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A research proposal on spectroscopy of gases and solids observed in the solar systemIt 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.
Document ID
19870003056
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Valero, F. P. J.
(NASA Ames Research Center Moffett Field, CA, United States)
Allamandola, L. J.
(NASA Ames Research Center Moffett Field, CA, United States)
Chackerian, C., Jr.
(NASA Ames Research Center Moffett Field, CA, United States)
Giver, L. P.
(NASA Ames Research Center Moffett Field, CA, United States)
Goorvitch, D.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 13, 2013
Publication Date
September 1, 1986
Publication Information
Publication: NASA, Washington Reports of Planetary Astronomy, 1985
Subject Category
Astronomy
Accession Number
87N12489
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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