Please use this identifier to cite or link to this item: https://apo.ansto.gov.au/dspace/handle/10238/12234
Title: Crystal structure of propio­nitrile (CH3CH2CN) determined using synchrotron powder X-ray diffraction
Authors: Brand, HEA
Gu, QF
Kimpton, JA
Auchettl, R
Ennis, C
Keywords: Crystal structure
Synchrotrons
X-ray diffraction
Thermal expansion
Ice
Planetary atmospheres
Satellites
Nitriles
Issue Date: Jan-2020
Publisher: International Union of Crystallography
Citation: Brand, H. E. A, Gu, Q., Kimpton, J. A., Auchettl, R.& Ennis, C.(2020). Crystal structure of propionitrile (CH3CH2CN) determined using synchrotron powder X-ray diffraction. Journal of Synchrotron Radiation 27, 1, 212-216. doi:10.1107/S1600577519015911
Abstract: The structure and thermal expansion of the astronomical molecule propio­nitrile have been determined from 100 to 150 K using synchrotron powder X-ray diffraction. This temperature range correlates with the conditions of Titan's lower stratosphere, and near surface, where propio­nitrile is thought to accumulate and condense into pure and mixed-nitrile phases. Propio­nitrile was determined to crystallize in space group, Pnma (No. 62), with unit cell a = 7.56183 (16) Å, b = 6.59134 (14) Å, c = 7.23629 (14), volume = 360.675 (13) Å3 at 100 K. The thermal expansion was found to be highly anisotropic with an eightfold increase in expansion between the c and b axes. These data will prove crucial in the computational modelling of propio­nitrile–ice systems in outer Solar System environments, allowing us to simulate and assign vibrational peaks in the infrared spectra for future use in planetary astronomy. © 2020 International Union of Crystallography
URI: https://doi.org/10.1107/S1600577519015911
https://apo.ansto.gov.au/dspace/handle/10238/12234
ISSN: 1600-5775
Appears in Collections:Journal Articles

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