Published July 22, 2005
| Supplemental Material
Journal Article
Open
Martian Surface Paleotemperatures from Thermochronology of Meteorites
- Creators
- Shuster, David L.
- Weiss, Benjamin P.
Chicago
Abstract
The temporal evolution of past martian surface temperatures is poorly known. We used thermochronology and published noble gas and petrographic data to constrain the temperature histories of the nakhlites and martian meteorite ALH84001. We found that the nakhlites have not been heated to more than 350°C since they formed. Our calculations also suggest that for most of the past 4 billion years, ambient near-surface temperatures on Mars are unlikely to have been much higher than the present cold (<0°C) state.
Additional Information
© 2005 American Association for the Advancement of Science. Received 4 April 2005; accepted 7 June 2005. We thank T. Swindle and D. Bogard for generously sharing their Ar data with us and for helpful discussions, along with T. Grove, A. Maloof, and J. Eiler. B.P.W. is supported by the NASA Mars Fundamental Research and NSF Geophysics programs.Attached Files
Supplemental Material - Shuster.SOM.pdf
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Additional details
- Eprint ID
- 51952
- DOI
- 10.1126/science.1113077
- Resolver ID
- CaltechAUTHORS:20141119-101159092
- NASA
- NSF
- Created
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2014-11-19Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field