Smythii basin topography and comparisons with Orientale

dc.contributor.authorStrain, Priscilla L.
dc.contributor.authorEl-Baz, Farouk
dc.date.accessioned2008-10-28T18:01:57Z
dc.date.available2008-10-28T18:01:57Z
dc.date.issued1979
dc.description.abstractThe Smythii basin has the most extensive topographic coverage of any lunar multi-ringed basin. Topographic data are used to study the morphology and morphometry of Smythii and to make comparisons with similar basins. The depth of the basin is shown to be over 8 km, which is comparable to that of Orientale. The inner ring reaches heights of 3.4 km, while the intermediate ring exhibits little relief. Lowest points in the basin are related to mare ridges. Basin volume is estimated to be 21 million cubic kilometers. Evidence suggests that significant differences in substrate characteristics may have existed for the Smythii and Orientale impacts.
dc.format.extent528285 bytes
dc.format.extent2609–2621
dc.format.mimetypeapplication/pdf
dc.identifier.citationStrain, Priscilla L. and El-Baz, Farouk. 1979. "<a href="https://repository.si.edu/handle/10088/6401">Smythii basin topography and comparisons with Orientale</a>." In <em>Proceedings of the 10th Lunar and Planetary Science Conference</em>. Houston, Texas ed. 2609–2621. 3
dc.identifier.urihttp://hdl.handle.net/10088/6401
dc.language.isoen_US
dc.relation.ispartofProceedings of the 10th Lunar and Planetary Science Conference 3
dc.titleSmythii basin topography and comparisons with Orientale
dc.typechapter
sro.description.unitNASM
sro.description.unitNASM-CEPS
sro.editionHouston, Texas
sro.identifier.itemID71563
sro.identifier.refworksID87780
sro.identifier.urlhttps://repository.si.edu/handle/10088/6401

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