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Spectrophotometry of faint comets: The asteroid approachObserving programs at optical (0.35-0.8 micron) and near-infrared (1.1-2.4 micron) wavelengths, directed at the acquisition of reflection spectra of faint and distant comets, are described. The ultimate goal is to obtain spectrophotometric measurements of comets for which a significant part of the light is expected to be reflected by the solid surface of the nucleus.
Document ID
19820006125
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Degewij, J. (Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 10, 2013
Publication Date
October 1, 1981
Publication Information
Publication: Mod. Observational Tech. for Comets
Subject Category
Astronomy
Accession Number
82N13998
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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