulnerable to extinction

0:12:52.280 --> 0:12:55.120
<v Speaker 1>if there's an environmental change, you know, we might look

0:12:55.160 --> 0:12:57.040
<v Speaker 1>back and say, like, how could such a silly animal

0:12:57.080 --> 0:13:01.400
<v Speaker 1>have existed where it's entire diet is dependent on bamboo

0:13:01.440 --> 0:13:04.840
<v Speaker 1>and they're really bad at mating in captivity. I think

0:13:04.880 --> 0:13:09.080
<v Speaker 1>we have this very narrow view in our own lifespan,

0:13:09.160 --> 0:13:12.040
<v Speaker 1>so it is it becomes kind of fascinating when we

0:13:12.160 --> 0:13:14.480
<v Speaker 1>zoom out and look at the history of the planet

0:13:14.520 --> 0:13:16.920
<v Speaker 1>and you're like, oh, yeah, we're just like little babies,

0:13:16.960 --> 0:13:20.079
<v Speaker 1>Like we're a little baby species. Yeah. And it's hard

0:13:20.120 --> 0:13:23.000
<v Speaker 1>for us because we tend to think in time scales

0:13:23.040 --> 0:13:28.000
<v Speaker 1>of hours, minutes, years, maybe centuries to understand processes that

0:13:28.120 --> 0:13:30.280
<v Speaker 1>go on that are much much slower. You know, it

0:13:30.280 --> 0:13:32.800
<v Speaker 1>took us a long time to appreciate how old the

0:13:32.800 --> 0:13:35.600
<v Speaker 1>Earth was. The first hints we had that it might

0:13:35.640 --> 0:13:38.880
<v Speaker 1>be billions of years old blew people's minds because it

0:13:38.960 --> 0:13:42.480
<v Speaker 1>was just such a strange concept. Understanding geological processes like

0:13:42.559 --> 0:13:46.160
<v Speaker 1>the formations of the continents and like glaciation work hard

0:13:46.240 --> 0:13:48.720
<v Speaker 1>for people because we don't tend to think in sort

0:13:48.760 --> 0:13:51.400
<v Speaker 1>of deep time, and yet we know that these processes

0:13:51.480 --> 0:13:54.520
<v Speaker 1>really do shape and influence the nature of the world

0:13:54.720 --> 0:13:57.240
<v Speaker 1>in which we live. And maybe most interesting and most

0:13:57.320 --> 0:14:00.800
<v Speaker 1>dramatic are the cataclysmic events, right is where if the

0:14:00.800 --> 0:14:03.840
<v Speaker 1>asteroid it hits somewhere different, maybe the dinosaurs wouldn't have

0:14:03.840 --> 0:14:06.320
<v Speaker 1>wiped out. Or if dinosaur scientists had looked up in

0:14:06.360 --> 0:14:09.679
<v Speaker 1>the sky and seen it coming and developed technology too diverted,

0:14:10.040 --> 0:14:12.520
<v Speaker 1>you know, then maybe things really would be different. I

0:14:12.559 --> 0:14:15.280
<v Speaker 1>love those moments when history could really take lots of

0:14:15.320 --> 0:14:19.920
<v Speaker 1>different courses. Yeah, dinosaur Matt Damon and a dinosaur Jennifer

0:14:19.960 --> 0:14:22.440
<v Speaker 1>Lawrence trying to figure things out. I wonder if the

0:14:22.440 --> 0:14:24.800
<v Speaker 1>dinosaur version of that movie would have been any better. Yeah,

0:14:24.800 --> 0:14:27.440
<v Speaker 1>I mean it is that. I do think about those

0:14:27.480 --> 0:14:30.600
<v Speaker 1>cataclysmic events quite a bit, you know, just the our

0:14:30.720 --> 0:14:33.840
<v Speaker 1>vulnerability of you know, as a single human, were relatively

0:14:33.920 --> 0:14:37.360
<v Speaker 1>vulnerable in our little fleshy bodies, but then our planet

0:14:37.400 --> 0:14:41.840
<v Speaker 1>also feels somewhat vulnerable just this like little paradise of

0:14:42.080 --> 0:14:46.040
<v Speaker 1>being able to be alive on it in a pretty

0:14:46.160 --> 0:14:51.160
<v Speaker 1>unforgiving universe. And then just that rock just traveling along

0:14:51.240 --> 0:14:55.520
<v Speaker 1>randomly could just you know, spell the end for an

0:14:55.680 --> 0:14:59.160
<v Speaker 1>entire planet of species. It's somewhat terrifying right to know

0:14:59.280 --> 0:15:01.600
<v Speaker 1>that these rocks are out there, and if one of

0:15:01.600 --> 0:15:03.600
<v Speaker 1>them falls into the gravity well of the Earth, it

0:15:03.720 --> 0:15:06.920
<v Speaker 1>could end all life on Earth, or some lives on Earth.

0:15:07.040 --> 0:15:09.840
<v Speaker 1>It certainly would not be a good day. And as

0:15:09.920 --> 0:15:12.960
<v Speaker 1>we saw in the nineties, these kind of things do happen,

0:15:13.120 --> 0:15:15.920
<v Speaker 1>like comic Shoemaker Levy, which came into the Solar System

0:15:16.000 --> 0:15:20.760
<v Speaker 1>smashed into Jupiter, creating fireballs bigger than planet Earth. So

0:15:20.840 --> 0:15:23.160
<v Speaker 1>this is not only something that happens than the deep

0:15:23.240 --> 0:15:25.760
<v Speaker 1>history of time, it's something that could happen. We don't

0:15:25.760 --> 0:15:29.400
<v Speaker 1>know when NASA is doing its best to track these asteroids,

0:15:29.400 --> 0:15:32.440
<v Speaker 1>but beyond that, we wonder, like, is it possible to

0:15:32.640 --> 0:15:35.960
<v Speaker 1>predict these events far in the future. Is there some

0:15:36.040 --> 0:15:39.720
<v Speaker 1>sort of like deep time process sort of like glaciation

0:15:40.120 --> 0:15:42.880
<v Speaker 1>or like formations of the continents which we can't yet

0:15:42.920 --> 0:15:45.680
<v Speaker 1>imagine because it happens on a galactic scale, which is

0:15:45.840 --> 0:15:50.080
<v Speaker 1>shaping these asteroid impacts, which is maybe creating patterns that

0:15:50.120 --> 0:15:53.120
<v Speaker 1>we could understand, which we could use to predict, so

0:15:53.160 --> 0:15:55.280
<v Speaker 1>we could know. Guys, we only got a million more

0:15:55.360 --> 0:15:58.680
<v Speaker 1>years before the next wave of killer asteroids. Better start

0:15:58.760 --> 0:16:01.640
<v Speaker 1>funding those spaceships. Yeah, I mean I'd like to know

0:16:01.920 --> 0:16:05.400
<v Speaker 1>because if an asteroid's coming in like the next year,

0:16:05.480 --> 0:16:09.120
<v Speaker 1>I know I can skip a dentist appointment. So don't

0:16:09.160 --> 0:16:13.600
<v Speaker 1>bother saving for retirement, folks. So on today's episode, we'll

0:16:13.600 --> 0:16:21.840
<v Speaker 1>be asking the question is there a pattern to major

0:16:21.960 --> 0:16:26.280
<v Speaker 1>asteroid impacts on Earth? And is it gonna benefit us

0:16:26.320 --> 0:16:30.040
<v Speaker 1>to know this or just make us scared? You can

0:16:30.080 --> 0:16:32.520
<v Speaker 1>short the stock market because you know all life on

0:16:32.600 --> 0:16:36.640
<v Speaker 1>Earth is going so put everything in gold, folks. This

0:16:36.720 --> 0:16:40.480
<v Speaker 1>is now a financial investment podcast. I believe that's illegal.

0:16:40.560 --> 0:16:43.520
<v Speaker 1>But also if the asteroid is made out of gold,

0:16:43.560 --> 0:16:46.200
<v Speaker 1>maybe you shouldn't invest in it because then we will

0:16:46.240 --> 0:16:50.240
<v Speaker 1>be inundated with gold and then also extremely dead. That's

0:16:50.280 --> 0:16:53.760
<v Speaker 1>not actual financial advice. Don't sue me. So you're saying

0:16:53.800 --> 0:16:56.840
<v Speaker 1>that when we're wiped out and the Ladybug civilization rises

0:16:56.920 --> 0:16:58.920
<v Speaker 1>up in our ashes, they're going to find so much

0:16:58.920 --> 0:17:01.480
<v Speaker 1>gold everywhere. It's just gonna be like they're paving their

0:17:01.560 --> 0:17:05.200
<v Speaker 1>streets in gold. Yeah, they're building their little Ladybug toilets

0:17:05.240 --> 0:17:07.800
<v Speaker 1>out of gold. So what is Ladybug Donald Trump then

0:17:07.880 --> 0:17:13.000
<v Speaker 1>going to do to make his bathroom extra bling well

0:17:13.040 --> 0:17:15.480
<v Speaker 1>as usual. I was wondering if people out there had

0:17:15.560 --> 0:17:18.480
<v Speaker 1>thought about if there was a pattern to major asteroid

0:17:18.560 --> 0:17:20.439
<v Speaker 1>impacts and if there was something we could do to

0:17:20.680 --> 0:17:24.000
<v Speaker 1>predict it. So thanks very much to everybody who participates

0:17:24.040 --> 0:17:26.960
<v Speaker 1>in these off the cuff answers on the virtual street.

0:17:27.040 --> 0:17:30.280
<v Speaker 1>If you would like to play this role for future episodes,

0:17:30.480 --> 0:17:32.879
<v Speaker 1>please don't be shy right to me. Two questions at

0:17:32.960 --> 0:17:35.240
<v Speaker 1>Daniel and Jorge dot com. So think about it for

0:17:35.240 --> 0:17:37.720
<v Speaker 1>a moment before you hear these answers. Do you think

0:17:37.800 --> 0:17:41.200
<v Speaker 1>there's a pattern to major asteroid impacts on Earth? Here's

0:17:41.200 --> 0:17:43.680
<v Speaker 1>what some listeners had to say. I think I heard

0:17:43.720 --> 0:17:46.600
<v Speaker 1>once it's like every thirty million years or something like that,

0:17:46.640 --> 0:17:50.240
<v Speaker 1>there's this massive asteroid that crashes into Earth and basically

0:17:50.240 --> 0:17:52.000
<v Speaker 1>wipes off all of the life on it. But I

0:17:52.000 --> 0:17:54.400
<v Speaker 1>don't really know. I don't think there's like any sort

0:17:54.440 --> 0:17:57.520
<v Speaker 1>of pattern to the distribution of asteroids. Those pods will

0:17:58.160 --> 0:18:00.919
<v Speaker 1>collide with Earth at some point in the post island,

0:18:01.160 --> 0:18:04.080
<v Speaker 1>so I don't think that there's a pattern of asteroid impacts.

0:18:04.080 --> 0:18:07.280
<v Speaker 1>It's orbital mechanics. Anything more than two bodies is pretty

0:18:07.320 --> 0:18:09.679
<v Speaker 1>chaotic and random, but I do think that there is

0:18:09.720 --> 0:18:13.520
<v Speaker 1>a governing frequency that decreases over time, so as our

0:18:13.600 --> 0:18:16.879
<v Speaker 1>Earth and Solar system get older, um impacts become less frequent.

0:18:17.119 --> 0:18:20.560
<v Speaker 1>I think you get some patterns with asteroids, because wouldn't

0:18:20.560 --> 0:18:24.240
<v Speaker 1>you get kind of like a cyclic almost resonant wave

0:18:24.320 --> 0:18:26.200
<v Speaker 1>function if you spend things up on a macro scale,

0:18:26.280 --> 0:18:28.520
<v Speaker 1>just since everything is orbiting, you could kind of mathematically

0:18:28.560 --> 0:18:31.760
<v Speaker 1>predict when it might fling stuff in our direction. I

0:18:31.800 --> 0:18:36.399
<v Speaker 1>don't know, well, hopefully if it's a pattern, it will

0:18:38.040 --> 0:18:43.600
<v Speaker 1>show us that no major asteroid will either art in

0:18:43.640 --> 0:18:49.080
<v Speaker 1>the future or until we are able to defend ourselves

0:18:49.720 --> 0:18:55.359
<v Speaker 1>properly to define them, because probably this is the most

0:18:55.400 --> 0:19:01.600
<v Speaker 1>difficult thing to just to see them in time for

0:19:01.680 --> 0:19:06.560
<v Speaker 1>us to prepare to do something about it. I really

0:19:06.600 --> 0:19:09.800
<v Speaker 1>do agree with the person who says that they hope

0:19:09.800 --> 0:19:13.200
<v Speaker 1>that no asteroid hits Earth until we're ready to defend ourselves,

0:19:13.240 --> 0:19:15.760
<v Speaker 1>because I feel like if we just learn like in

0:19:15.880 --> 0:19:17.840
<v Speaker 1>a hundred years we're going to get a big one,

0:19:17.920 --> 0:19:21.200
<v Speaker 1>but we have no way to do anything about it,

0:19:21.280 --> 0:19:23.040
<v Speaker 1>that would be a bit of a bomber. I'll be

0:19:23.119 --> 0:19:25.040
<v Speaker 1>honest with you, what do you mean we have no

0:19:25.080 --> 0:19:27.080
<v Speaker 1>way to do anything about it. You have no faith

0:19:27.119 --> 0:19:30.520
<v Speaker 1>in physicists and engineers to save the planet. It depends

0:19:30.560 --> 0:19:34.040
<v Speaker 1>on how fast you guys are at writing grant proposals.

0:19:34.080 --> 0:19:36.800
<v Speaker 1>I guess. So, if we've got an asteroid coming in

0:19:36.840 --> 0:19:38.719
<v Speaker 1>a hundred years, maybe you can do it. But if

0:19:38.720 --> 0:19:41.000
<v Speaker 1>it's like five weeks, do you think we could do

0:19:41.080 --> 0:19:43.760
<v Speaker 1>something about it? You know, the key really is to

0:19:43.920 --> 0:19:47.280
<v Speaker 1>discovering these things early on. If you see far in

0:19:47.359 --> 0:19:49.880
<v Speaker 1>advance that it's coming, that it only needs a little

0:19:49.920 --> 0:19:52.840
<v Speaker 1>bit of a push to not hit the Earth. It's

0:19:52.840 --> 0:19:55.320
<v Speaker 1>sort of like if somebody's firing a sniper shot from

0:19:55.359 --> 0:19:59.680
<v Speaker 1>five miles away, the tiniest little deviation in the direction

0:19:59.760 --> 0:20:02.240
<v Speaker 1>of their rifle means they're going to miss their target.

0:20:02.320 --> 0:20:04.119
<v Speaker 1>And so if you can figure out that this thing

0:20:04.200 --> 0:20:06.840
<v Speaker 1>is going to come in a hundred years, then even

0:20:06.840 --> 0:20:09.640
<v Speaker 1>the faintest little push, you could throw a rock at it,

0:20:09.840 --> 0:20:11.800
<v Speaker 1>or is that it with a laser, and they would

0:20:11.840 --> 0:20:14.480
<v Speaker 1>miss the Earth. You only have a few weeks of notice.

0:20:14.920 --> 0:20:16.840
<v Speaker 1>Then it's much much harder. You have to give it

0:20:16.880 --> 0:20:19.880
<v Speaker 1>a much bigger push. But actually, you know, this week,

0:20:20.000 --> 0:20:23.360
<v Speaker 1>as we record this episode, NASA is doing an amazing

0:20:23.480 --> 0:20:26.800
<v Speaker 1>test the dart probe is out there and it's about

0:20:26.840 --> 0:20:29.719
<v Speaker 1>to push on an asteroid to see if this works.

0:20:30.160 --> 0:20:32.679
<v Speaker 1>Can we actually find an asteroid and push on it

0:20:32.720 --> 0:20:35.520
<v Speaker 1>and see if we can change its direction. This is

0:20:35.560 --> 0:20:38.000
<v Speaker 1>not one that NASA thinks is going to hit the Earth.

0:20:38.080 --> 0:20:40.400
<v Speaker 1>This is just an experiment to see is it possible

0:20:40.440 --> 0:20:43.280
<v Speaker 1>to change its trajectory. Also, fortunately it's not one that

0:20:43.400 --> 0:20:45.720
<v Speaker 1>NASA thinks is going to hit the Earth after they

0:20:45.880 --> 0:20:48.919
<v Speaker 1>change its traject Right. I was about to say, I

0:20:49.000 --> 0:20:52.760
<v Speaker 1>really hope they double checked their math and their units,

0:20:52.960 --> 0:20:55.640
<v Speaker 1>because that would be a heck of all whoop. See

0:20:55.960 --> 0:20:59.280
<v Speaker 1>that is actually something people worry about developing these tools

0:20:59.520 --> 0:21:01.840
<v Speaker 1>that can affect the future of the human race. Like

0:21:02.160 --> 0:21:05.040
<v Speaker 1>if you can now aim asteroids, then you know some

0:21:05.200 --> 0:21:09.119
<v Speaker 1>super billain might decide to use that to threaten Earth

0:21:09.240 --> 0:21:12.639
<v Speaker 1>with asteroids. Right. Another direction people are working on is

0:21:12.800 --> 0:21:15.919
<v Speaker 1>zapping these things with lasers. That sounds like science fiction,

0:21:16.000 --> 0:21:18.280
<v Speaker 1>but you can get a powerful enough laser and zap

0:21:18.359 --> 0:21:21.119
<v Speaker 1>one side of the asteroid, then you can like vaporize

0:21:21.119 --> 0:21:22.840
<v Speaker 1>some of the rock and the ice and it can

0:21:22.840 --> 0:21:25.199
<v Speaker 1>give it a sideways push so that it doesn't hit

0:21:25.240 --> 0:21:27.360
<v Speaker 1>the Earth. There, people in Santa Barbara working on these

0:21:27.440 --> 0:21:30.239
<v Speaker 1>kind of super lasers. But also that does make me

0:21:30.320 --> 0:21:34.720
<v Speaker 1>worry about you know, like other applications of supers well,

0:21:34.720 --> 0:21:37.800
<v Speaker 1>like you're not firing this laser from Earth right because

0:21:37.920 --> 0:21:41.240
<v Speaker 1>I would imagine you'd scorch a few birds and maybe

0:21:41.280 --> 0:21:43.479
<v Speaker 1>a few planes if you did that. I don't think

0:21:43.480 --> 0:21:45.400
<v Speaker 1>they even have a prototype of this laser so far.

0:21:45.560 --> 0:21:48.320
<v Speaker 1>It's still in the exploratory studies. But there are a

0:21:48.480 --> 0:21:50.640
<v Speaker 1>range of solutions, and we actually have a whole podcast

0:21:50.680 --> 0:21:55.119
<v Speaker 1>episode about how to defend the Earth from asteroids, including

0:21:55.200 --> 0:21:58.800
<v Speaker 1>gravity tractors and laser beams and giving them a push.

0:21:58.840 --> 0:22:01.119
<v Speaker 1>It all depends on what the thing is made out of,

0:22:01.480 --> 0:22:03.119
<v Speaker 1>Like if it's a pile of rubble, it's kind of

0:22:03.119 --> 0:22:04.560
<v Speaker 1>hard to give it a push, or if it's a

0:22:04.560 --> 0:22:06.520
<v Speaker 1>big ball of ice, it's good to zap it with

0:22:06.560 --> 0:22:09.960
<v Speaker 1>a laser, And also really depends on spotting it early

0:22:10.080 --> 0:22:13.440
<v Speaker 1>and understanding where it comes from. We're gonna take a

0:22:13.520 --> 0:22:15.040
<v Speaker 1>quick break, but when we come back, we're going to

0:22:15.119 --> 0:22:18.240
<v Speaker 1>talk about the source of these deadly rocks that might

0:22:18.280 --> 0:22:20.640
<v Speaker 1>wipe out life on Earth, whether or not the data

0:22:20.720 --> 0:22:23.000
<v Speaker 1>suggests there are coming in a pattern, and what we

0:22:23.040 --> 0:22:25.919
<v Speaker 1>can do about it. So like what angle I should

0:22:26.000 --> 0:22:29.719
<v Speaker 1>keep my umbrella at. Essentially how many umbrellas you need

0:22:29.760 --> 0:22:45.240
<v Speaker 1>to buy? Actually, all right, we're back and we're talking

0:22:45.280 --> 0:22:49.879
<v Speaker 1>about whether there's a pattern to asteroid impact on Earth.

0:22:50.280 --> 0:22:52.960
<v Speaker 1>We have some pretty strong evidence that about sixty five

0:22:53.160 --> 0:22:56.280
<v Speaker 1>million years ago there was a huge impact or it

0:22:56.359 --> 0:22:59.200
<v Speaker 1>was something like five to ten kilometers wide, and it

0:22:59.320 --> 0:23:03.199
<v Speaker 1>struck the Earth the twenty thousand miles per hour. You

0:23:03.280 --> 0:23:05.920
<v Speaker 1>might wonder, like, why is it going so fast? Well,

0:23:06.160 --> 0:23:08.399
<v Speaker 1>most of the stuff out there in the Solar System

0:23:08.560 --> 0:23:11.120
<v Speaker 1>is whizzing around the Sun pretty fast. It's like we're

0:23:11.119 --> 0:23:12.919
<v Speaker 1>all the fast land on the freeway, and if somebody

0:23:12.920 --> 0:23:15.320
<v Speaker 1>comes at you at that speed, it's going to be

0:23:15.400 --> 0:23:18.120
<v Speaker 1>pretty fast. But also, the Earth has a lot of gravity,

0:23:18.480 --> 0:23:21.120
<v Speaker 1>so once something comes even near the Earth and then

0:23:21.280 --> 0:23:24.680
<v Speaker 1>falls to the surface, it gets accelerated by the Earth.

0:23:24.680 --> 0:23:26.960
<v Speaker 1>The Earth is like pulling it in, so by the

0:23:27.000 --> 0:23:29.800
<v Speaker 1>time it hits the ground, it has a lot of velocity.

0:23:29.920 --> 0:23:32.520
<v Speaker 1>And this asteroid impact, we think, wiped out about thirty

0:23:33.160 --> 0:23:36.439
<v Speaker 1>of the species on Earth at the time, including many

0:23:36.600 --> 0:23:39.080
<v Speaker 1>of the dinosaurs. Yeah, I mean, I think one of

0:23:39.119 --> 0:23:42.080
<v Speaker 1>the things that is important to remember is that this

0:23:42.119 --> 0:23:45.320
<v Speaker 1>did not just wipe out the dinosaurs, only it wiped

0:23:45.320 --> 0:23:49.920
<v Speaker 1>out anything and everything that was around, like a good

0:23:50.040 --> 0:23:53.520
<v Speaker 1>number of them, the things that ended up surviving. It

0:23:53.640 --> 0:23:57.840
<v Speaker 1>was not like a dinosaur seeking asteroid that targeted the

0:23:57.880 --> 0:24:01.600
<v Speaker 1>dinosaurs specifically. It just targeted anything that was not able

0:24:01.680 --> 0:24:06.400
<v Speaker 1>to survive. The fallout of what happened after the asteroid hit.

0:24:06.560 --> 0:24:08.199
<v Speaker 1>I mean, I'm sure there was a good amount of

0:24:08.200 --> 0:24:11.000
<v Speaker 1>death and the immediate aftermath of the asteroid, but a

0:24:11.040 --> 0:24:13.399
<v Speaker 1>lot of it was sort of both long and slow

0:24:13.520 --> 0:24:17.439
<v Speaker 1>drawn out extinction, and the exact causes of it aren't

0:24:17.840 --> 0:24:22.640
<v Speaker 1>precisely known. It's hard to find really accurate evidence of

0:24:22.720 --> 0:24:25.560
<v Speaker 1>what exactly happened. But you know, there are a lot

0:24:25.600 --> 0:24:29.959
<v Speaker 1>of theories about, you know, the ecosystems collapsing because of

0:24:30.359 --> 0:24:33.640
<v Speaker 1>the you know, massive amount of debris that cut out

0:24:33.680 --> 0:24:35.800
<v Speaker 1>the sun, and of course you don't have as much

0:24:35.920 --> 0:24:39.119
<v Speaker 1>vegetation and so you don't have as many big herbivores,

0:24:39.320 --> 0:24:42.040
<v Speaker 1>and then you don't have as many big carnivores. So

0:24:42.280 --> 0:24:45.040
<v Speaker 1>like that. It basically, you know how these ecosystems are

0:24:45.080 --> 0:24:48.280
<v Speaker 1>like these Jenga towers and you pull one thing out

0:24:48.320 --> 0:24:50.879
<v Speaker 1>and it can collapse. Well, like this asteroid hitting is

0:24:50.920 --> 0:24:53.520
<v Speaker 1>like a throwing a tennis ball at the Jenga tower,

0:24:53.760 --> 0:24:58.239
<v Speaker 1>and so only the things that were hardy enough, you know,

0:24:58.520 --> 0:25:01.920
<v Speaker 1>typically quite small as well, because they didn't require as

0:25:02.040 --> 0:25:05.719
<v Speaker 1>much food, we're able to survive. And not all the

0:25:05.720 --> 0:25:09.040
<v Speaker 1>dinosaurs one extinct, like we still have birds. Birds are

0:25:09.280 --> 0:25:12.520
<v Speaker 1>the surviving dinosaurs of this period, and they were small

0:25:12.640 --> 0:25:16.400
<v Speaker 1>enough that they were able to sort of escape the

0:25:16.520 --> 0:25:21.040
<v Speaker 1>uh starvation of these larger dinosaurs that had much more

0:25:21.400 --> 0:25:25.000
<v Speaker 1>intensive dietary needs. And that's, like, I think, to me,

0:25:25.160 --> 0:25:27.800
<v Speaker 1>is one of the more compelling theories of what happened. Yeah,

0:25:27.840 --> 0:25:29.959
<v Speaker 1>it's important to realize, as you say, that these are

0:25:30.000 --> 0:25:32.800
<v Speaker 1>not like dinosaurs seeking asteroids that didn't come and then

0:25:32.840 --> 0:25:35.600
<v Speaker 1>like hunt down all the dinosaurs and kill them one

0:25:35.640 --> 0:25:37.480
<v Speaker 1>by one. It really is a lot of the death

0:25:37.560 --> 0:25:40.600
<v Speaker 1>probably came from the change in the environment and all

0:25:40.600 --> 0:25:42.360
<v Speaker 1>this stuff is now up in the atmosphere and you're

0:25:42.359 --> 0:25:45.520
<v Speaker 1>blocking the sun's light and so, as you say, ecosystems

0:25:45.760 --> 0:25:48.240
<v Speaker 1>react to that, and now you have to survive in

0:25:48.240 --> 0:25:50.160
<v Speaker 1>a pretty new world. I don't know if anybody out

0:25:50.160 --> 0:25:53.720
<v Speaker 1>there it was a fan of the Dinosaurs sitcom aired

0:25:53.760 --> 0:25:56.040
<v Speaker 1>I think in the eighties and nineties, but the theories.

0:25:56.040 --> 0:25:59.840
<v Speaker 1>Finale of that episode actually features like basically an Aster

0:26:00.080 --> 0:26:03.360
<v Speaker 1>Royd winter where they're all hovering in their house as

0:26:03.400 --> 0:26:05.840
<v Speaker 1>the snow comes down and they're not expecting to see

0:26:05.840 --> 0:26:08.000
<v Speaker 1>the sun for years. It's sort of a bleak ending

0:26:08.119 --> 0:26:11.679
<v Speaker 1>to a comedy series. It was a huge bummer. I

0:26:11.720 --> 0:26:14.199
<v Speaker 1>think it was sort of a cautionary tale because it

0:26:14.280 --> 0:26:19.280
<v Speaker 1>was something about some dino corporation caused this to happen,

0:26:19.400 --> 0:26:22.280
<v Speaker 1>and so it was I think supposed to be an

0:26:22.359 --> 0:26:26.240
<v Speaker 1>environmental message about not destroying our own planet with global

0:26:26.280 --> 0:26:31.240
<v Speaker 1>warming or or whatever you know potential ramifications of destroying

0:26:31.240 --> 0:26:34.520
<v Speaker 1>our environment would be. And it wasn't a comedy. It

0:26:34.560 --> 0:26:38.560
<v Speaker 1>was like this lighthearted comedy with these big puppet dinosaurs

0:26:38.600 --> 0:26:41.440
<v Speaker 1>and like, you know, a dinosaur baby that would hit

0:26:41.640 --> 0:26:44.080
<v Speaker 1>the father with a frying pans. So it was as

0:26:44.119 --> 0:26:49.280
<v Speaker 1>if The Simpsons ended on basically a nuclear war and

0:26:49.359 --> 0:26:53.080
<v Speaker 1>everyone dies. How inappropriate to combine you know, hard hitting

0:26:53.080 --> 0:26:56.120
<v Speaker 1>science with ridiculous jokes. I mean, you choose that kind

0:26:56.160 --> 0:26:59.159
<v Speaker 1>of venue for talking about as a serious topic. Anyway,

0:26:59.280 --> 0:27:02.280
<v Speaker 1>let's keep making some jokes about how all the dinosaurs

0:27:02.440 --> 0:27:04.800
<v Speaker 1>were wiped out millions of years ago. But I think

0:27:04.840 --> 0:27:07.879
<v Speaker 1>it's important to understand where these things come from. Like,

0:27:08.160 --> 0:27:11.280
<v Speaker 1>these rocks don't just appear in space and get dropped

0:27:11.320 --> 0:27:13.640
<v Speaker 1>on the Earth. These are not like malevolent aliens. As

0:27:13.680 --> 0:27:17.199
<v Speaker 1>far as we know, these are parts of our Solar system.

0:27:17.280 --> 0:27:19.480
<v Speaker 1>When big misimpression is that these rocks might come from

0:27:19.480 --> 0:27:23.200
<v Speaker 1>really deep space, like from outside our Solar system to impact,

0:27:23.440 --> 0:27:26.919
<v Speaker 1>that's actually really quite rare because our star is pretty

0:27:26.920 --> 0:27:30.000
<v Speaker 1>far away from other stars. You know, there's many light

0:27:30.080 --> 0:27:32.640
<v Speaker 1>years between us and the next star, and many many

0:27:32.640 --> 0:27:35.399
<v Speaker 1>more between most stars. So there's only been a few

0:27:35.440 --> 0:27:38.520
<v Speaker 1>examples of times when we've even seen a rock come

0:27:38.720 --> 0:27:42.760
<v Speaker 1>from another Solar system and passed through hours like Omamua.

0:27:43.240 --> 0:27:45.880
<v Speaker 1>Most of the times when we're thinking about impacts on Earth,

0:27:46.040 --> 0:27:49.000
<v Speaker 1>we're talking about our own neighbors. We're talking about sources

0:27:49.040 --> 0:27:51.800
<v Speaker 1>in the Solar system. Isn't that the thing with like

0:27:51.960 --> 0:27:56.199
<v Speaker 1>murders and stuff, where stranger danger is pretty overly hyped

0:27:56.240 --> 0:27:58.919
<v Speaker 1>and it's usually someone you know that murders you. I

0:27:58.920 --> 0:28:02.160
<v Speaker 1>guess it's the same thing with asteroids. It's the asteroid

0:28:02.240 --> 0:28:05.040
<v Speaker 1>you know, your neighbor, that comes and destroys your planet.

0:28:05.160 --> 0:28:08.200
<v Speaker 1>Another good example of inappropriate humor, Katie wow Now we're

0:28:08.280 --> 0:28:10.720
<v Speaker 1>now we're joking about murders. I'm going to go to

0:28:10.760 --> 0:28:13.040
<v Speaker 1>podcast jail. No, But you're exactly right. And the thing

0:28:13.080 --> 0:28:16.840
<v Speaker 1>to understand is that the Solar System, like life on Earth,

0:28:16.960 --> 0:28:21.639
<v Speaker 1>has not stopped developing. It's a continuous, ongoing process. Solar

0:28:21.680 --> 0:28:23.760
<v Speaker 1>system is about four and a half billion years old,

0:28:23.800 --> 0:28:26.600
<v Speaker 1>and it's started from some huge cloud of gas and

0:28:26.720 --> 0:28:29.560
<v Speaker 1>dust and little bits of rock left over from the

0:28:29.640 --> 0:28:32.879
<v Speaker 1>death of other stars and coalesced into these planets and

0:28:32.920 --> 0:28:36.000
<v Speaker 1>all of these bits. But it's a dynamic, ongoing process.

0:28:36.040 --> 0:28:38.320
<v Speaker 1>And as we study our Solar system and compare it

0:28:38.400 --> 0:28:41.280
<v Speaker 1>to other solar systems, we understand that lots of things

0:28:41.360 --> 0:28:44.960
<v Speaker 1>are changing through that history of the Solar System. Planets

0:28:45.000 --> 0:28:47.960
<v Speaker 1>might even be changing position. We think that Jupiter amount

0:28:48.000 --> 0:28:50.120
<v Speaker 1>have formed in the outer part of the Solar System

0:28:50.320 --> 0:28:52.600
<v Speaker 1>and then taken a trip to the inner Solar System

0:28:52.640 --> 0:28:55.560
<v Speaker 1>before being pulled back out by Saturn into the outer

0:28:55.680 --> 0:28:58.400
<v Speaker 1>Solar System again. So don't think of the Solar system

0:28:58.480 --> 0:29:00.720
<v Speaker 1>is like a static place where it's finished and it's

0:29:00.720 --> 0:29:03.600
<v Speaker 1>going to be like this forever. It's still ongoing. And

0:29:03.640 --> 0:29:06.720
<v Speaker 1>that goes double for the little bits, not just the planets,

0:29:06.880 --> 0:29:09.760
<v Speaker 1>but the extra little rocks that didn't find their way

0:29:09.880 --> 0:29:12.160
<v Speaker 1>into a big planet. So we know, for example that

0:29:12.240 --> 0:29:15.960
<v Speaker 1>between Mars and Jupiter there's the asteroid belt. Right, These

0:29:16.000 --> 0:29:18.560
<v Speaker 1>are a bunch of little rocks that are not part

0:29:18.600 --> 0:29:21.440
<v Speaker 1>of any planet. And it's not just between Mars and Jupiter.

0:29:21.480 --> 0:29:24.440
<v Speaker 1>There are actually two blobs that are in Jupiter's orbit,

0:29:24.560 --> 0:29:27.080
<v Speaker 1>and like in the same ellipse where Jupiter goes around

0:29:27.080 --> 0:29:29.200
<v Speaker 1>the Sun is a blob that goes ahead of them

0:29:29.200 --> 0:29:31.680
<v Speaker 1>and a blob that goes behind them. That I think

0:29:31.840 --> 0:29:34.120
<v Speaker 1>is really cool. It shows you sort of why the

0:29:34.160 --> 0:29:38.760
<v Speaker 1>asteroids exist exist because of Jupiter's gravity. Jupiter's like this

0:29:38.880 --> 0:29:41.480
<v Speaker 1>huge bully in the outer Solar System. It wasn't for

0:29:41.560 --> 0:29:45.280
<v Speaker 1>Jupiter these rocks might coalesce into a planet. We did

0:29:45.280 --> 0:29:48.720
<v Speaker 1>an episode recently about like why planets get rings versus moons,

0:29:48.920 --> 0:29:51.400
<v Speaker 1>and the answer there was because of the tidal forces

0:29:51.440 --> 0:29:54.239
<v Speaker 1>of the planets, pulling those moons apart into rings if

0:29:54.240 --> 0:29:56.640
<v Speaker 1>they're too close. This is sort of a similar thing.

0:29:56.760 --> 0:29:59.600
<v Speaker 1>Jupiter is tugging on all of these guys, preventing them

0:29:59.600 --> 0:30:03.280
<v Speaker 1>from well lessen into a single larger thing. So you

0:30:03.320 --> 0:30:06.400
<v Speaker 1>have this huge collection of rocks. But again that's not static.

0:30:06.600 --> 0:30:08.360
<v Speaker 1>It used to be in the much earlier times in

0:30:08.400 --> 0:30:11.600
<v Speaker 1>the Solar System that the asteroid belt was much much richer,

0:30:11.640 --> 0:30:14.360
<v Speaker 1>There was much more mass. A lot of that has

0:30:14.400 --> 0:30:17.080
<v Speaker 1>gotten lost because it's a little bit unstable. Things fall

0:30:17.160 --> 0:30:19.280
<v Speaker 1>in towards the Sun or get knocked out of the

0:30:19.320 --> 0:30:22.560
<v Speaker 1>asteroid belt by collisions or just by Jupiter's gravity. What

0:30:22.800 --> 0:30:26.840
<v Speaker 1>causes something to get knocked out of stability? So you

0:30:26.880 --> 0:30:31.120
<v Speaker 1>have this asteroid built, what is the impetus for one

0:30:31.160 --> 0:30:34.160
<v Speaker 1>of these asteroids just deciding to go like, well, see

0:30:34.200 --> 0:30:36.520
<v Speaker 1>it and fall into the Sun. Think about it the

0:30:36.520 --> 0:30:38.120
<v Speaker 1>other direction. What do you have to do in order

0:30:38.120 --> 0:30:42.440
<v Speaker 1>to survive over billions of years? You have Jupiter's gravity

0:30:42.480 --> 0:30:45.480
<v Speaker 1>tugging at you, if all the other planets also tugging

0:30:45.520 --> 0:30:47.440
<v Speaker 1>at you even less, and of course the Sun. In

0:30:47.560 --> 0:30:50.040
<v Speaker 1>order to survive you have to somehow balance all of

0:30:50.080 --> 0:30:52.800
<v Speaker 1>those things for billions of years. So you start out

0:30:52.840 --> 0:30:55.120
<v Speaker 1>with a huge number of rocks, and nobody has organized

0:30:55.160 --> 0:30:56.680
<v Speaker 1>these right there, just sort of like out there in

0:30:56.720 --> 0:31:00.479
<v Speaker 1>the Solar System. They formed gravitationally, and most of them

0:31:00.480 --> 0:31:02.959
<v Speaker 1>are just not on trajectories that are going to survive.

0:31:02.960 --> 0:31:05.320
<v Speaker 1>They're gonna get tugged by Jupiter, or they're gonna get

0:31:05.400 --> 0:31:08.160
<v Speaker 1>yanked by Mars, or they're gonna feel Saturn's pull, and

0:31:08.160 --> 0:31:10.560
<v Speaker 1>then eventually they're gonna fall into the Sun or into

0:31:10.600 --> 0:31:14.200
<v Speaker 1>another planet. So it requires like a really delicate balance

0:31:14.240 --> 0:31:17.240
<v Speaker 1>of all of those gravitational factors in order to survive

0:31:17.360 --> 0:31:20.120
<v Speaker 1>this long, and as time goes on, you're less and

0:31:20.200 --> 0:31:22.760
<v Speaker 1>less likely to survive because you know, it's really chaotic.

0:31:22.840 --> 0:31:26.000
<v Speaker 1>Like you can orbit a single object pretty stable for

0:31:26.040 --> 0:31:28.840
<v Speaker 1>a long long time, you're just feeling gravity towards it.

0:31:28.920 --> 0:31:31.160
<v Speaker 1>You have the right angle you can orbit. Now you

0:31:31.160 --> 0:31:33.800
<v Speaker 1>add another object in the Solar System, another thing with

0:31:33.840 --> 0:31:37.880
<v Speaker 1>heavy gravity, becomes much more complicated to keep a stable orbit.

0:31:38.320 --> 0:31:41.280
<v Speaker 1>Like the Earth, for example, its orbit is constantly being

0:31:41.320 --> 0:31:44.760
<v Speaker 1>tweaked by Jupiter and by Saturn, these tiny little tugs,

0:31:44.880 --> 0:31:46.840
<v Speaker 1>and so it's hard to find a path which is

0:31:46.840 --> 0:31:50.080
<v Speaker 1>going to be stable over billions of years. It's amazing, frankly,

0:31:50.120 --> 0:31:52.800
<v Speaker 1>that any of these asteroids were able to survive this

0:31:52.960 --> 0:31:56.920
<v Speaker 1>fairly chaotic gravitational system that long. I mean that kind

0:31:56.920 --> 0:32:00.240
<v Speaker 1>of sounds similar to evolution, where you know, the rule

0:32:00.320 --> 0:32:03.360
<v Speaker 1>is simple. If you survive, you survive, and if you don't,

0:32:03.480 --> 0:32:06.680
<v Speaker 1>you get tossed into the Sun or pulled into the Sun. Yeah.

0:32:06.800 --> 0:32:09.920
<v Speaker 1>The difference here is that there's no way to reproduce, right,

0:32:09.960 --> 0:32:12.680
<v Speaker 1>there's no like way to replenish these meteors that we

0:32:12.760 --> 0:32:17.719
<v Speaker 1>know that we know of exactly unless like two planets

0:32:17.800 --> 0:32:20.360
<v Speaker 1>collide and create a lot of debris. But our model

0:32:20.400 --> 0:32:23.680
<v Speaker 1>of the asteroid belt is that it's like point one

0:32:23.840 --> 0:32:27.600
<v Speaker 1>percent of its original mass. The first hundred million years

0:32:27.600 --> 0:32:30.920
<v Speaker 1>of the Solar System were pretty chaotic collisions all the time,

0:32:30.960 --> 0:32:32.920
<v Speaker 1>and things were falling out of it. So the asteroid

0:32:32.920 --> 0:32:36.000
<v Speaker 1>belt we think now is much much less mass than

0:32:36.040 --> 0:32:37.880
<v Speaker 1>it used to be. In total, if you took like

0:32:38.040 --> 0:32:40.440
<v Speaker 1>all the asteroids and the asteroid belt and add them up,

0:32:40.480 --> 0:32:42.920
<v Speaker 1>it'd be less than five percent of the mass of

0:32:42.960 --> 0:32:47.120
<v Speaker 1>our moon. So there's not actually that much stuff out there.

0:32:47.520 --> 0:32:50.240
<v Speaker 1>Is That good news for us? Because the more stuff,

0:32:50.240 --> 0:32:52.160
<v Speaker 1>it seems like, the more likely we're going to get

0:32:52.240 --> 0:32:54.600
<v Speaker 1>hit by that stuff. That's very good news for us.

0:32:54.680 --> 0:32:57.840
<v Speaker 1>We want fewer asteroids because each one is like a bullet, right,

0:32:58.080 --> 0:33:00.640
<v Speaker 1>Any of these things, if they're bigger and like ten

0:33:00.720 --> 0:33:03.959
<v Speaker 1>kilometers or so and they hit the Earth, that's an

0:33:03.960 --> 0:33:07.960
<v Speaker 1>extinction event, right, that's really catastrophic. Some of these guys

0:33:07.960 --> 0:33:11.000
<v Speaker 1>are huge. Like there's a dwarf planet in the asteroid belt,

0:33:11.080 --> 0:33:15.760
<v Speaker 1>it's called Series, and it's nine fifty kilometers in diameter, right,

0:33:15.800 --> 0:33:18.400
<v Speaker 1>that would just obliterate the surface of the Earth completely.

0:33:18.600 --> 0:33:23.080
<v Speaker 1>That sounds pretty serious. So it seems like earlier on,

0:33:23.200 --> 0:33:26.480
<v Speaker 1>like we probably had more asteroid collisions near Earth, because

0:33:26.520 --> 0:33:29.880
<v Speaker 1>like the Moon has a bunch of craters, But has

0:33:29.920 --> 0:33:33.760
<v Speaker 1>the Moon been hit by asteroids more recently? Was that

0:33:33.800 --> 0:33:36.720
<v Speaker 1>like debris from Earth hitting the Moon? Why do we

0:33:36.880 --> 0:33:41.200
<v Speaker 1>have more craters Like that seemed to be old than

0:33:41.640 --> 0:33:45.000
<v Speaker 1>we are currently experiencing in terms of getting hit by

0:33:45.120 --> 0:33:47.640
<v Speaker 1>space rocks. Yeah, there's a few things going on there.

0:33:47.720 --> 0:33:50.160
<v Speaker 1>It's true that we have fewer space rocks hitting things

0:33:50.240 --> 0:33:52.640
<v Speaker 1>now than we used to in the very early days

0:33:52.680 --> 0:33:55.080
<v Speaker 1>of the Solar System, just because there are fewer and

0:33:55.120 --> 0:33:57.640
<v Speaker 1>we sort of run out and the trend is towards

0:33:58.040 --> 0:34:01.720
<v Speaker 1>things coalescing into larger objects. So we just have fewer

0:34:01.720 --> 0:34:04.120
<v Speaker 1>of these rocks, which means fewer impacts. But there still

0:34:04.160 --> 0:34:06.239
<v Speaker 1>are a lot of impacts. And if you look at

0:34:06.240 --> 0:34:08.760
<v Speaker 1>the Moon, there's a very rich history there of impacts

0:34:08.760 --> 0:34:11.520
<v Speaker 1>and you can see, for example, really big craters that

0:34:11.600 --> 0:34:14.879
<v Speaker 1>you can tell are old with smaller craters inside them,

0:34:14.920 --> 0:34:17.520
<v Speaker 1>and so you can use that to tell like which

0:34:17.560 --> 0:34:21.120
<v Speaker 1>ones happened first because of the small crater it happened first,

0:34:21.280 --> 0:34:23.759
<v Speaker 1>the big one would have obliterated it. So you can

0:34:23.800 --> 0:34:26.759
<v Speaker 1>tell the sort of like the layers of cratering there,

0:34:27.160 --> 0:34:29.120
<v Speaker 1>and you can use that to try to reconstruct something

0:34:29.120 --> 0:34:32.239
<v Speaker 1>about the history of cratering on the Moon. But yeah,

0:34:32.280 --> 0:34:35.120
<v Speaker 1>there was definitely more cratering earlier on. And remember that

0:34:35.160 --> 0:34:38.080
<v Speaker 1>the Moon doesn't really have much of an atmosphere, has

0:34:38.160 --> 0:34:41.520
<v Speaker 1>almost no atmosphere. We just did an episode about the

0:34:41.520 --> 0:34:45.000
<v Speaker 1>Moon's atmosphere. It's like a few molecules per cubic centimeter,

0:34:45.120 --> 0:34:47.719
<v Speaker 1>whereas the Earth is like ten to the nineteen the

0:34:47.800 --> 0:34:51.520
<v Speaker 1>molecules per cubic centimeter, and that's a huge shield. Any

0:34:51.640 --> 0:34:54.040
<v Speaker 1>rock that hits the Moon is going to cause a crater,

0:34:54.280 --> 0:34:56.400
<v Speaker 1>whereas the rock that hits the Earth, if it's not

0:34:56.480 --> 0:34:59.400
<v Speaker 1>big enough, is going to burn up in our atmosphere

0:34:59.440 --> 0:35:02.240
<v Speaker 1>and we're not going to see it. So every surface

0:35:02.280 --> 0:35:05.240
<v Speaker 1>of the Solar System is constantly getting bombarded by smaller

0:35:05.320 --> 0:35:08.960
<v Speaker 1>rocks and sometimes bigger ones Earth. We don't often notice

0:35:09.000 --> 0:35:11.960
<v Speaker 1>that because our atmosphere protects us, but a big enough

0:35:12.040 --> 0:35:14.000
<v Speaker 1>one is definitely going to make it to the surface

0:35:14.000 --> 0:35:16.200
<v Speaker 1>of the Earth and do some damage. Well, I want

0:35:16.200 --> 0:35:20.120
<v Speaker 1>to hear about how we can predict whether one of

0:35:20.120 --> 0:35:22.719
<v Speaker 1>these big ones are gonna hit us, But I think

0:35:22.840 --> 0:35:25.239
<v Speaker 1>first I'm going to take a quick break to hide

0:35:25.320 --> 0:35:40.960
<v Speaker 1>under the bed a little bit. So we've talked about

0:35:41.040 --> 0:35:45.080
<v Speaker 1>how there is a lot of asteroid activity, that there's

0:35:45.080 --> 0:35:49.480
<v Speaker 1>a lot of randomness and chaos to the movement of asteroids,

0:35:49.520 --> 0:35:53.000
<v Speaker 1>like from say like the asteroid belt to falling into

0:35:53.000 --> 0:35:56.919
<v Speaker 1>the Sun. So it seems like there's so much randomness

0:35:57.000 --> 0:35:59.759
<v Speaker 1>it would be like really hard to predict if one

0:35:59.800 --> 0:36:01.799
<v Speaker 1>of the these guys would come and hit us. It

0:36:01.840 --> 0:36:04.960
<v Speaker 1>does seem like a lot of the process is random, right,

0:36:05.080 --> 0:36:07.759
<v Speaker 1>Like what makes an asteroid hit the Earth or not

0:36:07.920 --> 0:36:10.160
<v Speaker 1>hit the Earth. It does seem like it just needs

0:36:10.160 --> 0:36:12.319
<v Speaker 1>to get tugged the right way gravitationally and then end

0:36:12.400 --> 0:36:13.880
<v Speaker 1>up on a path. You know, for those of you

0:36:13.920 --> 0:36:17.040
<v Speaker 1>out there who are more anxious, NASA is doing their best.

0:36:17.080 --> 0:36:19.600
<v Speaker 1>They have a bunch of telescopes now tracking these things,

0:36:19.680 --> 0:36:21.720
<v Speaker 1>and they think they know where all of the big

0:36:21.760 --> 0:36:24.319
<v Speaker 1>asteroids are, the ones that might do any damage to

0:36:24.360 --> 0:36:26.480
<v Speaker 1>the Earth. They can't find all the asteroids because they

0:36:26.520 --> 0:36:28.360
<v Speaker 1>get to be pretty small, but the bigger ones, and

0:36:28.480 --> 0:36:31.640
<v Speaker 1>especially the shinier ones, they've had a lot of opportunities

0:36:31.680 --> 0:36:33.879
<v Speaker 1>to see these things because the asteroid belt is pretty close,

0:36:33.920 --> 0:36:35.920
<v Speaker 1>so we get lots of chances. The things that are

0:36:35.960 --> 0:36:38.360
<v Speaker 1>harder to predict are the things that come from further

0:36:38.480 --> 0:36:41.280
<v Speaker 1>out in our own solar system. These seem a little

0:36:41.280 --> 0:36:44.319
<v Speaker 1>bit more random and harder to anticipate because they're on

0:36:44.400 --> 0:36:47.480
<v Speaker 1>longer time scales, and those are things like comets. So

0:36:47.600 --> 0:36:50.720
<v Speaker 1>out past the asteroid belt, that's something called the Kuiper

0:36:50.840 --> 0:36:53.880
<v Speaker 1>Belt is now past Neptune. It's like thirty a U

0:36:54.080 --> 0:36:56.640
<v Speaker 1>out there, and instead of just being rock, these things

0:36:56.680 --> 0:36:59.839
<v Speaker 1>are icy rocks out past the snow line, and so

0:37:00.239 --> 0:37:04.120
<v Speaker 1>it's cold enough for vapor to coalesce into ice. These

0:37:04.160 --> 0:37:07.160
<v Speaker 1>chunky ice balls can also get disrupted and then fall

0:37:07.239 --> 0:37:10.080
<v Speaker 1>towards the inner Solar system, and that's what we typically

0:37:10.120 --> 0:37:12.680
<v Speaker 1>call a comet to have a tail, because this ice

0:37:12.800 --> 0:37:15.400
<v Speaker 1>is getting boiled off as they get closer and closer

0:37:15.440 --> 0:37:17.919
<v Speaker 1>to the Sun, and the Kuiper Belt is responsible for

0:37:18.120 --> 0:37:21.400
<v Speaker 1>what we call short period commets, ones that loop around

0:37:21.400 --> 0:37:24.520
<v Speaker 1>every two hundred years or so. That doesn't seem very short, right.

0:37:24.560 --> 0:37:26.600
<v Speaker 1>The problem though, is that if it only comes every

0:37:26.600 --> 0:37:30.080
<v Speaker 1>two hundred years, and we've only had like telescope technology

0:37:30.120 --> 0:37:32.120
<v Speaker 1>for a few hundred years, and we don't get very

0:37:32.120 --> 0:37:35.440
<v Speaker 1>many chances to see these things and like understand their

0:37:35.560 --> 0:37:38.719
<v Speaker 1>orbit and predict very well whether they're going to hit

0:37:38.760 --> 0:37:41.600
<v Speaker 1>the Earth. How much lead time would we have, like

0:37:41.680 --> 0:37:45.879
<v Speaker 1>from first spotting a comment to it making contact with Earth,

0:37:46.040 --> 0:37:49.600
<v Speaker 1>Like how fast could it move from when we could

0:37:49.640 --> 0:37:53.080
<v Speaker 1>first feasibly see it too when it would hit us.

0:37:53.440 --> 0:37:55.319
<v Speaker 1>It's a great question, and we have an answer to

0:37:55.360 --> 0:37:58.279
<v Speaker 1>that because it's happened right Commas Shoemaker levee, which hit

0:37:58.360 --> 0:38:00.960
<v Speaker 1>Jupiter in the nineties. We knew that was going to

0:38:01.080 --> 0:38:04.080
<v Speaker 1>hit but only a few months in advance because it

0:38:04.120 --> 0:38:06.439
<v Speaker 1>comes from pretty far out in the Solar system where

0:38:06.440 --> 0:38:08.960
<v Speaker 1>it's hard to track, and then as it comes in

0:38:09.040 --> 0:38:11.480
<v Speaker 1>people can calculate its trajectory and see where it's going

0:38:11.520 --> 0:38:14.000
<v Speaker 1>to loop around this time, and that's how we knew

0:38:14.040 --> 0:38:16.239
<v Speaker 1>it was going to hit Jupiter. And so some of

0:38:16.280 --> 0:38:19.000
<v Speaker 1>these things can come sort of out of the darkness

0:38:19.160 --> 0:38:21.680
<v Speaker 1>and surprise us. The scary thing is that there are

0:38:21.719 --> 0:38:25.320
<v Speaker 1>also long period comets, these things from the ord cloud,

0:38:25.719 --> 0:38:28.359
<v Speaker 1>and there might be like trillions of things out there,

0:38:28.480 --> 0:38:32.440
<v Speaker 1>much much further out, very loosely held by the Sun's gravity,

0:38:32.520 --> 0:38:35.160
<v Speaker 1>and these things can give comments that have really long

0:38:35.239 --> 0:38:38.760
<v Speaker 1>periods five hundred years, a thousand years, maybe even longer,

0:38:39.160 --> 0:38:42.640
<v Speaker 1>you know, looping through our solar system once every million years.

0:38:42.800 --> 0:38:46.040
<v Speaker 1>And so this is another source of potential killers. And

0:38:46.080 --> 0:38:48.800
<v Speaker 1>one issue is that because they come from so far out,

0:38:49.200 --> 0:38:52.080
<v Speaker 1>when they come in, they're gonna be moving very very fast,

0:38:52.440 --> 0:38:56.279
<v Speaker 1>which makes them hard to predict and also very very dangerous.

0:38:56.680 --> 0:39:00.480
<v Speaker 1>So comets are harder to predict than asteroids and also

0:39:00.680 --> 0:39:03.880
<v Speaker 1>faster moving, so they're really something to be more worried

0:39:03.880 --> 0:39:07.080
<v Speaker 1>about than asteroids. Well I hate that, so thank you

0:39:07.120 --> 0:39:12.279
<v Speaker 1>for that, so ignoring that kind of mortal peril. Are

0:39:12.280 --> 0:39:16.720
<v Speaker 1>we able to predict asteroids better than we can predict

0:39:16.760 --> 0:39:22.320
<v Speaker 1>comments like ore? Is there some science to understanding when

0:39:22.480 --> 0:39:25.239
<v Speaker 1>asteroids would hit us? There is some science there, but

0:39:25.320 --> 0:39:27.719
<v Speaker 1>we're not great at predicting asteroids more than like a

0:39:27.760 --> 0:39:30.640
<v Speaker 1>couple hundred years out. The more measurements you have of

0:39:30.680 --> 0:39:33.440
<v Speaker 1>an object, the better you can predict its trajectory. If

0:39:33.440 --> 0:39:36.400
<v Speaker 1>you've seen an asteroid a hundred times or a thousand times,

0:39:36.520 --> 0:39:38.840
<v Speaker 1>then you have a good sense of exactly what direction

0:39:38.840 --> 0:39:41.680
<v Speaker 1>it's going in and what its velocity is, and you

0:39:41.719 --> 0:39:44.319
<v Speaker 1>can predict pretty well where it's going to go. In

0:39:44.320 --> 0:39:46.839
<v Speaker 1>the end, it always becomes chaotic because there's so many

0:39:46.880 --> 0:39:49.600
<v Speaker 1>things in the Solar System that can tug on it.

0:39:49.520 --> 0:39:52.239
<v Speaker 1>It makes it hard to predict. Comments are harder if

0:39:52.280 --> 0:39:54.560
<v Speaker 1>you don't have much data, if you've only seen it once,

0:39:54.640 --> 0:39:56.759
<v Speaker 1>or if you've never seen it before, where it's just

0:39:57.000 --> 0:39:59.080
<v Speaker 1>entering the Solar system, and you know, the things that

0:39:59.120 --> 0:40:02.359
<v Speaker 1>trigger asteroid or comets to fall into the Earth are

0:40:02.480 --> 0:40:07.279
<v Speaker 1>these gravitational tugs. Right the Solar system, like left to itself,

0:40:07.600 --> 0:40:11.600
<v Speaker 1>is pretty stable. There's some gravitational chaos internally, but something

0:40:11.640 --> 0:40:13.759
<v Speaker 1>that we need to think about our effects from other

0:40:13.960 --> 0:40:17.000
<v Speaker 1>Solar systems. You know, the Sun is moving through the

0:40:17.040 --> 0:40:20.120
<v Speaker 1>galaxy and right now it's pretty far from other stars,

0:40:20.200 --> 0:40:22.719
<v Speaker 1>but as time goes on, it gets closer to other

0:40:22.719 --> 0:40:24.960
<v Speaker 1>stars and further from other stars. It's sort of like

0:40:25.280 --> 0:40:28.960
<v Speaker 1>swimming through an ocean of the galaxy. And if you

0:40:29.000 --> 0:40:31.200
<v Speaker 1>have these things out there in the or cloud that

0:40:31.239 --> 0:40:34.000
<v Speaker 1>are sort of like very tenuously held by the Sun.

0:40:34.320 --> 0:40:36.719
<v Speaker 1>Then a little tug from something else out there might

0:40:36.800 --> 0:40:38.759
<v Speaker 1>not get out of the stable orbit it's been in

0:40:38.840 --> 0:40:42.160
<v Speaker 1>for billions of years and send it rocketing towards the

0:40:42.160 --> 0:40:46.680
<v Speaker 1>inner Solar System. We do have ways to predict things

0:40:46.719 --> 0:40:51.480
<v Speaker 1>that's not always completely accurate, but it's based on like probabilities.

0:40:51.480 --> 0:40:54.560
<v Speaker 1>So like if you have a coin and you're flipping it,

0:40:54.680 --> 0:40:58.560
<v Speaker 1>you can't really with complete accuracy predict whether it's going

0:40:58.600 --> 0:41:01.480
<v Speaker 1>to be heads or tails, but you have an idea

0:41:01.640 --> 0:41:04.040
<v Speaker 1>of if you flip it a bunch of times that

0:41:04.239 --> 0:41:07.160
<v Speaker 1>you know roughly fifty percent at the time it should

0:41:07.200 --> 0:41:09.680
<v Speaker 1>be heads and fifty percent of the time it should

0:41:09.719 --> 0:41:12.239
<v Speaker 1>be tails. So do we have a similar thing when

0:41:12.280 --> 0:41:15.960
<v Speaker 1>it comes to asteroids, Like maybe we can't precisely predict

0:41:16.040 --> 0:41:19.240
<v Speaker 1>when an asteroid would hit us, but we have an

0:41:19.280 --> 0:41:23.439
<v Speaker 1>idea of the rough probability of asteroid hitting us over

0:41:23.640 --> 0:41:26.600
<v Speaker 1>the history of our planet. We can look back into

0:41:26.680 --> 0:41:29.239
<v Speaker 1>our history and try to see if there are patterns

0:41:29.280 --> 0:41:31.800
<v Speaker 1>there to see if there is a periodicity. But before

0:41:31.800 --> 0:41:33.440
<v Speaker 1>we do that, it's fun to think about, like what

0:41:33.600 --> 0:41:36.960
<v Speaker 1>might be causing that periodicity, Like are there even conceivably

0:41:37.080 --> 0:41:41.440
<v Speaker 1>theories that might generate that kind of pattern, because a

0:41:41.480 --> 0:41:44.480
<v Speaker 1>pattern means that there's something underlying happening. There's some like

0:41:44.760 --> 0:41:48.440
<v Speaker 1>very slow process which is grinding forward, which is changing

0:41:48.480 --> 0:41:52.080
<v Speaker 1>the nature of the environment in a way that's predictable. Right.

0:41:52.120 --> 0:41:55.480
<v Speaker 1>That's periodic, the way like the seasons are periodic. Because

0:41:55.520 --> 0:41:57.760
<v Speaker 1>of the way the Earth goes around the Sun, people

0:41:57.760 --> 0:42:00.560
<v Speaker 1>have looked for these kinds of things in our galaxy,

0:42:00.680 --> 0:42:03.920
<v Speaker 1>like periodic events that happen over tens of millions of

0:42:04.000 --> 0:42:07.560
<v Speaker 1>years that might trigger asteroids and comments to hit the

0:42:07.560 --> 0:42:09.440
<v Speaker 1>Earth on some sort of time scale. And there's a

0:42:09.480 --> 0:42:12.239
<v Speaker 1>couple of candidates. One is sort of plausible and the

0:42:12.280 --> 0:42:14.920
<v Speaker 1>other one is kind of crazy and dramatic. The one

0:42:14.960 --> 0:42:17.719
<v Speaker 1>that's sort of plausible is that the Sun does have

0:42:17.920 --> 0:42:21.840
<v Speaker 1>a sort of thirty million year cycle in the galaxy.

0:42:22.000 --> 0:42:24.080
<v Speaker 1>So the Sun is going around the center of the galaxy,

0:42:24.080 --> 0:42:26.360
<v Speaker 1>and it takes a couple of hundred million years to

0:42:26.480 --> 0:42:29.279
<v Speaker 1>orbit the center of the galaxy. That's like one galactic year.

0:42:29.520 --> 0:42:32.120
<v Speaker 1>But the Sun is also wiggling sort of up and

0:42:32.320 --> 0:42:35.480
<v Speaker 1>down through the galactic plane. So if you imagine the

0:42:35.560 --> 0:42:37.640
<v Speaker 1>Sun like going around the center of the galaxy, it's

0:42:37.680 --> 0:42:41.280
<v Speaker 1>also going up and down above and below the galactic

0:42:41.320 --> 0:42:44.240
<v Speaker 1>plane as it does that, and that happens about every

0:42:44.360 --> 0:42:48.480
<v Speaker 1>thirty million years. We pass through the sort of plane

0:42:48.520 --> 0:42:50.720
<v Speaker 1>at the center of the galaxy and then go below

0:42:50.760 --> 0:42:53.719
<v Speaker 1>it and then come back up thirty million years later. So,

0:42:53.880 --> 0:42:57.239
<v Speaker 1>like I've always kind of thought of the Sun as

0:42:57.320 --> 0:43:01.440
<v Speaker 1>this pretty stable, massive or but now I'm thinking of

0:43:01.480 --> 0:43:04.840
<v Speaker 1>it like this rubber ducky that is like circling the

0:43:04.920 --> 0:43:08.320
<v Speaker 1>drain of the bathtub, kind of bobbing under the water

0:43:08.440 --> 0:43:11.279
<v Speaker 1>and over the water exactly. And as it moves through

0:43:11.320 --> 0:43:14.719
<v Speaker 1>the galaxy, its environment changes, we get further and closer

0:43:14.760 --> 0:43:17.640
<v Speaker 1>to other stars. The center of the galaxy. The galactic

0:43:17.680 --> 0:43:20.799
<v Speaker 1>plane is definitely the densest part of the galaxy. And

0:43:20.880 --> 0:43:23.800
<v Speaker 1>so it's not inconceivable that that kind of process my

0:43:23.920 --> 0:43:27.280
<v Speaker 1>trigger comets or Kuiper Belt objects out of their otherwise

0:43:27.280 --> 0:43:29.920
<v Speaker 1>stable orbit give it just the right kind of tug

0:43:30.200 --> 0:43:32.920
<v Speaker 1>that might cause them to fall towards the center of

0:43:32.960 --> 0:43:36.200
<v Speaker 1>the Solar system. So that's the more plausible theory. Then

0:43:36.200 --> 0:43:38.279
<v Speaker 1>there's a theory that was spread in a popular book

0:43:38.320 --> 0:43:42.200
<v Speaker 1>recently about whether dark matter killed the dinosaurs. This is

0:43:42.200 --> 0:43:44.840
<v Speaker 1>a book written by a couple of theorists at Harvard,

0:43:45.160 --> 0:43:48.440
<v Speaker 1>and they suggest that dark matter, which is this invisible

0:43:48.480 --> 0:43:50.600
<v Speaker 1>matter that we know is out there but we don't

0:43:50.640 --> 0:43:53.319
<v Speaker 1>really understand very much. That we know that there's much

0:43:53.360 --> 0:43:56.120
<v Speaker 1>more of it than there is normal matter, and we

0:43:56.200 --> 0:43:58.239
<v Speaker 1>think that it's shaped sort of the whole structure of

0:43:58.239 --> 0:44:01.719
<v Speaker 1>the galaxy. They imagine that dark matter might coalesced into

0:44:01.760 --> 0:44:05.439
<v Speaker 1>sort of like a disk, like a dark frisbee. Yeah,

0:44:05.960 --> 0:44:08.560
<v Speaker 1>like a big dark frisbee. And when the Sun passes

0:44:08.600 --> 0:44:10.920
<v Speaker 1>through this dark matter disc that maybe it's the dark

0:44:10.960 --> 0:44:13.720
<v Speaker 1>matter that's tugging on the things in the outer Solar

0:44:13.760 --> 0:44:17.360
<v Speaker 1>System and then knocking them in towards our safe little garden.

0:44:17.640 --> 0:44:20.520
<v Speaker 1>Is there any evidence for this? So is there any

0:44:20.560 --> 0:44:22.719
<v Speaker 1>evidence for this? You know, this is just a fun

0:44:22.840 --> 0:44:26.160
<v Speaker 1>speculative theory. These two Harvard theorists came up with a

0:44:26.239 --> 0:44:28.640
<v Speaker 1>theory of dark matter that would generate this kind of

0:44:28.680 --> 0:44:30.560
<v Speaker 1>disc and then they went hunting to see if there

0:44:30.600 --> 0:44:33.799
<v Speaker 1>was evidence in the history on our planet for some

0:44:33.840 --> 0:44:36.440
<v Speaker 1>sort of periodicity, so that would be like an explanation

0:44:36.480 --> 0:44:39.279
<v Speaker 1>for that. We don't have any direct evidence of the

0:44:39.400 --> 0:44:43.360
<v Speaker 1>dark matter frisbee existing at all. It's just like another

0:44:43.480 --> 0:44:47.239
<v Speaker 1>idea that might generate a sort of periodic tug on

0:44:47.280 --> 0:44:50.000
<v Speaker 1>the Solar system that would create it. If indeed there

0:44:50.120 --> 0:44:53.759
<v Speaker 1>is any periodicity in the asteroid impacts on Earth, it

0:44:53.800 --> 0:44:57.000
<v Speaker 1>sounds like a very convenient scapegoat to me, Like if I,

0:44:57.800 --> 0:45:00.640
<v Speaker 1>you know, knock over a vase, I'm like, well, hey,

0:45:00.680 --> 0:45:04.200
<v Speaker 1>it's that dark matter, frisbee. You know how it is exactly.

0:45:04.400 --> 0:45:06.120
<v Speaker 1>And so now I think it's time to answer your

0:45:06.160 --> 0:45:08.480
<v Speaker 1>question from a few minutes ago, which is is there

0:45:08.520 --> 0:45:11.360
<v Speaker 1>actually any evidence can we look back on the history

0:45:11.400 --> 0:45:15.080
<v Speaker 1>on Earth and see a pattern of strikes, because you know,

0:45:15.160 --> 0:45:16.960
<v Speaker 1>one good way to predict the feature is of course

0:45:17.040 --> 0:45:19.279
<v Speaker 1>to look at the past and to see if this

0:45:19.320 --> 0:45:22.239
<v Speaker 1>has happened at regular intervals in the past. And this

0:45:22.320 --> 0:45:24.680
<v Speaker 1>is challenging, right because people weren't around, we've not been

0:45:24.680 --> 0:45:27.480
<v Speaker 1>doing astronomy for like hundreds of millions of years to

0:45:27.520 --> 0:45:29.640
<v Speaker 1>take this kind of data. But the sort of two

0:45:29.680 --> 0:45:32.319
<v Speaker 1>categories of evidence that people have looked at to see

0:45:32.360 --> 0:45:35.279
<v Speaker 1>if there are patterns. One is biological and the other

0:45:35.400 --> 0:45:38.800
<v Speaker 1>is geological. So first people look at like the history

0:45:38.800 --> 0:45:40.560
<v Speaker 1>of life on Earth, and they look at the fossil

0:45:40.640 --> 0:45:44.160
<v Speaker 1>record for extinctions, and there are a lot of them.

0:45:44.360 --> 0:45:46.080
<v Speaker 1>You know, if you look back in the history of

0:45:46.160 --> 0:45:49.240
<v Speaker 1>life on Earth is many times when you've had massive

0:45:49.280 --> 0:45:53.239
<v Speaker 1>dieots and big decreases in the diversity of life on Earth. Yeah, yeah,

0:45:53.320 --> 0:45:57.200
<v Speaker 1>you have these like bottleneck events you can look at,

0:45:57.680 --> 0:46:00.640
<v Speaker 1>you know, these kind of genetic because it's like not

0:46:00.719 --> 0:46:03.520
<v Speaker 1>just in terms of you know, you'll have a massive

0:46:03.640 --> 0:46:06.759
<v Speaker 1>dump of fossils that you can look at and that

0:46:06.880 --> 0:46:08.880
<v Speaker 1>are kind of layered and so you can see like

0:46:09.040 --> 0:46:13.520
<v Speaker 1>where you get these uh, these basically evidence of all

0:46:13.560 --> 0:46:17.560
<v Speaker 1>these animals dying. You have interesting sort of genetic bottleneck

0:46:17.600 --> 0:46:20.600
<v Speaker 1>where you can see evidence of mass die offs. I

0:46:20.640 --> 0:46:24.480
<v Speaker 1>think we have this sort of nice notion that these

0:46:24.520 --> 0:46:28.960
<v Speaker 1>mass extinctions don't really happen because we have not really

0:46:29.280 --> 0:46:33.160
<v Speaker 1>been direct witnesses to a mass extinction and our human

0:46:33.640 --> 0:46:37.040
<v Speaker 1>species lifespan. But yeah, they do happen with you know,

0:46:37.400 --> 0:46:42.239
<v Speaker 1>some regularity, not too often, but it's something that it's

0:46:42.280 --> 0:46:45.400
<v Speaker 1>hard to think of happening to us because you know,

0:46:45.480 --> 0:46:48.440
<v Speaker 1>we like very much being alive on the planet. But yes,

0:46:48.480 --> 0:46:52.000
<v Speaker 1>it does happen exactly, and sometimes these processes only happen

0:46:52.160 --> 0:46:54.560
<v Speaker 1>in deep time or there's not things that we witness

0:46:54.680 --> 0:46:56.919
<v Speaker 1>day to day or year to year, but they still

0:46:57.000 --> 0:46:59.840
<v Speaker 1>are part of the larger cycle of life on Earth.

0:47:00.000 --> 0:47:02.120
<v Speaker 1>You just might not have been paying attention long enough

0:47:02.160 --> 0:47:05.080
<v Speaker 1>to notice. And so you know, sixty five million years

0:47:05.120 --> 0:47:07.920
<v Speaker 1>ago there was a big die off, like to the species.

0:47:07.960 --> 0:47:11.800
<v Speaker 1>Two fifty million years ago there was a huge die off.

0:47:11.960 --> 0:47:14.920
<v Speaker 1>And the boundary between the Permian and Triassic period that

0:47:14.960 --> 0:47:17.640
<v Speaker 1>I think people still don't even really understand, something like

0:47:17.800 --> 0:47:21.640
<v Speaker 1>fifty percent of species on Earth died out. And if

0:47:21.640 --> 0:47:24.920
<v Speaker 1>you look at like over time when have species died out?

0:47:24.920 --> 0:47:27.160
<v Speaker 1>And you do see these spikes and you wonder like

0:47:27.880 --> 0:47:30.160
<v Speaker 1>is there a pattern there? So people have done a

0:47:30.160 --> 0:47:32.680
<v Speaker 1>statistical analysis to see like can you fit this to

0:47:32.680 --> 0:47:35.760
<v Speaker 1>a periodic function? Is there like a gap between these

0:47:35.800 --> 0:47:39.000
<v Speaker 1>peaks that's pretty regular or not. The way to do

0:47:39.040 --> 0:47:42.560
<v Speaker 1>this mathematically is something called a Furrier analysis. For those

0:47:42.640 --> 0:47:46.359
<v Speaker 1>you like signal processing nerds out there, it's basically like

0:47:46.440 --> 0:47:49.960
<v Speaker 1>taking a sound and decomposing it into frequencies. You listen

0:47:50.000 --> 0:47:52.080
<v Speaker 1>to Bob Dylan, for example, and you can lower the base,

0:47:52.160 --> 0:47:54.160
<v Speaker 1>or you can raise the trouble, or you know, you

0:47:54.200 --> 0:47:57.360
<v Speaker 1>can change the frequencies. That's because all sound is actually

0:47:57.400 --> 0:47:59.719
<v Speaker 1>built up of a bunch of different frequencies, and you

0:47:59.760 --> 0:48:03.280
<v Speaker 1>can decomposed sound into those frequencies and say Bob Dylan

0:48:03.320 --> 0:48:06.040
<v Speaker 1>is more based than Lady Gaga or whatever. And so

0:48:06.080 --> 0:48:08.719
<v Speaker 1>in the same way, you can take any distribution and

0:48:08.840 --> 0:48:12.440
<v Speaker 1>you can break it down into basically sine waves and say, like,

0:48:12.760 --> 0:48:16.359
<v Speaker 1>what frequencies are more common in this distribution. And when

0:48:16.360 --> 0:48:18.520
<v Speaker 1>you do that and you look at the pattern of

0:48:18.680 --> 0:48:23.200
<v Speaker 1>die offs biologically, you don't see much evidence. There's like

0:48:23.480 --> 0:48:27.680
<v Speaker 1>maybe some weak evidence for periodic die offs every sixty

0:48:27.680 --> 0:48:31.520
<v Speaker 1>million years or every hundred and forty million years. Really

0:48:31.520 --> 0:48:35.000
<v Speaker 1>you don't see something every thirty million years, like this

0:48:35.080 --> 0:48:37.080
<v Speaker 1>cycle that we talked about where the Sun goes in

0:48:37.120 --> 0:48:39.600
<v Speaker 1>and out of the galactic plane that happens every thirty

0:48:39.640 --> 0:48:42.439
<v Speaker 1>million years, But we don't see a die off every

0:48:42.440 --> 0:48:44.719
<v Speaker 1>thirty million years. It doesn't look like life on Earth

0:48:44.719 --> 0:48:47.440
<v Speaker 1>has been wiped out by an asteroid impact every thirty

0:48:47.440 --> 0:48:50.600
<v Speaker 1>million years, right, So it doesn't seem like it's on

0:48:50.640 --> 0:48:53.560
<v Speaker 1>an exact schedule, But it seems like there's also the

0:48:53.640 --> 0:48:56.840
<v Speaker 1>chance that like it wouldn't happen every thirty million years,

0:48:57.080 --> 0:49:00.680
<v Speaker 1>but you know the chance of it happening every thirty

0:49:00.680 --> 0:49:04.200
<v Speaker 1>million years would slightly increase, but you would maybe skip

0:49:04.239 --> 0:49:08.200
<v Speaker 1>a bunch of potential die offs, because just by increasing

0:49:08.239 --> 0:49:11.000
<v Speaker 1>the chance of something doesn't guarantee that it's going to happen,

0:49:11.360 --> 0:49:13.919
<v Speaker 1>Which seems like a really difficult analysis to make because

0:49:13.960 --> 0:49:17.440
<v Speaker 1>we don't have, you know, that much time to work with,

0:49:17.480 --> 0:49:20.640
<v Speaker 1>because like the Earth is not like the oldest thing

0:49:20.719 --> 0:49:23.360
<v Speaker 1>in the universe. Yeah, don't understanding the fossil record and

0:49:23.360 --> 0:49:25.839
<v Speaker 1>our ability to analyze this thing doesn't really go much

0:49:25.880 --> 0:49:28.600
<v Speaker 1>further back than like five or six hundred million years

0:49:29.000 --> 0:49:31.720
<v Speaker 1>after like the Cambrian explosion and that kind of stuff.

0:49:31.760 --> 0:49:33.760
<v Speaker 1>But you're right, it could be sort of like every

0:49:33.800 --> 0:49:36.520
<v Speaker 1>thirty million years we play Russian roulette and sometimes we

0:49:36.600 --> 0:49:38.960
<v Speaker 1>win and sometimes we don't win. But then you would

0:49:39.000 --> 0:49:41.759
<v Speaker 1>see that appearing, right, even if it didn't happen every time,

0:49:42.040 --> 0:49:45.280
<v Speaker 1>you would see it appearing at that periodicity. It wouldn't

0:49:45.280 --> 0:49:47.879
<v Speaker 1>have to happen every time for this analysis to reveal it.

0:49:47.920 --> 0:49:50.000
<v Speaker 1>But you're right, Also, this is limited, like we don't

0:49:50.080 --> 0:49:52.799
<v Speaker 1>have that many examples, and so it could be that

0:49:52.800 --> 0:49:55.400
<v Speaker 1>it's there, we just haven't seen enough examples for it

0:49:55.440 --> 0:49:58.000
<v Speaker 1>to sort of rise out of the data statistically. But

0:49:58.080 --> 0:50:00.279
<v Speaker 1>currently when we look at the data, we can't say

0:50:00.280 --> 0:50:03.400
<v Speaker 1>that there's statistical evidence for any sort of periodicity in

0:50:03.440 --> 0:50:06.480
<v Speaker 1>the die off patterns of life on Earth. There's too

0:50:06.560 --> 0:50:10.080
<v Speaker 1>much noise, uh, and there's not really much evidence of

0:50:10.120 --> 0:50:13.920
<v Speaker 1>a signal. And maybe if we had many billions of

0:50:14.000 --> 0:50:16.600
<v Speaker 1>years to work with, we could have better data, but

0:50:16.719 --> 0:50:21.840
<v Speaker 1>we don't have that. And sadly, crocodiles and celia counts

0:50:21.960 --> 0:50:25.360
<v Speaker 1>and some of these really old species are not really

0:50:25.400 --> 0:50:30.120
<v Speaker 1>good at data collections. So exactly, the fascinating thing is

0:50:30.160 --> 0:50:33.200
<v Speaker 1>that all of these events, somebody was there, you know,

0:50:33.360 --> 0:50:36.360
<v Speaker 1>some life was there, some eyeball was around seeing these

0:50:36.400 --> 0:50:39.160
<v Speaker 1>things happen. Just like all of human history, though most

0:50:39.160 --> 0:50:42.480
<v Speaker 1>of it's forgotten, all of it was witnessed, right, there

0:50:42.520 --> 0:50:45.760
<v Speaker 1>was somebody who knew exactly what happened to humans twenty

0:50:45.800 --> 0:50:48.239
<v Speaker 1>thousand years ago. It's just all those people are dead

0:50:48.320 --> 0:50:50.640
<v Speaker 1>and they didn't write it down, and so all that

0:50:50.760 --> 0:50:54.440
<v Speaker 1>information is now lost. That's so frustrating. Sometimes some scientists

0:50:54.440 --> 0:50:56.279
<v Speaker 1>have turned to the interior of the Earth to try

0:50:56.280 --> 0:50:59.480
<v Speaker 1>to understand if there's evidence in the geologic record for

0:50:59.520 --> 0:51:03.040
<v Speaker 1>these impact, not just like did enough species die off,

0:51:03.120 --> 0:51:05.480
<v Speaker 1>because you know, maybe the asteroid hit, but it just

0:51:05.520 --> 0:51:08.120
<v Speaker 1>didn't cause a big die off. So instead they've looked

0:51:08.120 --> 0:51:10.800
<v Speaker 1>at like the Earth itself to see if there's evidence

0:51:10.920 --> 0:51:13.839
<v Speaker 1>for these impacts. And these guys were interested not just

0:51:13.960 --> 0:51:17.759
<v Speaker 1>in asteroid impacts, but also in slow geologic events that

0:51:17.800 --> 0:51:20.279
<v Speaker 1>could have caused die offs from within the Earth. Like

0:51:20.360 --> 0:51:23.560
<v Speaker 1>what if there's some crazy process inside the Earth that

0:51:23.600 --> 0:51:27.799
<v Speaker 1>causes supervolcanoes every fifty million years that causes a die

0:51:27.840 --> 0:51:31.640
<v Speaker 1>off or some other very like slow process that bubbles

0:51:31.719 --> 0:51:34.360
<v Speaker 1>up every x million years and we just haven't understood

0:51:34.400 --> 0:51:36.839
<v Speaker 1>it yet. You know, we've definitely discovered these kinds of

0:51:36.880 --> 0:51:39.480
<v Speaker 1>things in geology many times, so it's fun to sort

0:51:39.480 --> 0:51:43.040
<v Speaker 1>of imagine even deeper time processes. So these guys look

0:51:43.120 --> 0:51:46.440
<v Speaker 1>not just at evidence for asteroid collisions, but also like

0:51:46.680 --> 0:51:50.400
<v Speaker 1>just large marine extinctions or changes in the sea floor

0:51:50.719 --> 0:51:53.520
<v Speaker 1>or big volcanic events. And they did the same thing.

0:51:53.560 --> 0:51:55.640
<v Speaker 1>They did a four the analysis to look for a

0:51:55.760 --> 0:51:58.759
<v Speaker 1>repeating signal to see like is there a period to

0:51:58.840 --> 0:52:02.280
<v Speaker 1>sort of large theological events on the surface of the Earth.

0:52:02.360 --> 0:52:05.160
<v Speaker 1>And these guys in their paper, they actually claim to

0:52:05.320 --> 0:52:09.800
<v Speaker 1>discover a signal every twenty eight million years. They said

0:52:09.840 --> 0:52:14.960
<v Speaker 1>that there's strong statistical evidence for something bad happening every

0:52:15.040 --> 0:52:18.319
<v Speaker 1>twenty eight million years. But I actually have to take

0:52:18.400 --> 0:52:20.520
<v Speaker 1>issue with this paper. I read this paper and I

0:52:20.520 --> 0:52:23.880
<v Speaker 1>think that they've done these statistical analysis wrong. Oh boy,

0:52:24.160 --> 0:52:28.600
<v Speaker 1>some drama, getting ready for some some statistical analysis drama.

0:52:28.600 --> 0:52:30.719
<v Speaker 1>All right, let's go. Let's let's take them down. What

0:52:30.760 --> 0:52:33.360
<v Speaker 1>they did is they looked for the most common recurrence

0:52:33.440 --> 0:52:35.920
<v Speaker 1>and they found something abound twenty eight million years. But

0:52:36.040 --> 0:52:37.719
<v Speaker 1>you know, every time you're gonna look at your data,

0:52:37.719 --> 0:52:39.960
<v Speaker 1>you're gonna find something to be the most common. The

0:52:40.080 --> 0:52:43.399
<v Speaker 1>question is like, how likely is it to be that significant?

0:52:43.440 --> 0:52:45.080
<v Speaker 1>Is it really a big peak or is it just

0:52:45.080 --> 0:52:47.480
<v Speaker 1>sort of like the biggest peak among a bunch of

0:52:47.560 --> 0:52:50.080
<v Speaker 1>random noise. And so they tried to calculate this. They

0:52:50.080 --> 0:52:52.320
<v Speaker 1>try to say, like how likely is there to see

0:52:52.360 --> 0:52:55.080
<v Speaker 1>this big peak at twenty million years? Is this likely

0:52:55.120 --> 0:52:57.360
<v Speaker 1>to just be noise or is this something real? So

0:52:57.400 --> 0:52:59.400
<v Speaker 1>they ran a bunch of statistical tests to see, like

0:52:59.480 --> 0:53:01.520
<v Speaker 1>how like ease it to see something at twenty eight

0:53:01.560 --> 0:53:04.160
<v Speaker 1>million years, and they found those very unlikely to see

0:53:04.200 --> 0:53:07.080
<v Speaker 1>this kind of peak. And from that they conclude, oh,

0:53:07.120 --> 0:53:09.680
<v Speaker 1>while this must be real because it's very unlikely to

0:53:09.760 --> 0:53:13.440
<v Speaker 1>generate this from just random noise. Problem with this method

0:53:13.440 --> 0:53:15.840
<v Speaker 1>of statistical analysis is that they were only calculating the

0:53:15.840 --> 0:53:18.840
<v Speaker 1>probability of seeing a peak from random events at twenty

0:53:18.920 --> 0:53:21.759
<v Speaker 1>eight million years, whereas these random events also could have

0:53:21.800 --> 0:53:24.399
<v Speaker 1>generated peaks at thirty million years and fifteen million years,

0:53:24.440 --> 0:53:26.279
<v Speaker 1>and if they'd seen that in their data, they would

0:53:26.280 --> 0:53:28.799
<v Speaker 1>have happily written a Nature paper about that as well.

0:53:28.920 --> 0:53:31.600
<v Speaker 1>So I think they sort of overstate the case that

0:53:31.680 --> 0:53:35.200
<v Speaker 1>this thing rises above the random noise. And in my view,

0:53:35.280 --> 0:53:39.280
<v Speaker 1>there's no real statistical evidence here for the geologic record

0:53:39.400 --> 0:53:42.520
<v Speaker 1>having any sort of period of major events, so speaking

0:53:42.600 --> 0:53:46.360
<v Speaker 1>purely for a friend who may go a little cross

0:53:46.400 --> 0:53:52.000
<v Speaker 1>side when discussing statistics. So essentially they're basically kind of

0:53:52.120 --> 0:53:56.920
<v Speaker 1>pruning data points that would make this finding more likely,

0:53:57.320 --> 0:54:01.040
<v Speaker 1>whereas if they included in their analysis all the data points,

0:54:01.120 --> 0:54:04.319
<v Speaker 1>you would get a lot more evidence of noise. Yeah,

0:54:04.320 --> 0:54:06.920
<v Speaker 1>it's like saying, what's the chance of getting a random

0:54:06.960 --> 0:54:09.800
<v Speaker 1>peak at this number? It's pretty small. Well, what's the

0:54:09.880 --> 0:54:12.239
<v Speaker 1>chance of getting a random peak at any number? It's

0:54:12.239 --> 0:54:15.040
<v Speaker 1>going to be much much bigger, And that's the number

0:54:15.040 --> 0:54:17.600
<v Speaker 1>they really need to be accounting for, because they would

0:54:17.600 --> 0:54:20.279
<v Speaker 1>have accepted a peak but basically any number. Right now,

0:54:20.320 --> 0:54:22.640
<v Speaker 1>it is interesting that the peak they get is just

0:54:22.719 --> 0:54:26.279
<v Speaker 1>about at thirty million years. That is suggestive because we

0:54:26.320 --> 0:54:28.839
<v Speaker 1>know there is this process where the Sun goes in

0:54:28.880 --> 0:54:32.120
<v Speaker 1>and out of the galactic plane every thirty one million years,

0:54:32.480 --> 0:54:35.080
<v Speaker 1>though they measure there's to be twenty eight million years.

0:54:35.120 --> 0:54:36.920
<v Speaker 1>And that might not seem like a big difference to you,

0:54:37.000 --> 0:54:41.040
<v Speaker 1>but three million years is not a short amount of time. Yeah,

0:54:41.239 --> 0:54:45.640
<v Speaker 1>sounds circumstantial to me. Can you imagine if literature review

0:54:45.760 --> 0:54:48.480
<v Speaker 1>was like a courtroom that you actually got to kind

0:54:48.520 --> 0:54:52.760
<v Speaker 1>of be a big fancy city lawyer in court arguing

0:54:52.840 --> 0:54:56.000
<v Speaker 1>for against statistical analysis. I think that would make science

0:54:56.040 --> 0:54:59.920
<v Speaker 1>a lot more interesting. It would probably make it for

0:55:00.000 --> 0:55:03.080
<v Speaker 1>a lot more deep grudges also, and you know, for

0:55:03.120 --> 0:55:06.520
<v Speaker 1>answering our question about whether there's a pattern to asteroid

0:55:06.560 --> 0:55:09.200
<v Speaker 1>impacts on Earth, remember that this paper is thinking about

0:55:09.239 --> 0:55:13.240
<v Speaker 1>all geological events, supervolcanoes and all sorts of other stuff.

0:55:13.239 --> 0:55:15.040
<v Speaker 1>And if you look at most of these events the

0:55:15.080 --> 0:55:18.960
<v Speaker 1>boundaries between geological time scales. For example, only the event

0:55:19.000 --> 0:55:22.360
<v Speaker 1>it's sixty five million years ago in the geological record

0:55:22.600 --> 0:55:25.360
<v Speaker 1>shows a significant impact. You know, we can see like

0:55:25.440 --> 0:55:28.200
<v Speaker 1>the ash and the dust from that impact in the record.

0:55:28.200 --> 0:55:30.560
<v Speaker 1>If you dig down into the earth, you can find

0:55:30.640 --> 0:55:34.400
<v Speaker 1>that and see the impact the other transition periods and

0:55:34.440 --> 0:55:36.680
<v Speaker 1>the die offs that don't seem to align with any

0:55:36.760 --> 0:55:39.680
<v Speaker 1>asteroid impact. There's no like event. We can find no

0:55:39.840 --> 0:55:43.760
<v Speaker 1>evidence of ash and dust, so it seems pretty loose.

0:55:43.840 --> 0:55:45.600
<v Speaker 1>As far as we can tell right now, there is

0:55:45.680 --> 0:55:49.640
<v Speaker 1>no evidence of periodic asteroid impact on Earth, which is,

0:55:49.680 --> 0:55:51.759
<v Speaker 1>you know, good news because it means that another one

0:55:51.840 --> 0:55:54.440
<v Speaker 1>might not be coming. But it's bad news because it

0:55:54.640 --> 0:55:57.520
<v Speaker 1>means they might just be unpredictable. I mean, it's also

0:55:57.600 --> 0:56:00.480
<v Speaker 1>bad news if I really want to cancel my dentist

0:56:00.520 --> 0:56:04.799
<v Speaker 1>appointment and the next million years or so, you know.

0:56:05.000 --> 0:56:08.239
<v Speaker 1>I think another thing is that when the big one

0:56:08.360 --> 0:56:11.640
<v Speaker 1>hit Earth and you know, killed off the dinosaurs. Of

0:56:11.680 --> 0:56:13.719
<v Speaker 1>course a little more complicated than that. I mean, there

0:56:13.719 --> 0:56:18.160
<v Speaker 1>were also other things happening at the time, other geological

0:56:18.200 --> 0:56:22.760
<v Speaker 1>activity that was contributing to the extinction. So it wasn't

0:56:22.840 --> 0:56:26.080
<v Speaker 1>just the asteroid. They also think that there was volcanic

0:56:26.120 --> 0:56:29.600
<v Speaker 1>activity that had nothing to do with the asteroid that

0:56:29.800 --> 0:56:33.920
<v Speaker 1>was causing an impact on the environment. And so it

0:56:33.960 --> 0:56:38.479
<v Speaker 1>was just this kind of like poorly timed asteroid that

0:56:39.000 --> 0:56:41.239
<v Speaker 1>kind of helped put a nail in the coffin of

0:56:41.760 --> 0:56:47.359
<v Speaker 1>an already sort of precarious situation for the dinosaurs, and

0:56:47.440 --> 0:56:49.840
<v Speaker 1>so yeah, I think it seems like it'd be a

0:56:49.880 --> 0:56:55.319
<v Speaker 1>little too tidy in terms of finding. You know that

0:56:55.440 --> 0:56:58.080
<v Speaker 1>every thirty million years we get hit by an asteroid

0:56:58.120 --> 0:57:01.200
<v Speaker 1>and all the animals, you know, go oh no, except

0:57:01.280 --> 0:57:03.840
<v Speaker 1>for a lucky few of them that end up surviving.

0:57:03.920 --> 0:57:07.440
<v Speaker 1>But it does seem like the actual picture of it

0:57:07.480 --> 0:57:09.759
<v Speaker 1>would be a lot messier, have to do with a

0:57:09.760 --> 0:57:14.760
<v Speaker 1>lot more kind of just a confluence of environmental factors,

0:57:14.800 --> 0:57:17.560
<v Speaker 1>both on Earth and maybe you know, outside of Earth,

0:57:17.680 --> 0:57:21.720
<v Speaker 1>rather than just one kind of convenient every thirty million

0:57:21.800 --> 0:57:25.240
<v Speaker 1>years asteroids and backdown. You sound like the asteroids defense

0:57:25.360 --> 0:57:27.760
<v Speaker 1>lawyer saying, hey, look, it wasn't my client. Even if

0:57:27.800 --> 0:57:30.200
<v Speaker 1>they were there, there was other stuff going on. I

0:57:30.360 --> 0:57:34.080
<v Speaker 1>may be a simple country lawyer, but the evidence that

0:57:34.200 --> 0:57:39.080
<v Speaker 1>my asteroid was anywhere near those dinosaurs is purely circumstantial.

0:57:39.240 --> 0:57:41.160
<v Speaker 1>I'm going to call in Daniel Whiteson to argue about

0:57:41.160 --> 0:57:44.960
<v Speaker 1>the statistical analysis of this paper. Al Right, well, I

0:57:45.000 --> 0:57:48.000
<v Speaker 1>think you can rest easy then, knowing that a big

0:57:48.040 --> 0:57:52.400
<v Speaker 1>asteroid may not necessarily be on way to pulverize all

0:57:52.440 --> 0:57:56.760
<v Speaker 1>of us. That is the most like lackluster optimistic thing

0:57:56.800 --> 0:57:59.320
<v Speaker 1>I've ever heard. It's like you can rest easy knowing

0:57:59.400 --> 0:58:03.360
<v Speaker 1>that you not die a random and horrible death along

0:58:03.400 --> 0:58:06.640
<v Speaker 1>with everyone else on Earth. But hey, you know, glass

0:58:06.680 --> 0:58:09.320
<v Speaker 1>half full. You may not die of predictable periodic death,

0:58:09.440 --> 0:58:12.760
<v Speaker 1>but you may actually die a random, horrible death because

0:58:13.120 --> 0:58:17.320
<v Speaker 1>comments and asteroids are unpredictable, and especially comets are really

0:58:17.320 --> 0:58:20.000
<v Speaker 1>a source of danger. And we need to keep funding

0:58:20.000 --> 0:58:22.240
<v Speaker 1>those telescopes to look out there. We need to keep

0:58:22.280 --> 0:58:26.000
<v Speaker 1>developing these technologies to divert these objects if they do

0:58:26.080 --> 0:58:29.320
<v Speaker 1>come towards our wonderful planet. Oh, I see, this is

0:58:29.360 --> 0:58:32.800
<v Speaker 1>why you're blaming the asteroids. This is a shakedown for

0:58:32.920 --> 0:58:36.120
<v Speaker 1>funding for science, just trying to save the planet. I mean,

0:58:36.240 --> 0:58:39.200
<v Speaker 1>just a little little thing like saving the planet. How convenient?

0:58:40.680 --> 0:58:42.600
<v Speaker 1>All right, Well, thank you Katy very much for joining

0:58:42.760 --> 0:58:46.360
<v Speaker 1>us on this optimistic view of our situation in the

0:58:46.440 --> 0:58:50.640
<v Speaker 1>Solar System and offering your full throw defense of asteroids.

0:58:50.960 --> 0:58:54.200
<v Speaker 1>And thanks everybody for listening to another deep dive into

0:58:54.240 --> 0:58:57.480
<v Speaker 1>the deep history of life on Earth. Thanks for joining us.

0:58:57.480 --> 0:59:07.480
<v Speaker 1>Tune in next time, yea, thanks for listening, and remember

0:59:07.520 --> 0:59:10.360
<v Speaker 1>that Daniel and Jorge explain the universe is a production

0:59:10.440 --> 0:59:13.960
<v Speaker 1>of I heart radio. For more podcast from my heart Radio,

0:59:14.120 --> 0:59:17.680
<v Speaker 1>visit the i heart Radio app, Apple Podcasts, or wherever

0:59:17.800 --> 0:59:19.480
<v Speaker 1>you listen to your favorite shows.