
In regions of poorly cemented surface materials it is possible to create large features due to just the action of the wind. The equatorial region between Olympus Mons and Apollinaris Mons is dominated by wind etched regions. This region east of Apollinaris Mons contains just such a terrain. The direction of the wind aligns with the ridges and valleys. The dominant wind direction in this region is southeast to northwest; however, other wind directions can occur within a localized region.The top of this VIS image follows the regional trend, with a smaller central surface indicating winds perpendicular to the prevailing direction. Orbit Number: 72333 Latitude: -10.2083 Longitude: 179.736 Instrument: VIS Captured: 2018-04-05 02:02 https://photojournal.jpl.nasa.gov/catalog/PIA22577
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.
NASA ID
PIA22577
Date Created
June 29, 2018
Center
JPL
Media Type
image
Download this image in multiple resolutions. All NASA media are free for public use.
960px