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Jupiter and Saturn: Near-infrared spectral albedos
Authors:Roger N Clark  Thomas B McCord
Institution:1. Department of Earth and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA;2. Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu Hawaii 96822, USA
Abstract:The near-infrared (0.65–2.5μm) spectral albedo of Jupiter and Saturn with 1.5% spectral resolution is presented for the center of disk and for the limb. There is a distinct difference in the continuum slope between Jupiter and Saturn which may be attributed to a difference in the dust content or composition of the two atmospheres. There is an indication of limb brightening in the deepest CH4 bands on Saturn. No limb brightening is found for Jupiter.
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