| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701687 | Icarus | 2012 | 16 Pages |
Abstract
⺠Impacts creating craters larger than 200 km can demagnetize the entire crust of Mars. ⺠Craters and QCDS larger than 200 km in Tempe Terra have no magnetic signatures. ⺠The crust underlying the Tempe Terra on Mars is not appreciably magnetized. ⺠No strong core dynamo existed within the first about 100 Myr of Mars history.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Jafar Arkani-Hamed, Daniel Boutin,