Media Information

 
 
 
Collection:
NASA Planetary Photo Journal Collection
Title:
Colored Crater in Vastitas Borealis
Original Caption Released with Image:


Released 30 April 2004

This daytime visible color image was collected on September 4, 2002 during the Northern Spring season in Vastitas Borealis.

This daytime visible color image was collected on September 4, 2002 during the Northern Spring season in Vastitas Borealis. The THEMIS VIS camera is capable of capturing color images of the martian surface using its five different color filters. In this mode of operation, the spatial resolution and coverage of the image must be reduced to accommodate the additional data volume produced from the use of multiple filters. To make a color image, three of the five filter images (each in grayscale) are selected. Each is contrast enhanced and then converted to a red, green, or blue intensity image. These three images are then combined to produce a full color, single image. Because the THEMIS color filters don't span the full range of colors seen by the human eye, a color THEMIS image does not represent true color. Also, because each single-filter image is contrast enhanced before inclusion in the three-color image, the apparent color variation of the scene is exaggerated. Nevertheless, the color variation that does appear is representative of some change in color, however subtle, in the actual scene. Note that the long edges of THEMIS color images typically contain color artifacts that do not represent surface variation.

Image information: VIS instrument. Latitude 69.3, Longitude 40.9 East ( 319.1 West). 19 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.

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
Produced By:
Arizona State University
Mission:
2001 Mars Odyssey
Spacecraft:
2001 Mars Odyssey
Target Name:
Mars
Is a satellite of:
Sol (our sun)
Instrument:
Thermal Emission Imaging System
Product Size:
630 samples x 1275 lines
facet_what:
Sun
facet_what:
Crater
facet_what:
Mars
facet_what:
2001 Mars Odyssey
facet_what:
Thermal Emission Imaging System (THEMIS)
facet_where:
Jet Propulsion Laboratory
facet_where:
Denver
facet_where:
Mars
facet_where:
Arizona
facet_where:
California
facet_where:
Washington
facet_where:
Jet Propulsion Laboratory (JPL)
facet_where:
Washington, D.C.
facet_when:
30 April 2004
facet_when:
September 4, 2002
facet_when_year:
2002
facet_when_year:
2004
Image #:
PIA05863
UID:
SPD-PHOTJ-PIA05863
orignial url:

Colored Crater in Vastitas Borealis