"Investigations into Mercury’s mantle through the partial melting of En" by Richard M. Gwyn

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Date of Award

Fall 2024

Document Type

Masters Thesis

Department or Program Affiliation

Geology

Degree Name

Master of Science (MS)

Department

Geology

First Advisor

Boujibar, Asmaa

Second Advisor

Walowski, Kristina

Third Advisor

Mulcahy, Sean

Abstract

The mantle and surface of Mercury exhibit distinct characteristics that set it apart from other terrestrial bodies, largely due to its extremely low oxygen fugacity (fO₂). This reduced state has resulted in unique compositional features, such as the planet's depletion in FeO and enrichment in volatile elements (e.g., Na, K, S). These properties present a challenge in understanding terrestrial differentiation processes on Mercury. To investigate these features, I conducted high-pressure, high-temperature partial melting experiments on enstatite chondrite (EH) compositions, simulating Mercury-like conditions. These experimental results were paired with thermodynamic modeling (using pMELTS) to capture the effects of varying fO₂ on Mercury’s mantle compositions and melting behaviors. This study’s findings were compared to MESSENGER mission surface composition data to assess the feasibility of EH chondrites as Mercury’s primary building blocks.

This study demonstrates that fO₂ could be a key factor influencing Mercury’s mantle melting behavior and surface composition. At lower fO₂ conditions, silicon preferentially partitions into the metallic phase, resulting in silicate melts with elevated Mg/Si, Ca/Si and Al/Si ratios. Thermodynamic modeling enabled us to estimate partial melt compositions at 1 GPa and 1300-1650°C between the silicate solidus and liquidus. These resulting melt compositions closely align with the geochemical signatures observed on Mercury’s surface, as reported by MESSENGER. Silicate melt compositions range from picro-basalt to phonolite, highlighting how the reduced conditions of Mercury’s mantle are a key factor in generating its surface geochemical diversity. Variations in mantle fO₂ can drive complex magmatic differentiation and volcanic evolution in reduced planetary systems.

Type

Text

Keywords

Mercury, Mantle, Magma Ocean, Oxygen Fugacity, Enstatite Chondrites

Publisher

Western Washington University

OCLC Number

1483965402

Subject – LCSH

Mercury (Planet)--Geology; Magmas; Chondrites (Meteorites); Thermodynamics; Thermochemistry

Geographic Coverage

Mercury (Planet)

Format

application/pdf

Genre/Form

masters theses

Language

English

Rights

Copying of this document in whole or in part is allowable only for scholarly purposes. It is understood, however, that any copying or publication of this document for commercial purposes, or for financial gain, shall not be allowed without the author’s written permission.

Rights Statement

http://rightsstatements.org/vocab/NKC/1.0/

Included in

Geology Commons

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