Journal article
New perspectives on ancient Mars
Science (American Association for the Advancement of Science), Vol.307(5713), pp.1214-1220
25/Feb/2005
PMID: 15731435
Abstract
Mars was most active during its first billion years. The core, mantle, and crust formed within ∼50 million years of solar system formation. A magnetic dynamo in a convecting fluid core magnetized the crust, and the global field shielded a more massive early atmosphere against solar wind stripping. The Tharsis province became a focus for volcanism, deformation, and outgassing of water and carbon dioxide in quantities possibly sufficient to induce episodes of climate warming. Surficial and near-surface water contributed to regionally extensive erosion, sediment transport, and chemical alteration. Deep hydrothermal circulation accelerated crustal cooling, preserved variations in crustal thickness, and modified patterns of crustal magnetization.
Details
- Title
- New perspectives on ancient Mars
- Creators
- Sean C SOLOMON (Corresponding Author) - Carnegie Institution for ScienceOded AHARONSON - California Institute of TechnologyJonathan M AURNOU - University of California Los AngelesW. Bruce BANERDT - Jet Propulsion LaboratoryMichael H CARR - United States Geological SurveyAndrew J DOMBARD - Washington University in St. LouisHerbert V FREY - Goddard Space Flight CenterMatthew P GOLOMBEK - Jet Propulsion LaboratorySteven A HAUCK - Case Western Reserve UniversityJames W HEAD - Brown UniversityBruce M JAKOSKY - University of Colorado BoulderCatherine L JOHNSON - University of California, San DiegoPatrick J MCGOVERN - Lunar and Planetary InstituteGregory A NEUMANN - Massachusetts Institute of TechnologyRoger J PHILLIPS - Washington University in St. LouisDavid E SMITH - Goddard Space Flight CenterMaria T ZUBER - Massachusetts Institute of Technology
- Resource Type
- Journal article
- Publication Details
- Science (American Association for the Advancement of Science), Vol.307(5713), pp.1214-1220; 25/Feb/2005
- Publisher
- American Association for the Advancement of Science; Washington, DC
- Language
- English
- DOI
- https://doi.org/10.1126/science.1101812
- PMID
- 15731435
- Grant note
- This paper began as a series of scientific discussions held at meetings of the Mars Orbiting Laser Altimeter team on the Mars Global Surveyor mission. We thank J. Dickson, L. Montesi, and J. Roark for assistance with figure preparation. Support for this paper has been provided by NASA, through the Mars Exploration Program, the Planetary Geology and Geophysics Program, and the NASA Astrobiology Institute.
- Record Identifier
- 993269004503596
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