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NASA Picks Mars 2003 Science Team
NASA Picks Mars 2003 Science Team
29 May 2002
(Source: NASA Headquarters)

Donald Savage
NASA Headquarters, Washington
(Phone: 202/358-1547)

RELEASE: 02-100

NASA has selected 28 scientists for participation in the 2003 Mars Exploration Rover (MER) Mission. The mission consists of two separate, though identical, rovers scheduled for launch in mid-2003 and arrival at separate destinations on Mars in early 2004.

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 MER Program Office at NASA's Jet Propulsion Laboratory (JPL), Pasadena, Calif., and will become full MER science-team members, joining previously selected scientists as part of the Athena science team.

"The breadth, scope, and creativity of the scientists selected is very encouraging," said Dr. Ed Weiler, NASA Associate Administrator for Space Science, Headquarters, Washington. "By directly participating in NASA's next mission to the surface of Mars, they will help bring us closer to the long-term objective of our Mars Exploration Program -- understanding Mars as a planet and determining whether life ever existed there."

The MER mission science objectives include: (1) study rocks and soils for clues to past water activity; (2) investigate landing sites that have a high probability of containing evidence of the action of liquid water; (3) determine the distribution and composition of minerals, rocks and soils surrounding the landing sites; (4) determine the nature of local surface geologic processes; (5) calibrate and validate data from orbiting missions at each landing site; and (6) study the geologic processes for clues about the environmental conditions that existed when liquid water was present, and whether those environments were conducive for life.

  • Johannes Brueckner; Max Planck Institut fur Chemie, Mainz, Germany; Investigation of elemental composition of Martian soils and their relationship to global surface chemistry
  • Nathalie A. Cabrol; SETI Institute, Moffett Field, Calif.; Aqueous Sedimentary Processes at the MER sites
  • Wendy M. Calvin; University of Nevada, Reno; Mini-TES investigation for surface mineralogy and surface/orbit constraints on TES
  • Benton C. Clark; Lockheed Martin Corporation, Littleton, Colo.; Chemical Alteration Processes on Mars: Investigations and Implications
  • Larry S. Crumpler; New Mexico Museum of Natural History and Science, Albuquerque; Field Geology and Micro-surface Characteristics at MER Investigation Sites
  • Jack D. Farmer; Arizona State University, Tempe; Integrated Studies of Surface Geology and Mineralogy to Explore for Past Aqueous Environments
  • William H. Farrand; Space Science Institute, Boulder, Colo.; Major and Minor Components of the Surface Layer of Mars: An Investigation Using the MER Pancam and Mini-TES
  • William M. Folkner; JPL; Measurement of Mars Rotation Changes with the Mars Exploration Rovers
  • Matthew P. Golombek; JPL; Directing Long Range Rover Traverses using Orbital Surface Predictions and MER Ground Truth
  • John A. Grant; Smithsonian Institution, Washington; Constraining the Geologic Setting and Evolution of the MER Landing Site(s)
  • Ronald Greeley; Arizona State University, Tempe; Mars Exploration Rover: Study of Aeolian Features and Processes
  • John P. Grotzinger; Massachusetts Institute of Technology, Cambridge; Geological Analysis of Martian Sediments and Sedimentary Rocks
  • Stubbe Hviid; Max Planck Institut fur Aeronomie, Katlenburg-Lindau, Germany; Investigation of the production and composition of Martian soils and dust and their effect upon the Martian atmosphere
  • Jeffrey R. Johnson; U.S. Geological Survey, Flagstaff, Ariz.; Spectrophotometric Observations of Surface Materials at the MER Landing Sites
  • Geoffrey A. Landis; Ohio Aerospace Institute, Cleveland; Study of Solar Energy and Dust Accumulation on MER
  • Mark T. Lemmon; Texas A & M University, College Station; Investigation of the properties of Martian atmospheric dust and its effect on the illumination of the Martian surface
  • Rongxing Li; Ohio State University, Columbus; Surface Image-based High-precision Near Real-time Landing Site Mapping and Long-range Rover Localization for MER 2003 mission
  • Scott M. McLennan; State University of New York, Stony Brook; Sedimentary Petrology at the MER Sites
  • Douglas W. Ming; NASA Johnson Space Center, Houston; Identification and Processes of Formation for Phyllosilicates, Sulfates, and Other Chemical Weathering Products on Mars
  • Jeffrey E. Moersch; University of Tennessee, Knoxville; A Search for Aqueous Minerals with the Mars Exploration Rover Mini-TES Experiment
  • Timothy J. Parker; JPL; Sedimentary Stratigraphy and Geomorphology of the MER A and B Landing Sites
  • James W. Rice; Arizona State University, Tempe; MER Geomorphic and Sedimentological Investigations
  • Lutz Richter; DLR Institut fur Raumsimulation, Koln, Germany; Mars Soil Mechanics Investigations Using MER Rover Locomotion System Engineering Data
  • Michael D. Smith; NASA Goddard Space Flight Center, Greenbelt, Md.; Retrieval of Atmospheric Properties using mini-TES spectra
  • Peter H. Smith; University of Arizona, Tucson; The dust cycle monitored from MER
  • Robert Sullivan; Cornell University, Ithaca, N.Y.; Physical and Mechanical Properties of Martian Soils Along MER Traverses
  • Michael J. Wolff; Space Science Institute, Martinez, Ga.; Aerosol Studies and the Boundary Layer: Things are Looking Up
  • Albert S. Yen; JPL; Soil Formation without Liquid Water: An Assessment of the Meteoritic Contribution to the Martian Surface
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Last Updated: 29 May 2002