A theory of Earth's mass extinctions
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0:00 - 0:02So, I want to start out with
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0:02 - 0:04this beautiful picture from my childhood.
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0:04 - 0:06I love the science fiction movies.
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0:06 - 0:08Here it is: "This Island Earth."
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0:08 - 0:10And leave it to Hollywood to get it just right.
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0:10 - 0:12Two-and-a-half years in the making.
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0:12 - 0:15(Laughter)
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0:15 - 0:18I mean, even the creationists give us 6,000,
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0:18 - 0:20but Hollywood goes to the chase.
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0:20 - 0:24And in this movie, we see what we think is out there:
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0:24 - 0:27flying saucers and aliens.
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0:27 - 0:30Every world has an alien, and every alien world has a flying saucer,
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0:30 - 0:34and they move about with great speed. Aliens.
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0:35 - 0:38Well, Don Brownlee, my friend, and I finally got to the point
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0:38 - 0:41where we got tired of turning on the TV
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0:41 - 0:44and seeing the spaceships and seeing the aliens every night,
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0:44 - 0:47and tried to write a counter-argument to it,
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0:47 - 0:51and put out what does it really take for an Earth to be habitable,
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0:51 - 0:53for a planet to be an Earth, to have a place
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0:53 - 0:56where you could probably get not just life, but complexity,
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0:56 - 0:58which requires a huge amount of evolution,
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0:58 - 1:01and therefore constancy of conditions.
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1:01 - 1:04So, in 2000 we wrote "Rare Earth." In 2003, we then asked,
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1:04 - 1:09let's not think about where Earths are in space, but how long has Earth been Earth?
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1:09 - 1:11If you go back two billion years,
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1:11 - 1:13you're not on an Earth-like planet any more.
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1:13 - 1:17What we call an Earth-like planet is actually a very short interval of time.
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1:17 - 1:19Well, "Rare Earth" actually
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1:19 - 1:22taught me an awful lot about meeting the public.
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1:22 - 1:25Right after, I got an invitation to go to a science fiction convention,
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1:25 - 1:28and with all great earnestness walked in.
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1:28 - 1:30David Brin was going to debate me on this,
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1:30 - 1:34and as I walked in, the crowd of a hundred started booing lustily.
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1:34 - 1:37I had a girl who came up who said, "My dad says you're the devil."
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1:37 - 1:41You cannot take people's aliens away from them
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1:41 - 1:45and expect to be anybody's friends.
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1:45 - 1:47Well, the second part of that, soon after --
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1:47 - 1:50and I was talking to Paul Allen; I saw him in the audience,
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1:50 - 1:52and I handed him a copy of "Rare Earth."
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1:52 - 1:56And Jill Tarter was there, and she turned to me,
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1:56 - 1:59and she looked at me just like that girl in "The Exorcist."
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1:59 - 2:01It was, "It burns! It burns!"
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2:01 - 2:03Because SETI doesn't want to hear this.
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2:03 - 2:06SETI wants there to be stuff out there.
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2:06 - 2:09I really applaud the SETI efforts, but we have not heard anything yet.
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2:09 - 2:11And I really do think we have to start thinking
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2:11 - 2:14about what's a good planet and what isn't.
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2:14 - 2:17Now, I throw this slide up because it indicates to me that,
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2:17 - 2:21even if SETI does hear something, can we figure out what they said?
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2:21 - 2:23Because this was a slide that was passed
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2:23 - 2:27between the two major intelligences on Earth -- a Mac to a PC --
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2:27 - 2:30and it can't even get the letters right --
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2:30 - 2:32(Laughter)
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2:32 - 2:34-- so how are we going to talk to the aliens?
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2:34 - 2:37And if they're 50 light years away, and we call them up,
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2:37 - 2:39and you blah, blah, blah, blah, blah,
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2:39 - 2:42and then 50 years later it comes back and they say, Please repeat?
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2:42 - 2:44I mean, there we are.
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2:44 - 2:47Our planet is a good planet because it can keep water.
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2:47 - 2:51Mars is a bad planet, but it's still good enough for us to go there
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2:51 - 2:53and to live on its surface if we're protected.
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2:53 - 2:56But Venus is a very bad -- the worst -- planet.
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2:56 - 2:59Even though it's Earth-like, and even though early in its history
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2:59 - 3:02it may very well have harbored Earth-like life,
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3:02 - 3:05it soon succumbed to runaway greenhouse --
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3:05 - 3:07that's an 800 degrees [Fahrenheit] surface --
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3:07 - 3:10because of rampant carbon dioxide.
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3:10 - 3:13Well, we know from astrobiology that we can really now predict
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3:13 - 3:16what's going to happen to our particular planet.
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3:16 - 3:19We are right now in the beautiful Oreo
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3:19 - 3:22of existence -- of at least life on Planet Earth --
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3:22 - 3:25following the first horrible microbial age.
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3:25 - 3:28In the Cambrian explosion, life emerged from the swamps,
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3:28 - 3:30complexity arose,
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3:30 - 3:33and from what we can tell, we're halfway through.
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3:33 - 3:36We have as much time for animals to exist on this planet
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3:36 - 3:38as they have been here now,
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3:38 - 3:40till we hit the second microbial age.
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3:40 - 3:42And that will happen, paradoxically --
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3:42 - 3:44everything you hear about global warming --
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3:44 - 3:47when we hit CO2 down to 10 parts per million,
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3:47 - 3:49we are no longer going to have to have plants
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3:49 - 3:53that are allowed to have any photosynthesis, and there go animals.
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3:53 - 3:55So, after that we probably have seven billion years.
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3:55 - 3:58The Sun increases in its intensity, in its brightness,
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3:58 - 4:03and finally, at about 12 billion years after it first started,
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4:03 - 4:06the Earth is consumed by a large Sun,
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4:06 - 4:09and this is what's left.
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4:09 - 4:13So, a planet like us is going to have an age and an old age,
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4:13 - 4:17and we are in its golden summer age right now.
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4:17 - 4:19But there's two fates to everything, isn't there?
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4:19 - 4:22Now, a lot of you are going to die of old age,
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4:22 - 4:25but some of you, horribly enough, are going to die in an accident.
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4:25 - 4:27And that's the fate of a planet, too.
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4:27 - 4:31Earth, if we're lucky enough -- if it doesn't get hit by a Hale-Bopp,
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4:31 - 4:35or gets blasted by some supernova nearby
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4:35 - 4:38in the next seven billion years -- we'll find under your feet.
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4:38 - 4:40But what about accidental death?
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4:40 - 4:42Well, paleontologists for the last 200 years
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4:42 - 4:44have been charting death. It's strange --
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4:44 - 4:47extinction as a concept wasn't even thought about
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4:47 - 4:50until Baron Cuvier in France found this first mastodon.
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4:50 - 4:52He couldn't match it up to any bones on the planet,
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4:52 - 4:54and he said, Aha! It's extinct.
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4:54 - 4:57And very soon after, the fossil record started yielding
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4:57 - 5:00a very good idea of how many plants and animals there have been
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5:00 - 5:02since complex life really began to leave
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5:02 - 5:05a very interesting fossil record.
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5:05 - 5:08In that complex record of fossils,
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5:08 - 5:10there were times when lots of stuff
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5:10 - 5:12seemed to be dying out very quickly,
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5:12 - 5:14and the father/mother geologists
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5:14 - 5:16called these "mass extinctions."
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5:16 - 5:18All along it was thought to be either an act of God
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5:18 - 5:20or perhaps long, slow climate change,
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5:20 - 5:22and that really changed in 1980,
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5:22 - 5:25in this rocky outcrop near Gubbio,
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5:25 - 5:28where Walter Alvarez, trying to figure out
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5:28 - 5:31what was the time difference between these white rocks,
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5:31 - 5:33which held creatures of the Cretaceous period,
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5:33 - 5:35and the pink rocks above, which held Tertiary fossils.
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5:35 - 5:39How long did it take to go from one system to the next?
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5:39 - 5:41And what they found was something unexpected.
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5:41 - 5:44They found in this gap, in between, a very thin clay layer,
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5:44 - 5:47and that clay layer -- this very thin red layer here --
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5:47 - 5:49is filled with iridium.
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5:49 - 5:52And not just iridium; it's filled with glassy spherules,
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5:52 - 5:54and it's filled with quartz grains
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5:54 - 5:58that have been subjected to enormous pressure: shock quartz.
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5:58 - 6:00Now, in this slide the white is chalk,
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6:00 - 6:03and this chalk was deposited in a warm ocean.
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6:03 - 6:05The chalk itself's composed by plankton
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6:05 - 6:09which has fallen down from the sea surface onto the sea floor,
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6:09 - 6:12so that 90 percent of the sediment here is skeleton of living stuff,
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6:12 - 6:14and then you have that millimeter-thick red layer,
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6:14 - 6:16and then you have black rock.
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6:16 - 6:19And the black rock is the sediment on the sea bottom
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6:19 - 6:21in the absence of plankton.
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6:21 - 6:25And that's what happens in an asteroid catastrophe,
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6:25 - 6:28because that's what this was, of course. This is the famous K-T.
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6:28 - 6:30A 10-kilometer body hit the planet.
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6:30 - 6:34The effects of it spread this very thin impact layer all over the planet,
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6:34 - 6:37and we had very quickly the death of the dinosaurs,
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6:37 - 6:39the death of these beautiful ammonites,
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6:39 - 6:41Leconteiceras here, and Celaeceras over here,
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6:41 - 6:43and so much else.
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6:43 - 6:45I mean, it must be true,
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6:45 - 6:48because we've had two Hollywood blockbusters since that time,
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6:48 - 6:51and this paradigm, from 1980 to about 2000,
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6:51 - 6:56totally changed how we geologists thought about catastrophes.
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6:56 - 6:59Prior to that, uniformitarianism was the dominant paradigm:
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6:59 - 7:02the fact that if anything happens on the planet in the past,
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7:02 - 7:06there are present-day processes that will explain it.
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7:06 - 7:09But we haven't witnessed a big asteroid impact,
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7:09 - 7:11so this is a type of neo-catastrophism,
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7:11 - 7:14and it took about 20 years for the scientific establishment
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7:14 - 7:16to finally come to grips: yes, we were hit;
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7:16 - 7:20and yes, the effects of that hit caused a major mass extinction.
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7:21 - 7:23Well, there are five major mass extinctions
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7:23 - 7:26over the last 500 million years, called the Big Five.
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7:26 - 7:29They range from 450 million years ago
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7:29 - 7:31to the last, the K-T, number four,
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7:31 - 7:35but the biggest of all was the P, or the Permian extinction,
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7:35 - 7:37sometimes called the mother of all mass extinctions.
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7:37 - 7:40And every one of these has been subsequently blamed
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7:40 - 7:42on large-body impact.
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7:42 - 7:44But is this true?
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7:45 - 7:48The most recent, the Permian, was thought to have been an impact
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7:48 - 7:50because of this beautiful structure on the right.
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7:50 - 7:53This is a Buckminsterfullerene, a carbon-60.
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7:53 - 7:56Because it looks like those terrible geodesic domes
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7:56 - 7:58of my late beloved '60s,
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7:58 - 8:00they're called "buckyballs."
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8:00 - 8:02This evidence was used to suggest
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8:02 - 8:06that at the end of the Permian, 250 million years ago, a comet hit us.
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8:06 - 8:09And when the comet hits, the pressure produces the buckyballs,
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8:09 - 8:11and it captures bits of the comet.
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8:11 - 8:15Helium-3: very rare on the surface of the Earth, very common in space.
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8:16 - 8:18But is this true?
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8:18 - 8:22In 1990, working on the K-T extinction for 10 years,
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8:22 - 8:25I moved to South Africa to begin work twice a year
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8:25 - 8:27in the great Karoo desert.
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8:27 - 8:30I was so lucky to watch the change of that South Africa
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8:30 - 8:33into the new South Africa as I went year by year.
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8:33 - 8:35And I worked on this Permian extinction,
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8:35 - 8:38camping by this Boer graveyard for months at a time.
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8:38 - 8:41And the fossils are extraordinary.
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8:41 - 8:43You know, you're gazing upon your very distant ancestors.
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8:43 - 8:45These are mammal-like reptiles.
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8:45 - 8:48They are culturally invisible. We do not make movies about these.
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8:48 - 8:50This is a Gorgonopsian, or a Gorgon.
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8:50 - 8:54That's an 18-inch long skull of an animal
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8:54 - 8:58that was probably seven or eight feet, sprawled like a lizard,
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8:58 - 9:00probably had a head like a lion.
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9:00 - 9:02This is the top carnivore, the T-Rex of its time.
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9:02 - 9:04But there's lots of stuff.
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9:04 - 9:06This is my poor son, Patrick.
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9:06 - 9:07(Laughter)
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9:07 - 9:10This is called paleontological child abuse.
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9:10 - 9:12Hold still, you're the scale.
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9:12 - 9:17(Laughter)
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9:18 - 9:21There was big stuff back then.
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9:21 - 9:24Fifty-five species of mammal-like reptiles.
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9:24 - 9:27The age of mammals had well and truly started
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9:27 - 9:29250 million years ago ...
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9:29 - 9:32... and then a catastrophe happened.
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9:32 - 9:34And what happens next is the age of dinosaurs.
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9:34 - 9:38It was all a mistake; it should have never happened. But it did.
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9:38 - 9:40Now, luckily,
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9:40 - 9:43this Thrinaxodon, the size of a robin egg here:
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9:43 - 9:46this is a skull I've discovered just before taking this picture --
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9:46 - 9:48there's a pen for scale; it's really tiny --
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9:48 - 9:52this is in the Lower Triassic, after the mass extinction has finished.
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9:52 - 9:55You can see the eye socket and you can see the little teeth in the front.
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9:55 - 10:00If that does not survive, I'm not the thing giving this talk.
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10:00 - 10:04Something else is, because if that doesn't survive, we are not here;
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10:04 - 10:08there are no mammals. It's that close; one species ekes through.
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10:08 - 10:11Well, can we say anything about the pattern of who survives and who doesn't?
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10:11 - 10:13Here's sort of the end of that 10 years of work.
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10:13 - 10:16The ranges of stuff -- the red line is the mass extinction.
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10:16 - 10:18But we've got survivors and things that get through,
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10:18 - 10:22and it turns out the things that get through preferentially are cold bloods.
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10:22 - 10:26Warm-blooded animals take a huge hit at this time.
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10:27 - 10:29The survivors that do get through
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10:29 - 10:32produce this world of crocodile-like creatures.
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10:32 - 10:36There's no dinosaurs yet; just this slow, saurian, scaly, nasty,
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10:36 - 10:41swampy place with a couple of tiny mammals hiding in the fringes.
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10:41 - 10:44And there they would hide for 160 million years,
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10:44 - 10:47until liberated by that K-T asteroid.
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10:47 - 10:49So, if not impact, what?
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10:49 - 10:53And the what, I think, is that we returned, over and over again,
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10:53 - 10:56to the Pre-Cambrian world, that first microbial age,
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10:56 - 10:58and the microbes are still out there.
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10:58 - 11:00They hate we animals.
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11:00 - 11:02They really want their world back.
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11:02 - 11:06And they've tried over and over and over again.
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11:06 - 11:09This suggests to me that life causing these mass extinctions
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11:09 - 11:12because it did is inherently anti-Gaian.
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11:12 - 11:17This whole Gaia idea, that life makes the world better for itself --
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11:17 - 11:21anybody been on a freeway on a Friday afternoon in Los Angeles
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11:21 - 11:23believing in the Gaia theory? No.
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11:23 - 11:26So, I really suspect there's an alternative,
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11:26 - 11:28and that life does actually try to do itself in --
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11:28 - 11:30not consciously, but just because it does.
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11:30 - 11:34And here's the weapon, it seems, that it did so over the last 500 million years.
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11:34 - 11:37There are microbes which, through their metabolism,
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11:37 - 11:39produce hydrogen sulfide,
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11:39 - 11:42and they do so in large amounts.
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11:42 - 11:45Hydrogen sulfide is very fatal to we humans.
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11:45 - 11:49As small as 200 parts per million will kill you.
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11:51 - 11:55You only have to go to the Black Sea and a few other places -- some lakes --
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11:55 - 11:59and get down, and you'll find that the water itself turns purple.
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11:59 - 12:02It turns purple from the presence of numerous microbes
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12:02 - 12:05which have to have sunlight and have to have hydrogen sulfide,
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12:05 - 12:09and we can detect their presence today -- we can see them --
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12:09 - 12:11but we can also detect their presence in the past.
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12:11 - 12:13And the last three years have seen
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12:13 - 12:16an enormous breakthrough in a brand-new field.
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12:16 - 12:18I am almost extinct --
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12:18 - 12:20I'm a paleontologist who collects fossils.
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12:20 - 12:23But the new wave of paleontologists -- my graduate students --
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12:23 - 12:25collect biomarkers.
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12:25 - 12:29They take the sediment itself, they extract the oil from it,
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12:29 - 12:31and from that they can produce compounds
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12:31 - 12:35which turn out to be very specific to particular microbial groups.
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12:35 - 12:39It's because lipids are so tough, they can get preserved in sediment
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12:39 - 12:42and last the hundreds of millions of years necessary,
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12:42 - 12:44and be extracted and tell us who was there.
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12:44 - 12:47And we know who was there. At the end of the Permian,
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12:47 - 12:49at many of these mass extinction boundaries,
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12:49 - 12:53this is what we find: isorenieratene. It's very specific.
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12:53 - 12:57It can only occur if the surface of the ocean has no oxygen,
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12:57 - 13:00and is totally saturated with hydrogen sulfide --
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13:00 - 13:03enough, for instance, to come out of solution.
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13:03 - 13:07This led Lee Kump, and others from Penn State and my group,
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13:07 - 13:10to propose what I call the Kump Hypothesis:
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13:10 - 13:13many of the mass extinctions were caused by lowering oxygen,
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13:13 - 13:17by high CO2. And the worst effect of global warming, it turns out:
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13:17 - 13:20hydrogen sulfide being produced out of the oceans.
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13:20 - 13:22Well, what's the source of this?
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13:22 - 13:26In this particular case, the source over and over has been flood basalts.
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13:26 - 13:29This is a view of the Earth now, if we extract a lot of it.
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13:29 - 13:31And each of these looks like a hydrogen bomb;
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13:31 - 13:33actually, the effects are even worse.
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13:33 - 13:36This is when deep-Earth material comes to the surface,
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13:36 - 13:38spreads out over the surface of the planet.
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13:38 - 13:41Well, it's not the lava that kills anything,
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13:41 - 13:43it's the carbon dioxide that comes out with it.
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13:43 - 13:46This isn't Volvos; this is volcanoes.
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13:46 - 13:48But carbon dioxide is carbon dioxide.
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13:49 - 13:52So, these are new data Rob Berner and I -- from Yale -- put together,
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13:52 - 13:54and what we try to do now is
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13:54 - 13:57track the amount of carbon dioxide in the entire rock record --
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13:57 - 14:00and we can do this from a variety of means --
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14:00 - 14:02and put all the red lines here,
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14:02 - 14:05when these -- what I call greenhouse mass extinctions -- took place.
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14:05 - 14:07And there's two things that are really evident here to me,
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14:07 - 14:10is that these extinctions take place when CO2 is going up.
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14:10 - 14:13But the second thing that's not shown on here:
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14:13 - 14:16the Earth has never had any ice on it
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14:16 - 14:20when we've had 1,000 parts per million CO2.
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14:20 - 14:22We are at 380 and climbing.
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14:22 - 14:25We should be up to a thousand in three centuries at the most,
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14:25 - 14:29but my friend David Battisti in Seattle says he thinks a 100 years.
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14:29 - 14:31So, there goes the ice caps,
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14:31 - 14:35and there comes 240 feet of sea level rise.
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14:35 - 14:37I live in a view house now;
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14:37 - 14:39I'm going to have waterfront.
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14:39 - 14:43All right, what's the consequence? The oceans probably turn purple.
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14:43 - 14:46And we think this is the reason that complexity took so long
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14:46 - 14:48to take place on planet Earth.
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14:48 - 14:51We had these hydrogen sulfide oceans for a very great long period.
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14:51 - 14:55They stop complex life from existing.
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14:55 - 15:00We know hydrogen sulfide is erupting presently a few places on the planet.
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15:00 - 15:04And I throw this slide in -- this is me, actually, two months ago --
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15:04 - 15:08and I throw this slide in because here is my favorite animal, chambered nautilus.
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15:08 - 15:12It's been on this planet since the animals first started -- 500 million years.
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15:12 - 15:15This is a tracking experiment, and any of you scuba divers,
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15:15 - 15:18if you want to get involved in one of the coolest projects ever,
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15:18 - 15:20this is off the Great Barrier Reef.
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15:20 - 15:21And as we speak now,
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15:21 - 15:24these nautilus are tracking out their behaviors to us.
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15:24 - 15:28But the thing about this is that every once in a while
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15:28 - 15:30we divers can run into trouble,
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15:30 - 15:32so I'm going to do a little thought experiment here.
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15:32 - 15:35This is a Great White Shark that ate some of my traps.
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15:35 - 15:38We pulled it up; up it comes. So, it's out there with me at night.
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15:38 - 15:41So, I'm swimming along, and it takes off my leg.
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15:41 - 15:44I'm 80 miles from shore, what's going to happen to me?
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15:44 - 15:46Well now, I die.
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15:46 - 15:48Five years from now, this is what I hope happens to me:
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15:48 - 15:51I'm taken back to the boat, I'm given a gas mask:
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15:51 - 15:5480 parts per million hydrogen sulfide.
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15:54 - 15:58I'm then thrown in an ice pond, I'm cooled 15 degrees lower
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15:58 - 16:02and I could be taken to a critical care hospital.
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16:02 - 16:04And the reason I could do that is because we mammals
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16:04 - 16:07have gone through a series of these hydrogen sulfide events,
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16:07 - 16:09and our bodies have adapted.
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16:09 - 16:13And we can now use this as what I think will be a major medical breakthrough.
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16:13 - 16:15This is Mark Roth. He was funded by DARPA.
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16:15 - 16:19Tried to figure out how to save Americans after battlefield injuries.
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16:19 - 16:21He bleeds out pigs.
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16:21 - 16:24He puts in 80 parts per million hydrogen sulfide --
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16:24 - 16:27the same stuff that survived these past mass extinctions --
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16:27 - 16:29and he turns a mammal into a reptile.
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16:29 - 16:33"I believe we are seeing in this response the result of mammals and reptiles
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16:33 - 16:36having undergone a series of exposures to H2S."
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16:36 - 16:38I got this email from him two years ago;
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16:38 - 16:41he said, "I think I've got an answer to some of your questions."
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16:41 - 16:43So, he now has taken mice down
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16:43 - 16:47for as many as four hours, sometimes six hours,
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16:47 - 16:49and these are brand-new data he sent me on the way over here.
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16:49 - 16:54On the top, now, that is a temperature record of a mouse who has gone through --
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16:54 - 16:56the dotted line, the temperatures.
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16:56 - 16:58So, the temperature starts at 25 centigrade,
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16:58 - 16:59and down it goes, down it goes.
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16:59 - 17:01Six hours later, up goes the temperature.
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17:01 - 17:06Now, the same mouse is given 80 parts per million hydrogen sulfide
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17:06 - 17:08in this solid graph,
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17:08 - 17:10and look what happens to its temperature.
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17:10 - 17:12Its temperature drops.
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17:12 - 17:16It goes down to 15 degrees centigrade from 35,
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17:16 - 17:19and comes out of this perfectly fine.
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17:19 - 17:22Here is a way we can get people to critical care.
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17:22 - 17:27Here's how we can bring people cold enough to last till we get critical care.
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17:28 - 17:32Now, you're all thinking, yeah, what about the brain tissue?
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17:32 - 17:35And so this is one of the great challenges that is going to happen.
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17:35 - 17:37You're in an accident. You've got two choices:
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17:37 - 17:40you're going to die, or you're going to take the hydrogen sulfide
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17:40 - 17:43and, say, 75 percent of you is saved, mentally.
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17:43 - 17:45What are you going to do?
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17:45 - 17:48Do we all have to have a little button saying, Let me die?
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17:48 - 17:50This is coming towards us,
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17:50 - 17:52and I think this is going to be a revolution.
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17:52 - 17:55We're going to save lives, but there's going to be a cost to it.
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17:55 - 17:57The new view of mass extinctions is, yes, we were hit,
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17:57 - 17:59and, yes, we have to think about the long term,
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17:59 - 18:01because we will get hit again.
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18:01 - 18:03But there's a far worse danger confronting us.
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18:03 - 18:06We can easily go back to the hydrogen sulfide world.
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18:06 - 18:08Give us a few millennia --
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18:08 - 18:10and we humans should last those few millennia --
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18:10 - 18:14will it happen again? If we continue, it'll happen again.
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18:14 - 18:16How many of us flew here?
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18:16 - 18:18How many of us have gone through
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18:18 - 18:21our entire Kyoto quota
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18:21 - 18:23just for flying this year?
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18:23 - 18:26How many of you have exceeded it? Yeah, I've certainly exceeded it.
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18:26 - 18:29We have a huge problem facing us as a species.
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18:29 - 18:31We have to beat this.
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18:31 - 18:35I want to be able to go back to this reef. Thank you.
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18:35 - 18:41(Applause)
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18:41 - 18:43Chris Anderson: I've just got one question for you, Peter.
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18:43 - 18:45Am I understanding you right, that what you're saying here
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18:45 - 18:47is that we have in our own bodies
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18:47 - 18:51a biochemical response to hydrogen sulfide
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18:51 - 18:54that in your mind proves that there have been past mass extinctions
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18:54 - 18:56due to climate change?
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18:56 - 18:58Peter Ward: Yeah, every single cell in us
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18:58 - 19:01can produce minute quantities of hydrogen sulfide in great crises.
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19:02 - 19:03This is what Roth has found out.
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19:03 - 19:05So, what we're looking at now: does it leave a signal?
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19:05 - 19:07Does it leave a signal in bone or in plant?
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19:07 - 19:10And we go back to the fossil record and we could try to detect
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19:10 - 19:12how many of these have happened in the past.
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19:12 - 19:14CA: It's simultaneously
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19:14 - 19:17an incredible medical technique, but also a terrifying ...
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19:17 - 19:20PW: Blessing and curse.
- Title:
- A theory of Earth's mass extinctions
- Speaker:
- Peter Ward
- Description:
-
Asteroid strikes get all the coverage, but "Medea Hypothesis" author Peter Ward argues that most of Earth's mass extinctions were caused by lowly bacteria. The culprit, a poison called hydrogen sulfide, may have an interesting application in medicine.
- Video Language:
- English
- Team:
closed TED
- Project:
- TEDTalks
- Duration:
- 19:18
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TED edited English subtitles for A theory of Earth's mass extinctions | |
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TED edited English subtitles for A theory of Earth's mass extinctions | |
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TED edited English subtitles for A theory of Earth's mass extinctions | |
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TED added a translation |