+ CRISM Research
The Compact Reconnaissance Imaging Spectrometer
for Mars (CRISM) is a NASA sponsored instrument currently onboard the
Mars Reconnaissance Orbiter (MRO) which is in orbit around
Mars.
CRISM opened its cover in September of 2006 and
has begun taking images. Check out the first images here!
CRISM
is an infrared spectrometer that measures light from 0.4 microns to 4
microns. This region of the electromagnetic spectrum extends from what
we can see with our eyes (the visible) to what is commonly termed the
mid infra-red. Just like infrared sensors here on Earth, CRISM can
reveal patterns our eyes are not sensitive to, because molecules and
minerals react differently to infrared light.
CRISM does not, however, extend its greatest
sensitivity to the "thermal infrared" region where it may be able to
sense heat. This region has been covered at Mars by the Thermal
Emission Spectrometer (TES). TES was sensitive to heat, and in
particular, how heat was emitted from Martian materials, however
because Mars is so cold, it is very challenging to interpret the
information from TES. CRISM, by looking at reflected light from the
Sun, at over 500 wavelengths (for many so called "hyperspectral"
observations) will reveal at very fine spatial scale (down to about 18m
per pixel) between minerals on the surface.
I'm excited about what CRISM is going to reveal on
Mars, if you'd like to learn more, you can contact me or you can go to
a couple of related websites which are listed below. Periodically I'll
update this page with my latest work on CRISM data, I've included a few
teasers here already.
+ CRISM related websites
- '
CRISM @ APL' The CRISM site at the Johns Hopkins Applied
Physics Laboratory, where the instrument was built and where it is run.
- ' CRISM @ JPL' The CRISM site at
the Jet Propulsion Laboratory.
- ' MRO @ JPL' The Mars
Reconnaissance Orbiter site at the Jet Propulsion Laboratory.
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+ Recent CRISM Papers
Here you will find the full text
of some of my recent papers regarding CRISM in pdf format.
- 'Louth Crater: Evolution of a layered water
ice mound' with S. Byrne, L. Tornabene and T. Roush
(2008) Icarus 196 433-445
- 'High
resolution Observations of Korolev Crater and Mrs Chippy's Ring during
Summer by CRISM and HiRISE',
with S. Byrne, T. Roush, K.E. Herkenhoff, J.L. Bishop,
C. Hansen, R.O. Green, P. Russell, A. McEwen, S.L. Murchie and the
CRISM and HiRISE teams, (2007) LPSC
XXXVIII, abstract 2308
- 'Mars
Polar Targets for the CRISM' with J. Bishop and R. Green,
(2006) Mars Water Workshop, NASA
Ames Research Center, Feb 22-23
- 'Hydrothermal
Mars through the CRISM: Which
hydroxyl band and why', (2005) LPSC XXXVI, abstract
1091
- 'MR
PRISM: A Spectral Analysis tool for the
CRISM', (2006) SPIE
Optics and Photonics, San Diego, 13-17Aug, paper
6309-28
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