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Soil Diversity and Hydration as Observed by ChemCam at Gale Crater, Mars

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Title Soil Diversity and Hydration as Observed by ChemCam at Gale Crater, Mars
Names Meslin, P.-Y. (creator)
Gasnault, O. (creator)
Forni, O. (creator)
Schröder, S. (creator)
Cousin, A. (creator)
Berger, G. (creator)
Clegg, S. M. (creator)
Lasue, J. (creator)
Maurice, S. (creator)
Sautter, V. (creator)
Le Mouélic, S. (creator)
Wiens, R. C. (creator)
Fabre, C. (creator)
Goetz, W. (creator)
Bish, D. (creator)
Mangold, N. (creator)
Ehlmann, B. (creator)
Lanza, N. (creator)
Harri, A.-M. (creator)
Anderson, R. (creator)
Rampe, E. (creator)
McConnochie, T. H. (creator)
Pinet, P. (creator)
Blaney, D. (creator)
Léveillé, R. (creator)
Archer, D. (creator)
Barraclough, B. (creator)
Bender, S. (creator)
Blake, D. (creator)
Blank, J. G. (creator)
Bridges, N. (creator)
Clark, B. C. (creator)
DeFlores, L. (creator)
Delapp, D. (creator)
Dromart, G. (creator)
Dyar, M. D. (creator)
Fisk, M. (creator)
Gondet, B. (creator)
Grotzinger, J. (creator)
Herkenhoff, K. (creator)
Johnson, J. (creator)
Lacour, J.-L. (creator)
Langevin, Y. (creator)
Leshin, L. (creator)
Lewin, E. (creator)
Madsen, M. B. (creator)
Melikechi, N. (creator)
Mezzacappa, A. (creator)
Mischna, M. A. (creator)
Moores, J. E. (creator)
Newsom, H. (creator)
Ollila, A. (creator)
Perez, R. (creator)
Renno, N. (creator)
Sirven, J.-B. (creator)
Tokar, R. (creator)
de la Torre, M. (creator)
d’Uston, L. (creator)
Vaniman, D. (creator)
Yingst, A. (creator)
MSL Science Team (creator)
Date Issued 2013-09-27 (iso8601)
Note To the best of our knowledge, one or more authors of this paper were federal employees when contributing to this work.
This is the publisher’s final pdf. The published article is copyrighted by American Association for the Advancement of Science and can be found at: http://www.aaas.org/publications/.
Abstract Abstract: The ChemCam instrument, which provides insight into martian soil chemistry at the submillimeter scale, identified two principal soil types along the Curiosity rover traverse: a fine-grained mafic type and a locally derived, coarse-grained felsic type. The mafic soil component is representative of widespread martian soils and is similar in composition to the martian dust. It possesses a ubiquitous hydrogen signature in ChemCam spectra, corresponding to the hydration of the amorphous phases found in the soil by the CheMin instrument. This hydration likely accounts for an important fraction of the global hydration of the surface seen by previous orbital measurements. ChemCam analyses did not reveal any significant exchange of water vapor between the regolith and the atmosphere. These observations provide constraints on the nature of the amorphous phases and their hydration.
Genre Article
Topic Emission spectrometer data
Identifier Meslin, P., Sautter, V., Le Mouélic, S., Wiens, R. C., Fabre, C., Goetz, W., . . . MSL Sci Team. (2013). Soil diversity and hydration as observed by ChemCam at gale crater, mars. Science (New York, N.Y.), 341(6153), 1238670. doi:10.1126/science.1238670

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