GRS evidence and the possibility of paleooceans on Mars

Autor: Lucia Marinangeli, John Keller, Daniel M. Janes, Roberto Furfaro, Alberto G. Fairén, Gian Gabriele Ori, J. C. Ferris, Trent M. Hare, Dirk Schulze-Makuch, Javier Ruiz, Kris Kerry, Michael Finch, Victor R. Baker, William V. Boynton, Jeffrey S. Kargel, Shawn J. Wheelock, William C. Mahaney, Kyeong Ja Kim, Suniti Karunatillake, James M. Dohm, Goro Komatsu
Přispěvatelé: Korea Institute of Geoscience and Mineral Resource, Ministry of Science and Technology (South Korea)
Rok vydání: 2009
Předmět:
Zdroj: E-Prints Complutense. Archivo Institucional de la UCM
instname
Digital.CSIC. Repositorio Institucional del CSIC
E-Prints Complutense: Archivo Institucional de la UCM
Universidad Complutense de Madrid
Popis: 71 manuscript pages, 12 figures, 3 tables.-- Presented at the 2nd International Workshop on Exploring Mars and its Earth Analogues, Trento, Italy, June 19-23, 2007: http://digital.csic.es/handle/10261/8617
The Gamma Ray Spectrometer (Mars Odyssey spacecraft) has revealed elemental distributions of potassium (K), thorium (Th), and iron (Fe) on Mars that require fractionation of K (and possibly Th and Fe) consistent with aqueous activity. This includes weathering, evolution of soils, and transport, sorting, and deposition, as well as with the location of first-order geomorphological demarcations identified as possible paleoocean boundaries. The element abundances occur in patterns consistent with weathering in situ and possible presence of relict or exhumed paleosols, deposition of weathered materials (salts and clastic minerals), and eathering/transport under neutral to acidic brines. The abundances are explained by hydrogeology consistent with the possibly overlapping alternatives of paleooceans and/or heterogeneous rock compositions from diverse provenances (e.g, differing igneous compositions).
We are grateful to the Gamma Ray Spectrometer Team whose diligent efforts have yielded tremendous fruit. Kyeong Kim is partially supported by the Basic Research Project (08-3611) of the Korea Institute of Geoscience and Mineral Resources (KIGAM) funded by the Ministry of Science and Technology (MOST) of Korea.
Databáze: OpenAIRE