Drilling for Life on Mars
Much has been
said about the life that once may have existed on Mars (see
our review of Donald Goldsmith's The Hunt for Life on Mars in our Winter 1998
issue). But what
about life that exists on Mars now? This is an ongoing
part of NASA's explanation of Mars, and how it is being done
was explained by
Carol Stoker of the NASA Ames Research Center on 4 August
2004 at the American
Association of Physics Teachers meeting in Sacramento (CA).
In her talk on
"Drilling for Life on Mars," Stoker began by describing
how the present conditions on Mars dictate where to search
for life there.
Because the atmospheric pressure on Mars is close to that of
the triple point of
water, water passes from solid to vapor state there; the
liquid water
considered to be essential to a life-producing and
sustaining environment can exist on
Mars only below ground.
Moreover, Mars lacks atmospheric ozone to absorb
solar ultraviolet radiation which destroys organic compounds
that might form on
the surface of the planet.
In fact, Mars
Odyssey neutron spectrometry shows that an ice-rich layer
is known to lie 1-5 km below the ice-free layer on the
surface of Mars,
especially in high latitudes (above 60 degrees). Below that, said Stoker, the ice
should be melted by internal heating. Drilling a couple of kilometers on Mars
is an ambitious project.
But, Stoker noted, gullies may expose outcropping of
the underground aquifer layer 100 meters below ground level,
after they are
cleaned off by a "Dust Devil." Finding extant life, she added, is more
important and more likely than recognizing extinct life,
which may require multiple
missions or (more likely) human exploration.
Before trying
this out on Mars, NASA is testing their drilling strategy
at Rio Tinto in Spain in their MARTE (Mars Astrobiology Rio
Tinto Experiment).
Stoker said that the Rio Tinto area in the Iberian pyrite
belt was chosen
because of its red color.
There conventional drilling technology, sampling, and
analysis will look for living organisms whose metabolism is
based on the
reduction of iron (to ferrous ion) and oxidation of sulfur
(from sulfide to
sulfate). Such
anaerobic bacteria have been found in the Rio Tinto, which has a pH
of 2.3, but they had never been found underground.
Formation of
sulfate in acidic environment would produce sulfuric acid, a
eutectic solution of which has a freezing point of
-16oC. Such a depressed
freezing point would enhance its likelihood on Mars. The detection of
jarosite (a hydrous sulfate of iron and potassium) on Mars
further encourages Stoker
to believe that an ecosystem like that at Rio Tinto exists
there, because
jarosite doesn't form above a pH of 3.
Stoker continued
by pointing out problems in drilling for subsurface life
on Earth that will not
occur on Mars:
1) introduction of surface organisms into the subsurface.
2) alteration of chemical properties.
3) destruction of anaerobic life by exposure to aerobic
environment.
She said that the core samples are protected against
atmospheric oxygen by
plastic liners and are analyzed in an anaerobic glove
chamber. Cultures have
been grown from the rock both aerobically and anaerobically,
with identification
of possible bacteria in SEM (Scanning Electron Microscope)
photos. Microbes
have been identified both above and below the water table,
she reported, with
resources to sustain them in the same layer.
Those interested
in learning more about MARTE can avail themselves of
eight hour-long on-line lectures (in either English or
Spanish) -- at the
following website:
The lecture titles are "Mission to Mars, the MARTE Project and
an Introduction to Rio Tinto, Spain," "The Wonders
of a Mars Analog: Biology
at Rio Tinto," "Subsurface Life," "Spain's
Iberian Pyrite Belt," "Issues and
challenges for Robotic Drilling," "Drilling on
Mars," "Molecular Biology
techniques for discovering life on Mars," and
"Sample Handling while Searching for
Life." The
first 18 frames of PowerPoint for the first lecture match those for
Stoker's talk to AAPT.