Aeolian abrasion of rocks as a mechanism to produce methane in the Martian atmosphere
Author:
Publisher
Springer Science and Business Media LLC
Subject
Multidisciplinary
Link
http://www.nature.com/articles/s41598-019-44616-2.pdf
Reference40 articles.
1. Webster, C. R. et al. Background levels of methane in Mars’ atmosphere show strong seasonal variations. Science 360, 1093–1096 (2018).
2. Webster, C. R. et al. Mars methane detection and variability at Gale crater. Science 347, 415–417 (2015).
3. Mumma, M. J. et al. Strong Release of Methane on Mars in Northern Summer 2003. Science 323, 1041–1045 (2009).
4. Moores, J. E. & Schuerger, A. C. UV degradation of accreted organics on Mars: IDP longevity, surface reservoir of organics, and relevance to the detection of methane in the atmosphere. Journal of Geophysical Research: Planets 117, E8 (2012).
5. Schuerger, A. C. et al. Methane from UV‐irradiated carbonaceous chondrites under simulated Martian conditions. Journal of Geophysical Research: Planets 117, E8 (2012).
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1. Advective Fluxes in the Martian Regolith as a Mechanism Driving Methane and Other Trace Gas Emissions to the Atmosphere;Geophysical Research Letters;2020-02-03
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