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Deciphering Martian climatic history using returned samples (1988)

Brigham, C. A. ; Krieger, D. B. ; Paige, D. A.

In: CASI

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Publication Date: 2013-08-31

Description: By necessity, a Mars sample return mission must sample the upper few meters of the Martian surface. This material was subjected to a wide variety of physical processes. Presently, the most important processes are believed to be wind-driven erosion and deposition, and water ice accumulation at higher latitudes. A sample return mission represents an opportunity to better understand and quantify these important geological processes. By obtaining sample cores at key locations, it may be possible to interpret much of recent Martian climatic history.

Keywords: LUNAR AND PLANETARY EXPLORATION

Type: Lunar and Planetary Inst., Workshop on Mars Sample Return Science; p 136-137

Format: application/pdf

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