PIA10946: Gypsum Dunes North of Phoenix Landing Site
 Target Name:  Mars
 Is a satellite of:  Sol (our sun)
 Mission:  Mars Reconnaissance Orbiter (MRO)
 Spacecraft:  Mars Reconnaissance Orbiter (MRO)
 Instrument:  CRISM
 Product Size:  1109 x 1500 pixels (w x h)
 Produced By:  Johns Hopkins University Applied Physics Laboratory / CRISM 
 Full-Res TIFF:  PIA10946.tif (4.997 MB)
 Full-Res JPEG:  PIA10946.jpg (202.4 kB)

Click on the image above to download a moderately sized image in JPEG format (possibly reduced in size from original)

Original Caption Released with Image:

This image of sulfate deposits, including gypsum, in the Olympia Undae region of Mars was taken by the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) at 0026 UTC on November 18, 2006 (7:26 p.m. EDT on November 17, 2006) near 80 degrees north latitude, 245 degrees east longitude. CRISM's image was taken in 544 colors covering 0.36-3.92 micrometers, and shows features as small as 20 meters (66 feet) across.

Named for a classic albedo feature, Olympia Undae is a large dune field that stretches some 1,100 kilometers (684 miles) across the northern polar regions of Mars, just south of the ice cap.

In 2005 CRISM's sibling instrument, OMEGA, on board Mars Express, captured data revealing that Olympia Undaeís dunes hold sulfate minerals including gypsum. With more than five times the spatial resolution of OMEGA, CRISM has captured greater detail of this region.

The top image reveals the location of CRISM data on a Mars Orbiter Laser Altimeter (MOLA) map. The area from which CRISM data were gathered is roughly 12 degrees north and 11 degrees east of the region where Phoenix recently landed.

The lower left image is an infrared, false-color image that reveals dark colored dunes overlying a lighter, rust-colored substrate. CRISM spectral data (lower right image) shows the region is inundated with sulfates. It also reveals that the darker dune material holds a higher concentration of the water-bearing calcium sulfate mineral gypsum. A full resolution targeted CRISM image taken just five degrees west of the image above, revealed greater gypsum concentrations along the dunesí crests (Gypsum at Olympia Undae).

On Earth, gypsum is the most common sulfate mineral and is widely found in sedimentary rocks. Itís frequently associated with evaporite salts and is often found as a thick layer beneath halite or rock salt. Although most often associated with evaporites, gypsum can also occur in layers with limestone and shale. Most people are familiar with gypsum in the form of plaster of Paris.

CRISM is one of six science instruments on NASA's Mars Reconnaissance Orbiter. Led by The Johns Hopkins University Applied Physics Laboratory, Laurel, Md., the CRISM team includes expertise from universities, government agencies and small businesses in the United States and abroad. NASA's Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Mars Reconnaissance Orbiter and the Mars Science Laboratory for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, built the orbiter.

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