An Impactor Origin for Lunar Magnetic Anomalies

Bringing Magnetic Materials to the Moon The Apollo missions to the Moon revealed that portions of the lunar crust are strongly magnetized. Lunar rocks are poor at recording the magnetic field, thus these magnetic anomalies have been difficult to explain. Based on numerical simulations of large-scale...

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Published in:Science
Main Authors: Wieczorek, Mark A., Weiss, Benjamin P., Stewart, Sarah T.
Format: Article in Journal/Newspaper
Language:English
Published: American Association for the Advancement of Science (AAAS) 2012
Subjects:
Online Access:http://dx.doi.org/10.1126/science.1214773
https://www.science.org/doi/pdf/10.1126/science.1214773
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spelling craaas:10.1126/science.1214773 2024-06-23T07:56:49+00:00 An Impactor Origin for Lunar Magnetic Anomalies Wieczorek, Mark A. Weiss, Benjamin P. Stewart, Sarah T. 2012 http://dx.doi.org/10.1126/science.1214773 https://www.science.org/doi/pdf/10.1126/science.1214773 en eng American Association for the Advancement of Science (AAAS) Science volume 335, issue 6073, page 1212-1215 ISSN 0036-8075 1095-9203 journal-article 2012 craaas https://doi.org/10.1126/science.1214773 2024-06-13T04:01:03Z Bringing Magnetic Materials to the Moon The Apollo missions to the Moon revealed that portions of the lunar crust are strongly magnetized. Lunar rocks are poor at recording the magnetic field, thus these magnetic anomalies have been difficult to explain. Based on numerical simulations of large-scale impacts, Wieczorek et al. (p. 1212 see the Perspective by Collins ) show that the vast majority of lunar magnetic anomalies can be explained by highly magnetic materials that originated outside the Moon and were delivered by the asteroid that hit the Moon and formed the South Pole–Aitken basin, the largest impact basin in the solar system. Article in Journal/Newspaper South pole AAAS Resource Center (American Association for the Advancement of Science) Aitken ENVELOPE(-44.516,-44.516,-60.733,-60.733) South Pole Science 335 6073 1212 1215
institution Open Polar
collection AAAS Resource Center (American Association for the Advancement of Science)
op_collection_id craaas
language English
description Bringing Magnetic Materials to the Moon The Apollo missions to the Moon revealed that portions of the lunar crust are strongly magnetized. Lunar rocks are poor at recording the magnetic field, thus these magnetic anomalies have been difficult to explain. Based on numerical simulations of large-scale impacts, Wieczorek et al. (p. 1212 see the Perspective by Collins ) show that the vast majority of lunar magnetic anomalies can be explained by highly magnetic materials that originated outside the Moon and were delivered by the asteroid that hit the Moon and formed the South Pole–Aitken basin, the largest impact basin in the solar system.
format Article in Journal/Newspaper
author Wieczorek, Mark A.
Weiss, Benjamin P.
Stewart, Sarah T.
spellingShingle Wieczorek, Mark A.
Weiss, Benjamin P.
Stewart, Sarah T.
An Impactor Origin for Lunar Magnetic Anomalies
author_facet Wieczorek, Mark A.
Weiss, Benjamin P.
Stewart, Sarah T.
author_sort Wieczorek, Mark A.
title An Impactor Origin for Lunar Magnetic Anomalies
title_short An Impactor Origin for Lunar Magnetic Anomalies
title_full An Impactor Origin for Lunar Magnetic Anomalies
title_fullStr An Impactor Origin for Lunar Magnetic Anomalies
title_full_unstemmed An Impactor Origin for Lunar Magnetic Anomalies
title_sort impactor origin for lunar magnetic anomalies
publisher American Association for the Advancement of Science (AAAS)
publishDate 2012
url http://dx.doi.org/10.1126/science.1214773
https://www.science.org/doi/pdf/10.1126/science.1214773
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_source Science
volume 335, issue 6073, page 1212-1215
ISSN 0036-8075 1095-9203
op_doi https://doi.org/10.1126/science.1214773
container_title Science
container_volume 335
container_issue 6073
container_start_page 1212
op_container_end_page 1215
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