Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin

Chasma Australe, 500 km long and up to 80 km wide, is the most remarkable of the martian south pole erosional reentrants carved in the polar layered deposits. We have interpreted Chasma Australe erosional and depositional features as evidence for a flood origin, which we have reconstructed using a m...

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Published in:Icarus
Main Authors: Anguita, Francisco, Babín Vich, Rosa Blanca, Benito, Gerardo, Gómez Ortiz, David, Collado, Ana, Rice, James W.
Format: Article in Journal/Newspaper
Language:English
Published: Elsevier Science B.V., Amsterdam 2000
Subjects:
Online Access:https://eprints.ucm.es/id/eprint/25615/
https://eprints.ucm.es/id/eprint/25615/1/1-s2.0-S0019103599962942-01.pdf
http://www.journals.elsevier.com/icarus/
https://doi.org/10.1006/icar.1999.6294
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spelling ftunivcmadrid:oai:www.ucm.es:25615 2023-05-15T18:22:11+02:00 Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin Anguita, Francisco Babín Vich, Rosa Blanca Benito, Gerardo Gómez Ortiz, David Collado, Ana Rice, James W. 2000 application/pdf https://eprints.ucm.es/id/eprint/25615/ https://eprints.ucm.es/id/eprint/25615/1/1-s2.0-S0019103599962942-01.pdf http://www.journals.elsevier.com/icarus/ https://doi.org/10.1006/icar.1999.6294 en eng Elsevier Science B.V., Amsterdam https://eprints.ucm.es/id/eprint/25615/1/1-s2.0-S0019103599962942-01.pdf info:eu-repo/semantics/openAccess Geología info:eu-repo/semantics/article PeerReviewed 2000 ftunivcmadrid https://doi.org/10.1006/icar.1999.6294 2022-05-12T19:56:37Z Chasma Australe, 500 km long and up to 80 km wide, is the most remarkable of the martian south pole erosional reentrants carved in the polar layered deposits. We have interpreted Chasma Australe erosional and depositional features as evidence for a flood origin, which we have reconstructed using a modified Manning equation. The main characteristics of the flow are a water velocity between 30 and 50 m s¡1 and discharge values between 7 x 10^8 and 3 x 10^9 m3 s-1, very near to MGS data-based estimations for martian outflow channels (D. E. Smith et al. 1998, Science 279, 1686–1692). We thus postulate that Chasma Australe originated in a catastrophic flood. The tectonic study of an area (roughly 20 million km2 in size) around Mars’ south pole included the measurement and projection in rose diagrams of more than 300 lineaments, of which 85 were wrinkle ridges and the rest straight scarps. The whole set of lineaments can be explained by a stress field with a d1 N10ºE in strike, the wrinkle ridges being reverse faults and the other lineaments direct and strike-slip faults. The straight layout of parts of Chasma Australe almost 200 km long suggests that the chasma was carved following a fracture network. The effectiveness of the erosional process (the canyon is up to 1000 m deep) leads us to suspect that this carving was preceded by a sapping period. Endogenetic and exogenetic processes would thus have contributed to the origin of this landform Article in Journal/Newspaper South pole Universidad Complutense de Madrid (UCM): E-Prints Complutense South Pole Icarus 144 2 302 312
institution Open Polar
collection Universidad Complutense de Madrid (UCM): E-Prints Complutense
op_collection_id ftunivcmadrid
language English
topic Geología
spellingShingle Geología
Anguita, Francisco
Babín Vich, Rosa Blanca
Benito, Gerardo
Gómez Ortiz, David
Collado, Ana
Rice, James W.
Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin
topic_facet Geología
description Chasma Australe, 500 km long and up to 80 km wide, is the most remarkable of the martian south pole erosional reentrants carved in the polar layered deposits. We have interpreted Chasma Australe erosional and depositional features as evidence for a flood origin, which we have reconstructed using a modified Manning equation. The main characteristics of the flow are a water velocity between 30 and 50 m s¡1 and discharge values between 7 x 10^8 and 3 x 10^9 m3 s-1, very near to MGS data-based estimations for martian outflow channels (D. E. Smith et al. 1998, Science 279, 1686–1692). We thus postulate that Chasma Australe originated in a catastrophic flood. The tectonic study of an area (roughly 20 million km2 in size) around Mars’ south pole included the measurement and projection in rose diagrams of more than 300 lineaments, of which 85 were wrinkle ridges and the rest straight scarps. The whole set of lineaments can be explained by a stress field with a d1 N10ºE in strike, the wrinkle ridges being reverse faults and the other lineaments direct and strike-slip faults. The straight layout of parts of Chasma Australe almost 200 km long suggests that the chasma was carved following a fracture network. The effectiveness of the erosional process (the canyon is up to 1000 m deep) leads us to suspect that this carving was preceded by a sapping period. Endogenetic and exogenetic processes would thus have contributed to the origin of this landform
format Article in Journal/Newspaper
author Anguita, Francisco
Babín Vich, Rosa Blanca
Benito, Gerardo
Gómez Ortiz, David
Collado, Ana
Rice, James W.
author_facet Anguita, Francisco
Babín Vich, Rosa Blanca
Benito, Gerardo
Gómez Ortiz, David
Collado, Ana
Rice, James W.
author_sort Anguita, Francisco
title Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin
title_short Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin
title_full Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin
title_fullStr Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin
title_full_unstemmed Chasma Australe, Mars: Structural Framework for a Catastrophic Outflow Origin
title_sort chasma australe, mars: structural framework for a catastrophic outflow origin
publisher Elsevier Science B.V., Amsterdam
publishDate 2000
url https://eprints.ucm.es/id/eprint/25615/
https://eprints.ucm.es/id/eprint/25615/1/1-s2.0-S0019103599962942-01.pdf
http://www.journals.elsevier.com/icarus/
https://doi.org/10.1006/icar.1999.6294
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://eprints.ucm.es/id/eprint/25615/1/1-s2.0-S0019103599962942-01.pdf
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container_title Icarus
container_volume 144
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