http://www.asu.edu/asunews/research/Mars-Leshin_120602.html

NASA Selects ASU-Directed SCIM Proposal as One of Four Finalists
for Mars Scout Mission

James Hathaway, [EMAIL PROTECTED]
Arizona State university
480-965-6375
December 6, 2002

NASA has selected a proposal for a mission that would
collect samples of martian atmospheric dust as one of four
finalists for the first Mars Scout mission (see NASA press
release). The proposal, directed by Arizona State University
geologist and cosmochemist Laurie Leshin, will receive a
$500,000 grant to complete its development prior to the
agency's final selection process, which will begin next
summer. The Mars Scout Program plans to mount at least one
(and perhaps several) Scout missions to Mars beginning in
2007, with budgets of up to $300 million per mission.

Leshin's proposal is called "Sample Collection for 
Investigation of Mars" (SCIM), and involves a mission that
would do a hit-and-run with the dusty Martian atmosphere. 
The proposed mission would perform the first return of a 
Martian sample at less cost, lower risk and in a shorter 
time frame than the far more complicated missions that 
will eventually be launched to collect samples from the 
planet's surface. For full details on the mission
proposal, including images and animations, see 

http://scim.asu.edu .

In brief, the proposal calls for a spacecraft to make a 
"high pass" of Mars, going within 25 miles of the planet's
surface and to collect samples from the Martian atmosphere 
for about one minute at about 12,300 miles per hour, before 
swinging back and beginning the return to earth. On the 
spacecraft, a light-weight and porous high-tech substance 
known as "aerogel" would cushion, trap and preserve dust 
particles. The aerogel collection device is similar to the 
device on the Stardust mission to collect dust streaming 
off of a comet.

Leshin projects that the aerogel would capture about 1000 
fine dust particles measuring 10 microns (1/100 of a millimeter) 
or larger. "Martian dust is an interesting thing because there 
is dust all over the Martian surface," said Leshin. "It's the 
ubiquitous layer - it's everywhere, yet we really know very 
little about it. It samples virtually the whole planet, yet it is 
so fine-grained that it is very hard to study when you're sitting 
there on the surface. You really need to bring it back to Earth to 
characterize it grain by grain. And each grain is like a little
rock from Mars."

Dr. Leshin is currently at the American Geophysical Union meeting 
in San Francisco, but can be reached by cellular phone at 
602-430-0067, or in her hotel at 415-771-1400, room 4282.

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