This image is located near the equator and the prime meridian of Mars in a region called Terra Meridiani. This is a unique area of Mars that displays layers of material that appear to be in the process of being stripped away. This exposing another layer of material directly underneath that is visible in the central portion of the image. Measurements from another instrument in orbit around Mars, the Thermal Emission Spectrometer on the Mars Global Surveyor, indicate that this region has a high concentration of a mineral called hematite. Grey hematite can form in both volcanic and water rich environments. It is not certain exactly how this mineral formed on Mars, but its presence along with the layering seen in this region makes this region of Mars particularly interesting. Among other possibilities, these layers could be volcanic ash deposits or plausibly sediments deposited in water. This region of Mars is very old and whatever process took place here, it happened long ago. This is one of the principal candidate sites for the next rover mission that will be sent to Mars in 2003.
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.
Name | Value | Additional Values |
---|---|---|
Target | Mars | |
System | ||
Target Type | Planet | |
Mission | 2001 Mars Odyssey | Mars Global Surveyor (MGS) |
Instrument Host | Mars Odyssey | Mars Global Surveyor |
Host Type | Orbiter | |
Instrument | Thermal Emission Imaging System (THEMIS) | |
Detector | ||
Extra Keywords | Grayscale, Thermal, Volcano, Water | |
Acquisition Date | ||
Release Date | 2002-12-19 | |
Date in Caption | ||
Image Credit | NASA/JPL/Arizona State University | |
Source | photojournal.jpl.nasa.gov/catalog/PIA04064 | |
Identifier | PIA04064 |