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The newspaper of The Johns Hopkins University August 22, 2005 | Vol. 34 No. 42
Powerful Mineral Mapper CRISM is Headed to Mars
APL-built spectrometer on NASA's Latest mission to the red planet

By Michael Buckley
Applied Physics Laboratory

With the August 12 launch of NASA�s Mars Reconnaissance Orbiter spacecraft from Cape Canaveral Air Force Station, Fla., the Compact Reconnaissance Imaging Spectrometer for Mars�or CRISM�joins the set of hightech detectives seeking traces of water on the red planet.

Built by Johns Hopkins� Applied Physics Laboratory, CRISM is the first visible-infrared spectrometer to fly on a NASA Mars mission. Its primary job: Look for the residue of minerals that form in the presence of water, the �fingerprints� left by evaporated hot springs, thermal vents, lakes or ponds on Mars when water could have existed on the surface.

With unprecedented clarity, CRISM will map areas on the martian surface down to house-sized scales�as small as 60 feet across�when the spacecraft is in its average orbit altitude of about 190 miles.

�CRISM plays a very important role in Mars exploration,� APL�s Scott Murchie, the instrument�s principal investigator, said. �Our data will identify sites most likely to have contained water and which would make the best potential landing sites for future missions seeking fossils or even traces of life on Mars.�

Though certain landforms provide evidence that water may once have flowed on Mars, Murchie said scientists have little evidence of sites containing mineral deposits created by long-term interaction between water and rock. The NASA Rover Opportunity found evidence for liquid water in Meridian Planum, a large plain near Mars� equator, but that is only one of many hundreds of sites where future spacecraft could land.

Peering through a telescope with a fourinch aperture, and with a greater capability to map spectral variations than any similar instrument sent to another planet, CRISM will read 544 �colors� in reflected sunlight to detect minerals in the surface. Its highest resolution is about 20 times sharper than any previous look at Mars in infrared wavelengths.

�At infrared wavelengths, rocks that look absolutely the same to human eyes become very different,� Murchie said. �CRISM has the capability to take images in which different rocks will �light up� in different colors.�

CRISM is mounted on a gimbal, allowing it to follow targets on the surface as the orbiter passes overhead. CRISM will spend the first half of a two-year orbit mission mapping Mars at 650-foot scales, searching for potential study areas. Several thousand promising sites will then be measured in detail at CRISM�s highest spatial and spectral resolution. CRISM will also monitor seasonal variations in dust and ice particles in the atmosphere, supplementing data gathered by the orbiter�s other instruments and providing new clues about the martian climate.

�CRISM will improve significantly on the mapping technology currently orbiting Mars,� said Peter Bedini of APL, CRISM project manager. �We�ll not only look for future landing sites, but we�ll be able to provide details on information the Mars Exploration Rovers are gathering now. There is a lot more to learn, and after CRISM and the Mars Reconnaissance Orbiter, there will still be more to learn. But with this mission we�re taking a big step in exploring and understanding Mars.�

As the Mars Reconnaissance Orbiter cruises to its destination, the CRISM operations team continues to fine-tune the software and systems it will use to command the instrument and receive, read, process and store a wealth of data from orbit�more than 10 terabytes when processed back on Earth, enough to fill more than 15,000 compact discs. The spacecraft is set to reach Mars in March, use aerobraking to circularize its orbit and settle into its science orbit by November 2006.

APL, which has built more than 150 spacecraft instruments over the past four decades, led the effort to develop, integrate and test CRISM. CRISM�s co-investigators are top planetary scientists from Brown University, the Jet Propulsion Laboratory, Northwestern University, the Space Science Institute, Washington University in St. Louis, University of Paris, the Applied Coherent Technology Corp. and NASA�s Goddard Space Flight Center, Ames Research Center and Johnson Space Center.

The Jet Propulsion Laboratory, a division of the California Institute of Technology, Pasadena, manages the Mars Reconnaissance Orbiter mission for NASA�s Science Mission Directorate.

For more information on CRISM and the Mars Reconnaissance Orbiter, including instrument images, go to


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