Volcanic Outgassing of CO2 and H2O on Mars
By Matthias Grott, A. Morschhauser, Doris Breuer, Ernst Hauber. 2011
164 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics
View Paper: https://www.semanticscholar.org/paper/846365ed26f6753a42161f903612c8a0007cfdd1
How researchers see this paper
The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.
In Astronomy and Astrophysics
- R. Wordsworth
- Francois Forget
- Ehouarn Millour
- J. Leconte
- M. Gudel
- Jean-Baptiste Madeleine
- James W. Head III
- F. Gaillard
In Geophysics
- R. Wordsworth
- F. Gaillard
- Bruno Scaillet
- Matthias Grott
- A. Morschhauser
- Ernst Hauber
- J. Leconte
- L. Noack
Citations in the corpus
- Outgassing History and Escape of the Martian Atmosphere and Water Inventory (2015, background): “The solid and dashed lines show the rates obtained with parameterized thermochemical evolution models assuming a global melt layer and melt generation in localized, hot mantle plumes, respectively (Grott et al. 2011; Morschhauser et al. 2011).”
- The Climate of Early Mars (2016, background): “The outgassing of CO2 into the Martian atmosphere with time is a function of the rate of volcanic activity and the chemical composition of the mantle (Grott et al. 2011).”
- A theoretical framework for volcanic degassing chemistry in a comparative planetology perspective and implications for planetary atmospheres (2014, methodology): “atmospheric pressure versus time lines are calculated using (Grott et al., 2011), which remains a reasonable approximation for our purpose.”
- Comparison of “warm and wet” and “cold and icy” scenarios for early Mars in a 3‐D climate model (2015, background): “…of the maximum atmospheric CO2 pressure during the Noachian are of order 1-2 bar [Phillips et al., 2001; Kite et al., 2014], with one study [Grott et al., 2011] pointing to lower values (∼ 0.25 bar) based on outgassing models that incorporate the lower estimated oxygen fugacity of typical…”
- 3D modelling of the early Martian Climate under a denser CO2 atmosphere: Temperatures and CO2 ice clouds. (2012, methodology): “To refine these conclusions, Grott et al. (2011) combined the”
- Origin and evolution of the atmospheres of early Venus, Earth and Mars (2018, background): “Volcanos and impacts during the late heavy bombardment (e.g., Bottke et al. 2012) period resulted in the build-up of a secondary CO2 atmosphere with a surface partial pressure that reached several hundred mbar (Grott et al. 2011; Lammer et al. 2013).”