Kevin W. Lewis

Affiliations: 
2009-2014 Geoscience Princeton University, Princeton, NJ 
 2014- Earth and Planetary Sciences Johns Hopkins University, Baltimore, MD 
Area:
Planetary Science
Website:
http://eps.jhu.edu/directory/kevin-lewis/
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"Kevin Lewis"
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Publications

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Lewis KW, Peters S, Gonter K, et al. (2019) A surface gravity traverse on Mars indicates low bedrock density at Gale crater. Science (New York, N.Y.). 363: 535-537
Ojha L, Lewis K, Karunatillake S, et al. (2018) The Medusae Fossae Formation as the single largest source of dust on Mars. Nature Communications. 9: 2867
Banham SG, Gupta S, Rubin DM, et al. (2018) Ancient Martian aeolian processes and palaeomorphology reconstructed from the Stimson formation on the lower slope of Aeolis Mons, Gale crater, Mars Sedimentology. 65: 993-1042
Lapotre MGA, Ewing RC, Weitz CM, et al. (2018) Morphologic Diversity of Martian Ripples: Implications for Large‐Ripple Formation Geophysical Research Letters. 45: 10,229-10,239
Edwards CS, Piqueux S, Hamilton VE, et al. (2018) The Thermophysical Properties of the Bagnold Dunes, Mars: Ground-Truthing Orbital Data Journal of Geophysical Research: Planets. 123: 1307-1326
Anderson RB, Edgar LA, Rubin DM, et al. (2018) Complex bedding geometry in the upper portion of Aeolis Mons, Gale crater, Mars Icarus. 314: 246-264
Ewing RC, Lapotre MGA, Lewis KW, et al. (2017) Sedimentary processes of the Bagnold Dunes: Implications for the eolian rock record of Mars. Journal of Geophysical Research. Planets. 122: 2544-2573
Edgar LA, Gupta S, Rubin DM, et al. (2017) Shaler: in situ analysis of a fluvial sedimentary deposit on Mars Sedimentology. 65: 96-122
Yingst RA, Cropper K, Gupta S, et al. (2016) Characteristics of pebble and cobble-sized clasts along the Curiosity rover traverse from sol 100 to 750: Terrain types, potential sources, and transport mechanisms Icarus. 280: 72-92
Kite ES, Sneed J, Mayer DP, et al. (2016) Evolution of major sedimentary mounds on Mars: Buildup via anticompensational stacking modulated by climate change Journal of Geophysical Research. 121: 2282-2324
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