Detection of solid C(triple bond)N bearing materials on solar system bodies

Details Detection of solid C(triple bond)N bearing materials on solar system bodies Detection of solid C(triple bond)N bearing materials on solar system bodies

Oct 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991plas.rept..155c&link_type=abstract

In NASA, Washington, Reports of Planetary Astronomy, 1991 p 155 (SEE N92-12792 03-89)

Astronomy and Astrophysics

Astronomy

Asteroids, Cn Emission, Comets, Iapetus, Solids, Uranus Rings, Astronomical Spectroscopy, Chemical Composition, Cyanides, Infrared Spectra, Solar System

Scientific paper

We found observational evidence for the presence of C(triple bond)N-bearing solid materials on four classes of Solar System bodies: comets, asteroids, the rings of Uranus, and Saturn's satellite Iapetus. Gaseous CN was known in comet spectra, and the IR spectra of Comet P/Halley show emission of the CN fundamental at 4.5 microns interpreted as solids containing CN- group in the grains of the inner coma. The presented data offer the first evidence for chemically related material on the other objects.

Affiliated with

Also associated with

No associations

Rating

Detection of solid C(triple bond)N bearing materials on solar system bodies does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Detection of solid C(triple bond)N bearing materials on solar system bodies, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Detection of solid C(triple bond)N bearing materials on solar system bodies will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1876982