Potential anomalies on a sphere: Applications to the thickness of the lunar crust

International audience A new technique for calculating potential anomalies on a sphere due to finite amplitude relie f has been developed. We show that by raising the topography to the nth power and expanding this field into spherical h annonics, potential anomalies due to topography on spherical de...

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Published in:Journal of Geophysical Research: Planets
Main Authors: Phillips, Roger, Wieczorek, Mark
Other Authors: Washington University in Saint Louis (WUSTL)
Format: Article in Journal/Newspaper
Language:English
Published: HAL CCSD 1998
Subjects:
Online Access:https://hal.archives-ouvertes.fr/hal-02458509
https://hal.archives-ouvertes.fr/hal-02458509/document
https://hal.archives-ouvertes.fr/hal-02458509/file/Wieczorek%20and%20Phillips%201998.pdf
https://doi.org/10.1029/97JE03136
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spelling ftccsdartic:oai:HAL:hal-02458509v1 2023-05-15T18:22:54+02:00 Potential anomalies on a sphere: Applications to the thickness of the lunar crust Phillips, Roger Wieczorek, Mark Washington University in Saint Louis (WUSTL) 1998 https://hal.archives-ouvertes.fr/hal-02458509 https://hal.archives-ouvertes.fr/hal-02458509/document https://hal.archives-ouvertes.fr/hal-02458509/file/Wieczorek%20and%20Phillips%201998.pdf https://doi.org/10.1029/97JE03136 en eng HAL CCSD Wiley-Blackwell info:eu-repo/semantics/altIdentifier/doi/10.1029/97JE03136 hal-02458509 https://hal.archives-ouvertes.fr/hal-02458509 https://hal.archives-ouvertes.fr/hal-02458509/document https://hal.archives-ouvertes.fr/hal-02458509/file/Wieczorek%20and%20Phillips%201998.pdf doi:10.1029/97JE03136 info:eu-repo/semantics/OpenAccess ISSN: 2169-9097 EISSN: 2169-9100 Journal of Geophysical Research. Planets https://hal.archives-ouvertes.fr/hal-02458509 Journal of Geophysical Research. Planets, Wiley-Blackwell, 1998, 103 (E1), pp.1715-1724. ⟨10.1029/97JE03136⟩ [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology info:eu-repo/semantics/article Journal articles 1998 ftccsdartic https://doi.org/10.1029/97JE03136 2021-12-12T01:24:44Z International audience A new technique for calculating potential anomalies on a sphere due to finite amplitude relie f has been developed. We show that by raising the topography to the nth power and expanding this field into spherical h annonics, potential anomalies due to topography on spherical density interfaces can be computed to arbitrary p recision. U sing a filter for downward continuing the Bouguer anomaly, we have computed a variety of crustal thickness maps for the Moon, assuining both a homogeneous as well as a dual-layered crust. The crustal thickness maps for the homogeneous model give plausible results, but this model is nor consistent with the seismic data, petrologi.c evidence, and geoid to topography ratios, all of which suggest some form of crustal stratification. Several dual-layered models were investigated, and it was found that only models with both upper and lower c rustal thickness variations could satisfy the gravity and topography data. These models predict that the entire upper crust has been excavat ed beneath the major nearside multiring b as itis. Additiona lly, significant amounts of lower crusta l material was excavated from these basins, especially beneath Crisium. T his m odel also predicts that mantle material should not have been excavated during the South-Pole A itken basin forming event, and that lower crus tal material should be exposed at the surface in this basin. Article in Journal/Newspaper South pole Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe) South Pole Journal of Geophysical Research: Planets 103 E1 1715 1724
institution Open Polar
collection Archive ouverte HAL (Hyper Article en Ligne, CCSD - Centre pour la Communication Scientifique Directe)
op_collection_id ftccsdartic
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
Phillips, Roger
Wieczorek, Mark
Potential anomalies on a sphere: Applications to the thickness of the lunar crust
topic_facet [SDU.STU.PL]Sciences of the Universe [physics]/Earth Sciences/Planetology
description International audience A new technique for calculating potential anomalies on a sphere due to finite amplitude relie f has been developed. We show that by raising the topography to the nth power and expanding this field into spherical h annonics, potential anomalies due to topography on spherical density interfaces can be computed to arbitrary p recision. U sing a filter for downward continuing the Bouguer anomaly, we have computed a variety of crustal thickness maps for the Moon, assuining both a homogeneous as well as a dual-layered crust. The crustal thickness maps for the homogeneous model give plausible results, but this model is nor consistent with the seismic data, petrologi.c evidence, and geoid to topography ratios, all of which suggest some form of crustal stratification. Several dual-layered models were investigated, and it was found that only models with both upper and lower c rustal thickness variations could satisfy the gravity and topography data. These models predict that the entire upper crust has been excavat ed beneath the major nearside multiring b as itis. Additiona lly, significant amounts of lower crusta l material was excavated from these basins, especially beneath Crisium. T his m odel also predicts that mantle material should not have been excavated during the South-Pole A itken basin forming event, and that lower crus tal material should be exposed at the surface in this basin.
author2 Washington University in Saint Louis (WUSTL)
format Article in Journal/Newspaper
author Phillips, Roger
Wieczorek, Mark
author_facet Phillips, Roger
Wieczorek, Mark
author_sort Phillips, Roger
title Potential anomalies on a sphere: Applications to the thickness of the lunar crust
title_short Potential anomalies on a sphere: Applications to the thickness of the lunar crust
title_full Potential anomalies on a sphere: Applications to the thickness of the lunar crust
title_fullStr Potential anomalies on a sphere: Applications to the thickness of the lunar crust
title_full_unstemmed Potential anomalies on a sphere: Applications to the thickness of the lunar crust
title_sort potential anomalies on a sphere: applications to the thickness of the lunar crust
publisher HAL CCSD
publishDate 1998
url https://hal.archives-ouvertes.fr/hal-02458509
https://hal.archives-ouvertes.fr/hal-02458509/document
https://hal.archives-ouvertes.fr/hal-02458509/file/Wieczorek%20and%20Phillips%201998.pdf
https://doi.org/10.1029/97JE03136
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source ISSN: 2169-9097
EISSN: 2169-9100
Journal of Geophysical Research. Planets
https://hal.archives-ouvertes.fr/hal-02458509
Journal of Geophysical Research. Planets, Wiley-Blackwell, 1998, 103 (E1), pp.1715-1724. ⟨10.1029/97JE03136⟩
op_relation info:eu-repo/semantics/altIdentifier/doi/10.1029/97JE03136
hal-02458509
https://hal.archives-ouvertes.fr/hal-02458509
https://hal.archives-ouvertes.fr/hal-02458509/document
https://hal.archives-ouvertes.fr/hal-02458509/file/Wieczorek%20and%20Phillips%201998.pdf
doi:10.1029/97JE03136
op_rights info:eu-repo/semantics/OpenAccess
op_doi https://doi.org/10.1029/97JE03136
container_title Journal of Geophysical Research: Planets
container_volume 103
container_issue E1
container_start_page 1715
op_container_end_page 1724
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