CoMA: A high resolution Time-Of-Flight Secondary Ion Mass Spectrometer (TOF-SIMS) for in situ analysis of cometary matter

Details CoMA: A high resolution Time-Of-Flight Secondary Ion Mass Spectrometer (TOF-SIMS) for in situ analysis of cometary matter CoMA: A high resolution Time-Of-Flight Secondary Ion Mass Spectrometer (TOF-SIMS) for in situ analysis of cometary matter

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992acm..proc..683z&link_type=abstract

In Lunar and Planetary Inst., Asteroids, Comets, Meteors 1991 p 683-686 (SEE N93-19113 06-90)

Computer Science

Comet Nuclei, Comet Rendezvous Asteroid Flyby Mission, Dust Collectors, Secondary Ion Mass Spectrometry, Time Of Flight Spectrometers, Chemical Composition, Cometary Atmospheres, In Situ Measurement, Space Rendezvous, Spaceborne Experiments

Scientific paper

A lot of clues concerning the origin of the solar system can be found by
sending an exploring spacecraft to a rendezvous with a comet. The space
experiment CoMA, which will measure the elemental, isotopic, and
molecular composition of cometary dust grains is described. It will be
flown on NASA's Comet Rendezvous Asteroid Flyby (CRAF) mission.

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