Magma ocean evolution on GJ 1132 b
Overview
Thermal and volatile evolution of GJ 1132 b’s mantle and atmosphere during its magma ocean phase.
Date |
08/21/20 |
Author |
Patrick Barth |
Planet name |
GJ 1132 b |
Initial water content |
100 TO |
Modules |
AtmEsc, MagmOc, STELLAR |
Approx. runtime |
3 minutes |
To run this example
python makeplot.py
Expected output

Evolution of various planetary parameters for the magma ocean evolution of GJ 1132 b with an initial water inventory that is 100 that of the modern Earth. The planet radiatively cools with VPLanet’s grey atmosphere model. Counter-clockwise from top left: Mantle and surface temperature; water masses in the different reservoirs; atmospheric pressures; atmospheric net cooling flux; melt fraction of the magma ocean (not including solidified mantle); mass fraction of water and Fe2O3 in the melt; oxygen mass in different reservoirs; solidification radius of the magma ocean.