Localized erosion at the edge of crater floors may be caused by hydrothermal alteration due to focusing of fluid flow around an impact melt sheet following crater formation, coupled with hydrothermal self-sealing under the center of the crater. Additional information is contained in the original extended abstract.
Central Remnant Craters on Mars - Localization of Hydrothermal Alteration at the Edge of Crater Floors?
2001-01-01
Conference paper
No indication
English
Photometric properties of lunar crater floors
TIBKAT | 1964
|British Library Conference Proceedings | 1996
|NTRS | 1965
|How Cold are the Floors of Lunar Polar Shadowed Craters?
NTRS | 2010
|