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Geochemistry of Carbonates on Mars: Implications for Climate History and Nature of Aqueous Environments

Niles, Paul B. and Catling, David C. and Berger, Gilles and Chassefière, Eric and Ehlmann, Bethany L. and Michalski, Joseph R. and Morris, Richard and Ruff, Steven W. and Sutter, Brad (2013) Geochemistry of Carbonates on Mars: Implications for Climate History and Nature of Aqueous Environments. Space Science Reviews, 174 (1-4). pp. 301-328. ISSN 0038-6308. doi:10.1007/s11214-012-9940-y. https://resolver.caltech.edu/CaltechAUTHORS:20130131-095255817

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Abstract

Ongoing research on martian meteorites and a new set of observations of carbonate minerals provided by an unprecedented series of robotic missions to Mars in the past 15 years help define new constraints on the history of martian climate with important crosscutting themes including: the CO_2 budget of Mars, the role of Mg-, Fe-rich fluids on Mars, and the interplay between carbonate formation and acidity. Carbonate minerals have now been identified in a wide range of localities on Mars as well as in several martian meteorites. The martian meteorites contain carbonates in low abundances (<1 vol.%) and with a wide range of chemistries. Carbonates have also been identified by remote sensing instruments on orbiting spacecraft in several surface locations as well as in low concentrations (2–5 wt.%) in the martian dust. The Spirit rover also identified an outcrop with 16 to 34 wt.% carbonate material in the Columbia Hills of Gusev Crater that strongly resembled the composition of carbonate found in martian meteorite ALH 84001. Finally, the Phoenix lander identified concentrations of 3–6 wt.% carbonate in the soils of the northern plains. The carbonates discovered to date do not clearly indicate the past presence of a dense Noachian atmosphere, but instead suggest localized hydrothermal aqueous environments with limited water availability that existed primarily in the early to mid-Noachian followed by low levels of carbonate formation from thin films of transient water from the late Noachian to the present. The prevalence of carbonate along with evidence for active carbonate precipitation suggests that a global acidic chemistry is unlikely and a more complex relationship between acidity and carbonate formation is present.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1007/s11214-012-9940-yDOIUNSPECIFIED
http://link.springer.com/article/10.1007%2Fs11214-012-9940-yPublisherUNSPECIFIED
ORCID:
AuthorORCID
Ehlmann, Bethany L.0000-0002-2745-3240
Sutter, Brad0000-0002-3036-170X
Additional Information:© 2012 US Government. Received: 20 January 2012; accepted: 29 September 2012; published online: 25 October 2012. Thoughtful reviews were provided by Ralph Harvey and Jim Bell which greatly improved the manuscript. Thanks to M. Toplis and the ISSI conference organizers for coordinating this review and promoting interesting discussions. E. Chassefière acknowledges support from CNRS EPOV interdisciplinary program.
Funders:
Funding AgencyGrant Number
CNRS EPOV interdisciplinary programUNSPECIFIED
Subject Keywords:Mars; Carbonate; Climate; CO2; Water; Meteorites; Spectroscopy; Acidity; Atmosphere
Issue or Number:1-4
DOI:10.1007/s11214-012-9940-y
Record Number:CaltechAUTHORS:20130131-095255817
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130131-095255817
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:36708
Collection:CaltechAUTHORS
Deposited By: Jason Perez
Deposited On:31 Jan 2013 21:14
Last Modified:09 Nov 2021 23:24

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