Sośnicka M, Lüders V. Phase transitions in natural C-O-H-N-S fluid inclusions - implications for gas mixtures and the behavior of solid H
2S at low temperatures.
Nat Commun 2021;
12:6975. [PMID:
34848726 PMCID:
PMC8633383 DOI:
10.1038/s41467-021-27269-6]
[Citation(s) in RCA: 1] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Key Words] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/27/2020] [Accepted: 11/08/2021] [Indexed: 11/09/2022] Open
Abstract
C-O-H-N-S-bearing fluids are known as one of the most challenging geochemical systems due to scarcity of available experimental data. H2S-rich fluid systems were recognized in a wide array of world-class mineral deposits and hydrocarbon reservoirs. Here we report on a nature of low-temperature (T ≥ -192 °C) phase transitions observed in natural CH4-H2S-CO2-N2-H2O fluid inclusions, which are modeled as closed thermodynamic systems and thus serve as natural micro-laboratories representative of the C-O-H-N-S system. For the first time, we document solid-solid H2S (α ↔ β ↔ γ) transitions, complex clathrates and structural transformations of solid state H2S in natural inclusion gas mixtures. The new data on Raman spectroscopic features and a complete sequence of phase transition temperatures in the gas mixtures contribute to scientific advancements in fluid geochemistry. Enhanced understanding of the phase equilibria in the C-O-H-N-S system is a prerequisite for conscientious estimation of P-T-V-X properties, necessary to model the geologic evolution of hydrocarbon and mineral systems. Our findings are a driver for the future research expeditions to extraterrestrial H2S-rich planetary systems owing to their low temperature environments.
Collapse