Mineralogy of an active eolian sediment from the Namib dune, Gale crater, Mars

dc.contributor.author Achilles, C. N.
dc.contributor.author Treiman, Allan H.
dc.contributor.author https://orcid.org/0000-0002-8073-2839
dc.contributor.author Craig, Patricia I.
dc.contributor.author https://orcid.org/0000-0003-4080-4997
dc.coverage.spatial Mars (Planet)
dc.date.accessioned 2020-04-13T20:43:05Z
dc.date.available 2020-04-13T20:43:05Z
dc.date.issued 2017-11-30
dc.description.abstract Curiosity's recent traverse through an active basaltic eolian deposit, informally named the Bagnold Dune Field (Figure 1), provided the opportunity for a multi‐instrument investigation of the geomorphology, chemistry, and mineralogy of the dunes. en
dc.description.statementofresponsibility C. N. Achilles, R. T. Downs, D. W. Ming, E. B. Rampe, R. V. Morris, A. H. Treiman, S. M. Morrison, D. F. Blake, D. T. Vaniman, R. C. Ewing, S. J. Chipera, A. S. Yen, T. F. Bristow, B. L. Ehlmann, R. Gellert, R. M. Hazen, K. V. Fendrich, P. I. Craig, J. P. Grotzinger, D. J. Des Marais, J. D. Farmer, P. C. Sarrazin, J. M. Morookian
dc.format.extent Pages 2344-2361
dc.format.mimetype application/pdf
dc.identifier.citation Achilles, C. N., et al. (2017), Mineralogyof an active eolian sediment from theNamib dune, Gale crater, Mars,J. Geophys. Res. Planets, 122, 2344–2361,doi:10.1002/2017JE005262 en
dc.identifier.other DOI: https://doi.org/10.1002/2017JE005262
dc.identifier.uri https://hdl.handle.net/20.500.11753/1493
dc.language.iso en en
dc.publisher American Geophysical Union en
dc.relation.ispartofseries LPI contribution ; no. 2117
dc.rights.license Attribution-NonCommercial-NoDerivatives 4.0 International (CC BY-NC-ND 4.0)
dc.subject Mars (Planet) en
dc.subject Sand dunes en
dc.subject Mineralogy en
dc.title Mineralogy of an active eolian sediment from the Namib dune, Gale crater, Mars en
dc.type Article en
Files
Original bundle
Now showing 1 - 1 of 1
No Thumbnail Available
Name:
LPI-002117.pdf
Size:
3.91 MB
Format:
Adobe Portable Document Format
Description:
LPI Contribution 2117