Title |
Orbital Identification of Carbonate-Bearing Rocks on Mars
|
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Published in |
Science, December 2008
|
DOI | 10.1126/science.1164759 |
Pubmed ID | |
Authors |
Bethany L. Ehlmann, John F. Mustard, Scott L. Murchie, Francois Poulet, Janice L. Bishop, Adrian J. Brown, Wendy M. Calvin, Roger N. Clark, David J. Des Marais, Ralph E. Milliken, Leah H. Roach, Ted L. Roush, Gregg A. Swayze, James J. Wray |
Abstract |
Geochemical models for Mars predict carbonate formation during aqueous alteration. Carbonate-bearing rocks had not previously been detected on Mars' surface, but Mars Reconnaissance Orbiter mapping reveals a regional rock layer with near-infrared spectral characteristics that are consistent with the presence of magnesium carbonate in the Nili Fossae region. The carbonate is closely associated with both phyllosilicate-bearing and olivine-rich rock units and probably formed during the Noachian or early Hesperian era from the alteration of olivine by either hydrothermal fluids or near-surface water. The presence of carbonate as well as accompanying clays suggests that waters were neutral to alkaline at the time of its formation and that acidic weathering, proposed to be characteristic of Hesperian Mars, did not destroy these carbonates and thus did not dominate all aqueous environments. |
Mendeley readers
Geographical breakdown
Country | Count | As % |
---|---|---|
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Germany | 2 | <1% |
France | 1 | <1% |
Italy | 1 | <1% |
Canada | 1 | <1% |
United Kingdom | 1 | <1% |
Belgium | 1 | <1% |
Mexico | 1 | <1% |
Unknown | 292 | 95% |
Demographic breakdown
Readers by professional status | Count | As % |
---|---|---|
Student > Ph. D. Student | 76 | 25% |
Researcher | 70 | 23% |
Student > Master | 34 | 11% |
Student > Bachelor | 30 | 10% |
Professor > Associate Professor | 17 | 6% |
Other | 36 | 12% |
Unknown | 44 | 14% |
Readers by discipline | Count | As % |
---|---|---|
Earth and Planetary Sciences | 155 | 50% |
Physics and Astronomy | 39 | 13% |
Agricultural and Biological Sciences | 16 | 5% |
Engineering | 11 | 4% |
Chemistry | 8 | 3% |
Other | 23 | 7% |
Unknown | 55 | 18% |