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Dusting Off The Mars Manual

File Photo: This black and white image of Mermaid Dune was extracted from the green color plane of Soujourner's rear color camera. The rover right rear wheel is seen at bottom left and the shadow of the Alpha Proton X-ray Spectrometer (APXS) is at bottom center. The dune surface occupies the upper right half of the image. The contact between Mermaid and the underlying ground surface extends from the upper left to the APXS shadow. The surface of the dune exhibits a granular texture. The image resolution is about 1 mm/pixel, so the granularity may represent sand particles or cohesive clods of dust.
  • Image source: NSSDC Collection
  • Los Angeles - Jun 20, 2002
    Dr. Geoffrey A. Landis, an aerospace engineer at NASA's Glenn Research Center, Cleveland, thinks he knows what it takes to explore Mars. And the Agency believes him. Landis' proposal, "Study of Solar Energy and Dust Accumulation on the Rovers," was one of 28 scientific studies of Mars recently selected by NASA for the 2003 Mars Exploration Rover Mission.

    His proposal calls for the use of Mars Exploration Rover (MER) instrumentation to study the intensity, spatial and spectral distribution of solar energy on the Mars surface, and to compare the measured values with various models of solar distribution.

    Landis will measure three additional properties: the rate of deposition and removal of atmospheric dust on the rover's solar arrays; the operating temperature of the solar arrays on Mars; and the degradation (if any) of the solar power system in the Martian environment. Finally, data derived from these measurements will be used to determine the optical properties of atmospheric and deposited dust.

    "I'm really looking forward to working on this mission," says Landis.

    "The two MER vehicles are going to be much larger and more capable than the Sojourner rover. They can traverse longer distances and make better measurements. This is an exciting mission-I expect that we'll learn a lot about what the surface of Mars is like."

    Landis, who resides in Berea, Ohio, has previous Mars mission experience working on 1997's successful Mars Pathfinder expedition as a science investigator of the rover, Sojourner. He and a team of Glenn engineers built a miniature instrument to look for dust accumulation on the rover's solar panels. Giant storms raise large amounts of dust into the Mars atmosphere, and dust settling can degrade solar arrays.

    Landis' experiment showed almost 20% loss of solar array power during two months on Mars. While not detrimental to the Sojourner mission, such a trend poses a concern for longer missions. Understanding solar power on Mars is important to future exploration, including possible human missions.

    The selected proposals were judged to have the best science value among 84 proposals submitted to NASA last December in response to the Mars Exploration Rover Announcement of Opportunity. Each selected investigation will work with the Mars Exploration Rover Program Office at the Jet Propulsion Laboratory, Pasadena, Calif., and will become full mission science-team members, joining previously selected scientists as part of the Athena payload science team. The MER rover mission will send twin rovers to the surface of Mars, landing in January and February 2004.

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    Martian Scientists Hope To Stir Up A Devil Of A Storm
    Tucson - May 21, 2002
    Scientists from several nations begin an unprecedented 3-and-1/2-week pilot field experiment on the Santa Cruz flats near Eloy, Ariz., today, May 20, to discover how dust devils may affect atmospheres on Earth and on Mars.



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