|
Gusev Crater Windstreaks
- Click the image above for a larger view
- Full-Res JPEG (685 x 1428) (79.5 kB)
- Full-Res TIFF (685 x 1428) (681.8 kB)
Caption:
Context image
Today's VIS image shows some of the numerous dark linear streaks on the floor of Gusev Crater. These streaks are formed by wind action. The dark streaks are where dust devils have removed the surface dust, revealing the darker rock beneath. Gusev Crater is the home of the MER Spirit lander.
Orbit Number: 65898 Latitude: -14.5 Longitude: 175.545 Instrument: VIS Captured: 2016-10-21 21:54
Background Info:
Please see the THEMIS Data Citation Note for details on crediting THEMIS images.
NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Science Mission Directorate, Washington, D.C. The Thermal Emission Imaging System (THEMIS) was developed by Arizona State University, Tempe, in collaboration with Raytheon Santa Barbara Remote Sensing. The THEMIS investigation is led by Dr. Philip Christensen at Arizona State University. Lockheed Martin Astronautics, Denver, is the prime contractor for the Odyssey project, and developed and built the orbiter. Mission operations are conducted jointly from Lockheed Martin and from JPL, a division of the California Institute of Technology in Pasadena.
Cataloging Keywords:
| Name | Value | Additional Values |
|---|---|---|
| Target | Mars | |
| System | ||
| Target Type | Planet | |
| Mission | 2001 Mars Odyssey | Mars Exploration Rover (MER) |
| Instrument Host | Mars Odyssey | Spirit (MER-A) |
| Host Type | Orbiter | Rover |
| Instrument | Thermal Emission Imaging System (THEMIS) | |
| Detector | ||
| Extra Keywords | Crater, Dust, Grayscale, Thermal | |
| Acquisition Date | ||
| Release Date | 2016-12-12 | |
| Date in Caption | 2016-10-21 | |
| Image Credit | NASA/JPL-Caltech/ASU | |
| Source | photojournal.jpl.nasa.gov/catalog/PIA21187 | |
| Identifier | PIA21187 | |
