Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars
A broad pitted plain and an elongated low rise occur near the south pole of Mars between a region of major cavi (Cavi Angusti) and a regionally smooth and broad valley (Argentea Planum). Viking, Mars Global Surveyor (MGS), and Odyssey data reveal a densely pitted plain covering ∼6750 km^2, and con...
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ftcaltechauth:oai:authors.library.caltech.edu:xje0k-h7643 2024-06-23T07:53:51+00:00 Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars Dickson, James Head, James W. 2006-03 https://doi.org/10.1016/j.pss.2005.12.010 unknown Elsevier https://doi.org/10.1016/j.pss.2005.12.010 oai:authors.library.caltech.edu:xje0k-h7643 eprintid:72397 resolverid:CaltechAUTHORS:20161129-103258413 info:eu-repo/semantics/closedAccess Other Planetary and Space Science, 54(3), 251-272, (2006-03) Mars Dorsa Argentea Formation Glacial Lake Kettle Hole Polar processes info:eu-repo/semantics/article 2006 ftcaltechauth https://doi.org/10.1016/j.pss.2005.12.010 2024-06-12T03:04:27Z A broad pitted plain and an elongated low rise occur near the south pole of Mars between a region of major cavi (Cavi Angusti) and a regionally smooth and broad valley (Argentea Planum). Viking, Mars Global Surveyor (MGS), and Odyssey data reveal a densely pitted plain covering ∼6750 km^2, and containing >300 irregularly shaped, steep-walled and flat-floored depressions with a mean diameter of ∼3.5 km. At the southernmost (poleward) extent of this plain are 12 north/south trending linear valleys that are characterized by theater-shaped heads abutting a major cavi within Cavi Angusti. The pitted plain, which abuts Cavi Angusti to the southwest, is separated from the floor of Argentea Planum by a smooth, elongated low rise that extends parallel to the plain for ∼200 km. These unusual features are all found within the Hesperian-aged circumpolar Dorsa Argentea Formation, which has been interpreted by some workers to be an ice-rich glacier-related deposit. We interpret the pitted plain to represent the maximum northern extent of the Angusti lobe ice deposit. The pits are analogous in morphology and distribution to terrestrial kettle holes, which form from the melting of isolated ice-blocks surrounded and partly buried by sediment, to leave hollows. The linear valleys are consistent with sapping valleys formed from the release of an elevated groundwater table, fed by meltwater lakes. On the basis of these characteristics, relationships and analogs, we interpret the marginal facies to represent an ice-sheet/lake contact environment that existed during Hesperian time. © 2006 Elsevier Ltd. Received 6 January 2005; received in revised form 12 December 2005; accepted 14 December 2005. This work was partially supported by the NASA Mars Data Analysis Program, which is gratefully acknowledged. Thanks are extended to David R. Marchant for productive discussions about glacial landforms and processes and the geology of Cape Cod. Article in Journal/Newspaper Ice Sheet South pole Caltech Authors (California Institute of Technology) Broad Valley ENVELOPE(-57.869,-57.869,-63.526,-63.526) Glacial Lake ENVELOPE(-129.463,-129.463,58.259,58.259) South Pole Planetary and Space Science 54 3 251 272 |
institution |
Open Polar |
collection |
Caltech Authors (California Institute of Technology) |
op_collection_id |
ftcaltechauth |
language |
unknown |
topic |
Mars Dorsa Argentea Formation Glacial Lake Kettle Hole Polar processes |
spellingShingle |
Mars Dorsa Argentea Formation Glacial Lake Kettle Hole Polar processes Dickson, James Head, James W. Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars |
topic_facet |
Mars Dorsa Argentea Formation Glacial Lake Kettle Hole Polar processes |
description |
A broad pitted plain and an elongated low rise occur near the south pole of Mars between a region of major cavi (Cavi Angusti) and a regionally smooth and broad valley (Argentea Planum). Viking, Mars Global Surveyor (MGS), and Odyssey data reveal a densely pitted plain covering ∼6750 km^2, and containing >300 irregularly shaped, steep-walled and flat-floored depressions with a mean diameter of ∼3.5 km. At the southernmost (poleward) extent of this plain are 12 north/south trending linear valleys that are characterized by theater-shaped heads abutting a major cavi within Cavi Angusti. The pitted plain, which abuts Cavi Angusti to the southwest, is separated from the floor of Argentea Planum by a smooth, elongated low rise that extends parallel to the plain for ∼200 km. These unusual features are all found within the Hesperian-aged circumpolar Dorsa Argentea Formation, which has been interpreted by some workers to be an ice-rich glacier-related deposit. We interpret the pitted plain to represent the maximum northern extent of the Angusti lobe ice deposit. The pits are analogous in morphology and distribution to terrestrial kettle holes, which form from the melting of isolated ice-blocks surrounded and partly buried by sediment, to leave hollows. The linear valleys are consistent with sapping valleys formed from the release of an elevated groundwater table, fed by meltwater lakes. On the basis of these characteristics, relationships and analogs, we interpret the marginal facies to represent an ice-sheet/lake contact environment that existed during Hesperian time. © 2006 Elsevier Ltd. Received 6 January 2005; received in revised form 12 December 2005; accepted 14 December 2005. This work was partially supported by the NASA Mars Data Analysis Program, which is gratefully acknowledged. Thanks are extended to David R. Marchant for productive discussions about glacial landforms and processes and the geology of Cape Cod. |
format |
Article in Journal/Newspaper |
author |
Dickson, James Head, James W. |
author_facet |
Dickson, James Head, James W. |
author_sort |
Dickson, James |
title |
Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars |
title_short |
Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars |
title_full |
Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars |
title_fullStr |
Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars |
title_full_unstemmed |
Evidence for an Hesperian-aged South Circum-Polar Lake Margin Environment on Mars |
title_sort |
evidence for an hesperian-aged south circum-polar lake margin environment on mars |
publisher |
Elsevier |
publishDate |
2006 |
url |
https://doi.org/10.1016/j.pss.2005.12.010 |
long_lat |
ENVELOPE(-57.869,-57.869,-63.526,-63.526) ENVELOPE(-129.463,-129.463,58.259,58.259) |
geographic |
Broad Valley Glacial Lake South Pole |
geographic_facet |
Broad Valley Glacial Lake South Pole |
genre |
Ice Sheet South pole |
genre_facet |
Ice Sheet South pole |
op_source |
Planetary and Space Science, 54(3), 251-272, (2006-03) |
op_relation |
https://doi.org/10.1016/j.pss.2005.12.010 oai:authors.library.caltech.edu:xje0k-h7643 eprintid:72397 resolverid:CaltechAUTHORS:20161129-103258413 |
op_rights |
info:eu-repo/semantics/closedAccess Other |
op_doi |
https://doi.org/10.1016/j.pss.2005.12.010 |
container_title |
Planetary and Space Science |
container_volume |
54 |
container_issue |
3 |
container_start_page |
251 |
op_container_end_page |
272 |
_version_ |
1802645689683935232 |