Global tectonic patterns of the Moon

Planetary tectonics provide a record of the myriad of processes that shape planetary surfaces and interiors. While there is a long history of mapping and modeling planetary tectonics, stresses from disparate processes are not generally captured by a single model. We present a comprehensive and gener...

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Published in:Icarus
Main Authors: Matsuyama, I., Keane, J. T., Trinh, A., Beuthe, M., Watters, T. R.
Format: Article in Journal/Newspaper
Language:English
Published: Elsevier 2021
Subjects:
Online Access:https://authors.library.caltech.edu/108403/
https://authors.library.caltech.edu/108403/1/1-s2.0-S0019103520305364-main.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20210311-133741100
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spelling ftcaltechauth:oai:authors.library.caltech.edu:108403 2023-05-15T18:22:48+02:00 Global tectonic patterns of the Moon Matsuyama, I. Keane, J. T. Trinh, A. Beuthe, M. Watters, T. R. 2021-04 application/pdf https://authors.library.caltech.edu/108403/ https://authors.library.caltech.edu/108403/1/1-s2.0-S0019103520305364-main.pdf https://resolver.caltech.edu/CaltechAUTHORS:20210311-133741100 en eng Elsevier https://authors.library.caltech.edu/108403/1/1-s2.0-S0019103520305364-main.pdf Matsuyama, I. and Keane, J. T. and Trinh, A. and Beuthe, M. and Watters, T. R. (2021) Global tectonic patterns of the Moon. Icarus, 358 . Art. No. 114202. ISSN 0019-1035. doi:10.1016/j.icarus.2020.114202. https://resolver.caltech.edu/CaltechAUTHORS:20210311-133741100 <https://resolver.caltech.edu/CaltechAUTHORS:20210311-133741100> other Article PeerReviewed 2021 ftcaltechauth https://doi.org/10.1016/j.icarus.2020.114202 2021-11-18T19:04:27Z Planetary tectonics provide a record of the myriad of processes that shape planetary surfaces and interiors. While there is a long history of mapping and modeling planetary tectonics, stresses from disparate processes are not generally captured by a single model. We present a comprehensive and general stress and tectonics model that can consider multiple stress-generating mechanisms simultaneously. The model is applicable to mass loading with arbitrary geometry, rotational and orbital perturbations, and arbitrary elastic lithosphere thicknesses. This wholistic approach to tectonic modeling has important implications for understanding both lunar evolution and tectonics across the solar system. We apply this model to the Moon, which exhibits a global pattern of thrust faults. The ubiquitous presence of young thrust faults suggests that isotropic contraction plays a dominant role. However, their non-random orientation requires additional stress-generating mechanisms that are not isotropic. Best-fit solutions correspond to models combining isotropic contraction with orbit recession, despinning, and South Pole-Aitken ejecta loading and the corresponding true polar wander. Contraction and despinning assuming an elastic shell with a thinner equatorial region can lead to misfits that are smaller than those assuming a constant thickness elastic shell. The young age of the faults favors recent contraction and recession; however, unrelaxed stresses from older processes combined with recent contractional stresses can also generate young faults. This possibility is supported by the Moon's ability to preserve a fossil figure. Article in Journal/Newspaper South pole Caltech Authors (California Institute of Technology) Aitken ENVELOPE(-44.516,-44.516,-60.733,-60.733) South Pole Icarus 358 114202
institution Open Polar
collection Caltech Authors (California Institute of Technology)
op_collection_id ftcaltechauth
language English
description Planetary tectonics provide a record of the myriad of processes that shape planetary surfaces and interiors. While there is a long history of mapping and modeling planetary tectonics, stresses from disparate processes are not generally captured by a single model. We present a comprehensive and general stress and tectonics model that can consider multiple stress-generating mechanisms simultaneously. The model is applicable to mass loading with arbitrary geometry, rotational and orbital perturbations, and arbitrary elastic lithosphere thicknesses. This wholistic approach to tectonic modeling has important implications for understanding both lunar evolution and tectonics across the solar system. We apply this model to the Moon, which exhibits a global pattern of thrust faults. The ubiquitous presence of young thrust faults suggests that isotropic contraction plays a dominant role. However, their non-random orientation requires additional stress-generating mechanisms that are not isotropic. Best-fit solutions correspond to models combining isotropic contraction with orbit recession, despinning, and South Pole-Aitken ejecta loading and the corresponding true polar wander. Contraction and despinning assuming an elastic shell with a thinner equatorial region can lead to misfits that are smaller than those assuming a constant thickness elastic shell. The young age of the faults favors recent contraction and recession; however, unrelaxed stresses from older processes combined with recent contractional stresses can also generate young faults. This possibility is supported by the Moon's ability to preserve a fossil figure.
format Article in Journal/Newspaper
author Matsuyama, I.
Keane, J. T.
Trinh, A.
Beuthe, M.
Watters, T. R.
spellingShingle Matsuyama, I.
Keane, J. T.
Trinh, A.
Beuthe, M.
Watters, T. R.
Global tectonic patterns of the Moon
author_facet Matsuyama, I.
Keane, J. T.
Trinh, A.
Beuthe, M.
Watters, T. R.
author_sort Matsuyama, I.
title Global tectonic patterns of the Moon
title_short Global tectonic patterns of the Moon
title_full Global tectonic patterns of the Moon
title_fullStr Global tectonic patterns of the Moon
title_full_unstemmed Global tectonic patterns of the Moon
title_sort global tectonic patterns of the moon
publisher Elsevier
publishDate 2021
url https://authors.library.caltech.edu/108403/
https://authors.library.caltech.edu/108403/1/1-s2.0-S0019103520305364-main.pdf
https://resolver.caltech.edu/CaltechAUTHORS:20210311-133741100
long_lat ENVELOPE(-44.516,-44.516,-60.733,-60.733)
geographic Aitken
South Pole
geographic_facet Aitken
South Pole
genre South pole
genre_facet South pole
op_relation https://authors.library.caltech.edu/108403/1/1-s2.0-S0019103520305364-main.pdf
Matsuyama, I. and Keane, J. T. and Trinh, A. and Beuthe, M. and Watters, T. R. (2021) Global tectonic patterns of the Moon. Icarus, 358 . Art. No. 114202. ISSN 0019-1035. doi:10.1016/j.icarus.2020.114202. https://resolver.caltech.edu/CaltechAUTHORS:20210311-133741100 <https://resolver.caltech.edu/CaltechAUTHORS:20210311-133741100>
op_rights other
op_doi https://doi.org/10.1016/j.icarus.2020.114202
container_title Icarus
container_volume 358
container_start_page 114202
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