Photochemical Escape from Mars as a Climate Driver: How Important?
Abstract
Photochemical escape is the primary loss process for O, C, and N atoms from Mars. But C rates are 10 times lower than O, setting up a conundrum: where did all the carbon from an early thick CO2 atmosphere go?
- Publication:
-
Ninth International Conference on Mars
- Pub Date:
- July 2019
- Bibcode:
- 2019LPICo2089.6033L