SETI public: Fw: Spirit Lowers Front Wheels, Looks Around in Infrared

From: LARRY KLAES (ljk4_at_msn.com)
Date: Fri Jan 09 2004 - 17:53:33 PST

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    ----- Original Message -----
    From: NASA Jet Propulsion Laboratory
    Sent: Friday, January 09, 2004 7:49 PM
    To: ljk4_at_msn.com
    Subject: Spirit Lowers Front Wheels, Looks Around in Infrared

    MEDIA RELATIONS OFFICE
    JET PROPULSION LABORATORY
    CALIFORNIA INSTITUTE OF TECHNOLOGY
    NATIONAL AERONAUTICS AND SPACE ADMINISTRATION
    PASADENA, CALIFORNIA 91109. TELEPHONE (818) 354-5011
    http://jpl.convio.net/site/R?i=tzBD39HPM6pO-3BCLCXxIg.. http://jpl.convio.net/site/R?i=F2NYBsMzVOlO-3BCLCXxIg..

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

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

    NEWS RELEASE: 2004-013 January 9, 2004

    Spirit Lowers Front Wheels, Looks Around in Infrared

    NASA's Spirit, the first of two Mars Exploration Rovers on the martian
    surface, has stood up and extended its front wheels while continuing
    to delight its human partners with new information about its
    neighborhood within Mars' Gusev Crater.

    Traces of carbonate minerals showed up in the rover's first survey of
    the site with its infrared sensing instrument, called the miniature
    thermal emission spectrometer or Mini-TES. Carbonates form in the
    presence of water, but it's too early to tell whether the amounts
    detected come from interaction with water vapor in Mars' atmosphere or
    are evidence of a watery local environment in the past, scientists
    emphasized.

    "We came looking for carbonates. We have them. We're going to chase
    them," said Dr. Phil Christensen of Arizona State University, Tempe,
    leader of the Mini-TES team. Previous infrared readings from Mars
    orbit have revealed a low concentration of carbonates distributed
    globally. Christensen has interpreted that as the result of dust
    interaction with atmospheric water. First indications are that the
    carbonate concentration near Spirit may be higher than the Mars global
    average.

    After the rover drives off its lander platform, infrared measurements
    it takes as it explores the area may allow scientists to judge whether
    the water indicated by the nearby carbonates was in the air or in a
    suspected ancient lake.

    "The beauty is we know how to find out," said Dr. Steve Squyres of
    Cornell University, Ithaca, N.Y., principal investigator for the
    mission. "Is the carbonate concentrated in fluffy dust? That might
    favor the atmospheric hypothesis. Is it concentrated in coarser
    material? That might favor the water hypothesis."

    Spirit accomplished a key step late Thursday in preparing for rolling
    off the lander. In anticipation, the flight team at NASA Jet
    Propulsion Laboratory in Pasadena, Calif., played Bob Marley's "Get
    Up, Stand Up" as wake-up music for the sixth morning on Mars, said
    JPL's Matt Wallace, mission manager. In the following hours, the
    rover was raised by a lift mechanism under its belly, and its front
    wheels were fully extended. Then the rover was set back down, raised
    again and set down again to check whether suspension mechanisms had
    latched properly.

    Pictures returned from the rover's navigation camera and front
    hazard-identification camera, plus other data, confirmed success.

    "We are very, very, very pleased to see the rover complete the most
    critical part of the stand-up process," Wallace said. Next steps
    include retracting the lift mechanism and extending the rear wheels.

    A tug on airbag tendons by the airbag retraction motor Thursday
    evening did not lower puffed up portions of airbag material that are a
    potential obstacle to driving the rover straight forward to exit the
    lander. The most likely path for driving off will be to turn 120
    degrees to the right before rolling off. "This is something we have
    practiced many times. We are very comfortable doing it," Wallace said.

    The earliest scenario for getting the rover off the lander, if all
    goes smoothly, is Spirit's 13th or 14th day on Mars, Jan. 16 or 17.

    "We're proceeding in a measured, temperate way," said JPL's Peter
    Theisinger, project manager for the Mars Exploration Rover project.
    "This is a priceless asset. It is fully functioning. It is sitting in
    a beautiful scientific target. We're not going to take any
    inappropriate risks."

    While preparing to learn more about what Mars rocks are made of,
    Christensen announced an educational project to involve school
    children and other people in getting rocks from all over Earth for
    comparison. "Send me your rocks and we'll see if there are rocks in
    your back yard that are similar to what we're seeing on Mars," he
    said. Information about how to send rocks to Arizona State University
    is on the rovers' Web site at http://jpl.convio.net/site/R?i=rgFJvG7H8DNO-3BCLCXxIg..
    http://jpl.convio.net/site/R?i=XQMasusuI_JO-3BCLCXxIg.. .

    Spirit's twin Mars Exploration Rover, Opportunity, will reach Mars on
    Jan. 25 (Universal Time and EST; Jan. 24 PST). The rovers' main task
    is to spend three months exploring for clues in rocks and soil about
    whether past environments near the landing sites were ever watery and
    possibly suitable to sustain life.
    JPL, a division of the California Institute of Technology, manages the
    Mars Exploration Rover project for NASA's Office of Space Science,
    Washington.

    -end-


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