[meteorite-list] NASA Selects 28 Participating Scientists For Mars Rover Mission

From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu Apr 22 10:04:54 2004
Message-ID: <200205292127.OAA05251_at_zagami.jpl.nasa.gov>

Donald Savage
Headquarters, Washington May 29, 2002
(Phone: 202/358-1547)

RELEASE: 02-100

NASA SELECTS 28 PARTICIPATING SCIENTISTS FOR MARS ROVER
MISSION

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.
 
The selected investigators are:

* 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

                      - end -
Received on Wed 29 May 2002 05:27:32 PM PDT