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Table · dataset · 2021

Replication Data for: Degradation of Small Simple and Large Complex Lunar Craters: Not a Simple Scale Dependence

Listed in TRR170-DB

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

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Where it is published

Catalogue records · 1

Topics

Provenance · 1 source records, 9 field assertions
SourceKeyLast seenRaw
TRR170-DBdoi:10.35003/C1K4CZ14 h agoJSON v1
FieldAssertionExtractorEvidence
concepts[field].dataverse_subject:astronomy-and-astrophysicssource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0/subjects
concepts[field].dataverse_subject:computer-and-information-sciencesource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0/subjects
concepts[field].local:field:astronomymapping · planetary data portal orgconnector:planetary_data_portal_org@1.0.0/subjects
created_datesource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0
descriptionsource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0/description
publication_datesource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0
titlesource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0/name
updated_datesource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0
version_labelsource · planetary data portal orgconnector:planetary_data_portal_org@1.0.0