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Galilean satellite eclipse studies I. Observations and satellite characteristics
Authors:Thomas F. Greene  Dale W. Smith  Richard W. Shorthill
Affiliation:1. Department of Astronomy, University of Washington, Seattle, Washington 98105, USA;2. Boeing Aerospace Company, Seattle, Washington 98124, USA;3. Geospace Sciences Laboratory, University of Utah Research Institute, Salt Lake City, Utah 84108, USA
Abstract:Spectrophotometric light curves of 12 Galilean satellite eclipses are reported. The observations were made in 20 to 30 channels over the wavelength range 3240 to 10,500 Å using the 200-in. telescope. The initial data processing is described. These data measure the Jovian aerosol content in the lower stratosphere and uppermost troposhere and the methane abundance in the lower stratosphere. The data are consistent with a lack of limb darkening on the Galilean satellites. The orbit of Callisto is shown to be inclined 0.08 ± 0.02° to the equatorial plane of Jupiter.
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