Regional variations in the stability and diffusion of water-ice in the Martian regolith
Geologic evidence suggests subsurface water-ice has played an important role in the formation of Martian landforms. Forms of mass-wasting such as debris aprons and flow patterns on valley floors suggest creep deformation of ice-laden soil, while thermokarst and chaotic terrain suggest once extensive...
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1992
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ftnasantrs:oai:casi.ntrs.nasa.gov:19920019799 2023-05-15T18:32:57+02:00 Regional variations in the stability and diffusion of water-ice in the Martian regolith Mellon, Michael T. Jakosky, Bruce M. Unclassified, Unlimited, Publicly available JAN 1, 1992 http://ntrs.nasa.gov/search.jsp?R=19920019799 unknown http://ntrs.nasa.gov/search.jsp?R=19920019799 Accession ID: 92N29042 No Copyright CASI 91 Lunar and Planetary Inst., Workshop on the Martian Surface and Atmosphere Through Time; p 105-106 1992 ftnasantrs 2012-02-15T19:21:29Z Geologic evidence suggests subsurface water-ice has played an important role in the formation of Martian landforms. Forms of mass-wasting such as debris aprons and flow patterns on valley floors suggest creep deformation of ice-laden soil, while thermokarst and chaotic terrain suggest once extensive deposits of ground ice that were later removed. The global distribution of ice-related morphology was mapped. The mapping showed regional variation, in both latitude and longitude, in the distribution of debris aprons, concentric fill craters, and 'softened' crater profiles. Other/Unknown Material Thermokarst NASA Technical Reports Server (NTRS) |
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Open Polar |
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NASA Technical Reports Server (NTRS) |
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ftnasantrs |
language |
unknown |
topic |
91 |
spellingShingle |
91 Mellon, Michael T. Jakosky, Bruce M. Regional variations in the stability and diffusion of water-ice in the Martian regolith |
topic_facet |
91 |
description |
Geologic evidence suggests subsurface water-ice has played an important role in the formation of Martian landforms. Forms of mass-wasting such as debris aprons and flow patterns on valley floors suggest creep deformation of ice-laden soil, while thermokarst and chaotic terrain suggest once extensive deposits of ground ice that were later removed. The global distribution of ice-related morphology was mapped. The mapping showed regional variation, in both latitude and longitude, in the distribution of debris aprons, concentric fill craters, and 'softened' crater profiles. |
format |
Other/Unknown Material |
author |
Mellon, Michael T. Jakosky, Bruce M. |
author_facet |
Mellon, Michael T. Jakosky, Bruce M. |
author_sort |
Mellon, Michael T. |
title |
Regional variations in the stability and diffusion of water-ice in the Martian regolith |
title_short |
Regional variations in the stability and diffusion of water-ice in the Martian regolith |
title_full |
Regional variations in the stability and diffusion of water-ice in the Martian regolith |
title_fullStr |
Regional variations in the stability and diffusion of water-ice in the Martian regolith |
title_full_unstemmed |
Regional variations in the stability and diffusion of water-ice in the Martian regolith |
title_sort |
regional variations in the stability and diffusion of water-ice in the martian regolith |
publishDate |
1992 |
url |
http://ntrs.nasa.gov/search.jsp?R=19920019799 |
op_coverage |
Unclassified, Unlimited, Publicly available |
genre |
Thermokarst |
genre_facet |
Thermokarst |
op_source |
CASI |
op_relation |
http://ntrs.nasa.gov/search.jsp?R=19920019799 Accession ID: 92N29042 |
op_rights |
No Copyright |
_version_ |
1766217173055832064 |