NASA Satellite Finds Interior of Mars Is Colder

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May 15, 2008

Dwayne Brown
Headquarters, Washington
202-358-1726
dwayne.c.brown@xxxxxxxx 

Whitney Clavin
Jet Propulsion Laboratory, Pasadena, Calif.
818-354-4673
whitney.clavin@xxxxxxxxxxxx 

RELEASE: 08-128

NASA SATELLITE FINDS INTERIOR OF MARS IS COLDER

WASHINGTON -- New observations from NASA's Mars Reconnaissance Orbiter 
indicate that the crust and upper mantle of Mars are stiffer and 
colder than previously thought.

The findings suggest any liquid water that might exist below the 
planet's surface and any possible organisms living in that water, 
would be located deeper than scientists had suspected.

"We found that the rocky surface of Mars is not bending under the load 
of the north polar ice cap," said Roger Phillips of the Southwest 
Research Institute in Boulder, Colo. Phillips is the lead author of a 
new report appearing in this week's online version of Science. "This 
implies that the planet's interior is more rigid, and thus colder, 
than we thought before." 

The discovery was made using the Shallow Radar (SHARAD) instrument on 
the Orbiter, which has provided the most detailed pictures to date of 
the interior layers of ice, sand and dust that make up the north 
polar cap on Mars. The radar images reveal long, continuous layers 
stretching up to 600 miles or about one-fifth the length of the 
United States. 

"In our first glimpses inside the polar ice using the radar on Mars 
Reconnaissance Orbiter, we can clearly see stacks of icy material 
that trace the history of Mars' climate," said Jeffrey Plaut from 
NASA's Jet Propulsion Laboratory in Pasadena, Calif. Plaut is a 
science team member and a co-author of the paper. "Radar has opened 
up a new avenue for studying Mars' past."

The radar pictures show a smooth, flat border between the ice cap and 
the rocky Martian crust. On Earth, the weight of a similar stack of 
ice would cause the planet's surface to sag. The fact that the 
Martian surface is not bending means that its strong outer shell, or 
lithosphere, a combination of its crust and upper mantle, must be 
very thick and cold.

"The lithosphere of a planet is the rigid part. On Earth, the 
lithosphere is the part that breaks during an earthquake," said 
Suzanne Smrekar, deputy project scientist for Mars Reconnaissance 
Orbiter at JPL. "The ability of the radar to see through the ice cap 
and determine that there is no bending of the lithosphere gives us a 
good idea of present day temperatures inside Mars for the first 
time." 

Temperatures in the outer portion of a rocky planet like Mars increase 
with depth toward the interior. The thicker the lithosphere, the more 
gradually the temperatures increase. The discovery of a thicker 
Martian lithosphere therefore implies that any liquid water lurking 
in aquifers below the surface would have to be deeper than previously 
calculated, where temperatures are warmer. Scientists speculate that 
any life on Mars associated with deep aquifers also would have to be 
buried deeper in the interior.

The radar pictures also reveal four zones of finely spaced layers of 
ice and dust separated by thick layers of nearly pure ice. Scientists 
think this pattern of thick ice-free layers represents cycles of 
climate change on Mars on a time scale of roughly one million years. 
Such climate changes are caused by variations in the tilt of the 
planet's rotational axis and in the eccentricity of its orbit around 
the sun. The observations support the idea that the north polar ice 
cap is geologically active and relatively young, at about 4 million 
years. 

On May 25, NASA's Phoenix Mars Lander is scheduled to touch down not 
far from the north polar ice cap. It will further investigate the 
history of water on Mars, and is expected to get the first up close 
look at ice on the Red Planet.

The SHARAD was provided by the Italian Space Agency, and its 
operations are led by the InfoCom Department, University of Rome "La 
Sapienza." Thales Alenia Space Italia, in Rome, is the Italian Space 
Agency's prime contractor for the radar instrument. Astro Aerospace, 
of Carpinteria, Calif., a business unit of Los Angeles-based Northrop 
Grumman Corp., developed the instrument's antenna as a subcontractor 
to Thales Alenia Space Italia. 

The Mars Reconnaissance Orbiter mission is managed by JPL for NASA's 
Science Mission Directorate in Washington. Lockheed Martin Space 
Systems in Denver was the prime contractor for the orbiter and 
supports its operations. 

For more detailed information about the Mars Reconnaissance Orbiter, 
visit:

http://www.nasa.gov/mro

	
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