USRA Houston Repository
Geochemical variation in the Stimson formation of Gale crater: Provenance, mineral sorting, and a comparison with modern Martian dunes
JavaScript is disabled for your browser. Some features of this site may not work without it.
| dc.contributor.author | Bedford, Candice | |
| dc.contributor.author | https://orcid.org/0000-0002-0783-1064 | |
| dc.contributor.author | Schwenzer, Susanne Petra | |
| dc.contributor.author | Bridges, John C. | |
| dc.contributor.author | Banham, Steven | |
| dc.contributor.author | Wiens, Roger | |
| dc.contributor.author | Gasnault, Olivier M. | |
| dc.contributor.author | Rampe, Elizabeth | |
| dc.contributor.author | Frydenvang, Jens | |
| dc.contributor.author | Gasda, Patrick J. | |
| dc.contributor.author | https://orcid.org/0000-0002-9608-0759 | |
| dc.coverage.spatial | Mars (Planet) | |
| dc.date.accessioned | 2020-02-10T21:50:45Z | |
| dc.date.available | 2020-02-10T21:50:45Z | |
| dc.date.issued | 2020-05 | |
| dc.identifier.citation | Bedford, C.C., S.P. Schwenzer, J.C. Bridges, S. Banham, R.C. Wiens, O. Gasnault, E.B. Rampe, J. Frydenvang, and P.J. Gasda. 2020. "Geochemical variation in the Stimson formation of Gale crater: Provenance, mineral sorting, and a comparison with modern Martian dunes". Icarus. 341: 2020-05. | en |
| dc.identifier.other | https://doi.org/10.1016/j.icarus.2020.113622 | |
| dc.identifier.uri | https://hdl.handle.net/20.500.11753/1420 | |
| dc.description.abstract | A ChemCam geochemical study of the ancient aeolian Stimson formation in Gale crater. The geochemical effect of mineral sorting in the ancient dunes has been preserved. The Stimson dunes were transported SW-NE, opposite to the modern Bagnold dunes. A subalkaline basaltic source region is suggested for the Stimson formation. | en |
| dc.description.statementofresponsibility | C.C. Bedford, S.P. Schwenzer, J.C. Bridges, S. Banham, R.C. Wiens, O. Gasnault, E. B. Rampe, J. Frydenvang, P.J. Gasda | |
| dc.format.extent | 22 pages | |
| dc.format.mimetype | application/pdf | |
| dc.language.iso | en | en |
| dc.publisher | Elsevier | en |
| dc.relation.ispartofseries | LPI contribution ; no. 2244 | |
| dc.subject | Mars (Planet) | en |
| dc.subject | Geochemistry | en |
| dc.subject.lcc | QB641 | |
| dc.title | Geochemical variation in the Stimson formation of Gale crater: Provenance, mineral sorting, and a comparison with modern Martian dunes | en |
| dc.type | Article | en |
| dc.rights.license | This is an open access article distributed under the terms of the Creative Commons CC-BY license, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. You are not required to obtain permission to reuse this article. |
Files in this item
This item appears in the following Collection(s)
-
LPI Contributions
Documents the scientific research, meetings, and outreach products from the LPI.