Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8134564 | Icarus | 2018 | 12 Pages |
Abstract
The orbital data products of Ceres, including global LAMO image mosaic and global HAMO DTM with a resolution of 35â¯m/pixel and 135â¯m/pixel respectively, are utilized in this research to create a global catalogue of impact craters with diameterâ¯â¥â¯1â¯km, and their morphometric parameters are calculated. Statistics shows: (1) There are 29,219 craters in the catalogue, and the craters have a various morphologies, e.g., polygonal crater, floor fractured crater, complex crater with central peak, etc.; (2) The identifiable smallest crater size is extended to 1â¯km and the crater numbers have been updated when compared with the crater catalogue (Dâ¯â¥â¯20â¯km) released by the Dawn Science Team; (3) The d/D ratios for fresh simple craters, obviously degraded simple crater and polygonal simple crater are 0.11â¯Â±â¯0.04, 0.05â¯Â±â¯0.04 and 0.14â¯Â±â¯0.02 respectively. (4) The d/D ratios for non-polygonal complex crater and polygonal complex crater are 0.08â¯Â±â¯0.04 and 0.09â¯Â±â¯0.03. The global crater catalogue created in this work can be further applied to many other scientific researches, such as comparing d/D with other bodies, inferring subsurface properties, determining surface age, and estimating average erosion rate.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Gou Sheng, Yue Zongyu, Di Kaichang, Liu Zhaoqin,