Abstract
Geochemical and geophysical processes controlled by the presence of water have a large impact both on Earth and within the icy moons of the outer Solar System. Here, three projects relating to hydrous systems are presented. In the first, the partitioning of F and Cl between amphibole and melt at conditions relevant to hydrous arc magmas was investigated using experimental runs, where it is determined that F is moderately compatible in amphibole at crustal conditions. This result indicates that the Cl/F ratio of erupted lavas may be controlled by amphibole cumulates at depth. In the second project, the strength of icy moon seafloors was modeled, where it was determined that common sources of stress cannot drive fault motion in the present day, indicating that little unaltered rock may be exposed to the seafloor. In the final project, the effect of ammonia on H2 production during serpentinization was determined through paired high and low temperature experiments. It is found that the presence of ammonia lowers the rate of serpentine formation at high temperatures and lowers H2 production at low temperatures.
Committee Chair
Paul Byrne
Committee Members
Jeffrey Catalano; Michael Krawczynski; Tansu Daylan; William McKinnon
Degree
Doctor of Philosophy (PhD)
Author's Department
Earth & Planetary Sciences
Document Type
Dissertation
Date of Award
8-11-2026
Language
English (en)
DOI
https://doi.org/10.7936/eqk5-z403
Recommended Citation
Dawson, Henry, "Investigation of Mineral Formation and Alteration in Hydrous Systems" (2026). Arts & Sciences Graduate Student Theses and Dissertations. 3825.
The definitive version is available at https://doi.org/10.7936/eqk5-z403