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Mars ExplorationConference Paper

Preliminary Geological Map of the Peace Vallis Fan Integrated with In Situ Mosaics From the Curiosity Rover, Gale Crater, Mars

Curiosity20191 min read123 words
Sumner, D. Y., Palucis, M., Dietrich, B., Calef, F., Stack, K. M., Ehlmann, B., Bridges, J., Dromart, J., Eigenbrode, J., Farmer, J., Grant, J., Grotzinger, J., Hamilton, V., Hardgrove, C., Kah, L., Leveille, R., Mangold, N., Rowland, S., and Williams, R.
Goddard Space Flight Center

A geomorphically defined alluvial fan extends from Peace Vallis on the NW wall of Gale Crater, Mars into the Mars Science Laboratory (MSL) Curiosity rover landing ellipse. Prior to landing, the MSL team mapped the ellipse and surrounding areas, including the Peace Vallis fan. Map relationships suggest that bedded rocks east of the landing site are likely associated with the fan, which led to the decision to send Curiosity east. Curiosity's mast camera (Mastcam) color images are being used to refine local map relationships. Results from regional mapping and the first 100 sols of the mission demonstrate that the area has a rich geological history. Understanding this history will be critical for assessing ancient habitability and potential organic matter preservation at Gale Crater.


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