Seasonal Flows in Asimov Crater
Seasonal flows called recurring slope lineae RSL grow down warm slopes in the summer, fade when they become inactive, then re-form the following year when the slopes warm up again from the Sun. This observation is from NASA Mars Reconnaissance Orbiter
Usage Rights
Most NASA images are in the public domain and free to use. Credit NASA as the source. Check NASA's media usage guidelines for details. Images featuring identifiable individuals may require additional permissions.
Details
NASA ID
PIA18561
Date Created
May 20, 2015
Center
JPL
Media Type
image
Downloads
Download this image in multiple resolutions. All NASA media are free for public use.
