Complexity in low-temperature phase diagrams of planetary ices: phase transition in bischofite, MgCl2.6H2O
Abstract
Bischofite, MgCL2.6H2O is a marine evaporite that may be present also on or inside icy satellites. It has a monoclinic structure formed of [Mg(H2O)6]2- octahedral cations and individual chlorine ions. The structure is quasihexagonal with a distorted hexagonal-close packed arrangement of the two structural groups. . This structure has C2/m space group. First-principles calculations based on density functional perturbation theory indicate the presence of unstable imaginary phonon modes in the zone-center. They are characterized by 153i cm-1 and 57i cm-1 imaginary wavenumbers. Both these modes correspond to tilting of the water molecules. We then investigate these lattice instabilities and find a new structure that is present at low temperatures. The phase transition to this new structure involves the break of the symmetry with the loss of the m symmetry plane and of the inversion center. The new structure is polar with C2 space group.
- Publication:
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AGU Fall Meeting Abstracts
- Pub Date:
- December 2010
- Bibcode:
- 2010AGUFMMR11C1890B
- Keywords:
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- 3672 MINERALOGY AND PETROLOGY / Planetary mineralogy and petrology;
- 5422 PLANETARY SCIENCES: SOLID SURFACE PLANETS / Ices;
- 5460 PLANETARY SCIENCES: SOLID SURFACE PLANETS / Physical properties of materials;
- 5470 PLANETARY SCIENCES: SOLID SURFACE PLANETS / Surface materials and properties