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Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover
by
Glotch, T. D.
, Gorelick, N.
, Fergason, R. L.
, Calvin, W. M.
, Morris, R. V.
, Hayes, A.
, Golombek, M. P.
, Mehall, G. L.
, Hamilton, V. E.
, Knudson, A. T.
, McSween, H. Y.
, Rogers, A. D.
, Budney, C.
, Moersch, J. E.
, Johnson, J. R.
, Anwar, S.
, Arvidson, R. E.
, Smith, M. D.
, Ruff, S. W.
, Blaney, D. L.
, Graff, T. G.
, Wyatt, M. B.
, Bandfield, J. L.
, Mehall, L. K.
, Wolff, M. J.
, Christensen, P. R.
, Squyres, S. W.
in
Absorption spectra
/ Basalt
/ Bound water
/ Carbonates
/ Climate
/ Coatings
/ Disturbed soils
/ Dust
/ Equipment and supplies
/ Experiments
/ Geologic Sediments
/ Geology
/ Impact craters
/ Interferometry
/ Iron Compounds
/ Least Squares Statistics
/ Lunar And Planetary Science And Exploration
/ Magnesium Compounds
/ Mars
/ Mars (Planet)
/ Mineralogy
/ Minerals
/ Olivine
/ Oxides
/ Physical properties
/ Properties
/ Research Articles and Reports
/ Rocks
/ Silicates
/ Sodic soils
/ Space exploration
/ Spectrum Analysis
/ Success
/ Temperature
/ Water
2004
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Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover
by
Glotch, T. D.
, Gorelick, N.
, Fergason, R. L.
, Calvin, W. M.
, Morris, R. V.
, Hayes, A.
, Golombek, M. P.
, Mehall, G. L.
, Hamilton, V. E.
, Knudson, A. T.
, McSween, H. Y.
, Rogers, A. D.
, Budney, C.
, Moersch, J. E.
, Johnson, J. R.
, Anwar, S.
, Arvidson, R. E.
, Smith, M. D.
, Ruff, S. W.
, Blaney, D. L.
, Graff, T. G.
, Wyatt, M. B.
, Bandfield, J. L.
, Mehall, L. K.
, Wolff, M. J.
, Christensen, P. R.
, Squyres, S. W.
in
Absorption spectra
/ Basalt
/ Bound water
/ Carbonates
/ Climate
/ Coatings
/ Disturbed soils
/ Dust
/ Equipment and supplies
/ Experiments
/ Geologic Sediments
/ Geology
/ Impact craters
/ Interferometry
/ Iron Compounds
/ Least Squares Statistics
/ Lunar And Planetary Science And Exploration
/ Magnesium Compounds
/ Mars
/ Mars (Planet)
/ Mineralogy
/ Minerals
/ Olivine
/ Oxides
/ Physical properties
/ Properties
/ Research Articles and Reports
/ Rocks
/ Silicates
/ Sodic soils
/ Space exploration
/ Spectrum Analysis
/ Success
/ Temperature
/ Water
2004
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Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover
by
Glotch, T. D.
, Gorelick, N.
, Fergason, R. L.
, Calvin, W. M.
, Morris, R. V.
, Hayes, A.
, Golombek, M. P.
, Mehall, G. L.
, Hamilton, V. E.
, Knudson, A. T.
, McSween, H. Y.
, Rogers, A. D.
, Budney, C.
, Moersch, J. E.
, Johnson, J. R.
, Anwar, S.
, Arvidson, R. E.
, Smith, M. D.
, Ruff, S. W.
, Blaney, D. L.
, Graff, T. G.
, Wyatt, M. B.
, Bandfield, J. L.
, Mehall, L. K.
, Wolff, M. J.
, Christensen, P. R.
, Squyres, S. W.
in
Absorption spectra
/ Basalt
/ Bound water
/ Carbonates
/ Climate
/ Coatings
/ Disturbed soils
/ Dust
/ Equipment and supplies
/ Experiments
/ Geologic Sediments
/ Geology
/ Impact craters
/ Interferometry
/ Iron Compounds
/ Least Squares Statistics
/ Lunar And Planetary Science And Exploration
/ Magnesium Compounds
/ Mars
/ Mars (Planet)
/ Mineralogy
/ Minerals
/ Olivine
/ Oxides
/ Physical properties
/ Properties
/ Research Articles and Reports
/ Rocks
/ Silicates
/ Sodic soils
/ Space exploration
/ Spectrum Analysis
/ Success
/ Temperature
/ Water
2004
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Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover
Journal Article
Initial Results from the Mini-TES Experiment in Gusev Crater from the Spirit Rover
2004
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Overview
The Miniature Thermal Emission Spectrometer (Mini-TES) on Spirit has studied the mineralogy and thermophysical properties at Gusev crater. Undisturbed soil spectra show evidence for minor carbonates and bound water. Rocks are olivinerich basalts with varying degrees of dust and other coatings. Dark-toned soils observed on disturbed surfaces may be derived from rocks and have derived mineralogy (±5 to 10%) of 45% pyroxene (20% Ca-rich pyroxene and 25% pigeonite), 40% sodic to intermediate plagioclase, and 15% olivine (forsterite 45% ±5 to 10). Two spectrally distinct coatings are observed on rocks, a possible indicator of the interaction of water, rock, and airfall dust. Diurnal temperature data indicate particle sizes from 40 to 80 µm in hollows to ~0.5 to 3 mm in soils.
Publisher
American Association for the Advancement of Science,The American Association for the Advancement of Science
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