The Formation of MgS & MgO Monomers and Dimers from Magnesium, Oxygen, and Sulfur Hydrides
The reaction of SH + MgH is shown in this quantum chemical study to be an energetically downhill pathway leading to the astronomically known MgS molecule as well as H<sub>2</sub>. Hence, the formation of MgS in the gas phase is now shown to be a possible contributor to this diatomic molecule's observed astronomical abundance. Similarly, MgO can form through a related process with OH + MgH, but the energy costs are higher, implying that MgH could be consumed in reactions with SH faster than those with OH. Hence, MgS may be more abundant than MgO as a result in line with current astronomical observations. Additionally, further additions of MgS/MgO can lead to the dimers of these molecules, indicating that the formation of nanoclusters is possible. These structures could be the building blocks for larger dust grains and mineral-based materials that populate protoplanetary disks and, ultimately, lead to rocky bodies.
Authors
- Ryan C. Fortenberry (ORCID: https://orcid.org/0000-0003-4716-8225)
- Kailey M. Bell
Institutions
- University of Mississippi (US)
Publication Details
- Journal
- Molecules
- Published
- 2025-04-08
- DOI
- https://doi.org/10.3390/molecules30081650
- Citations
- 2
- Primary Topic
- Inorganic Fluorides and Related Compounds
- Type
- article
- Field-Weighted Citation Impact
- 1.07
Funders
- National Aeronautics and Space Administration