Abstract
The structure and thermal expansion of the astronomical molecule propionitrile have been determined from 100 to 150K 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 100K. 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.
Author supplied keywords
Cite
CITATION STYLE
Brand, H. E. A., Gu, Q., Kimpton, J. A., Auchettl, R., & Ennisb, C. (2020). Crystal structure of propionitrile (CH3CH2CN) determined using synchrotron powder X-ray diffraction Brand Helen E. A. Journal of Synchrotron Radiation, 27, 212–216. https://doi.org/10.1107/S1600577519015911
Register to see more suggestions
Mendeley helps you to discover research relevant for your work.