The crosscutting relationships observed in this image from NASA's Mars Odyssey spacecraft can be used to determine the relative timing of graben and channel formations.
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Crosscutting Grabens


Released 21 April 2003

The crosscutting relationships observed in this THEMIS image can be used to determine the relative timing of graben and channel formations. Several north-west/south-east trending fractures are observed to crosscut north-east/south-west formations.

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.

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.

Image information: VIS instrument. Latitude 43.2, Longitude 269.4 East (90.6 West). 19 meter/pixel resolution.

Image details

ID#:
PIA04471

Date added:
2003-04-21

Target:
Mars

Mission:
2001 Mars Odyssey

Spacecraft:
2001 Mars Odyssey

Instruments:
Thermal Emission Imaging System

Rating:



Views:
3,133

Full-Res TIFF:
PIA04471.tif (3.24 MB)

Full-Res JPG:
PIA04471.jpg (0.58 MB)

Image credit:
NASA/JPL/Arizona State University