Elasticity of methane hydrate phases at high pressure

Determination of the full elastic constants (cij) of methane hydrates (MHs) at extreme pressure-temperature environments is essential to our understanding of the elastic, thermodynamic, and mechanical properties of methane in MH reservoirs on Earth and icy satellites in the solar system. Here, we ha...

Full description

Bibliographic Details
Published in:The Journal of Chemical Physics
Main Authors: Beam, Jennifer, Yang, Jing, Liu, Jin, Liu, Chujie, Lin, Jung-Fu
Other Authors: Burke Undergraduate Research Fund of the Department of Geological Sciences, the University of Texas, Extreme Physics and Chemistry Program of the Deep Carbon Observatory, Seed Grant of the Jackson School of Geosciences
Format: Article in Journal/Newspaper
Language:English
Published: AIP Publishing 2016
Subjects:
Methane hydrate
Online Access:http://dx.doi.org/10.1063/1.4946795
https://pubs.aip.org/aip/jcp/article-pdf/doi/10.1063/1.4946795/15511595/154501_1_online.pdf
Description
Summary:Determination of the full elastic constants (cij) of methane hydrates (MHs) at extreme pressure-temperature environments is essential to our understanding of the elastic, thermodynamic, and mechanical properties of methane in MH reservoirs on Earth and icy satellites in the solar system. Here, we have investigated the elastic properties of singe-crystal cubic MH-sI, hexagonal MH-II, and orthorhombic MH-III phases at high pressures in a diamond anvil cell. Brillouin light scattering measurements, together with complimentary equation of state (pressure-density) results from X-ray diffraction and methane site occupancies in MH from Raman spectroscopy, were used to derive elastic constants of MH-sI, MH-II, and MH-III phases at high pressures. Analysis of the elastic constants for MH-sI and MH-II showed intriguing similarities and differences between the phases′ compressional wave velocity anisotropy and shear wave velocity anisotropy. Our results show that these high-pressure MH phases can exhibit distinct elastic, thermodynamic, and mechanical properties at relevant environments of their respective natural reservoirs. These results provide new insight into the determination of how much methane exists in MH reservoirs on Earth and on icy satellites elsewhere in the solar system and put constraints on the pressure and temperature conditions of their environment.

Similar Items