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Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.     

Tabatha Thompson 202-358-3895
NASA Headquarters, Washington

Lori Stiles 520-626-4402                        
University of Arizona, Tucson

News Release: 2007-017                                          Feb. 15, 2007

NASA Mars Orbiter Sees Effects of Ancient Underground Fluids 

SAN FRANCISCO - Liquid or gas flowed through cracks penetrating underground 
rock 
on ancient Mars, according to a report based on some of the first observations 
by NASA's 
Mars Reconnaissance Orbiter. These fluids may have produced conditions to 
support 
possible habitats for microbial life. 

These ancient patterns were revealed when the most powerful telescopic camera 
ever sent 
to Mars began examining the planet last year. The camera showed features as 
small as 
approximately 3 feet (one meter) across. Mineralization took place deep 
underground, 
along faults and fractures. These mineral deposits became visible after 
overlying layers 
were eroded away throughout millions of years. 

Dr. Chris Okubo, a geologist at the University of Arizona, Tucson, discovered 
the 
patterns in an image of exposed layers in a Martian canyon named Candor Chasma. 
The 
image was taken in September 2006 by the High Resolution Imaging Science 
Experiment 
camera aboard the orbiter.

"What caught my eye was the bleaching or lack of dark material along the 
fracture. That 
is a sign of mineral alteration by fluids that moved through those joints," 
said Okubo. "It 
reminded me of something I had seen during field studies in Utah, that is 
light-tone 
zones, or 'haloes,' on either side of cracks through darker sandstone."

Dr. Alfred McEwen, the camera's principal investigator from the University of 
Arizona, 
Tucson, said, "This result shows how orbital observations can identify features 
of 
particular interest for future exploration on the surface or in the subsurface 
or by sample 
return. The alteration along fractures, concentrated by the underground fluids, 
marks 
locations where we can expect to find key information about chemical and 
perhaps 
biologic processes in a subsurface environment that may have been habitable." 

The haloes visible along fractures seen in the Candor Chasma image appear to be 
slightly 
raised relative to surrounding, darker rock. This is evidence that the 
circulating fluids 
hardened the lining of the fractures, as well as bleaching it. The harder 
material would 
not erode away as quickly as softer material farther from the fractures.

The most likely origin for these features is that minerals that were dissolved 
in water 
came out of solution and became part of the rock material lining the fractures. 
 Another 
possibility is that the circulating fluid was a gas, which may or may not have 
included 
water vapor in its composition, Okubo said.

Similar haloes adjacent to fractures show up in images that the high-resolution 
camera 
took of other places on Mars after the initial Candor Chasma image. "We are 
excited to 
be seeing geological features too small to have been noticed previously," Okubo 
said.  

"This publication is just the first of many, many to come. The analysis is 
based on test 
observations taken even before the start of our main science phase. Since then, 
Mars 
Reconnaissance Orbiter has returned several terabits of science data, 
sustaining a pace 
greater than any other deep space mission. This flood of data will require 
years of study 
to exploit their full value, forever increasing our understanding of Mars and 
its history of 
climate change," said  Dr. Richard Zurek, project scientist for Mars 
Reconnaissance 
Orbiter at NASA's Jet Propulsion Laboratory, Pasadena, Calif.

Okubo and McEwen report the findings in the Feb. 16 edition of the journal 
Science.  
Images showing the haloes along fractures are available at 
http://www.nasa.gov/mission_pages/MRO/news/20070215.html .

JPL, a division of the California Institute of Technology, manages the mission 
for 
NASA's Science Mission Directorate, Washington.  Lockheed Martin Space Systems, 
Denver, is the prime contractor for the project and built the spacecraft.  The 
University of 
Arizona operates the High Resolution Imaging Science Experiment camera. Ball 
Aerospace and Technology Corp., Boulder, Colo., built the camera.

-end- 



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