NARRATOR: Is there life beyond Earth?
To find out, we might look no farther
than the planet next door.
Mars may be our best hope for resolving the ultimate mystery
of creation.
MAN: It is the one planet
out there that is Earth-like enough
that we can imagine that life might have taken hold
on that world.
MAN: If we go to Mars, will we find that, yes,
the same events that led to life on Earth
happened independently on this other planet?
MAN: And if we find evidence on our very next planet, Mars,
then you have to say
that has to be so common across the Milky Way,
across the universe, you know that we are not alone.
NARRATOR: Mars has more in common with our world
than any place we know of in the universe.
But it's still a world away.
Getting an astronaut there to search for life is beyond us.
So for now we must resort to the next best thing...
(electronic whirring)
Robots.
Mars today is a busy place.
Three satellites orbit it.
Three landers ponder its surface.
They're finding a wealth of clues.
MAN: Holy smokes! I'm just blown away by this.
MAN: When that first data comes down,
the sense of astonishment is indescribable.
Oh, wow!
MAN: We would never have thought
of looking for organisms like this on Mars.
NARRATOR: But they're also discovering that, in its past,
Mars had some dark secrets.
Life can survive in pretty harsh conditions,
but there are limits.
MAN: Around four billion years ago,
there was a cataclysmic event.
MAN: And this was big.
This thing went wham-- right into the planet.
NARRATOR: Four and a half billion years ago, two young planets emerged,
both brimming with promise.
But something went very wrong with Earth's twin.
Is there life on Mars?
Up next on NOVA.
MajoNARRATOR: for NOVA Mars eludes us.
Even as this planet surrenders its secrets,
it remains stubbornly guarded about one...
The question we have come in pursuit of, above all others.
STEVE SQUYRES: The geology is fascinating,
the climate is interesting, atmospheric science.
There is any number of things that you can study
about the planet, but to me what makes Mars special
is its potential as an abode for life.
NARRATOR: If there's life on Mars,
there could be life throughout the universe.
CHRIS McKAY: If it happened twice,
right here in our own solar system, then we would have,
for the first time, a good answer to the question,
Is the universe full of life?
The answer would be yes.
PETER SMITH: The Holy Grail of Mars exploration
is finding some form of Martian biology,
what's often called the Second Genesis.
Did life start on Earth and Mars?
Did it evolve in a totally different way
than Earth-life did?
NARRATOR: Peter Smith has been involved with seven missions to Mars.
Each has only driven home how difficult it is to get there.
MAN: This is the Mars Polar Lander Mission Control
at the Jet Propulsion Center.
NARRATOR: 1999.
The Mars Polar Lander is about to touch down on the surface.
Smith and his team should get word any moment.
They wait...
There's nothing worse than no signal.
NARRATOR: ...and wait, for a signal that never comes.
SMITH: I was trying
to hold out a little hope that maybe it landed
and the communication link hadn't quite set up yet,
but I had the worst sinking feeling.
MAN: The mood doesn't look too good over there.
NARRATOR: During its descent, the Polar Lander disappeared.
SMITH: You felt like
somebody very close to you in your life,
someone you love very dearly, had died
through some tragic accident.
NARRATOR: At the time, Smith was already preparing his next mission,
another lander called Mars Surveyor.
But after the failure of Polar Lander,
NASA canceled the mission.
SMITH: Oh, it was just miserable.
All fell apart.
All my house of cards just collapsed.
NARRATOR: Smith didn't give up.
His plan: To take the technology from those failed missions
out of mothballs, and repurpose it for another lander.
Every precaution would be taken to make sure
this one would make it.
He christens the new mission with a name apropos: Phoenix.
SMITH: We are rising from the ashes,
and we're going back to Mars.
MISSION CONTROL: Zero and liftoff.
SMITH: And so, Phoenix it is.
Sending a mission to Mars
is somewhat like hitting a golf ball across the solar system.
We'll see if we got our hole in one.
NARRATOR: Nine months later.
Smith is back on track to search for signs of life on Mars.
MAN: Three, two, one, mark...
NARRATOR: Mission Control at NASA's Jet Propulsion Laboratory.
If Phoenix lands,
it'll be thanks to the engineers here today who made it happen.
But no one knows better than Smith what could go wrong.
Standing by for touchdown.
Touchdown signal detected.
(cheering)
NARRATOR: Finally, Peter Smith has arrived on Mars.
SMITH: By gosh, we are going and doing it.
We have a great chance of making a new discovery on Mars.
It's the thrill of my life.
NARRATOR: Now that Phoenix has landed,
NASA is sharing supervision of the mission with scientists
at the University of Arizona, where Smith is based.
Phoenix is in the far north of Mars,
so it has just three months before the polar sun will begin
to set for the long winter,
and with it will go the lander's power supply.
Time is already running out.
This is the 39th time we've tried to reach Mars
and only the seventh time we've actually landed there.
It is a quest years in the making.
The first to attempt it were the Soviets.
During the 1960s, they launched eight missions.
They failed eight times.
It wasn't until the late '70s
that we'd get our first close view of the Martian surface,
with the two Viking Landers.
Each bears a $60 million box,
packed with three biology experiments
that are, in their day, state of the art.
They're designed to test the soil
for the presence of organisms.
A member of the science team is Carl Sagan.
SAGAN: There may be warm, wet kinds of organisms in a dormant state.
It may be that by dropping them in liquid water,
Viking might have a very pleasant surprise
in detecting such organisms.
MAN: Now the screen for touchdown.
Touchdown! We have touchdown.
NARRATOR: Hopes are running high.
Many people are ready to exclude
the possibility of large organisms on Mars,
but I see no reason to do that.
And I think it's possible that, for example,
the Viking Lander camera may pick up
organisms that happen to be walking by the Viking Lander.
A silicon-based giraffe will be detectable
if it walks by the Viking Lander camera.
NARRATOR: But when the pictures come in,
there are no signs of giraffes.
As the experiments proceed, the news gets bleaker.
SMITH: That this was devoid of life,
that Mars was just a barren desert,
that it may have been interesting
four billion years ago,
but today it's lacking in those ingredients
that would allow life to flourish.
NARRATOR: Those ingredients for life are common on Earth.
Billions of years ago,
life as we know it needed three things to begin.
One is an energy source, like heat--
from the volcanic fury
of the Earth below and the sun's rays from above.
Two are organics-- carbon-based molecules;
not living things, but the building blocks of life.
But the third is scarce in our solar system:
the medium that helps the chemicals intermingle.
The most important requirement for life is liquid water,
and that's the defining requirement for life
in terms of our solar system.
There's plenty of energy, there's plenty of carbon,
there's plenty of other elements
on all the planets in our solar system.
What's rare is liquid water.
NARRATOR: Not only did Viking find no life, but no water, either.
Mars was pronounced a wasteland.
DAN McCLEESE: It was really a bummer.
Mars was "dead," unquote.
That was kind of the outcome in the newspapers.
And so we had a hiatus of missions to Mars of 20 years.
NARRATOR: Mars slipped away from the limelight.
Then, in 1996, NASA scientists unveil a Martian rock,
a meteorite that had landed in Antarctica,
which appears to hold the fossilized traces
of microscopic life.
Or so they think.
It turns out the formations they found could have been produced
by volcanic activity.
"Follow the microbe" has not gotten NASA far.
Instead, another strategy replaces it.
ANDY KNOLL: Certainly, life as we understand it requires water.
So NASA's explorational mantra has been "follow the water."
And that's a pretty reasonable first step.
NARRATOR: 2004-- NASA is putting wheels on the ground...
(cheering)
...times two.
The Mars rovers Spirit and Opportunity have landed
and are ready to roam the planet.
The hunt for signs of water-- present or past-- is on.
Opportunity is at a spot called Meridiani Planum...
Oh, look at this one.
Look at this!
NARRATOR: And right away,
the first pictures it sends home are stunning.
(team cheering)
Previous missions had sent photos of sheer desolation.
Look at that!
NARRATOR: But now, not far from the lander is bedrock,
the first ever seen on Mars.
STEVE SQUYRES: Holy smokes!
(laughter)
I'm sorry, I'm just... I'm just blown away by this.
NAAT Bedrock is a recod of ancient environments...
and a dream come true for mission leader Steve Squyres.
SQUYRES: This is the sweetest spot I've ever seen.
(laughter)
That outcrop in the distance is just out of this world.
I can't wait to get there.
(laughter)
SQUYRES: Most of the rock on Mars is volcanic lava flow.
This is something else.
This is an unusual Martian rock,
at least compared to what we've seen everywhere else.
The fact that these rocks are layered
says that one possible origin for these
is that they were laid down in liquid water.
We do not know what's going on here, but the beauty of it is
we have preserved in front of us a record that will answer that
and we have on our rover
a toolkit of gizmos that will tell us that answer.
NARRATOR: One gizmo is a camera on the end of the robotic arm.
It finds a puzzle never before seen on Mars:
tiny, smooth spheres, like so many blueberries.
Could they be the product of water?
The pellets probably formed in the cavities of wet soil,
perhaps in a salty ocean floor.
You should circle that one.
NARRATOR: If the team can find certain salts in the rock,
it will clinch the ancient presence of water.
The place to find those chemical clues
isn't on the surface.
They would have seeped underground...
if only the team could look there.
They can.
The rovers come equipped with a drill--
the Rock Abrasion Tool, or RAT--
as shown in this NASA animation.
But the man in charge of the RAT is worried.
STEVE GOREVAN: I thought that before landing
we had roughly been able
to approximate anything that Mars was going to throw at us.
Of course, what I neglected to think about was a rock
that would be spitting out blueberries.
What we're afraid of happening is that we're going to dislodge
one of the spherules
and that it's going to be like a pinball machine
between the RAT and the surface of the rock.
And this could be something that causes us some problems.
NARRATOR: The pressure is on to pick a rock to test.
GOREVAN: That spot for RATting has to be chosen now.
And I mean literally
in the next, uh, well, it should be chosen in the next...
it should be chosen in the next hour.
WOMAN: What is this rock?
GOREVAN: That's McKittrick.
NARRATOR: They've selected a spot that's blueberry-free.
Hopefully.
This, this, I can't stand this.
It's like... I wish it was over.
MAN: That's good, contact switch is tripped.
MAN: Are you ready to give a formal "Go"
for the RAT sequence, Master?
Yes, I think we are.
MISSION MANAGER: More definitive.
MAN: We're go to RAT.
Go to RAT. I like that. Okay.
You are clear to command.
GOREVAN: On my mark: 3, 2, 1, mark.
MAN: The RAT has been engaged.
GOREVAN: I don't care if we find chili under there.
(laughing): I don't care.
I just want to make that thing work.
NARRATOR: The result?
Yes! You see that hole?
NARRATOR: Direct from Mars, a cleanly RATted hole.
SQUYRES: It's the most important hole we've ever dug.
NARRATOR: Finally, they can check the rock's chemistry.
A spectrometer onboard is able to read each chemical
as a different wavelength,
breaking them down like a prism does light.
The rock is as much as 40% sulfate salt,
a mineral that's only produced by soil interacting with water.
That clinches it-- water was once here.
SQUYRES: That's beautiful, man.
It's so different from anything we've seen before.
That's great!
Whew!
SQUYRES: There's an awful lot of sulfate salt in this rock,
and that's very, very hard to explain away
other than water having been massively involved
in creating this stuff.
If you tasted this thing, you'd taste the salt.
It's a very, very salt-rich rock.
It looks like what geologists call an evaporite deposit.
Evaporites form when you have liquid water
with lots of stuff dissolved in it
and the water evaporates away and it leaves stuff behind.
NARRATOR: That stuff includes the blueberries.
They hardened long ago
when these rocks were saturated with water,
and they remained
after the softer, surrounding rock eroded away.
SQUYRES: So we think we're parked
on what was once the shore of a salty sea on Mars.
That's pretty cool.
NARRATOR: The rovers have proven,
even if they're finding no water on Mars now,
it once flowed here,
probably over three and a half billion years ago.
But that doesn't necessarily mean
there were living things here.
It would have taken more to generate life.
Amid its shallow seas, could Mars have produced
that energy it takes to stir up a primordial soup?
In search of clues, Spirit sets off on a journey
of 1.4 miles and two months
to explore the rugged Columbia Hills.
But the trek takes such a toll on the rover,
it might not make it to its destination.
SQUYRES: This is one beat-up vehicle.
This thing has traveled for three kilometers;
it's coated with dust.
We've got a gimpy wheel.
That front right wheel is hurting.
NARRATOR: Spirit is down to five wheels,
and there's no one to change a tire on Mars.
Its rovings may be over.
The team troubleshoots with their duplicate model at JPL.
WOMAN: If we're going backwards, and it's not a lead wheel...
It takes some, but it still has the pressure.
Any time you drive that wheel...
SQUYRES: We've got this dead weight
hanging off the front of the rover
in contact with the ground.
And so when we drive now,
we have to drive that vehicle differently.
We have to drive it backwards.
We always drive backwards,
dragging the dead wheel as we go.
And we drag the wheel, we go very slowly.
It's kind of painful to watch.
NARRATOR: But the setback turns up a surprise.
It, against all expectations,
led to the most important discovery Spirit has made.
As we drag that dead wheel through the soil,
it digs this wonderful hundreds-of-meters-long trench
in the dirt.
And we looked at the soil in the trench
and it was as white as bright snow.
NARRATOR: The white patches revealed by the gimpy wheel
is another telltale mineral--
silica, the stuff of sand and glass.
This soil is 90% silica.
It would have taken a lot of heat
to generate that concentration.
Perhaps hot springs like the ones on Earth
existed on Mars over three and a half billion years ago.
SQUYRES: This is a place where there was hot water
and maybe steam and it would come out of the ground.
And that provides, at least locally, an environmental niche
that would be suitable for life.
RRATOR: On our planet,
in these crucibles of hydrothermal activity,
the most ancient bacteria may have first emerged.
Liquid water...
energy.
When Mars and Earth were young,
they might have both had what it takes to create organisms.
Roughly three and a half billion years ago,
life may have had everything going for it on Mars.
McKAY: There's a real distinct parallel
between early Mars and early Earth.
There's a real parallel there that strengthens the case
for there being life on... having been life on Mars.
NARRATOR: But Andy Knoll is skeptical.
KNOLL: Let's think about the requirements of life.
Almost all of life on Earth
exists within a fairly narrow band
of environmental conditions.
NARRATOR: Not all water sustains life.
KNOLL: It's not enough just to say water was there.
The real question is the properties of water.
NARRATOR: The way the rovers found water was by detecting salt.
So how salty were those seas?
KNOLL: It turns out that Meridiani Planum
was way saltier than anything that's known to sustain life.
NARRATOR: If water is too salty or acidic, it can be deadly.
Three and a half billion years ago,
the waters of Meridiani, where Opportunity is, could have been
up to a thousand times saltier than Earth's oceans.
SQUYRES: It was pretty nasty stuff.
This was not nice pure water by any stretch of the imagination.
It was very acidic-- it was acid, sulfuric acid--
and it was very salty, it was a brine.
So, it would have been a very challenging place for life.
NARRATOR: What made the waters of Mars turn to poison?
A crucial clue is revealed
when Opportunity ventures to its next destination.
The walls of Victoria Crater offer the chance to study
the geological record.
The deeper, the older.
SQUYRES: Young rocks at the top, older rocks at the bottom.
You're doing a trip through time on Mars,
and the deeper you go, the further back you're going.
And we use those craters
to provide us with access to other rocks below the surface.
NARRATOR: The base of these cliffs could have formed
thousands of years before the rocks at the top.
Was Mars wet then?
Sure enough, Victoria's walls are lined with distinct bands.
Like the Grand Canyon, they are classic sedimentary layers,
the product of era after era of water.
Opportunity discovers that, moving forward in time,
the salt concentration steadily increases.
That means the amount of water bearing that salt was dwindling.
KNOLL: At Victoria,
we have evidence for some water early,
less water later, still less water since then.
It was evaporating and the result was
it got saltier and saltier and saltier and saltier.
NARRATOR: It appears Mars evaporated to death.
But why?
What could wring an entire planet dry?
Earth is able to stay wet and warm because its water is held
in the protection of a blanketing atmosphere.
The Martian atmosphere is today
less than one percent as dense as ours,
though it must have once been robust,
since water did flow here.
What happened to it?
Chances are the sun destroyed Mars' atmosphere
by relentlessly bombarding it with solar wind.
Earth's atmosphere is protected from the sun
by a powerful magnetic field.
That's generated by a spinning molten core, creating a dynamo.
McCLEESE: We're lucky on Earth; we wouldn't be here otherwise.
The magnetic field actually shields the atmosphere and us.
What it does is it manages to keep that solar wind
from blowing the atmosphere away.
NARRATOR: But then Mars is a tenth the mass of Earth.
It doesn't seem large enough
to generate a strong magnetic field.
In fact, does Mars even have a molten core to begin with?
Answers are emerging from a new age of Martian exploration.
Satellites dispatched by NASA and the European Space Agency
have been circling Mars.
The orbiters, for me,
are kind of the unsung heroes of Mars.
The global perspective is the thing that really gives you
the understanding of how the planet works.
NARRATOR: With data collected from the satellite Mars Odyssey,
scientists were able to model
the longest canyon in the solar system.
It stretches the length of the continental U.S.
and could fit the Los Angeles city basin
within the width of its walls.
With satellites, they are reconstructing
the volcanic history of Mars, the planet that produced
the solar system's largest volcano.
Olympus Mons spans an area the size of Arizona
and rises to three times the height of Everest.
Volcanoes are no longer active on Mars,
but their presence means
that at one time the planet did have a molten core.
Still, how could such a small planet pump up enough juice
to power a magnetic field?
Some scientists believe that Mars got a little help
from a visitor from space...
a giant asteroid.
Four billion years ago,
the solar system was a violent place.
KNOLL: There was an influx of meteors,
and in fact there are craters on Mars
into which you could fit Australia.
NARRATOR: The theory is, one object got caught in Mars' orbit.
SUE SMREKAR: There could have been a body
that was circling Mars and circling Mars.
And it's possible
that asteroids circling Mars created so much heat
and so much, um, deformation inside
that it actually started a dynamo.
NARRATOR: With sheer tidal force,
the asteroid may have churned the planet's molten core,
powering up its magnetic field and its atmosphere in turn.
At least for a time.
What, then, went wrong?
So on Mars we ask the question,
well, where is the magnetic field?
NARRATOR: Earth's magnetic field is one powerful cloak.
But that's not what the orbiters find on Mars.
McCLEESE: With the Mars Global Surveyor, we put a magnetometer--
a very, very sensitive experiment-- onboard.
We put it into close orbit.
And lo and behold, it found
the trace of an ancient magnetic field on the planet.
NARRATOR: Unlike Earth, Mars today has
countless small magnetic fields pock-marking its surface.
Like shrapnel left at a bomb site,
they seem like the aftermath of some violent event,
one that may have also left another clue at the scene:
Mars is misshapen.
SMREKAR: We could see that the Southern Highlands
were much more heavily cratered and much higher.
The north is much lower, much smoother.
NARRATOR: Mars has a clear division cutting straight through it.
The north is much less weathered than the south.
The reason?
The leading theory is Mars suffered a massive collision.
Perhaps that asteroid drew too close.
McCLEESE: I mean, this was big.
And the idea is that this thing went, wham!
Right into the planet.
Pushed the atmosphere away from the planet,
just literally blew the atmosphere away.
The object may have changed forever the south and the north,
making the two very, very different.
And it may have been the way, finally,
that the dynamo changed the way in which it was operating,
and so the magnetic field went away.
NARRATOR: In one staggering blow, Mars may have lost the driving force
behind its molten core and its magnetic field.
Stripped of its protective cloak,
the planet was forever left exposed
to a searing assault of solar wind,
preventing its atmosphere from reforming.
In the areas where the rovers have been traveling, it appears
that over three billion years ago Mars was transformed--
from a warm, wet place, possibly brimming with early life,
to an arid, acidic corpse.
But is it certain that any and all life on the planet
was wiped out?
There's part of me, I must admit, that would root
for the idea of Martian life.
Is it impossible that life exists on Mars?
No, but I think it's not the odds-on bet.
I would take up Andy on his bet.
I think the chance of finding life on Mars is high,
or I wouldn't be spending my time and energy
searching for it.
NARRATOR: Chris McKay holds out hope that some organisms may have held on,
adapting to a harsher world.
Now, to find out if there could be life on Mars,
he's headed for the ends of the Earth.
McKAY: We're on our way up into the far north of the Arctic.
The polar regions are
a prime target for searching for evidence of life.
NARRATOR: It's summer at Axel Heiberg.
But, come winter, this island can get down to 40 below.
McKay has come to study a remarkable feature.
Here flow two springs that are up to ten times saltier
than seawater.
Salt at this concentration is usually poisonous.
Could microbes survive these waters?
McKay has reason to think so.
On Earth, searching for life is easy.
No matter where you look, just about,
you find evidence of life.
NARRATOR: To what lengths will life go?
It faces challenges world over.
In the driest, hottest desert, microbes thrive.
In the ocean's sunless depths as well.
Even in the bowels of the Earth,
in caves seething with toxic fumes and scalding acid.
At almost every limit, life prevails.
Salty as the springs of Axel Heiberg are, they harbor
miniature ecosystems.
McKAY: We find a dark, rich soil right above the ice
full of all sorts of bacteria.
It looks kind of like the soil you find
in a forest floor-- it's that rich.
NARRATOR: So if life is this resilient on Earth, how about on Mars?
Could it have survived
on a planet stripped of its atmosphere?
Somehow, somewhere could it have adapted to harsher conditions
and found refuge?
Maybe we've just been looking in all the wrong places.
The sites the rovers explored
were both along the Martian equator.
But there's more to a planet than just two spots.
SMREKAR: Imagine if you just went to Death Valley
or you just landed on the arctic tundra, you know.
You would get incredibly different view of the Earth.
Sure, where the rovers landed could have been an acid wash.
Very salty.
Not very friendly to life.
But I bet if we landed in another place,
we might find something different.
NARRATOR: It would have to be a place that somehow retained
those same life-friendly ingredients:
liquid water, not too salty or acidic;
an energy source;
and nurturing organic molecules.
"Following the water" calls for at least one more stop,
and this time, NASA is aiming for a spot on Mars
where water may still exist.
We've long known the Martian ice caps in the north and south
are made of carbon dioxide-- dry ice.
But some held out hopes water lies beneath it.
In 2002, the satellite Odyssey was able to peer
below the surface to tell which elements are present.
Odyssey actually discovered hydrogen
in the upper three feet of soil.
NARRATOR: A vast reservoir of hydrogen, marked blue here.
Could that "H" be a sign of H2O?
If there's still water on Mars, this is where to look for it.
It's time for the Phoenix Lander to take up the hunt,
under the leadership of Peter Smith.
SMITH: The polar north on Mars
potentially was once liquid water.
We don't know that for a fact; we're going there to find out.
NARRATOR: Tucson, Arizona, is now Mars Central.
This is the latest image.
This is where it came down.
NARRATOR: Unlike the rovers,
this robot is not just looking for signs of a watery past.
It's taking the search for life one step closer.
Its goal?
To look for water and to assess habitability.
That is, in the past,
was the planet able to support life, and did it?
NARRATOR: Phoenix will focus on one area and dig.
It's not designed to detect life itself, but it can tell
if conditions here were once right for it.
RESEARCHER: Outstanding!
(excited murmuring)
NARRATOR: The first "sol," or Martian day, and already it looks
like the team has landed in the right place.
SMITH: This is the most ice-rich area outside of the polar cap.
NARRATOR: The lander uses a camera on its arm to peer under itself.
It discovered that the descent thrusters had, by chance,
cleared a patch of soil away, revealing what might be ice.
SMITH: This is an interesting place we've landed.
If you came out here with a broom,
you could sweep off that...
it's only two inches of soil over ice.
You could actually sweep off all that soil off into a corner
and you would have almost a skating rink
with some interesting bumps on it.
MAN: Hey, Matt, did you see
the color picture of what UA dug up?
No-- no, I haven't.
Unidentified white stuff in there.
Oh, wow!
NARRATOR: But whether it's carbon dioxide ice or water ice
or something else is the question.
That white stuff, wow!
This material we think is ice.
SMITH: We found some very bluish ice-like material
that has the science team arguing incessantly
about whether it's ice or salt or some other exotic material.
That's not permafrost. That is ice.
NARRATOR: That bluish, ice-like material turns up as nuggets
in a ditch Phoenix dug.
The team intentionally leaves the area undisturbed
and watches.
These two...
MARK LEMMON: We were trying to put the pictures up on the screens
as fast as we could, compare them to the pictures
that we'd taken a few days before.
And it just took seconds of looking at the picture
to say, "Yes, stuff has changed."
NARRATOR: Lo and behold, the clumps disappear.
Oh, is that pretty.
NARRATOR: The reason?
They vaporized.
That wouldn't happen to carbon dioxide ice--
not at 26 below zero.
Only water is going to actually sublimate away
at those temperatures.
We watched it just poof, go away,
over the course of a couple days.
NARRATOR: For the first time, we have touched water on another planet.
And yet, how does that help the chances for life on Mars?
Microbes need liquid water.
Is the Martian north hiding that somewhere?
McKAY: Phoenix is the first Mars mission ever
to actually come in contact with real H2O.
It's ice, but there it is.
Water, frozen solid.
And the question then is, was it ever liquid?
NARRATOR: Phoenix can find out.
The robotic lab has an instrument onboard
that can detect if the soil here has come in contact
with liquid water.
It's called TEGA, and it can distinguish different chemicals
by heating them in a small oven.
Each boils off at a different temperature.
Let's do another tool-frame rotation of negative point one.
Minus point one tool frame.
NARRATOR: Working with an exact model of Phoenix,
the team's been running simulations in Arizona
with dirt that's dry and granular--
characteristics they expect Mars dirt to have.
All they need now is to get Phoenix
a scoop of the real thing so TEGA can run its test.
RESEARCHER: The right stuff slid.
It's the stuff on the screen.
NARRATOR: Sample after sample is delivered.
But to the TEGA oven below.
There's the full ten-minute shake right there.
Okay, so the bottom line is we didn't get any dirt.
NARRATOR: Martian soil is surprisingly sticky.
SMITH: Well, the TEGA instrument has not been
a stellar performer, unfortunately.
It's had a lot of little problems.
Now, are these just growth pains
or learning difficulties,
or is it really an instrument on the way out?
This has been a very emotional ride.
NARRATOR: The best minds in space science are devoted to one thing:
getting dirt past a screen.
So far, the dirt is winning.
Finally...
The TEGA oven is full!
No! Really?
Yay!
It's been a long time coming,
but boy it's sweet when it's here, right?
WOMAN: Okay, can we be happy now?
We can be happy now.
NARRATOR: Soon there's more reason to be happy:
TEGA's ovens turn up carbonates--
chalk-like minerals that form in the presence
of liquid H2O.
Water-- liquid water-- was at this spot on Mars.
But how could that be?
Temperatures recorded in the Martian polar north
have never gotten warmer than 13 below zero.
How could the ice here have ever melted?
Another satellite, the Mars Reconnaissance Orbiter,
found a clue.
Probing the polar cap by bouncing radio waves down,
like sonar, it discovered distinct layers of dust and ice,
laid down through a succession of climates, colder and warmer.
McCLEESE: How do you get layers on planets?
Well, you get cycles of hot and cold
over the surface of the planet.
NARRATOR: And what makes the temperature change so much?
That happens over phases that last millions of years,
as the globe tilts more or less toward the sun.
A planet spins like a top.
The Earth has a large moon that helps to stabilize it,
so it rotates relatively steadily.
But the two moons Mars has are both small,
so it's more prone to wobbling.
Over the course of millions of years, it can tilt a lot.
Five million years ago,
the Martian north pole was angled at 45 degrees.
McKAY: So the amount of sunlight that it receives in a day
would be twice what it's receiving now.
So imagine five million years ago
it could have been as warm as the polar regions on Earth.
NARRATOR: This part of Mars may have been warmer
as recently as five million years ago--
long after the planet's atmosphere got ruined--
warm enough to be wet.
Did that make the north life-friendly?
Not if conditions here were extremely acidic or salty,
like where the rovers landed.
To find out how life-friendly this area was,
Phoenix will use a second lab, called MECA.
It will test its sample's properties not by heating it up,
but by adding water it's brought along.
MICHAEL HECHT: It stirs it up to determine what comes out of the soil,
what kind of tea does this Martian soil make.
(all chatting)
NARRATOR: Step one is getting a sample into a cell.
After TEGA's troubles, no one is taking that for granted.
I don't see anything changing down here at all.
NARRATOR: Looking at the visuals from Mars,
it's hard to tell if the soil actually got delivered.
The team can only hold out hopes their experiment is underway.
SUZANNE YOUNG: Just waiting, that part was agony.
Every second was an hour.
It was definitely the longest hour of my life.
NARRATOR: Then...
All right, here we go.
There it is.
More is coming.
HECHT: When that first data comes down from Mars and you suddenly see
these wiggles on the screen
just like you've seen in the laboratory,
the sense of astonishment is indescribable, just seeing it.
We know for the first time the pH of Mars.
NARRATOR: The pH-- the level of how acidic the soil is.
I want a number from zero to twelve.
HECHT: Something that people have been speculating about
for years and years and years.
Give us a number from zero to twelve.
NARRATOR: There's a surprise...
It's basic.
It's basic?
NARRATOR: It's not acidic-- a reading of 8.3,
the kind of soil asparagus could grow in.
So far, so good for life.
Next, what's that salt content in the sample?
HECHT: Beautiful!
(laughs)
Oh, that is gorgeous.
NARRATOR: It's unexpectedly low.
Another plus for life.
McKAY: At the Phoenix site
we find relatively pure ice.
We find neutral conditions.
We find salts, but at low levels.
SAMUEL KOUNAVES: For a lot of us it's a new view of Mars.
It obviously is not super salty,
it's obviously not super acidic or super basic.
Bacteria might enjoy this stuff.
So some organisms might be able to survive
if the other part of the environment was good.
NARRATOR: But that's a big if.
Just when all readings are pointing
to a life-friendly environment, one comes up that's baffling.
HECHT: After the initial analysis,
that's where things started getting truly interesting.
Michaelina, take a look at this.
NARRATOR: There's an unexpected chemical called perchlorate.
HECHT: It was about the farthest thing from our imagination
that we might find there.
NARRATOR: On our planet, perchlorate is a toxic chemical
manufactured for rocket fuel and fireworks.
It's rare in the natural world,
except in the most forbidding deserts on Earth.
HECHT: This stuff, liquid perchlorate,
is not a material that microbes can very easily live in.
It's not a very friendly environment.
KOUNAVES: Life can survive
in pretty harsh conditions, but there are limits.
NARRATOR: What are the chances of life amid perchlorate?
It's a new question for Mars scientists.
Not for John Coates.
COATES: People have said that the presence of perchlorate on Mars
is indicative that life couldn't be present,
that this compound is too toxic.
But that statement is not true.
NARRATOR: At a lab in Berkeley, California,
Coates and his team have been quietly studying
a group of microbes that is about to attract some attention.
These are his subjects--
organisms that thrive on perchlorate,
consuming it as we do the air we breathe...
a trait that could come in handy
on oxygen-deprived Mars.
The Martians we've long sought may be like these bacteria,
called dechloromonas.
COATES: We would never have thought of looking for organisms like this
on Mars.
Now that we know that this compound is present on Mars,
it certainly opens up that as a life-form
that could potentially have existed on Mars.
NARRATOR: Could dechloromonas or its alien counterpart
have ever stood a chance on Mars?
Phoenix will never know.
Its experiments done, the team disperses.
As the Martian polar night descends,
the lander's solar power dwindles.
Phoenix will soon be entombed in dry ice, never to awaken.
The search for signs of Martian life
will fall to the next mission.
The Mars Science Lab-- MSL--
will be the size of a small car.
It will be bristling with technology...
an array of imagers, sampling tools and labs
that will make its predecessors seem quaint.
McKAY: I'm very excited about MSL.
In an interesting way,
it's a complement to the Phoenix mission.
To me, we've already followed the water.
We know there's water on Mars.
Check on the water.
The next thing we need to do
in terms of a strategy for life search is follow the organics.
Find organics.
NARRATOR: We have come a long way in meeting our neighbor next door.
We've gone from envisioning it as barren and moon-like
to a place as diverse as it is familiar.
A world that could well have harbored life.
We can now imagine the day, billions of years past,
when two planets took their turn round the sun,
neck and neck in the race to claim life's course.
We know what happened on Earth.
But the other was dealt a blow.
If there's proof on Mars of a life-filled past,
it is still waiting to be discovered.
On NOVA's "Is There Life on Mars?" Web site,
check out our Q&A with a NASA astrophysicist,
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