[meteorite-list] Curiosity Rover Finds Evidence of Mars Crust Contributing to Atmosphere

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Fri, 30 Sep 2016 14:53:28 -0700 (PDT)
Message-ID: <201609302153.u8ULrSFQ002897_at_zagami.jpl.nasa.gov>

http://www.jpl.nasa.gov/news/news.php?feature=6631

Curiosity Finds Evidence of Mars Crust Contributing to Atmosphere
Jet Propulsion Laboratory
September 29, 2016

NASA's Curiosity rover has found evidence that chemistry in the surface
material on Mars contributed dynamically to the makeup of its atmosphere
over time. It's another clue that the history of the Red Planet's atmosphere
is more complex and interesting than a simple legacy of loss.

The findings come from the rover's Sample Analysis at Mars, or SAM, instrument
suite, which studied the gases xenon and krypton in Mars' atmosphere.
The two gases can be used as tracers to help scientists investigate the
evolution and erosion of the Martian atmosphere. A lot of information
about xenon and krypton in Mars' atmosphere came from analyses of Martian
meteorites and measurements made by the Viking mission.

"What we found is that earlier studies of xenon and krypton only told
part of the story," said Pamela Conrad, lead author of the report and
SAM's deputy principal investigator at NASA's Goddard Space Flight Center
in Greenbelt, Maryland. "SAM is now giving us the first complete in situ
benchmark against which to compare meteorite measurements."

Of particular interest to scientists are the ratios of certain isotopes
- or chemical variants - of xenon and krypton. The SAM team ran a series
of first-of-a-kind experiments to measure all the isotopes of xenon and
krypton in the Martian atmosphere. The experiments are described in a
paper published in Earth and Planetary Science Letters.

The team's method is called static mass spectrometry, and it's good for
detecting gases or isotopes that are present only in trace amounts. Although
static mass spectrometry isn't a new technique, its use on the surface
of another planet is something only SAM has done.

Overall, the analysis agreed with earlier studies, but some isotope ratios
were a bit different than expected. When working on an explanation for
those subtle but important differences, the researchers realized that
neutrons might have gotten transferred from one chemical element to another
within the surface material on Mars. The process is called neutron capture,
and it would explain why a few selected isotopes were more abundant than
previously thought possible.

In particular, it looks as if some of the barium surrendered neutrons
that got picked up by xenon to produce higher-than-expected levels of
the isotopes xenon-124 and 126. Likewise, bromine might have surrendered
some of its neutrons to produce unusual levels of krypton-80 and krypton-82.

These isotopes could have been released into the atmosphere by impacts
on the surface and by gas escaping from the regolith, which is the soil
and broken rocks of the surface.

"SAM's measurements provide evidence of a really interesting process in
which the rock and unconsolidated material at the planet's surface have
contributed to the xenon and krypton isotopic composition of the atmosphere
in a dynamic way," said Conrad.

The atmospheres of Earth and Mars exhibit very different patterns of xenon
and krypton isotopes, particularly for xenon-129. Mars has much more of
it in the atmosphere than does Earth.

"The unique capability to measure in situ the six and nine different isotopes
of krypton and xenon allows scientists to delve into the complex interactions
between the Martian atmosphere and crust," said Michael Meyer, lead scientist
for the Mars Exploration Program at NASA Headquarters in Washington. "Discovering
these interactions through time allows us to gain a greater understanding
of planetary evolution."

NASA's Mars Science Laboratory Project is using Curiosity to determine
if life was possible on Mars and study major changes in Martian environmental
conditions. NASA studies Mars to learn more about our own planet, and
in preparation for future human missions to Mars. NASA's Jet Propulsion
Laboratory, a division of the California Institute of Technology in Pasadena,
manages the project for NASA's Science Mission Directorate in Washington.

For more information about SAM, visit:

http://ssed.gsfc.nasa.gov/sam

SAM experiment data are archived in the Planetary Data System, online
at:

http://pds.nasa.gov

For more information about Curiosity, visit:

http://www.nasa.gov/msl

The research paper is available at:

http://dx.doi.org/10.1016/j.epsl.2016.08.028

News Media Contact
Written by Elizabeth Zubritsky

Guy Webster Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6278
guy.webster at jpl.nasa.gov

Dwayne Brown / Laurie Cantillo
NASA Headquarters, Washington
202-358-1726 / 202-358-1077
dwayne.c.brown at nasa.gov / laura.l.cantillo at nasa.gov

2016-249
Received on Fri 30 Sep 2016 05:53:28 PM PDT