dc.date.accessioned
2023-05-23T15:19:55Z
dc.date.available
2023-05-23T15:19:55Z
dc.identifier
https://doi.org/10.35003/AVDEXW
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/39441
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-39158
dc.description
• We present 3D evolution models of the Moon coupled to its early bombardment history.
• Thermal anomalies induced by impacts on the Moon decay within 100–200 Myrs.
• Ejecta deposits modify surface heat flux even on long timescales.
• Surface insulation may maintain bombardment-induced anomalies until present.
• Impact bombardment may alter lunar contraction history.
dc.subject
Computer and Information Science
dc.subject
internal evolution
dc.subject
mantle convection
dc.subject
Impact processes
dc.title
Replication Data for: The role of impact bombardment history in lunar evolution
dcterms.accessRights.openaire
metadata only access
