Channels and valleys on Mars: cold climate features formed as a result of a thickening cryosphere
- 1 November 1996
- journal article
- Published by Elsevier in Planetary and Space Science
- Vol. 44 (11) , 1411-1423
- https://doi.org/10.1016/s0032-0633(96)00053-0
Abstract
No abstract availableThis publication has 33 references indexed in Scilit:
- Evolution of water reservoirs on Mars from D/H ratios in the atmosphere and crustNature, 1995
- Evidence, Age, and Thickness of a Frozen Paleolake in Utopia Planitia, MarsIcarus, 1994
- Earth and Mars: Water inventories as clues to accretional historiesIcarus, 1992
- Water in SNC Meteorites: Evidence for a Martian HydrosphereScience, 1992
- Ancient aqueous sedimentation on MarsIcarus, 1991
- Magnitude of a catastrophic flood event at Kasei Valles, MarsGeology, 1990
- Polygenic eruptions on Alba Patera, MarsBulletin of Volcanology, 1988
- HDO in the Martian atmosphere: Implications for the abundance of crustal waterIcarus, 1988
- Deuterium on Mars: The Abundance of HDO and the Value of D/HScience, 1988
- Martian Valleys: Morphology, Distribution, Age, and OriginScience, 1980