Astronomy and Astrophysics – Astronomy
Scientific paper
Sep 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986plas.rept..167v&link_type=abstract
In NASA, Washington Reports of Planetary Astronomy, 1985 p 167-168 (SEE N87-12407 03-89)
Astronomy and Astrophysics
Astronomy
Astronomical Spectroscopy, Cosmic Gases, Planetary Atmospheres, Spaceborne Astronomy, Faint Objects, Ice Formation, Volatility
Scientific paper
It is well recognized and accepted that the interpretation and analysis of any type of remote planetary spectroscopic observation requires that basic molecular parameters be available. Furthermore, the newly developed capabilities of air, ground, and space borne spectrometers trained on bodies in the solar system are producing results which are extremely difficult to understand on the basis of available data. This is particularly true in the case of spectral features arising from gases and volatiles condensed as ices. With the objective to continue to extend the understanding of spectroscopic observations of solar system objects (including comets) , laboratory studies of both gas phase molecules and ices and dusts are proposed.
Allamandola Louis J.
Chackerian Charles Jr.
Giver Lawrence P.
Goorvitch David
Valero Francisco P. J.
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