Magma ocean thermal evolution model for determining basal pressure of last equilibration (bPLE)
- 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.
|Type of resource
|software, multimedia, text
|[ca. November 2022 - November 2023]
|December 20, 2023
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