Martian flow features, moraine-like ridges, and gullies: Terrestrial analogs and interrelationships
Ridges that resemble terrestrial moraines are commonly visible at the foot of many mid-latitude crater walls in Mars Global Surveyor Mars Orbiter Camera images. These moraine-like ridges are often associated with hillside gullies, mantling material, and glacier-like flows, and are usually in contact...
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| Veröffentlicht in: | Icarus (New York, N.Y. 1962) N.Y. 1962), 2005-04, Vol.174 (2), p.321-335 |
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| container_title | Icarus (New York, N.Y. 1962) |
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| creator | Arfstrom, John Hartmann, William K. |
| description | Ridges that resemble terrestrial moraines are commonly visible at the foot of many mid-latitude crater walls in Mars Global Surveyor Mars Orbiter Camera images. These moraine-like ridges are often associated with hillside gullies, mantling material, and glacier-like flows, and are usually in contact with crater fill, suggesting possible interrelationships. We consider terrestrial glacier systems that may be analogs of martian moraine-like ridges and glacier-like flows and suggest that the formation of some gullies and crater fill is intimately tied to ice deposition, ice flow, and rock-glacier processes. Upper limits on age suggest the possibility that many of these features formed during the last, or last few, high obliquity cycles. |
| doi_str_mv | 10.1016/j.icarus.2004.05.026 |
| format | Article |
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Upper limits on age suggest the possibility that many of these features formed during the last, or last few, high obliquity cycles.</description><subject>Astronomy</subject><subject>Crater fill</subject><subject>Earth, ocean, space</subject><subject>Exact sciences and technology</subject><subject>Glaciers</subject><subject>Mars climate</subject><subject>Moraines</subject><subject>Recent gullies</subject><subject>Solar system</subject><issn>0019-1035</issn><issn>1090-2643</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2005</creationdate><recordtype>article</recordtype><recordid>eNqNkc-L1TAQx4Mo-Fz9Dzz0oidbZ5I2bTwIsuiusOJlPYdpOn3mmdc-k3bF_97Ut-BNhYGBmc_8_ArxHKFCQP36UHlHcU2VBKgraCqQ-oHYIRgopa7VQ7EDQFMiqOaxeJLSAQCazqidcJ8oLp6mYgzzj2JkWtbI6VVxnCP5icvgv3ER_bDfgjQNxX4NwXN6U9xyzOQSPYWcoDDv02_AT8uWCbT4eUpf_Sk9FY9GComf3fsL8eXD-9vL6_Lm89XHy3c3patNs5Qs25Z1P-ih6xQikdRkembsthuaHrUb0ZFyZgCnsR6yGY3GyL4dezTqQrw89z3F-fuad7NHnxyHQBPPa7KyU51ptPwniK1qQan6P0DZoFZtBusz6OKcUuTRnqI_UvxpEeymkT3Ys0Z208hCY7NGuezFfX9KjsIYaXI-_anVrYQGMHNvzxzn9915jjY5z5PjwUd2ix1m__dBvwASy6om</recordid><startdate>20050401</startdate><enddate>20050401</enddate><creator>Arfstrom, John</creator><creator>Hartmann, William K.</creator><general>Elsevier Inc</general><general>Elsevier</general><scope>IQODW</scope><scope>AAYXX</scope><scope>CITATION</scope><scope>7TG</scope><scope>KL.</scope><scope>8FD</scope><scope>H8D</scope><scope>L7M</scope></search><sort><creationdate>20050401</creationdate><title>Martian flow features, moraine-like ridges, and gullies: Terrestrial analogs and interrelationships</title><author>Arfstrom, John ; Hartmann, William K.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c495t-e277e6bd6d88311aa26a9bee1826435b16cf1ca3c9d0c614d14d961992b7fb193</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2005</creationdate><topic>Astronomy</topic><topic>Crater fill</topic><topic>Earth, ocean, space</topic><topic>Exact sciences and technology</topic><topic>Glaciers</topic><topic>Mars climate</topic><topic>Moraines</topic><topic>Recent gullies</topic><topic>Solar system</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Arfstrom, John</creatorcontrib><creatorcontrib>Hartmann, William K.</creatorcontrib><collection>Pascal-Francis</collection><collection>CrossRef</collection><collection>Meteorological & Geoastrophysical Abstracts</collection><collection>Meteorological & Geoastrophysical Abstracts - Academic</collection><collection>Technology Research Database</collection><collection>Aerospace Database</collection><collection>Advanced Technologies Database with Aerospace</collection><jtitle>Icarus (New York, N.Y. 1962)</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Arfstrom, John</au><au>Hartmann, William K.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Martian flow features, moraine-like ridges, and gullies: Terrestrial analogs and interrelationships</atitle><jtitle>Icarus (New York, N.Y. 1962)</jtitle><date>2005-04-01</date><risdate>2005</risdate><volume>174</volume><issue>2</issue><spage>321</spage><epage>335</epage><pages>321-335</pages><issn>0019-1035</issn><eissn>1090-2643</eissn><coden>ICRSA5</coden><abstract>Ridges that resemble terrestrial moraines are commonly visible at the foot of many mid-latitude crater walls in Mars Global Surveyor Mars Orbiter Camera images. 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| ispartof | Icarus (New York, N.Y. 1962), 2005-04, Vol.174 (2), p.321-335 |
| issn | 0019-1035 1090-2643 |
| language | eng |
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| source | Elsevier ScienceDirect Journals Complete |
| subjects | Astronomy Crater fill Earth, ocean, space Exact sciences and technology Glaciers Mars climate Moraines Recent gullies Solar system |
| title | Martian flow features, moraine-like ridges, and gullies: Terrestrial analogs and interrelationships |
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