Magma ocean thermal evolution model for determining basal pressure of last equilibration (bPLE)

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Abstract/Contents

Abstract: This is a modified version of the magma ocean thermal evolution model of Schaefer et al. (2016) Astrophysical Journal, 829:63. This code has been modified for habitable zone planets, and to test different solidus and liquidus temperatures as well as the solidus-liquidus offset. There are two versions of the code included to do calculations for Earth and Mars. This model is use in support of the paper " Ferric iron evolution during crystallization of the Earth and Mars" by Laura Schaefer, Kaveh Pahlevan, and Lindy Elkins-Tanton, submitted to Journal of Geophysical Research: Planets.

Author	Schaefer, Laura

Related item	Preferred citation Schaefer et al. (2016) ApJ, 829: 63, doi:10.3847/004-637X/829/2/63
DOI	https://doi.org/10.25740/rk050tc3031, https://doi.org/10.25740/rk050tc3031
Location	https://purl.stanford.edu/rk050tc3031

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License: This work is licensed under a Creative Commons Attribution 4.0 International license (CC BY).

Preferred citation: Schaefer, L. (2023). Magma ocean thermal evolution model for determining basal pressure of last equilibration (bPLE). Stanford Digital Repository. Available at https://purl.stanford.edu/rk050tc3031. https://doi.org/10.25740/rk050tc3031.

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