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Infrared observations of the dark side of Iapetus
Authors:LA Lebofsky  MA Feierberg  AT Tokunaga
Institution:Lunar and Planetary Laboratory, University of Arizona, Tucson, Arizona 85721, USA;Institute for Astronomy, University of Hawaii, Honolulu, Hawaii 96822, USA
Abstract:Broadband (J, H, K, L, and L′) and narrowband (2.8–3.8 μm) circularly variable filter photometric observations were made of the dark side of Iapetus (Eastern Elongation). The data show a 3-μm absorption feature which is too deep to be a residual water frost feature from the bright material around the poles. Laboratory simulations show that the dark material must have a strong 3-μm absorption and could be a hydrated silicate mixed with a small amount of water frost.
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