Spectrophotometry of faint comets: The asteroid approach

Details Spectrophotometry of faint comets: The asteroid approach Spectrophotometry of faint comets: The asteroid approach

Oct 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981motc.conf...63d&link_type=abstract

In its Mod. Observational Tech. for Comets p 63-69 (SEE N82-13989 04-89)

Astronomy and Astrophysics

Astronomy

Albedo, Brightness, Comets, Reflectance, Spectrophotometry, Astronomical Photometry, Data Acquisition, Space Observations (From Earth), Spectroscopic Analysis, Surface Properties

Scientific paper

Observing 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.

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