Eolian controlled modification of the martian south polar layered deposits

Data from the Mars Orbiter Laser Altimeter (MOLA) and Mars Orbiter Camera (MOC) aboard the Mars Global Surveyor (MGS) mission and the Thermal Emission Imaging System (THEMIS) aboard the Mars Odyssey mission have revealed unique surface features in a particular region of the South Polar Layered Depos...

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Published in:Icarus
Main Authors: Koutnik, Michelle R., Byrne, Shane, Murray, Bruce C., Toigo, Anthony D., Crawford, Zane A.
Format: Article in Journal/Newspaper
Language:unknown
Published: Elsevier 2005
Subjects:
Online Access:https://doi.org/10.1016/j.icarus.2004.09.015
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record_format openpolar
spelling ftcaltechauth:oai:authors.library.caltech.edu:r8k9n-zww83 2024-10-13T14:10:23+00:00 Eolian controlled modification of the martian south polar layered deposits Koutnik, Michelle R. Byrne, Shane Murray, Bruce C. Toigo, Anthony D. Crawford, Zane A. 2005-04 https://doi.org/10.1016/j.icarus.2004.09.015 unknown Elsevier https://doi.org/10.1016/j.icarus.2004.09.015 eprintid:44836 info:eu-repo/semantics/closedAccess Other Icarus, 174(2), 490-501, (2005-04) 3rd International Conference on Mars Polar Science and Exploration, Lake Louise, Canada, Oct. 13-17, 2003 Mars surface Ices Wind Polar info:eu-repo/semantics/article 2005 ftcaltechauth https://doi.org/10.1016/j.icarus.2004.09.015 2024-09-25T18:46:40Z Data from the Mars Orbiter Laser Altimeter (MOLA) and Mars Orbiter Camera (MOC) aboard the Mars Global Surveyor (MGS) mission and the Thermal Emission Imaging System (THEMIS) aboard the Mars Odyssey mission have revealed unique surface features in a particular region of the South Polar Layered Deposits (SPLD). The dominant morphology is large-scale quasi-parallel grooves that extend for hundreds of kilometers with only tens of meters of vertical relief, that we have termed here the "Wire Brush" terrain. The grooves are also transected by disjointed, yet roughly continuous, low-relief sinuous ridges that cross roughly perpendicular to the trend-direction of the large-scale grooves and show only tens of meters of relief. We interpret these ridges to be eroded remnants of folded layers. At the northern end of the large-scale grooves there are non-symmetric mounds. They are frequently preceded by a significant depression and/or trailing grooves that are parallel to the Wire Brush trend. We find that a two-stage process involving winds that intermittently remove a low-density crust exposing the underlying ice to ablation is the interpretation that best explains the multitude of features observed here. These features appear to be currently inactive indicating higher winds in previous epochs. © 2004 Elsevier Inc. Received 9 March 2004; revised 27 August 2004. We thank Oz Pathare (Caltech), Bernard Hallet (University of Washington), Eric Kolb (University of Arizona), and Ken Tanaka (USGS) for their contributions and useful discussions. We are grateful to Lori Fenton and an anonymous reviewer for detailed constructive reviews that greatly improved this manuscript. Article in Journal/Newspaper Polar Science Caltech Authors (California Institute of Technology) Fenton ENVELOPE(161.917,161.917,-74.333,-74.333) Hallet ENVELOPE(6.662,6.662,63.003,63.003) Icarus 174 2 490 501
institution Open Polar
collection Caltech Authors (California Institute of Technology)
op_collection_id ftcaltechauth
language unknown
topic Mars
surface
Ices
Wind
Polar
spellingShingle Mars
surface
Ices
Wind
Polar
Koutnik, Michelle R.
Byrne, Shane
Murray, Bruce C.
Toigo, Anthony D.
Crawford, Zane A.
Eolian controlled modification of the martian south polar layered deposits
topic_facet Mars
surface
Ices
Wind
Polar
description Data from the Mars Orbiter Laser Altimeter (MOLA) and Mars Orbiter Camera (MOC) aboard the Mars Global Surveyor (MGS) mission and the Thermal Emission Imaging System (THEMIS) aboard the Mars Odyssey mission have revealed unique surface features in a particular region of the South Polar Layered Deposits (SPLD). The dominant morphology is large-scale quasi-parallel grooves that extend for hundreds of kilometers with only tens of meters of vertical relief, that we have termed here the "Wire Brush" terrain. The grooves are also transected by disjointed, yet roughly continuous, low-relief sinuous ridges that cross roughly perpendicular to the trend-direction of the large-scale grooves and show only tens of meters of relief. We interpret these ridges to be eroded remnants of folded layers. At the northern end of the large-scale grooves there are non-symmetric mounds. They are frequently preceded by a significant depression and/or trailing grooves that are parallel to the Wire Brush trend. We find that a two-stage process involving winds that intermittently remove a low-density crust exposing the underlying ice to ablation is the interpretation that best explains the multitude of features observed here. These features appear to be currently inactive indicating higher winds in previous epochs. © 2004 Elsevier Inc. Received 9 March 2004; revised 27 August 2004. We thank Oz Pathare (Caltech), Bernard Hallet (University of Washington), Eric Kolb (University of Arizona), and Ken Tanaka (USGS) for their contributions and useful discussions. We are grateful to Lori Fenton and an anonymous reviewer for detailed constructive reviews that greatly improved this manuscript.
format Article in Journal/Newspaper
author Koutnik, Michelle R.
Byrne, Shane
Murray, Bruce C.
Toigo, Anthony D.
Crawford, Zane A.
author_facet Koutnik, Michelle R.
Byrne, Shane
Murray, Bruce C.
Toigo, Anthony D.
Crawford, Zane A.
author_sort Koutnik, Michelle R.
title Eolian controlled modification of the martian south polar layered deposits
title_short Eolian controlled modification of the martian south polar layered deposits
title_full Eolian controlled modification of the martian south polar layered deposits
title_fullStr Eolian controlled modification of the martian south polar layered deposits
title_full_unstemmed Eolian controlled modification of the martian south polar layered deposits
title_sort eolian controlled modification of the martian south polar layered deposits
publisher Elsevier
publishDate 2005
url https://doi.org/10.1016/j.icarus.2004.09.015
long_lat ENVELOPE(161.917,161.917,-74.333,-74.333)
ENVELOPE(6.662,6.662,63.003,63.003)
geographic Fenton
Hallet
geographic_facet Fenton
Hallet
genre Polar Science
genre_facet Polar Science
op_source Icarus, 174(2), 490-501, (2005-04)
3rd International Conference on Mars Polar Science and Exploration, Lake Louise, Canada, Oct. 13-17, 2003
op_relation https://doi.org/10.1016/j.icarus.2004.09.015
eprintid:44836
op_rights info:eu-repo/semantics/closedAccess
Other
op_doi https://doi.org/10.1016/j.icarus.2004.09.015
container_title Icarus
container_volume 174
container_issue 2
container_start_page 490
op_container_end_page 501
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