POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT

International audience Introduction: Here, we describe and evaluate: a) the presence and distribution in Utopia Planitia (UP), Mars (40-50 o N, 110-124 o E), of small-sized polygons , (10-25 m in diameter), with low centres (lcps) or high centres (hcps) relative to their margins; b) the spatial ,...

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Main Authors: Soare, R.J., Conway, Susan J., Mc Keown, L, E, Williams, J-P, Godin, E, Hawkswell, J
Other Authors: Dawson College, Laboratoire de Planétologie et Géodynamique UMR 6112 (LPG), Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST), Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Format: Conference Object
Language:English
Published: HAL CCSD 2019
Subjects:
Ice
Online Access:https://hal.science/hal-02396172
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spelling ftinsu:oai:HAL:hal-02396172v1 2023-11-12T04:14:05+01:00 POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT Soare, R.J. Conway, Susan J. Mc Keown, L, E Williams, J-P Godin, E Hawkswell, J Dawson College Laboratoire de Planétologie et Géodynamique UMR 6112 (LPG) Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST) Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS) The Woodlands, Texas, United States 2019-03 https://hal.science/hal-02396172 en eng HAL CCSD hal-02396172 https://hal.science/hal-02396172 50th Lunar and Planetary Science Conference https://hal.science/hal-02396172 50th Lunar and Planetary Science Conference, Mar 2019, The Woodlands, Texas, United States [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology info:eu-repo/semantics/conferenceObject Conference papers 2019 ftinsu 2023-11-01T17:26:56Z International audience Introduction: Here, we describe and evaluate: a) the presence and distribution in Utopia Planitia (UP), Mars (40-50 o N, 110-124 o E), of small-sized polygons , (10-25 m in diameter), with low centres (lcps) or high centres (hcps) relative to their margins; b) the spatial , perhaps periglacial, association of these polygons and thermokarst-like depressions or basins; and, c) statistical data that support the hypothesis that ice-wedges underlie lcp/hcp margins. LCPs/HCPs on Earth: Geographically-expansive complexes of ice-wedge polygons (be they lcps or hcps), thermokarst, thermokarst lakes and alases, i.e. thermokarst depressions of basins absent of water, are commonplace in the Tuktoyaktuk Coastlands (TC) of northern Canada and the Yamal peninsula (YP) of eastern Russia [1-4]. In these and similar arctic-regions sur-face/near-surface water is abundant, freeze-thaw cycling is ubiquitous and the permafrost is ice-rich to depth [1-4, Fig. 1]. Ice-rich permafrost comprises excess ice: "the volume of ice in the ground which exceeds the total pore-volume that the ground would have under natural unfro-zen-conditions" [5]. Ice lenses, veins, wedges or larger masses of consolidated ice are typical examples of excess ice [5]. Thermokarst comprises excess ice. This makes it particularly sensitive to volumetric inflation as ice ag-grades, when mean temperatures remain stable or fall, or volumetric deflation as ice degrades, when mean temperatures rise and meltwater is evacuated by drainage or evaporation from the thaw zone. Fig. 1. Near-surface ice and ice wedges at Peninsula Point, SW of Tuktoyaktuk: (a-c) recessional terraces resulting from thermal destabilisation of coastline. (d) Surface depressions above degrading ice-wedges; massive-ice exposures cen-tre/centre left. Image credit, R. Soare. Spatially-associated assemblages of lcps and hcps also are geological markers of climate change. Stable or falling mean-temperatures engender ice-wedge aggrad-ation and the uplift of polygon margins. ... Conference Object Arctic Climate change Ice permafrost Thermokarst wedge* Yamal Peninsula Institut national des sciences de l'Univers: HAL-INSU Arctic Canada Tuktoyaktuk ENVELOPE(-133.006,-133.006,69.425,69.425) Yamal Peninsula ENVELOPE(69.873,69.873,70.816,70.816)
institution Open Polar
collection Institut national des sciences de l'Univers: HAL-INSU
op_collection_id ftinsu
language English
topic [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology
spellingShingle [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology
Soare, R.J.
Conway, Susan J.
Mc Keown, L, E
Williams, J-P
Godin, E
Hawkswell, J
POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT
topic_facet [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology
description International audience Introduction: Here, we describe and evaluate: a) the presence and distribution in Utopia Planitia (UP), Mars (40-50 o N, 110-124 o E), of small-sized polygons , (10-25 m in diameter), with low centres (lcps) or high centres (hcps) relative to their margins; b) the spatial , perhaps periglacial, association of these polygons and thermokarst-like depressions or basins; and, c) statistical data that support the hypothesis that ice-wedges underlie lcp/hcp margins. LCPs/HCPs on Earth: Geographically-expansive complexes of ice-wedge polygons (be they lcps or hcps), thermokarst, thermokarst lakes and alases, i.e. thermokarst depressions of basins absent of water, are commonplace in the Tuktoyaktuk Coastlands (TC) of northern Canada and the Yamal peninsula (YP) of eastern Russia [1-4]. In these and similar arctic-regions sur-face/near-surface water is abundant, freeze-thaw cycling is ubiquitous and the permafrost is ice-rich to depth [1-4, Fig. 1]. Ice-rich permafrost comprises excess ice: "the volume of ice in the ground which exceeds the total pore-volume that the ground would have under natural unfro-zen-conditions" [5]. Ice lenses, veins, wedges or larger masses of consolidated ice are typical examples of excess ice [5]. Thermokarst comprises excess ice. This makes it particularly sensitive to volumetric inflation as ice ag-grades, when mean temperatures remain stable or fall, or volumetric deflation as ice degrades, when mean temperatures rise and meltwater is evacuated by drainage or evaporation from the thaw zone. Fig. 1. Near-surface ice and ice wedges at Peninsula Point, SW of Tuktoyaktuk: (a-c) recessional terraces resulting from thermal destabilisation of coastline. (d) Surface depressions above degrading ice-wedges; massive-ice exposures cen-tre/centre left. Image credit, R. Soare. Spatially-associated assemblages of lcps and hcps also are geological markers of climate change. Stable or falling mean-temperatures engender ice-wedge aggrad-ation and the uplift of polygon margins. ...
author2 Dawson College
Laboratoire de Planétologie et Géodynamique UMR 6112 (LPG)
Université d'Angers (UA)-Université de Nantes - UFR des Sciences et des Techniques (UN UFR ST)
Université de Nantes (UN)-Université de Nantes (UN)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
format Conference Object
author Soare, R.J.
Conway, Susan J.
Mc Keown, L, E
Williams, J-P
Godin, E
Hawkswell, J
author_facet Soare, R.J.
Conway, Susan J.
Mc Keown, L, E
Williams, J-P
Godin, E
Hawkswell, J
author_sort Soare, R.J.
title POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT
title_short POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT
title_full POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT
title_fullStr POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT
title_full_unstemmed POSSIBLE ICE-WEDGE POLYGONS IN UTOPIA PLANITIA, MARS, AND THEIR POLEWARD LATITUDINAL GRADIENT
title_sort possible ice-wedge polygons in utopia planitia, mars, and their poleward latitudinal gradient
publisher HAL CCSD
publishDate 2019
url https://hal.science/hal-02396172
op_coverage The Woodlands, Texas, United States
long_lat ENVELOPE(-133.006,-133.006,69.425,69.425)
ENVELOPE(69.873,69.873,70.816,70.816)
geographic Arctic
Canada
Tuktoyaktuk
Yamal Peninsula
geographic_facet Arctic
Canada
Tuktoyaktuk
Yamal Peninsula
genre Arctic
Climate change
Ice
permafrost
Thermokarst
wedge*
Yamal Peninsula
genre_facet Arctic
Climate change
Ice
permafrost
Thermokarst
wedge*
Yamal Peninsula
op_source 50th Lunar and Planetary Science Conference
https://hal.science/hal-02396172
50th Lunar and Planetary Science Conference, Mar 2019, The Woodlands, Texas, United States
op_relation hal-02396172
https://hal.science/hal-02396172
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