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Far-infrared photometry of Titan and Iapetus
Authors:R.F. Loewenstein  D.A. Harper  R.H. Hildebrand  Harvey Moseley  Ed Shaya  J. Smith
Affiliation:1. Yerkes Observatory, University of Chicago, Williams Bay, Wisconsin 53191, USA;1. Enrico Fermi Institute, University of Chicago, 5630 Ellis Avenue, Chicago, Illinois 60637, USA;2. Goddard Spaceflight Center, Code 693.2, Greenbelt, Maryland 20771, USA
Abstract:Titan was observed in four broad passbands between 35 and 150 μm. The brightness temperature in this interval is roughly constant at 76 ± 3°K. Integrating Titan's spectrum from 5 to 150 μm yields an effective temperature of 86 ± 3°K. Both the bright and dark hemispheres of Iapetus were observed in one broadband filter with λe ~ 66 μm. The brightness temperatures for these two sides of Iapetus are 96 ± 9°K and 114 ± 10°K, respectively. The bright-side Bond albedo is calculated to be 0.61?0.22+0.16.
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