Large impact crater histories of Mars: The effect of different model crater age techniques
By Stuart J. Robbins, B. Hynek, R. Lillis, William Bottke. 2013
145 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Atmospheric Science
View Paper: https://www.semanticscholar.org/paper/92617da8ca302c53e18e3c61ce245083298e79f0
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In Astronomy and Astrophysics
In Atmospheric Science
Citations in the corpus
- Origin and evolution of the atmospheres of early Venus, Earth and Mars (2018, background): “Maybe Mars had once a short period of proto-plate tectonics (Frey 2006; Yin 2012), but this most likely stopped during the pre-Noachian period together with the Martian magnetic dynamo (Dehant et al. 2007, and references therein; Lillis et al. 2008, 2013; Robbins et al. 2013).”
- Geologic Constraints on Early Mars Climate (2018, background): “The Early/Middle Noachian may be the most erosive time in Mars history – with 1 km of column-averaged sediment transport inferred (Robbins et al. 2013, Irwin et al. 2013).”