Abstract
Propene (C3H6) has been measured in the planetary atmospheres of Earth and Titan, and may be detected in the giant planets by infrared spectroscopy. Propene infrared absorption cross sections have been determined in the 2680–3220 cm−1 and 450–1250 cm−1 regions by high-resolution Fourier transform spectroscopy with H2 and N2, respectively, as broadening gases. Samples of propene were held at 202, 232, 265, 297 K.
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