Water and Lava Both Seem Viable for the Formation of One of Mars' Densest and Largest Channel Networks
Abstract
100s of km long Axius Valles on <1° slope imply formation by low-viscosity liquid. Setting, morphology, discharge rate compatible with water or certain lavas.
- Publication:
-
51st Annual Lunar and Planetary Science Conference
- Pub Date:
- March 2020
- Bibcode:
- 2020LPI....51.1088B