Status Report

NASA Mars Odyssey THEMIS Image: A Question of Interpretation

By SpaceRef Editor
July 22, 2004
Filed under , , ,

Medium image for 20040722a

Image Context:

Context image for 20040722a
Context image credit: NASA/Mars Orbiter Laser Altimeter (MOLA) Team
[ Find on map: Javascript version ]

[ Find on map: CGI version ]

ParameterValue ParameterValue
Latitude-6.7 &nbsp InstrumentVIS
Longitude174.7E (185.3W) &nbsp Resolution (m)19
Image Size (pixels)3059×1369 &nbsp Image Size (km)58.1×26

Full data on this image has now been released via the THEMIS Data Releases website.

The atmosphere of Mars is a dynamic system. Water-ice clouds, fog, and hazes can make imaging the surface from space difficult. Dust storms can grow from local disturbances to global sizes, through which imaging is impossible. Seasonal temperature changes are the usual drivers in cloud and dust storm development and growth.

Eons of atmospheric dust storm activity has left its mark on the surface of Mars. Dust carried aloft by the wind has settled out on every available surface; sand dunes have been created and moved by centuries of wind; and the effect of continual sand-blasting has modified many regions of Mars, creating yardangs and other unusual surface forms.

It is often difficult to determine if wind eroded
surface represent the youngest activity in a region. Wind
eroded landforms can be covered by later materials and
the exhumed long after they were initially formed. This
image illustrates how difficult it can be to interpret
the surface of Mars.

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 Credit: NASA/JPL/Arizona State University


Show Full-Size Image (GIF)
] [ Show Full-Size Image (JPG) ]


Show Full-Size Image (PNG)
] [ Show Full-Size Image (TIF) ]


Printer-friendly version

SpaceRef staff editor.