2001 Mars Odyssey Mission Summary

被引：0
作者：
R.S. Saunders
R.E. Arvidson
G.D. Badhwar
W.V. Boynton
P.R. Christensen
F.A. Cucinotta
W.C. Feldman
R.G. Gibbs
C. Kloss
M.R. Landano
R.A. Mase
G.W. McSmith
M.A. Meyer
I.G. Mitrofanov
G.D. Pace
J.J. Plaut
W.P. Sidney
D.A. Spencer
T.W. Thompson
C.J. Zeitlin
机构：
[1] Jet Propulsion Laboratory,Department of Earth and Planetary Sciences
[2] Washington University,Department of Planetary Sciences, Lunar and Planetary Laboratory
[3] Johnson Space Center,Department of Geological Sciences
[4] NASA,National Space Biomedical Research Institute
[5] University of Arizona,undefined
[6] Arizona State University,undefined
[7] NASA Headquarters,undefined
[8] Los Alamos National Laboratory,undefined
[9] The Russian Aviation and Space Agency's Institute for Space Research (IKI),undefined
[10] Laboratory of Space Gamma Ray Spectroscopy,undefined
[11] Lockheed Martin Astronautics,undefined
[12] Baylor College of Medicine,undefined
[13] Science Applications International Corporation,undefined
来源：
Space Science Reviews | 2004年 / 110卷
关键词：
Mars Global Surveyor; Martian Surface; Neutron Spectrometer; Deep Space Network; Planetary Data System;
D O I：
暂无
中图分类号：
学科分类号：
摘要：
The 2001 Mars Odyssey spacecraft, now in orbit at Mars, will observe the Martian surface at infrared and visible wavelengths to determine surface mineralogy and morphology, acquire global gamma ray and neutron observations for a full Martian year, and study the Mars radiation environment from orbit. The science objectives of this mission are to: (1) globally map the elemental composition of the surface, (2) determine the abundance of hydrogen in the shallow subsurface, (3) acquire high spatial and spectral resolution images of the surface mineralogy, (4) provide information on the morphology of the surface, and (5) characterize the Martian near-space radiation environment as related to radiation-induced risk to human explorers.
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页码：1 / 36
页数：35
相关论文
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  • [1] Badhwar G. D.(2004)Martian Radiation Environment Experiment (MARIE) Space Science Reviews 110 131-142
  • [2] Boynton W. V.(2002)Distribution of Hydrogen in the Near Surface of Mars: Evidence for Subsurface Ice Deposits Science 297 81-85
  • [3] Feldman W. C.(2004)The Mars Odyssey Gamma-Ray Spectrometer Instrument Suite Space Science Reviews 110 37-83
  • [4] Squyres S.W.(2004)The Thermal Emission Imaging System (THEMIS) for the Mars 2001 Odyssey Mission Space Science Reviews 110 85-130
  • [5] Prettyman T. H.(2003)Formation of Recent Martian Gullies through Melting of Extensive Water-Ice Snow Deposits Nature 422 45-48
  • [6] Bruckner J.(2004)In Memoriam, Gautam D. Badhwar (1940-2001) Space Science Reviews 110 157-159
  • [7] Evans L. G.(2002)Global Distribution of Neutrons from Mars: Results from Mars Odyssey Science 297 75-78
  • [8] Reedy R. C.(2002)Maps of Subsurface Hydrogen from the High Energy Neutron Detector, Mars Odyssey Science 297 78-81
  • [9] Starr R.(2004)Radiation Climate Map for Analyzing Risks to Astronauts on the Mars Surface from Galactic Cosmic Rays Space Science Reviews 110 143-156
  • [10] Arnold J. R.(2003)Exposed Water Ice Discovered Near the South Pole of Mars Science 299 1048-1051
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