Optical characteristics of the Galilean satellites of Jupiter in the 0.347-0.792 micron spectral range. I - Dependence of reflectivity on the orbital phase angle near opposition

Details Optical characteristics of the Galilean satellites of Jupiter in the 0.347-0.792 micron spectral range. I - Dependence of reflectivity on the orbital phase angle near opposition Optical characteristics of the Galilean satellites of Jupiter in the 0.347-0.792 micron spectral range. I - Dependence of reflectivity on the orbital phase angle near opposition

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985kfnt....1...29d&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 1, July-Aug. 1985, p. 29-36. In Russian.

Physics

2

Galilean Satellites, Infrared Spectra, Jupiter Satellites, Orbital Elements, Phase Shift, Spectral Reflectance, Ultraviolet Spectra, Callisto, Electrophotometry, Interference Grating, Io, Near Infrared Radiation, Optical Properties, Radio Filters

Scientific paper

Photoelectric observations of the Galilean satellites were performed at 0.347-0.792 micron using 11 interference filters (Delta lambda/lambda = 2 percent). The dependence of the reflectivity of the satellites on the orbital phase angle near opposition (alpha not greater than 1.2 deg) was determined. The most significant reflectivity variations (approximately 40 percent) were observed for Io in the ultraviolet (0.347 micron). The smallest variations (5-7 percent) were observed for Callisto for the whole spectral range investigated.

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