Role of artesian groundwater in forming Martian permafrost features

Various landforms possibly related to formation (growth), movement, or decay of ground ice have been identified on Mars, including fretted terrain (ft) and associated lobate debris aprons (lda), the chaotic terrain, concentric crater fills (ccf), polygonal ground, softened terrain, small domes that...

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Bibliographic Details
Main Author: Howard, Alan D.
Format: Other/Unknown Material
Language:unknown
Published: 1991
Subjects:
Ice
Online Access:http://hdl.handle.net/2060/19920001553
id ftnasantrs:oai:casi.ntrs.nasa.gov:19920001553
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spelling ftnasantrs:oai:casi.ntrs.nasa.gov:19920001553 2023-05-15T16:36:52+02:00 Role of artesian groundwater in forming Martian permafrost features Howard, Alan D. Unclassified, Unlimited, Publicly available Jun 1, 1991 application/pdf http://hdl.handle.net/2060/19920001553 unknown Document ID: 19920001553 Accession ID: 92N10771 http://hdl.handle.net/2060/19920001553 No Copyright CASI LUNAR AND PLANETARY EXPLORATION NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1990; p 120-122 1991 ftnasantrs 2015-03-15T05:02:13Z Various landforms possibly related to formation (growth), movement, or decay of ground ice have been identified on Mars, including fretted terrain (ft) and associated lobate debris aprons (lda), the chaotic terrain, concentric crater fills (ccf), polygonal ground, softened terrain, small domes that are possibly pingos, and curvilinear (fingerprint) features (cuf). Glaciers may also have been present. Some of these may involve ice derived from artesian groundwater. Topical areas of discussion are: Mars groundwater and the location of permafrost features; the ft, lda, ccf, and cuf; role of artesian groundwater in formation of fretted terrain, lobate debris blankets, and concentric crater fills; sources of glacial ice; and pingos and other pseudovolcanic structures. Other/Unknown Material Ice permafrost NASA Technical Reports Server (NTRS)
institution Open Polar
collection NASA Technical Reports Server (NTRS)
op_collection_id ftnasantrs
language unknown
topic LUNAR AND PLANETARY EXPLORATION
spellingShingle LUNAR AND PLANETARY EXPLORATION
Howard, Alan D.
Role of artesian groundwater in forming Martian permafrost features
topic_facet LUNAR AND PLANETARY EXPLORATION
description Various landforms possibly related to formation (growth), movement, or decay of ground ice have been identified on Mars, including fretted terrain (ft) and associated lobate debris aprons (lda), the chaotic terrain, concentric crater fills (ccf), polygonal ground, softened terrain, small domes that are possibly pingos, and curvilinear (fingerprint) features (cuf). Glaciers may also have been present. Some of these may involve ice derived from artesian groundwater. Topical areas of discussion are: Mars groundwater and the location of permafrost features; the ft, lda, ccf, and cuf; role of artesian groundwater in formation of fretted terrain, lobate debris blankets, and concentric crater fills; sources of glacial ice; and pingos and other pseudovolcanic structures.
format Other/Unknown Material
author Howard, Alan D.
author_facet Howard, Alan D.
author_sort Howard, Alan D.
title Role of artesian groundwater in forming Martian permafrost features
title_short Role of artesian groundwater in forming Martian permafrost features
title_full Role of artesian groundwater in forming Martian permafrost features
title_fullStr Role of artesian groundwater in forming Martian permafrost features
title_full_unstemmed Role of artesian groundwater in forming Martian permafrost features
title_sort role of artesian groundwater in forming martian permafrost features
publishDate 1991
url http://hdl.handle.net/2060/19920001553
op_coverage Unclassified, Unlimited, Publicly available
genre Ice
permafrost
genre_facet Ice
permafrost
op_source CASI
op_relation Document ID: 19920001553
Accession ID: 92N10771
http://hdl.handle.net/2060/19920001553
op_rights No Copyright
_version_ 1766027188250869760