dc.creator
Riedel, Christian
dc.creator
Minton, David A.
dc.creator
Michael, Gregory
dc.creator
Bogert, Carolyn H. van der
dc.creator
Hiesinger, Harald
dc.date.accessioned
2023-05-23T15:19:56Z
dc.date.available
2023-05-23T15:19:56Z
dc.identifier
https://doi.org/10.35003/C1K4CZ
dc.identifier.uri
https://refubium.fu-berlin.de/handle/fub188/39447
dc.identifier.uri
http://dx.doi.org/10.17169/refubium-39164
dc.description
• We model the surface evolution for a pre-Nectarian lunar surface unit• Relative to their size, large craters are less destructive to the surrounding terrain than small simple craters• A simple scale dependence from small to large craters does not explain the per-crater contribution to topographic diffusion of large craters
dc.subject
Astronomy and Astrophysics
dc.subject
Computer and Information Science
dc.subject
Surface evolution
dc.subject
Crater equilibrium
dc.title
Replication Data for: Degradation of Small Simple and Large Complex Lunar Craters: Not a Simple Scale Dependence
dcterms.accessRights.openaire
metadata only access
