Journal
ICARUS
Volume 330, Issue -, Pages 11-15Publisher
ACADEMIC PRESS INC ELSEVIER SCIENCE
DOI: 10.1016/j.icarus.2019.04.020
Keywords
InSight Lander; SEIS; Mars; Seismic velocities; Basalt
Categories
Funding
- University of Strasbourg
Ask authors/readers for more resources
The theoretical predictions for the P- and S-wave velocity of basalt with pore spaces filled with gaseous CO2, liquid water, or water ice presented herein could help improve interpretations of the seismic data collected by NASA's InSight lander, which landed on the Martian surface in November 2018.
Authors
I am an author on this paper
Click your name to claim this paper and add it to your profile.
Reviews
Recommended
No Data Available