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

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Gamma Rays in a Spectrum from the Mars Odyssey Gamma-ray Spectrometer*

R. C. Reedy, L. G. Evans, J. Brückner, K. J. Kim, and W. V. Boynton, Inst. of Meteoritics, MSC03-2050, Univ. New Mexico, Albuquerque, NM 87131 USA ([email protected]), ([email protected]), Science Programs, Computer Sciences Corp., Lanham, MD 20706 USA ([email protected]), Max-Planck-Institut für Chemie, D-55020 Mainz, Germany ([email protected]), Lunar & Planetary Laboratory, Univ....

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IGNEOUS AND AQUEOUS PROCESSES ON MARS: EVIDENCE FROM MEASUREMENTS OF K AND Th BY THE MARS ODYSSEY GAMMA RAY SPECTROMETER

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Erosion rates at the Mars Exploration Rover landing sites and long-term climate change on Mars

[1] Erosion rates derived from the Gusev cratered plains and the erosion of weak sulfates by saltating sand at Meridiani Planum are so slow that they argue that the present dry and desiccating environment has persisted since the Early Hesperian. In contrast, sedimentary rocks at Meridiani formed in the presence of groundwater and occasional surface water, and many Columbia Hills rocks at Gusev ...

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Comparing Quantitative Morphology of Clasts at Three Landing Sites on Mars: Mars

Background. Much of the sedimentary transport and depositional history of Mars may be recorded in the morphologic characteristics of the individual rocks or particles that make up its sedimentary clast population (defined as a rock fragment or grain resulting from the breakdown of larger rocks or bedrock). Measuring morphology is crucial; it retains the best record of sorting and abrasive effec...

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Evolution of the Martian Crust: Evidence from Preliminary Potassium and Thorium Measurements by Mars Odyssey Gamma-ray Spectrometer

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ژورنال

عنوان ژورنال: Journal of Geophysical Research: Planets

سال: 2007

ISSN: 0148-0227

DOI: 10.1029/2006je002859