Ferric iron evolution in magma ocean models

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Abstract/Contents

Abstract: This deposit contains the model code and output for the paper "Ferric iron evolution during crystallization of the Earth and Mars" by Laura Schaefer, Kaveh Pahlevan, and Lindy Elkins-Tanton, which has been submitted for publication at the Journal of Geophysical Research: Planets. The code calculates the bulk oxide evolution of a magma ocean during fractional crystallization and is based on the model of Elkins-Tanton et al. (2003). The code is modified to include the partitioning behavior of ferric iron. We include all model output calculations for the different magma ocean configurations for Earth and Mars, as well as different initial Fe3+/FeT values.

Type of resource	software, multimedia, text, Dataset
Date created	[ca. June 2017 - December 2023]
Date modified	June 14, 2024; June 25, 2024
Publication date	December 20, 2023

Author	Schaefer, Laura
Author	Elkins-Tanton, Lindy

DOI	https://doi.org/10.25740/yg376bh0915, https://doi.org/10.25740/yg376bh0915
Location	https://purl.stanford.edu/yg376bh0915

Use and reproduction: User agrees that, where applicable, content will not be used to identify or to otherwise infringe the privacy or confidentiality rights of individuals. Content distributed via the Stanford Digital Repository may be subject to additional license and use restrictions applied by the depositor.
License: This work is licensed under a Creative Commons Attribution 4.0 International license (CC BY).

Preferred citation: Schaefer, L. (2023). Ferric iron evolution in magma ocean models. Stanford Digital Repository. Available at https://purl.stanford.edu/yg376bh0915. https://doi.org/10.25740/yg376bh0915.

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