Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures

Periglacial surface structures like ice wedge polygons and thermokarst depressions are widely distributed in Siberian permafrost landscapes. Features of comparable morphology occur also on the Martian surface, especially in mid-latitude regions. We present polygon structures and thermokarst phenomen...

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Bibliographic Details
Main Authors: Grosse, G., Hauber, E., van Gasselt, S., Reiss, D., Lanz, J., Schirrmeister, L.
Format: Conference Object
Language:unknown
Published: 2002
Subjects:
Ice
Online Access:http://elib.dlr.de/18515/
id ftdlr:oai:elib.dlr.de:18515
record_format openpolar
spelling ftdlr:oai:elib.dlr.de:18515 2023-05-15T14:25:33+02:00 Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures Grosse, G. Hauber, E. van Gasselt, S. Reiss, D. Lanz, J. Schirrmeister, L. 2002 http://elib.dlr.de/18515/ unknown Grosse, G. und Hauber, E. und van Gasselt, S. und Reiss, D. und Lanz, J. und Schirrmeister, L. (2002) Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures. Water in the Upper Martian Surface, Workshop, April 17-19, 2002, Potsdam. Institut für Weltraumsensorik und Planetenerkundung Konferenzbeitrag NonPeerReviewed 2002 ftdlr 2016-03-28T20:20:12Z Periglacial surface structures like ice wedge polygons and thermokarst depressions are widely distributed in Siberian permafrost landscapes. Features of comparable morphology occur also on the Martian surface, especially in mid-latitude regions. We present polygon structures and thermokarst phenomena of different shapes and sizes, which were observed within the last four years during several German-Russian expeditions in Northern Yakutia. The morphology of the structures is studied quantitatively by air-borne and satellite imagery. Additionally, the geological and hydrological conditions for the formation of the periglacial features are described. Similar quantitative analyses of Martian analogue features have been carried out in order to obtain information on the lithological and hydrological environment in which they formed. These structures are often situated close to the mouths of the large outflow channel systems on Mars. Therefore, it is assumed that water from the flood events that carved the outflow channels oozed away into the ground forming a permafrost layer. Depth and thickness of this layer is not known. A model derived from rampart crater data (see Costard & Kargel, Icarus 114, 1994) for the ice content in Acidalia Planitia, proposes a ground ice layer > 2500 m thick below a layer of fluvial sediments containing ice segregations ~ 940 - 1000 m thick. By comparing the results of both terrestrial and martian investigations we will try to draw conclusions for the genesis of the observed structures on Mars as well as the depth and thickness of the possible permafrost layer. Conference Object Arctic Arctic Ice permafrost Thermokarst wedge* Yakutia German Aerospace Center: elib - DLR electronic library Arctic
institution Open Polar
collection German Aerospace Center: elib - DLR electronic library
op_collection_id ftdlr
language unknown
topic Institut für Weltraumsensorik und Planetenerkundung
spellingShingle Institut für Weltraumsensorik und Planetenerkundung
Grosse, G.
Hauber, E.
van Gasselt, S.
Reiss, D.
Lanz, J.
Schirrmeister, L.
Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures
topic_facet Institut für Weltraumsensorik und Planetenerkundung
description Periglacial surface structures like ice wedge polygons and thermokarst depressions are widely distributed in Siberian permafrost landscapes. Features of comparable morphology occur also on the Martian surface, especially in mid-latitude regions. We present polygon structures and thermokarst phenomena of different shapes and sizes, which were observed within the last four years during several German-Russian expeditions in Northern Yakutia. The morphology of the structures is studied quantitatively by air-borne and satellite imagery. Additionally, the geological and hydrological conditions for the formation of the periglacial features are described. Similar quantitative analyses of Martian analogue features have been carried out in order to obtain information on the lithological and hydrological environment in which they formed. These structures are often situated close to the mouths of the large outflow channel systems on Mars. Therefore, it is assumed that water from the flood events that carved the outflow channels oozed away into the ground forming a permafrost layer. Depth and thickness of this layer is not known. A model derived from rampart crater data (see Costard & Kargel, Icarus 114, 1994) for the ice content in Acidalia Planitia, proposes a ground ice layer > 2500 m thick below a layer of fluvial sediments containing ice segregations ~ 940 - 1000 m thick. By comparing the results of both terrestrial and martian investigations we will try to draw conclusions for the genesis of the observed structures on Mars as well as the depth and thickness of the possible permafrost layer.
format Conference Object
author Grosse, G.
Hauber, E.
van Gasselt, S.
Reiss, D.
Lanz, J.
Schirrmeister, L.
author_facet Grosse, G.
Hauber, E.
van Gasselt, S.
Reiss, D.
Lanz, J.
Schirrmeister, L.
author_sort Grosse, G.
title Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures
title_short Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures
title_full Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures
title_fullStr Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures
title_full_unstemmed Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures
title_sort periglacial features on earth (siberian arctic) and possible martian analogues: quantitative morphology of patterned ground and thermokarst structures
publishDate 2002
url http://elib.dlr.de/18515/
geographic Arctic
geographic_facet Arctic
genre Arctic
Arctic
Ice
permafrost
Thermokarst
wedge*
Yakutia
genre_facet Arctic
Arctic
Ice
permafrost
Thermokarst
wedge*
Yakutia
op_relation Grosse, G. und Hauber, E. und van Gasselt, S. und Reiss, D. und Lanz, J. und Schirrmeister, L. (2002) Periglacial Features on Earth (Siberian Arctic) and Possible Martian Analogues: Quantitative Morphology of Patterned Ground and Thermokarst Structures. Water in the Upper Martian Surface, Workshop, April 17-19, 2002, Potsdam.
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