Composition of conglomerates analyzed by the Curiosity rover: Implications for Gale Crater crust and sediment sources
Journal of Geophysical Research
By: Nicolas Mangold, L.M. Thompson, O. Forni, C. Fabre, L. Le Deit, R. C. Wiens, A.J. Williams, R. Williams, Ryan B. Anderson, Diana L. Blaney, Fred J. Calef, Agnes Cousin, Samuel M. Clegg, Gilles Dromart, William E. Dietrich, Kenneth S. Edgett, Martin R. Fisk, Olivier Gasnault, Ralf Gellert, John P. Grotzinger, Linda C. Kah, Stephane Le Mouelic, Scott M. McLennan, Sylvestre Maurice, Pierre-Yves Meslin, Horton E. Newsom, Marisa C. Palucis, William Rapin, Violaine Sautter, Kirsten L. Siebach, Katherine M. Stack, Dawn Y. Sumner, and Aileen Yingst
Links
- More Information:
- Open Access Version: External Repository
- Download citation as: RIS | Dublin Core
Abstract
| Publication type | Article |
|---|---|
| Publication Subtype | Journal Article |
| Title | Composition of conglomerates analyzed by the Curiosity rover: Implications for Gale Crater crust and sediment sources |
| Series title | Journal of Geophysical Research |
| DOI | 10.1002/2015JE004977 |
| Volume | 121 |
| Issue | 3 |
| Publication Date | March 16, 2016 |
| Year Published | 2016 |
| Language | English |
| Publisher | American Geophysical Union |
| Publisher location | Washington, D.C. |
| Contributing office(s) | Astrogeology Science Center |
| Description | 35 p. |
| First page | 353 |
| Last page | 387 |
| Other Geospatial | Gale, crater on Mars near the northwestern part of the Aeolis quadrangle at 5.4°S 137.8°E; 154 km (96 mi) in diameter; estimated to be about 3.5-3.8 billion years old. |
| Online Only (Y/N) | N |
| Additional Online Files (Y/N) | N |