Chemical compositions at Mars landing sites subject to Mars Odyssey Gamma Ray Spectrometer constraints-Reference-Cited by-同舟云学术

Chemical compositions at Mars landing sites subject to Mars Odyssey Gamma Ray Spectrometer constraints

Published:2007-08 Issue:E8 Volume:112 Page:
ISSN:0148-0227
Container-title:Journal of Geophysical Research: Planets
language:en
Short-container-title:J. Geophys. Res.

Author:

Karunatillake Suniti¹,Keller John M.²,Squyres Steven W.¹,Boynton William V.³,Brückner Johannes⁴,Janes Daniel M.³,Gasnault Olivier⁵,Newsom Horton E.⁶

Affiliation:

1. Department of Astronomy; Cornell University; Ithaca New York USA

2. Physics Department; California Polytechnic State University; San Luis Obispo California USA

3. Lunar and Planetary Laboratory; University of Arizona; Tucson Arizona USA

4. Abteilung Geochemie; Max-Planck-Institut für Chemie; Mainz Germany

5. Centre d'Etude Spatiale des Rayonnements/Centre National de la Recherche Scientifique/Université Paul Sabatier Toulouse; Toulouse France

6. Institute of Meteoritics and Department of Earth and Planetary Sciences; University of New Mexico; Albuquerque New Mexico USA

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://onlinelibrary.wiley.com/wol1/doi/10.1029/2006JE002859/fullpdf

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5. Overview of the Spirit Mars Exploration Rover Mission to Gusev Crater: Landing site to Backstay Rock in the Columbia Hills;Arvidson;J. Geophys. Res.,2006

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