New constraints on Titan's stratospheric n-butane abundance
Curiously, n-butane has yet to be detected at Titan, though it is predicted to be present in a wide range of abundances that span over 2.5 orders of magnitude. We have searched infrared spectroscopic observations of Titan for signals from n-butane (n-C4H10) in Titan's stratosphere. Three sets o...
Hoofdauteurs: | Steffens, BL, Nixon, CA, Sung, K, Irwin, PGJ, Lombardo, NA, Pereira, E |
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Formaat: | Journal article |
Taal: | English |
Gepubliceerd in: |
American Astronomical Society
2022
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