Liquid CO2 breakout and the formation of recent small gullies on Mars
By D. Musselwhite, T. Swindle, Jonathan I. Lunine. 2001
148 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Environmental Chemistry
View Paper: https://www.semanticscholar.org/paper/1cf751851e32fc27236ede9319fa751388dcef19
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In Astronomy and Astrophysics
- Michael D. Smith
- Michael J. Wolff
- R. Haberle
- B. Cantor
- James F. Bell III
- R. Clancy
- A. S. McEwen
- M. Ravine
Citations in the corpus
- Context Camera Investigation on board the Mars Reconnaissance Orbiter (2007, background): “[15] A few hypotheses for the origin of the gullies center on release of subsurface CO2 [Musselwhite et al., 2001; Hoffman, 2002]; Stewart and Nimmo [2002] considered it unlikely that sufficient quantities of CO2 could be trapped beneath the surface.”
- Long-term monitoring of martian gully formation and evolution with MRO/HiRISE (2015, background): “Proposed water-free formation processes include dry mass wasting (Treiman, 2003; Shinbrot et al., 2004), liquid CO2 aquifers (Musselwhite et al., 2001), and avalanching or sublimation of seasonal CO2 frost (Hoffman, 2002; Ishii and Sasaki, 2004; Balme et al., 2006; Cedillo-Flores et al., 2011).”