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Date: Tue, 29 Nov 2005 16:57:30 -0800
From: NASA Jet Propulsion Laboratory <[EMAIL PROTECTED]>
To: "[EMAIL PROTECTED]" <[EMAIL PROTECTED]>
Subject: NASA Rover Helps Reveal Possible Secrets of Martian Life

MEDIA RELATIONS OFFICE
JET PROPULSION LABORATORY
CALIFORNIA INSTITUTE OF TECHNOLOGY
NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
PASADENA, CALIF. 91109 TELEPHONE (818) 354-5011
http://www.jpl.nasa.gov

Guy Webster (818) 354-6278/5011
Jet Propulsion Laboratory, Pasadena, Calif.

George Deutsch/Erica Hupp (202) 358-1324/1237
NASA Headquarters, Washington

News Release: 2005-167                                                  
November 29, 2005

NASA Rover Helps Reveal Possible Secrets of Martian Life

Life may have had a tough time getting started in the ancient environment that 
left its mark in the
Martian rock layers examined by NASA's Opportunity rover. The most thorough 
analysis yet of the
rover's discoveries reveals the challenges life may have faced in the harsh 
Martian environment.

"This is the most significant set of papers our team has published," said Dr. 
Steve Squyres of Cornell
University, Ithaca, N.Y. He is principal investigator for the science 
instruments on Opportunity and
its twin Mars Exploration Rover, Spirit. The lengthy reports reflect more 
thorough analysis of
Opportunity's findings than earlier papers.

Scientists have been able to deduce that conditions in the Meridiani Planum 
region of Mars were
strongly acidic, oxidizing, and sometimes wet. Those conditions probably posed 
stiff challenges to
the potential origin of Martian life.

Based on Opportunity's data, nine papers by 60 researchers in volume 240, issue 
1 of the journal
Earth and Planetary Science Letters discuss what this part of the Martian 
Meridiani Planum region
was like eons ago. The papers present comparisons to some harsh habitats on 
Earth and examine the
ramifications for possible life on Mars.

Dr. Andrew Knoll of Harvard University, Cambridge, Mass., a co-author of the paper, 
said, "Life that
had evolved in other places or earlier times on Mars, if any did, might adapt 
to Meridiani conditions,
but the kind of chemical reactions we think were important to giving rise to 
life on Earth simply
could not have happened at Meridiani."

Scientists analyzed data about stacked sedimentary rock layers 23 feet thick, 
exposed inside
"Endurance Crater." They identified three divisions within the stack. The 
lowest, oldest portion had
the signature of dry sand dunes; the middle portion had windblown sheets of 
sand.  Particles in those
two layers were produced in part by previous evaporation of liquid water. The 
upper portion, with
some layers deposited by flowing water, corresponded to layers Opportunity 
found earlier inside a
smaller crater near its landing site.

Materials in all three divisions were wet both before and after the layers were 
deposited by either
wind or water. Researchers described chemical evidence that the sand grains 
deposited in the layers
had been altered by water before the layers formed. Scientists analyzed how 
acidic water moving
through the layers after they were in place caused changes such as the 
formation of hematite-rich
spherules within the rocks.

Experimental and theoretical testing reinforces the interpretation of changes 
caused by acidic water
interacting with the rock layers. "We made simulated Mars rocks in our 
laboratory, then infused
acidic fluids through them," said researcher Nicholas Tosca from the State 
University of New York,
Stony Brook. "Our theoretical model shows the minerals predicted to form when 
those fluids
evaporate bear a remarkable similarity to the minerals identified in the Meridiani 
outcrop."

The stack of layers in Endurance Crater resulted from a changeable environment 
perhaps 3.5 to 4
billion years ago. The area may have looked like salt flats occasionally 
holding water, surrounded by
dunes. The White Sands region in New Mexico bears a similar physical 
resemblance. For the
chemistry and mineralogy of the environment, an acidic river basin named Rio 
Tinto, in Spain,
provides useful similarities, said Dr. David Fernandez-Remolar of Spain's 
Centro de Astrobiologia
and co-authors.

Many types of microbes live in the Rio Tinto environment, one of the reasons 
for concluding that
ancient Meridiani could have been habitable. However, the organisms at Rio 
Tinto are descended
from populations that live in less acidic and stressful habitats. If Meridiani 
had any life, it might have
had to originate in a different habitat.

"You need to be very careful when you are talking about the prospect for life on 
Mars," Knoll said.
"We've looked at only a very small parcel of Martian real estate. The 
geological record Opportunity
has examined comes from a relatively short period out of Mars' long history."

NASA's Jet Propulsion Laboratory, Pasadena, Calif., manages the Mars 
Exploration Rover project.
Images and information about the rovers and their discoveries are available at
http://www.nasa.gov/vision/universe/solarsystem/mer_main.html .

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