[meteorite-list] NASA Trapped Mars Rover Finds Evidence of Subsurface Water

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu, 28 Oct 2010 10:11:41 -0700 (PDT)
Message-ID: <201010281711.o9SHBfaJ028991_at_zagami.jpl.nasa.gov>

Oct. 28, 2010

Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.brown at nasa.gov

Guy Webster
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-6278
guy.webster at jpl.nasa.gov
RELEASE: 10-278

NASA TRAPPED MARS ROVER FINDS EVIDENCE OF SUBSURFACE WATER

PASADENA, Calif. -- The ground where NASA's Mars Exploration Rover
Spirit became stuck last year holds evidence that water, perhaps as
snow melt, trickled into the subsurface fairly recently and on a
continuing basis.

Stratified soil layers with different compositions close to the
surface led the rover science team to propose that thin films of
water may have entered the ground from frost or snow. The seepage
could have happened during cyclical climate changes during periods
when Mars tilted farther on its axis. The water may have moved down
into the sand, carrying soluble minerals deeper than less-soluble
ones. Spin-axis tilt varies over timescales of hundreds of thousands
of years.

The relatively insoluble minerals near the surface include what is
thought to be hematite, silica and gypsum. Ferric sulfates, which are
more soluble, appear to have been dissolved and carried down by
water. None of these minerals is exposed at the surface, which is
covered by wind-blown sand and dust.

"The lack of exposures at the surface indicates the preferential
dissolution of ferric sulfates must be a relatively recent and
ongoing process since wind has been systematically stripping soil and
altering landscapes in the region Spirit has been examining," said
Ray Arvidson of Washington University in St. Louis, deputy principal
investigator for the twin rovers Spirit and Opportunity.

Analysis of these findings appears in a report in the Journal of
Geophysical Research published by Arvidson and 36 co-authors about
Spirit's operations from late 2007 until just before the rover
stopped communicating in March.

The twin Mars rovers finished their three-month prime missions in
April 2004, then kept exploring in bonus missions. One of Spirit's
six wheels quit working in 2006.

In April 2009, Spirit's left wheels broke through a crust at a site
called "Troy" and churned into soft sand. A second wheel stopped
working seven months later. Spirit could not obtain a position
slanting its solar panels toward the sun for the winter, as it had
for previous winters. Engineers anticipated it would enter a
low-power, silent hibernation mode, and the rover stopped
communicating March 22. Spring begins next month at Spirit's site,
and NASA is using the Deep Space Network and the Mars Odyssey orbiter
to listen if the rover reawakens.

Researchers took advantage of Spirit's months at Troy last year to
examine in great detail soil layers the wheels had exposed, and also
neighboring surfaces. Spirit made 13 inches of progress in its last
10 backward drives before energy levels fell too low for further
driving in February. Those drives exposed a new area of soil for
possible examination if Spirit does awaken and its robotic arm is
still usable.

"With insufficient solar energy during the winter, Spirit goes into a
deep-sleep hibernation mode where all rover systems are turned off,
including the radio and survival heaters," said John Callas, project
manager for Spirit and Opportunity at NASA's Jet Propulsion
Laboratory, in Pasadena, Calif. "All available solar array energy
goes into charging the batteries and keeping the mission clock
running."

The rover is expected to have experienced temperatures colder than it
has ever before, and it may not survive. If Spirit does get back to
work, the top priority is a multi-month study that can be done
without driving the rover. The study would measure the rotation of
Mars through the Doppler signature of the stationary rover's radio
signal with enough precision to gain new information about the
planet's core. The rover Opportunity has been making steady progress
toward a large crater, Endeavour, which is now approximately 5 miles
away.

Spirit, Opportunity, and other NASA Mars missions have found evidence
of wet Martian environments billions of years ago that were possibly
favorable for life. The Phoenix Mars Lander in 2008 and observations
by orbiters since 2002 have identified buried layers of water ice at
high and middle latitudes and frozen water in polar ice caps. These
newest Spirit findings contribute to an accumulating set of clues
that Mars may still have small amounts of liquid water at some
periods during ongoing climate cycles.

NASA's Jet Propulsion Laboratory manages the rovers for the agency's
Science Mission Directorate in Washington.

For more about the rovers, see:

http://www.nasa.gov/rovers
        
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Received on Thu 28 Oct 2010 01:11:41 PM PDT