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- W2000690116 abstract "The morphology of Titan's infrared spectral features reveals a pattern of differences with respect to Saturn's bands. Titan's bands exhibit a progressive washing out with increasing wavelength relative to the corresponding bands in Saturn's spectrum. Unidentified absorption features of apparently gaseous origin appear in the long-wavelength wing of Titan's 1-μm CH4 band complex with considerably greater strength. Greater absorption is also observed in the 1.1 μm region. Not all of the phenomena can be explained by enhance CH4 absorption, so Titan's spectrum implies the existence of another spectroscopically active gas. Several candidates for this gas are briefly considered. In a number of ways, Titan's far infrared spectral features approximate those in the spectrum of Uranus more closely than those in the spectrum of Saturn. This is further support for the concept of an optically deep atmosphere for Titan." @default.
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- W2000690116 date "1974-02-01" @default.
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- W2000690116 title "Titan: Unidentified strong absorptions in the photometric infrared" @default.
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- W2000690116 doi "https://doi.org/10.1016/0019-1035(74)90134-1" @default.
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