Smythii basin topography and comparisons with Orientale
| dc.contributor.author | Strain, Priscilla L. | |
| dc.contributor.author | El-Baz, Farouk | |
| dc.date.accessioned | 2008-10-28T18:01:57Z | |
| dc.date.available | 2008-10-28T18:01:57Z | |
| dc.date.issued | 1979 | |
| dc.description.abstract | The 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.extent | 528285 bytes | |
| dc.format.extent | 2609–2621 | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Strain, 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.uri | http://hdl.handle.net/10088/6401 | |
| dc.language.iso | en_US | |
| dc.relation.ispartof | Proceedings of the 10th Lunar and Planetary Science Conference 3 | |
| dc.title | Smythii basin topography and comparisons with Orientale | |
| dc.type | chapter | |
| sro.description.unit | NASM | |
| sro.description.unit | NASM-CEPS | |
| sro.edition | Houston, Texas | |
| sro.identifier.itemID | 71563 | |
| sro.identifier.refworksID | 87780 | |
| sro.identifier.url | https://repository.si.edu/handle/10088/6401 |