Crustal thickness and support of topography on Venus
The topography of a terrestrial planet can be supported by several mechanisms: (1) crustal thickness variations, (2) density variations in the crust and mantle, (3) dynamic support, and (4) lithospheric stresses. Each of these mechanisms could play a role in compensating topography on Venus, and we...
| Main Authors: | , , |
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| Other Authors: | |
| Format: | Article |
| Language: | en_US |
| Published: |
American Geophysical Union
2014
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| Online Access: | http://hdl.handle.net/1721.1/85638 https://orcid.org/0000-0003-2652-8017 |