New maximum constraints on the era of martian valley network formation

Author:

Morgan Alexander M.ORCID

Publisher

Elsevier BV

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference61 articles.

1. Amazonian-aged fluvial system and associated ice-related features in Terra Cimmeria, Mars;Adeli;Icarus,2016

2. Bahia, R.S., Bohacek, E.V., Braat, L., et al., 2023. A major missing component – aeolian-fluvial interaction on ancient Mars. 54th Lunar and Planetary Science Conference, Abstract 1193.

3. Implications of the shear stress river incision model for the timescale of postorogenic decay of topography;Baldwin;J. Geophys. Res. Solid Earth,2003

4. The dual nature of the martian crust: young lavas and old clastic materials;Bandfield;Icarus,2013

5. Long-term precipitation and late-stage valley network formation: landform simulations of Parana Basin, Mars;Barnhart;J. Geophys. Res. E Planets,2009

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