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New Perspectives on Ancient Mars

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Solomon, Sean C., Aharonson, Oded, Aurnou, Jonathan M., Banerdt, W. Bruce, Carr, Michael H., Dombard, Andrew J., Frey, Herbert V., Golombek, Matthew P., Hauck, Steven A., Head, James W., Jakosky, Bruce M., Johnson, Catherine L., McGovern, Patrick J., Neumann, Gregory A., Phillips, Roger J., Smith, David E., Zuber, Maria T.·2005·Science

DOI 10.1126/science.1101812

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Abstract

Mars was most active during its first billion years. The core, mantle, and crust formed within â¼50 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.

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Authors: Solomon, S. C., Aharonson, O., Aurnou, J. M., Banerdt, W. B., Carr, M. H., Dombard, A. J., Frey, H. V., Golombek, M. P., Hauck, S. A., Head, J. W., Jakosky, B. M., Johnson, C. L., McGovern, P. J., Neumann, G. A., Phillips, R. J., Smith, D. E., & Zuber, M. T.
Affiliations: California Institute of Technology (US)
Corresponding author: Solomon, Sean C.
ORCID: Solomon, Sean C.
Aharonson, Oded
Aurnou, Jonathan M.
Banerdt, W. Bruce
Carr, Michael H.
Dombard, Andrew J.
Golombek, Matthew P.
Hauck, Steven A.
Head, James W.
Jakosky, Bruce M.
Johnson, Catherine L.
McGovern, Patrick J.
Neumann, Gregory A.
Phillips, Roger J.
Smith, David E.
Zuber, Maria T.
Venue: Science
Publisher: American Association for the Advancement of Science (AAAS)
Published: 2005-02-25
Volume: 307
Issue: 5713
Pages: 1214-1220
ISSN: 0036-8075 (ISSN-L)
1095-9203
DOI: 10.1126/science.1101812
OpenAlex: W2110777688
Cited by: 316
References: 97
Citations by year: 2026: 5 · 2025: 13 · 2024: 8 · 2023: 13 · 2022: 14 · 2021: 10 · 2020: 9 · 2019: 7 · 2018: 13 · 2017: 13 · 2016: 12 · 2015: 16 · 2014: 15 · 2013: 7 · 2012: 22
FWCI: 2.82
Type: journal article
Language: en
Open access: green
escholarship.org
Locations: Science (publishedVersion)
PubMed (publishedVersion)
eScholarship (California Digital Library) (submittedVersion)
CaltechAUTHORS (California Institute of Technology) (submittedVersion)
NASA STI Repository (National Aeronautics and Space Administration) (submittedVersion)
Topics: Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Planetary Science and Exploration
Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
Physical Sciences › Earth and Planetary Sciences › Geochemistry and Petrology › Geological and Geochemical Analysis
Keywords: early Mars, magnetic dynamo, crustal magnetization, Tharsis volcanism, outgassing, carbon dioxide, global warming, water erosion, sediment transport, hydrothermal circulation, crustal cooling, crustal thickness, crustal deformation
MeSH terms: Atmosphere, Climate, Extraterrestrial Environment, Magnetics, Temperature, Water, Mars

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