TED2015
Nathalie Cabrol: How Mars might hold the secret to the origin of life
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While we like to imagine little green men, it's far more likely that life on other planets will be microbial. Planetary scientist Nathalie Cabrol takes us inside the search for microbes on Mars, a hunt which counterintuitively leads us to the remote lakes of the Andes mountains. This extreme environment — with its thin atmosphere and scorched land — approximates the surface of Mars about 3.5 billion years ago. How microbes adapt to survive here may just show us where to look on Mars — and could help us understand why some microbial pathways lead to civilization while others are a dead end.
Nathalie Cabrol - Planetary explorer
To determine how life might persist on Mars, Nathalie Cabrol explores one of Earth’s most extreme environments: high-elevation Andean lakes and deserts. Full bio
To determine how life might persist on Mars, Nathalie Cabrol explores one of Earth’s most extreme environments: high-elevation Andean lakes and deserts. Full bio
Double-click the English transcript below to play the video.
00:12
Well, you know, sometimes
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the most important things come
in the smallest packages.
in the smallest packages.
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I am going to try to convince you,
in the 15 minutes I have,
in the 15 minutes I have,
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that microbes have a lot to say
about questions such as,
about questions such as,
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"Are we alone?"
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and they can tell us more about
not only life in our solar system
not only life in our solar system
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but also maybe beyond,
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and this is why I am tracking them down
in the most impossible places on Earth,
in the most impossible places on Earth,
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in extreme environments where conditions
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are really pushing them
to the brink of survival.
to the brink of survival.
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Actually, sometimes me too,
when I'm trying to follow them too close.
when I'm trying to follow them too close.
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But here's the thing:
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We are the only advanced civilization
in the solar system,
in the solar system,
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but that doesn't mean that there is
no microbial life nearby.
no microbial life nearby.
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In fact, the planets
and moons you see here
and moons you see here
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could host life -- all of them --
and we know that,
and we know that,
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and it's a strong possibility.
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And if we were going to find life
on those moons and planets,
on those moons and planets,
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then we would answer questions such as,
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are we alone in the solar system?
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Where are we coming from?
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Do we have family in the neighborhood?
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Is there life beyond our solar system?
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And we can ask all those questions
because there has been a revolution
because there has been a revolution
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in our understanding
of what a habitable planet is,
of what a habitable planet is,
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and today, a habitable planet is a planet
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that has a zone where
water can stay stable,
water can stay stable,
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but to me this is a horizontal
definition of habitability,
definition of habitability,
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because it involves a distance to a star,
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but there is another
dimension to habitability,
dimension to habitability,
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and this is a vertical dimension.
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Think of it as
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conditions in the subsurface of a planet
where you are very far away from a sun,
where you are very far away from a sun,
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but you still have water,
energy, nutrients,
energy, nutrients,
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which for some of them means food,
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and a protection.
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And when you look at the Earth,
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very far away from any sunlight,
deep in the ocean,
deep in the ocean,
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you have life thriving
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and it uses only chemistry
for life processes.
for life processes.
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So when you think of it
at that point, all walls collapse.
at that point, all walls collapse.
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You have no limitations, basically.
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And if you have been looking
at the headlines lately,
at the headlines lately,
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then you will see that we have
discovered a subsurface ocean
discovered a subsurface ocean
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on Europa, on Ganymede,
on Enceladus, on Titan,
on Enceladus, on Titan,
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and now we are finding a geyser
and hot springs on Enceladus,
and hot springs on Enceladus,
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Our solar system is turning
into a giant spa.
into a giant spa.
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For anybody who has gone to a spa
knows how much microbes like that, right?
knows how much microbes like that, right?
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(Laughter)
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So at that point, think also about Mars.
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There is no life possible
at the surface of Mars today,
at the surface of Mars today,
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but it might still be hiding underground.
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So, we have been making progress
in our understanding of habitability,
in our understanding of habitability,
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but we also have been making progress
in our understanding
in our understanding
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of what the signatures
of life are on Earth.
of life are on Earth.
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03:17
And you can have what we call
organic molecules,
organic molecules,
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and these are the bricks of life,
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and you can have fossils,
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and you can minerals, biominerals,
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which is due to the reaction
between bacteria and rocks,
between bacteria and rocks,
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and of course you can have
gases in the atmosphere.
gases in the atmosphere.
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And when you look at those
tiny green algae
tiny green algae
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on the right of the slide here,
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they are the direct descendants
of those who have been pumping oxygen
of those who have been pumping oxygen
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a billion years ago
in the atmosphere of the Earth.
in the atmosphere of the Earth.
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When they did that, they poisoned
90 percent of the life
90 percent of the life
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at the surface of the Earth,
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but they are the reason why
you are breathing this air today.
you are breathing this air today.
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But as much as our understanding grows
of all of these things,
of all of these things,
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there is one question
we still cannot answer,
we still cannot answer,
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and this is, where are we coming from?
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And you know, it's getting worse,
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because we won't be able
to find the physical evidence
to find the physical evidence
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of where we are coming from
on this planet,
on this planet,
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and the reason being is that anything that
is older than four billion years is gone.
is older than four billion years is gone.
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All record is gone,
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erased by plate tectonics and erosion.
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This is what I call the Earth's
biological horizon.
biological horizon.
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Beyond this horizon we don't know
where we are coming from.
where we are coming from.
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So is everything lost? Well, maybe not.
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And we might be able to find
evidence of our own origin
evidence of our own origin
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in the most unlikely place,
and this place in Mars.
and this place in Mars.
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How is this possible?
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Well clearly at the beginning
of the solar system,
of the solar system,
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Mars and the Earth were bombarded
by giant asteroids and comets,
by giant asteroids and comets,
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and there were ejecta
from these impacts all over the place.
from these impacts all over the place.
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Earth and Mars kept throwing rocks
at each other for a very long time.
at each other for a very long time.
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Pieces of rocks landed on the Earth.
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Pieces of the Earth landed on Mars.
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So clearly, those two planets may have
been seeded by the same material.
been seeded by the same material.
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So yeah, maybe Granddady is sitting
there on the surface and waiting for us.
there on the surface and waiting for us.
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But that also means that we can go to Mars
and try to find traces of our own origin.
and try to find traces of our own origin.
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Mars may hold that secret for us.
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This is why Mars is so special to us.
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But for that to happen,
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Mars needed to be habitable
at the time when conditions were right.
at the time when conditions were right.
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So was Mars habitable?
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We have a number of missions
telling us exactly the same thing today.
telling us exactly the same thing today.
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At the time when life
appeared on the Earth,
appeared on the Earth,
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Mars did have an ocean,
it had volcanoes, it had lakes,
it had volcanoes, it had lakes,
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and it had deltas like the beautiful
picture you see here.
picture you see here.
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This picture was sent by the Curiosity
rover only a few weeks ago.
rover only a few weeks ago.
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It shows the remnants of a delta,
and this picture tells us something:
and this picture tells us something:
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water was abundant
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and stayed founting at the surface
for a very long time.
for a very long time.
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This is good news for life.
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Life chemistry takes a long time
to actually happen.
to actually happen.
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So this is extremely good news,
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but does that mean that if we go there,
life will be easy to find on Mars?
life will be easy to find on Mars?
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Not necessarily.
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Here's what happened:
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At the time when life exploded
at the surface of the Earth,
at the surface of the Earth,
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then everything went south for Mars,
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literally.
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The atmosphere was
stripped away by solar winds,
stripped away by solar winds,
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Mars lost its magnetosphere,
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and then cosmic rays and U.V.
bombarded the surface
bombarded the surface
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and water escaped to space
and went underground.
and went underground.
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So if we want to be able to understand,
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if we want to be able to find those traces
of the signatures of life
of the signatures of life
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at the surface of Mars, if they are there,
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we need to understand what was
the impact of each of these events
the impact of each of these events
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on the preservation of its record.
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Only then will we be able
to know where those signatures are hiding,
to know where those signatures are hiding,
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and only then will we be able
to send our rover to the right places
to send our rover to the right places
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where we can sample those rocks
that may be telling us something
that may be telling us something
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really important about who we are,
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or, if not, maybe telling us
that somewhere, independently,
that somewhere, independently,
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life has appeared on another planet.
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So to do that, it's easy.
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You only need to go back
3.5 billion years ago
3.5 billion years ago
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in the past of a planet.
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We just need a time machine.
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Easy, right?
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Well, actually, it is.
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Look around you -- that's planet Earth.
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This is our time machine.
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Geologists are using it
to go back in the past of our own planet.
to go back in the past of our own planet.
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I am using it a little bit differently.
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I use planet Earth to go
in very extreme environments
in very extreme environments
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where conditions were similar
to those of Mars
to those of Mars
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at the time when the climate changed,
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and there I'm trying
to understand what happened.
to understand what happened.
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What are the signatures of life?
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What is left? How are we going to find it?
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So for one moment now
I'm going to take you with me
I'm going to take you with me
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on a trip into that time machine.
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And now, what you see here,
we are at 4,500 meters in the Andes,
we are at 4,500 meters in the Andes,
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but in fact we are less than a billion
years after the Earth and Mars formed.
years after the Earth and Mars formed.
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The Earth and Mars will have looked
pretty much exactly like that --
pretty much exactly like that --
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volcanoes everywhere,
evaporating lakes everywhere,
evaporating lakes everywhere,
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minerals, hot springs,
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and then you see those mounds
on the shore of those lakes?
on the shore of those lakes?
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Those are built by the descendants
of the first organisms
of the first organisms
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that gave us the first fossil on Earth.
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But if we want to understand what's
going on, we need to go a little further.
going on, we need to go a little further.
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And the other thing about those sites
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is that exactly like on Mars
three and a half billion years ago,
three and a half billion years ago,
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the climate is changing very fast,
and water and ice are disappearing.
and water and ice are disappearing.
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But we need to go back to that time
when everything changed on Mars,
when everything changed on Mars,
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and to do that, we need to go higher.
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Why is that?
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Because when you go higher,
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the atmosphere is getting thinner,
it's getting more unstable,
it's getting more unstable,
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the temperature is getting cooler,
and you have a lot more U.V. radiation.
and you have a lot more U.V. radiation.
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Basically,
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you are getting to those conditions
on Mars when everything changed.
on Mars when everything changed.
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So I was not promising anything about
a leisurely trip on the time machine.
a leisurely trip on the time machine.
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You are not going to be sitting
in that time machine.
in that time machine.
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You have to haul 1,000 pounds
of equipment to the summit
of equipment to the summit
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of this 20,000-foot volcano
in the Andes here.
in the Andes here.
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That's about 6,000 meters.
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And you also have to sleep
on 42-degree slopes
on 42-degree slopes
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and really hope that there won't
be any earthquake that night.
be any earthquake that night.
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But when we get to the summit,
we actually find the lake we came for.
we actually find the lake we came for.
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At this altitude, this lake is
experiencing exactly the same conditions
experiencing exactly the same conditions
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as those on Mars
three and a half billion years ago.
three and a half billion years ago.
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And now we have to change our voyage
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into an inner voyage inside that lake,
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and to do that, we have to remove
our mountain gear
our mountain gear
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and actually don suits and go for it.
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But at the time we enter that lake,
at the very moment we enter that lake,
at the very moment we enter that lake,
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we are stepping back
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three and a half billion years
in the past of another planet,
in the past of another planet,
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and then we are going to get
the answer came for.
the answer came for.
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Life is everywhere, absolutely everywhere.
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Everything you see in this picture
is a living organism.
is a living organism.
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Maybe not so the diver,
but everything else.
but everything else.
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But this picture is very deceiving.
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Life is abundant in those lakes,
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but like in many places on Earth
right now and due to climate change,
right now and due to climate change,
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there is a huge loss in biodiversity.
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In the samples that we took back home,
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36 percent of the bacteria in those lakes
were composed of three species,
were composed of three species,
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and those three species are the ones
that have survived so far.
that have survived so far.
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Here's another lake,
right next to the first one.
right next to the first one.
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The red color you see here
is not due to minerals.
is not due to minerals.
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It's actually due to the presence
of a tiny algae.
of a tiny algae.
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In this region, the U.V. radiation
is really nasty.
is really nasty.
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Anywhere on Earth, 11
is considered to be extreme.
is considered to be extreme.
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During U.V. storms there,
the U.V. Index reaches 43.
the U.V. Index reaches 43.
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SPF 30 is not going to do anything
to you over there,
to you over there,
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and the water is so
transparent in those lakes
transparent in those lakes
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that the algae has
nowhere to hide, really,
nowhere to hide, really,
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and so they are developing
their own sunscreen,
their own sunscreen,
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and this is the red color you see.
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But they can adapt only so far,
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and then when all the water
is gone from the surface,
is gone from the surface,
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microbes have only one solution left:
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They go underground.
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And those microbes, the rocks
you see in that slide here,
you see in that slide here,
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well, they are actually
living inside rocks
living inside rocks
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and they are using the protection
of the translucence of the rocks
of the translucence of the rocks
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to get the good part of the U.V.
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and discard the part that could
actually damage their DNA.
actually damage their DNA.
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And this is why we are taking our rover
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to train them to search
for life on Mars in these areas,
for life on Mars in these areas,
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because if there was life on Mars
three and a half billion years ago,
three and a half billion years ago,
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it had to use the same strategy
to actually protect itself.
to actually protect itself.
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Now, it is pretty obvious
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that going to extreme environments
is helping us very much
is helping us very much
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for the exploration of Mars
and to prepare missions.
and to prepare missions.
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So far, it has helped us to understand
the geology of Mars.
the geology of Mars.
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It has helped to understand the past
climate of Mars and its evolution,
climate of Mars and its evolution,
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but also its habitability potential.
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Our most recent rover on Mars
has discovered traces of organics.
has discovered traces of organics.
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Yeah, there are organics
at the surface of Mars.
at the surface of Mars.
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And it also discovered traces of methane.
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And we don't know yet
if the methane in question
if the methane in question
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is really from geology or biology.
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Regardless, what we know is
that because of the discovery,
that because of the discovery,
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the hypothesis that there is still
life present on Mars today
life present on Mars today
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remains a viable one.
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So by now, I think I have convinced you
that Mars is very special to us,
that Mars is very special to us,
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but it would be a mistake to think
that Mars is the only place
that Mars is the only place
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in the solar system that is interesting
to find potential microbial life.
to find potential microbial life.
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And the reason is because
Mars and the Earth
Mars and the Earth
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could have a common root
to their tree of life,
to their tree of life,
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but when you go beyond Mars,
it's not that easy.
it's not that easy.
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Celestial mechanics
is not making it so easy
is not making it so easy
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for an exchange
of material between planets,
of material between planets,
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and so if we were to discover
life on those planets,
life on those planets,
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it would be different from us.
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It would be a different type of life.
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But in the end, it might be just us,
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it might be us and Mars,
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or it can be many trees of life
in the solar system.
in the solar system.
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I don't know the answer yet,
but I can tell you something:
but I can tell you something:
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No matter what the result is,
no matter what that magic number is,
no matter what that magic number is,
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it is going to give us a standard
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by which we are going to be able
to measure the life potential,
to measure the life potential,
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abundance and diversity
beyond our own solar system.
beyond our own solar system.
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And this can be achieved
by our generation.
by our generation.
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This can be our legacy,
but only if we dare to explore.
but only if we dare to explore.
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Now, finally,
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if somebody tells you that looking
for alien microbes is not cool
for alien microbes is not cool
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because you cannot have
a philosophical conversation with them,
a philosophical conversation with them,
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let me show you why and how
you can tell them they're wrong.
you can tell them they're wrong.
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Well, organic material
is going to tell you
is going to tell you
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about environment, about complexity
and about diversity.
and about diversity.
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DNA, or any information carrier,
is going to tell you about adaptation,
is going to tell you about adaptation,
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about evolution, about survival,
about planetary changes
about planetary changes
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and about the transfer of information.
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All together, they are telling us
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what started as a microbial pathway,
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and why what started
as a microbial pathway
as a microbial pathway
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sometimes ends up as a civilization
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or sometimes ends up as a dead end.
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Look at the solar system,
and look at the Earth.
and look at the Earth.
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On Earth, there are many
intelligent species,
intelligent species,
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but only one has achieved technology.
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Right here in the journey
of our own solar system,
of our own solar system,
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there is a very, very powerful message
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that says here's how we should look
for alien life, small and big.
for alien life, small and big.
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So yeah, microbes are talking
and we are listening,
and we are listening,
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and they are taking us,
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one planet at a time
and one moon at a time,
and one moon at a time,
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towards their big brothers out there.
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And they are telling us about diversity,
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they are telling us about
abundance of life,
abundance of life,
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and they are telling us
how this life has survived thus far
how this life has survived thus far
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to reach civilization,
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intelligence, technology
and, indeed, philosophy.
and, indeed, philosophy.
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Thank you.
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(Applause)
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ABOUT THE SPEAKER
Nathalie Cabrol - Planetary explorerTo determine how life might persist on Mars, Nathalie Cabrol explores one of Earth’s most extreme environments: high-elevation Andean lakes and deserts.
Why you should listen
While hunting for life in the fragile biomes of the Andes, Nathalie Cabrol has braved earthquakes, set a diving record and gathered data on the threats faced by mountain ecosystems in the face of climate change.
But Cabrol’s eyes are always fixed on Mars, which may have once had a climate similar to Earth’s mountain deserts. As a science team member for NASA, Cabrol helps design interplanetary experiments for the Martian Spirit rover, and researches new technologies for future missions to Mars and beyond.
Nathalie Cabrol | Speaker | TED.com