PIA03677: Dust Slides


Dust Slides

Caption:

Context image for PIA03677 Linear Clouds
Context image for PIA03677
Linear Clouds

Dust slides are common in the dust covered region called Lycus Sulci. A large fracture is also visible in this image.

Image information: VIS instrument. Latitude 28.1°N, Longitude 226.3°E. 18 meter/pixel resolution.

Note: this THEMIS visual image has not been radiometrically nor geometrically calibrated for this preliminary release. An empirical correction has been performed to remove instrumental effects. A linear shift has been applied in the cross-track and down-track direction to approximate spacecraft and planetary motion. Fully calibrated and geometrically projected images will be released through the Planetary Data System in accordance with Project policies at a later time.

Background Info:

NASA's Jet Propulsion Laboratory manages the 2001 Mars Odyssey mission for NASA's Office of Space Science, 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 Mars
Target Type Planet
Mission 2001 Mars Odyssey
Instrument Host 2001 Mars Odyssey
Host Type Orbiter
Instrument Thermal Emission Imaging System (THEMIS)
Detector
Extra Keywords Dust, Grayscale
Acquisition Date
Release Date 2006-01-17
Date in Caption
Image Credit NASA/JPL/ASU
Source photojournal.jpl.nasa.gov/catalog/PIA03677
Identifier PIA03677