Origin of acidic surface waters and the evolution of atmospheric chemistry on early Mars-Reference-Cited by-同舟云学术

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Origin of acidic surface waters and the evolution of atmospheric chemistry on early Mars

Published:2010-04-04 Issue:5 Volume:3 Page:323-326
ISSN:1752-0894
Container-title:Nature Geoscience
language:en
Short-container-title:Nature Geosci

Author:

Hurowitz Joel A.,Fischer Woodward W.,Tosca Nicholas J.,Milliken Ralph E.

Publisher

Springer Science and Business Media LLC

Subject

General Earth and Planetary Sciences

Link

http://www.nature.com/articles/ngeo831.pdf

Reference30 articles.

1. Grotzinger, J. P. et al. Stratigraphy and sedimentology of a dry to wet eolian depositional system, Burns formation, Meridiani Planum, Mars. Earth Planet. Sci. Lett. 240, 11–72 (2005).

2. Squyres, S. W. et al. Exploration of Victoria Crater by the Mars rover Opportunity. Science 324, 1058–1061 (2009).

3. McLennan, S. M. et al. Provenance and diagenesis of the evaporite-bearing Burns formation, Meridiani Planum, Mars. Earth Planet. Sci. Lett. 240, 95–121 (2005).

4. Tosca, N. J. et al. Geochemical modelling of evaporation processes on Mars: Insight from the sedimentary record at Meridiani Planum. Earth Planet. Sci. Lett. 240, 122–148 (2005).

5. Andrews-Hanna, J. C., Phillips, R. J. & Zuber, M. T. Meridiani Planum and the global hydrology of Mars. Nature 446, 163–166 (2007).

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