Abstract
Four bands of propane C3H8 and two of methyl acetylene C3H4 have been identified in the Voyager IR spectrum of Titan. Stratospheric abundances of 2 × 10-5 for C3H8 and 3 × 10-8 for C3H 4 have been determined for the mid-latitude region. A feature at 1,154 cm-1, previously assigned solely to CH3D, is now identified at least in part due to C3H8. © 1981 Nature Publishing Group.
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CITATION STYLE
APA
Maguire, W. C., Hanel, R. A., Jennings, D. E., Kunde, V. G., & Samuelson, R. E. (1981). C3H8 and C3H4 in Titan’s atmosphere. Nature, 292(5825), 683–686. https://doi.org/10.1038/292683a0
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