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Infrared reflectance spectra of Hyperion,Titania, and Triton
Authors:Larry A Lebofsky  George H Rieke  Marcia J Lebofsky
Institution:1. Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721, USA;2. Steward Observatory, University of Arizona, Tucson, Arizona 85721, USA
Abstract:Medium-resolution infrared (1–2.5 μm; Δλ/λ ∽ 0.05) photometry of Triton, Titania, and Hyperion and medium-resolution (1.5–2.4 μm; Δλ/λ ? 0.01) spectroscopy of Triton are presented. Hyperion and Titania have spectra roughly similar to the laboratory spectrum of water frost, while the spectrum of Triton is inconsistent with the spectra of frosts likely to be major surface constituents.
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