dc.creator
Potter, R.W.K.
dc.creator
Morbidelli, A.
dc.date.accessioned
2023-05-23T15:21:23Z
dc.date.available
2023-05-23T15:21:23Z
dc.identifier
https://doi.org/10.35003/ZUBECS
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/39506
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-39224
dc.description
•Giant impact on the nearside of the Moon can reproduce the crustal thickness asymmetry between the nearside and farside
•The nearside lowlands and KREEP materials on the lunar surface can be explained by the giant impact scenario
•Giant impact predicts that the Moon has a significant 182W anomaly after the Moon formation, as expected by the collision formation of the Moon
dc.relation
The GRAIL crustal thickness data can be accessed online via the GRAIL Crustal Thickness Archive (http://www.ipgp.fr/~wieczor/).
dc.subject
Astronomy and Astrophysics
dc.subject
Crustal thickness asymmetry
dc.title
Replication Data for: Are the Moon's Nearside‐Farside Asymmetries the Result of a Giant Impact ?
dcterms.accessRights.openaire
metadata only access
