A co-crystal between benzene and ethane: a potential evaporite material for Saturn's moon Titan
Using synchrotron X-ray powder diffraction, the structure of a co-crystal between benzene and ethane formed in situ at cryogenic conditions has been determined, and validated using dispersion-corrected density functional theory calculations. The structure comprises a lattice of benzene molecules hos...
Main Authors: | Helen E. Maynard-Casely, Robert Hodyss, Morgan L. Cable, Tuan Hoang Vu, Martin Rahm |
---|---|
Format: | Article |
Language: | English |
Published: |
International Union of Crystallography
2016-05-01
|
Series: | IUCrJ |
Subjects: | |
Online Access: | http://scripts.iucr.org/cgi-bin/paper?S2052252516002815 |
Similar Items
-
Dinaride evaporite mélange: Diagenesis of the Kosovo polje evaporites
by: Anita Kulušić, et al.
Published: (2014-02-01) -
The mineralogy and water content of paradox basin evaporite deposits
by: Conner, Trent Gregory
Published: (2008) -
A New Digital Terrain Model of the Huygens Landing Site on Saturn's Largest Moon, Titan
by: C. Daudon, et al.
Published: (2020-12-01) -
Chemical deposits in evaporite caves: an overview
by: Paolo Forti
Published: (2017-06-01) -
Simulations de laboratoire de la photodynamique VUV de l’atmosphère de Titan
by: Tigrine, Sarah
Published: (2017)