White Mars: A New Model for Mars' Surface and Atmosphere Based on CO2

By N. Hoffman. 2000

174 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Environmental Chemistry

View Paper: https://www.semanticscholar.org/paper/1d767b2bf14a9eeb4e189a9cb947b09d33ac6fae

How researchers see this paper

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In Astronomy and Astrophysics

1. Jonathan I. Lunine
2. Adam Burrows
3. Jon Fortney
4. J. D. Kirkpatrick
5. A. Burgasser

Citations in the corpus

• Liquid CO2 breakout and the formation of recent small gullies on Mars (2001, background): “However, we do not take as extreme a view as Hoffman [2000], who attributes all surface fluid activity on Mars to CO2.”
• Flow discharge and sediment transport models for estimating a minimum timescale of hydrological activity and channel and delta formation on Mars (2005, unknown): “…Goldspiel and Squyres , 1991; Irwin et al. , 2004], which is a vital piece of the past climate puzzle and may help to decide between scenarios ranging between a cold, dry and windy ‘‘white’’ Mars, and a warm, wet and wild ‘‘blue’’ Mars [ Hoffman , 2000; Baker , 2001] and the duration of such eras.”
• Signature of life on exoplanets: Can Darwin produce false positive detections? (2002, background): “The CO2 content is indeed supposed to have been much larger in the past (Kahn 1985; Pollack et al. 1987; Hoffman 2000).”