CRISM (Compact Reconnaissance Imaging Spectrometer for Mars)
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Beginning 12 Aug. 2005, 11:43:00 UTC
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CRISM Downloads

Want to download information from the website but can’t find it? Here are all of the downloadable documents the CRISM website has to offer!

CRISM View



CRISM View is a first-of-its-kind opportunity to watch Mars through the “eyes” of the Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) – as if you were riding along with it on the Mars Reconnaissance Orbiter!
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JCAT



The Java CRISM Analysis Tool (JCAT) can be used to view CRISM data downloaded from the Planetary Data System (PDS) Geosciences Node at Washington University in St. Louis.
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What is CRISM?

The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) is 1 of 6 science experiments on the Mars Reconnaissance Orbiter, which takes measurements of both the surface and the atmosphere of Mars.

CRISM data are used to find minerals’ spectral signatures on Mars. Different minerals form in different settings, ranging from ancient lakes and deltas to volcanic lava flows. We use the mineral evidence to understand how different geologic processes have shaped the planet over time.  CRISM also observes the polar ice caps and atmosphere to understand seasonal and year-to-year variations in the Martian weather.

Featured Images

  • Mars Reconnaissance Orbiter Preparing for Years Ahead             

  • Mars Gullies Likely Not Formed By Liquid Water             

  • Evidence Builds for Old Under-Ice Volcanoes on Mars             

  • New CRISM Data Products Offer Greater Accessibility to Mars Researchers             

  • Study Finds Evidence for More Recent Clay Formation on Mars               

  • NASA Confirms Evidence That Liquid Water Flows on Today’s Mars               

  • What Happened to Early Mars' Atmosphere? New Study Eliminates One Theory

  • Martian glass: Window into possible past life?                                                  

  • APL’s ​​C. Beck describes how CRISM helps researchers understand the history and formation of Valles Marineris.                         

  • Ancient Martian lake system records two water-related events                         

  • CRISM Reveals New Images of Comet Siding Spring's Coma                          

  • CRISM (shown here on NASA's Mars Reconnaissance Orbiter) delivers important new science and shows the way for past, present and future Mars rovers.

  • MESDT (Mars Exploration Student Data Teams) participants discuss Martian geology.

Latest News

February 9, 2018
Mars Reconnaissance Orbiter Preparing for Years Ahead
Teams operating the two instruments aboard NASA's Mars Reconnaissance Orbiter (MRO) named most often in research papers -- the High Resolution Imaging Science Experiment (HiRISE) camera and the CRISM mineral-mapper -- are dealing with challenges but are ready to continue providing valuable observations. [more]

January 11, 2018
Steep Slopes on Mars Reveal Structure of Buried Ice
Researchers using CRISM and other instruments have found eight sites where thick deposits of ice beneath Mars' surface are exposed in faces of eroding slopes. [more]

July 29, 2016
Mars Gullies Likely Not Formed By Liquid Water
New findings using CRISM data show that gullies on modern Mars are most likely not being formed by flowing liquid water. This new evidence will allow researchers to further narrow theories as to the mechanisms behind the formation of gullies on Mars. [more]

June 15, 2016
Spectroscopy on Mars: A Look at What’s Been Uncovered About the Red Planet
In this interview by Spectroscopy Editors, CRISM Co-Investigator Ray Arvidson discusses "how spectroscopy has played a significant role in the Mars expeditions, including the confirmation of the former presence of water on the Red Planet." [more]

May 3, 2016
CRISM Reveals Clues about Volcanoes Under Ice on Ancient Mars
Volcanoes erupted beneath an ice sheet on Mars billions of years ago, far from any ice sheet on the Red Planet today, new evidence from CRISM suggests. [more]

March 17, 2016
New CRISM Data Products Offer Greater Accessibility to Mars Researchers
CRISM has acquired tens of thousands of targeted, high-resolution, hyperspectra Mars observations – and now, thanks to two new data products in the Planetary Data System, that data will be much more accessible to researchers. [more]

All Mars Reconnaissance Orbiter Mission Updates

Team Profiles

Team profile collage Read about the career paths that led members of the CRISM team into space exploration.

CRISM Spectral Library

The MRO CRISM Spectral Library is an analysis tool for interpreting CRISM data. it currently contains 2,260 spectral analyses of 1,134 Mars-analog samples, all measured under desiccating conditions so that materials that adsorb water look as they would on Mars. This was made avaialble to the community through the PDS on the day that MRO entered Mars orbit!

The MICA Files »

The MICA Files is a compilation of published descriptions and type locations of unique spectral features identified on Mars by using data from CRISM. Learn more »

Hi-Res Image Map


Thousands of CRISM high-resolution images are available in easy-to-view format accessible through a searchable map. More are being added as they are converted from the full spectral data... [ more ]

Revealing Questions

Why should we study Mars?

Lots of reasons!  One is that Mars is made up of the same raw solar system materials that came together to form the planet Earth.  However, on Earth, plate tectonics has recycled almost all of the oldest rocks; consequently, we know little about what Earth was like when it was very young - when asteroids and comets were heavily bombarding the planet, and oceans and life were just getting started. Mars, on the other hand, does not have plate tectonics and so the record of that earliest period is still there for us to see. By understanding the geological evolution of Mars we will come to better understand what early Earth could have been like. Another reason is that Mars is a laboratory for studying weather. Like Earth it has seasons, ice caps, and winter frost. Unlike Earth, it lacks oceans. That makes Mars a simpler test case for models of how weather works.

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CRISM Facts

MRO's Primary Science Phase started in November 2006 and ended in November 2008. MRO is now in an extended mission.

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