dc.date.accessioned
2023-05-23T15:21:16Z
dc.date.available
2023-05-23T15:21:16Z
dc.identifier
https://doi.org/10.35003/MCI3M3
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/39470
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-39188
dc.description
• We provide relationships between impactor size, gravity signal and farside basin size as a function of cooling history and formation time;
• Gravity anomalies serve as a measure of basin size as impacts altered morphology and crustal thickness models simplify subsurface structure;
• Our basin formation models agree with the assumed formation time based on crater chronology and the estimated cooling history of the Moon.
dc.subject
Astronomy and Astrophysics
dc.subject
Computer and Information Science
dc.title
Replication Data for: Numerical investigation of lunar basin formation constrained by gravity signature
dcterms.accessRights.openaire
metadata only access
