Impact‐induced hydrothermal activity on early Mars
By Oleg Abramov, D. Kring. 2005
283 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/2885ed28817ea03d01aab9472849d6b249f953e4
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
- Jean-Baptiste Madeleine
- B. Charnay
- James W. Head III
- S. Stewart
- Alberto G. Fairén
In Atmospheric Science
- R. Wordsworth
- Francois Forget
- Ehouarn Millour
- Jean-Baptiste Madeleine
- S. Stewart
- Alberto G. Fairén
- S. Schwenzer
- L. E. Senft
Citations in the corpus
- Impact-generated hydrothermal systems capable of forming phyllosilicates on Noachian Mars (2009, background): “As discussed in detail previously (Abramov and Kring, 2005), substantial volumes of these altered systems were available and suitable for biological activity if life existed on early Mars.”
- Exploration of hydrothermal targets on Mars (2007, background): “This period, often referred to as the Lunar Cataclysm, lasted 20 to 200 million years (Abramov and Kring, 2005; Strom et al., 2005), during which time hydrothermal heat generated by impact events may have exceeded that generated by volcanic activity (Kring, 2000).”
- Impact-generated hydrothermal systems on Earth and Mars (2013, background): “These observations are particularly important with respect to Mars, where the focus of impact-generated hydrothermal models has exclusively focused on crater interiors (e.g., Rathbun and Squyres, 2002; Abramov and Kring, 2005; Schwenzer and Kring, 2009).”
- Global modelling of the early Martian climate under a denser CO2 atmosphere: Water cycle and ice evolution (2012, background): “Such an approach could be particularly revealing in localised studies of cases where geothermal processes or residual heating due to impacts may have been important [e.g., Abramov and Kring, 2005].”
- Impact crater formation in icy layered terrains on Mars (2006, background): “Calculations show that the presence of a crater lake in the hydrothermal system will increase the amount of circulation but decrease the lifetime of the system (Abramov and Kring 2005).”