SETI public: Fw: Healthy Rover Shows Its New Neighborhood on Mars

From: LARRY KLAES (ljk4_at_msn.com)
Date: Mon Jan 05 2004 - 04:50:19 PST

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    ----- Original Message -----
    From: NASA Jet Propulsion Laboratory
    Sent: Sunday, January 04, 2004 8:15 PM
    To: ljk4_at_msn.com
    Subject: Healthy Rover Shows Its New Neighborhood on Mars

    Donald Savage (202) 358-1547
    NASA Headquarters, Washington, D.C.

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

    NEWS RELEASE: 2004-004 January 4, 2004

    Healthy Rover Shows Its New Neighborhood On Mars

    NASA's Spirit Rover is starting to examine its new
    surroundings, revealing a vast flatland well suited to the
    robot's unprecedented mobility and scientific toolkit.

    "Spirit has told us that it is healthy," Jennifer Trosper of
    NASA's Jet Propulsion Laboratory, Pasadena, Calif., said
    today. Trosper is Spirit mission manager for operations on
    Mars' surface. The rover remains perched on its lander
    platform, and the next nine days or more will be spent
    preparing for egress, or rolling off, onto the martian
    surface.

    With only two degrees of tilt, with the deck toward the
    front an average of only about 37 centimeters (15 inches)
    off the ground, and with apparently no large rocks blocking
    the way, the lander is in good position for egress. "The
    egress path we're working toward is straight ahead," Trosper
    said.

    The rover's initial images excited scientists about the
    prospects of exploring the region after the roll-off.

    "My hat is off to the navigation team because they did a
    fantastic job of getting us right where we wanted to be,"
    said Dr. Steve Squyres of Cornell University, Ithaca, N.Y.,
    principal investigator for the science payload. By
    correlating images taken by Spirit with earlier images from
    spacecraft orbiting Mars, the mission team has determined
    that the rover appears to be in a region marked with
    numerous swaths where dust devils have removed brighter dust
    and left darker gravel behind.

    "This is our new neighborhood," Squyres said. "We hit the
    sweet spot. We wanted someplace where the wind had cleared
    off the rocks for us. We've landed in a place that's so
    thick with dust devil tracks that a lot of the dust has been
    blown away."

    The terrain looks different from any of the sites examined
    by NASA's three previous successful landers -- the two
    Vikings in 1976 and Mars Pathfinder in 1987.

    "What we're seeing is a section of surface that is
    remarkably devoid of big boulders, at least in our immediate
    vicinity, and that's good news because big boulders are
    something we would have trouble driving over," Squyres said.
    "We see a rock population that is different from anything
    we've seen elsewhere on Mars, and it comes out very much in
    our favor."
    Spirit arrived at Mars Jan. 3 (EST and PST; Jan. 4
    Universal Time) after a seven month journey. Its task
    is to spend the next three months exploring for clues
    in rocks and soil about whether the past environment at
    this part of Mars was ever watery and suitable to
    sustain life.

    Spirit's twin Mars Exploration Rover, Opportunity, will
    reach its landing site on the opposite side of Mars on Jan.
    25 (EST and Universal Time; Jan. 24 PST) to begin a similar
    examination of a site on the opposite side of the planet
    from Gusev Crater.
    JPL, a division of the California Institute of
    Technology, manages the Mars Exploration Rover project
    for NASA's Office of Space Science, Washington.
    Additional information about the project is available
    from JPL at:

                   http://jpl.convio.net/site/R?i=M4QDO0RFVIBO-3BCLCXxIg..
    http://jpl.convio.net/site/R?i=0FGl6EHuFPdO-3BCLCXxIg..
                                  
    and from Cornell University at:

                     http://jpl.convio.net/site/R?i=1eGcrfgm7tFO-3BCLCXxIg. http://jpl.convio.net/site/R?i=bYJQns_85-pO-3BCLCXxIg..

                                  
                                -end-


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