MINIATURE INTEGRATED CAMERA AND IMAGING SPECTROMETER
Artist's rendering by Don Foley
Artist's rendering by Don Foley (copyright)
If NASA is to conduct missions with smaller spacecraft, it is essential
to have correspondingly smaller science instruments. One of the advanced
technologies DS1 tested is the Miniature Integrated Camera Spectrometer
(MICAS), conceived and developed by a team from the United States
Geological Survey, the University of Arizona, Boston University,
Rockwell, SSG, and JPL. In one 12-kg package, it includes two black and
white cameras, an ultraviolet imaging spectrometer, and an infrared
imaging spectrometer plus all the thermal and electronic control. All
sensors share a single 10-cm-diameter telescope. With a structure and
mirror of highly stable SiC, no moving parts are required; the detectors
are electronically shuttered. Spacecraft pointing directs individual
detectors to the desired targets.
An imaging spectrometer allows the construction of a picture in which
each small element of the picture, known as a pixel, contains
information on the spectrum of light; that is, the light is broken into
its individual colors, as when you look through a prism. The imaging
spectrometers in DS1 work in the ultraviolet and infrared, and the
resulting data allows scientists to determine, among other things, the
chemical composition of objects being viewed. DS1 determined the
chemical composition of asteroid Braille with its infrared spectrometer.
Traditional spacecraft would have 3 separate devices to accomplish all
the functions of this one.
The ultraviolet detector did not function properly. But, as with all the
technologies on DS1, the purpose of the testing was to determine how
well it worked to reduce the cost and risk for future missions, so this
was a worthwhile experiment.
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