| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 5486942 | Icarus | 2018 | 5 Pages |
Abstract
- Sesquinary mass influx is capable of significant impact to the surface geology of Phobos. This can exceed the flux of solar system impactors.
- Sesquinary impacts have likely controlled the surface properties of Phobos for the last 20-25Â million years.
- The top â¼30â¯cm of Phobos regolith may largely consist of reaccreted sesquinary ejecta material.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Michael Nayak,