| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701559 | Icarus | 2012 | 9 Pages |
Abstract
⺠LRO NAC data allow 3D optical roughness imagery of the crater Giordano Bruno (GB). ⺠Some flows seen on the GB inner wall can be regolith taluses, not impact melt. ⺠The GB whirlpool structure may be formed by viscous fluxes from crater flanks. ⺠GB is a young crater with an age that is on the order of 1 My.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Yuriy Shkuratov, Vadim Kaydash, Gorden Videen,