Coupled thermal-orbital models show lava planets undergo two-stage migration from ~0.1 AU requiring initial eccentricities >=0.9 and sustained forcing, with migration rate depending on mantle state.
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Top-heavy thermochemical geodynamo simulations show heterogeneous outer boundary heat flux reproduces observed longitudinal inclination anomaly variations, while elevated chemical driving reduces longitudinal structures and promotes polar radial field minima.
Barnard's Star planets have masses 0.19-0.84 M_earth, are tidally locked, unlikely to retain primary atmospheres, and possess mantles rich in ferropericlase with less than half Earth's water capacity and radiogenic heating.
citing papers explorer
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Coupled orbital and interior structure evolution of lava planets
Coupled thermal-orbital models show lava planets undergo two-stage migration from ~0.1 AU requiring initial eccentricities >=0.9 and sustained forcing, with migration rate depending on mantle state.
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Paleomagnetic signatures of core-mantle interactions inferred from top-heavy thermochemical geodynamo simulations
Top-heavy thermochemical geodynamo simulations show heterogeneous outer boundary heat flux reproduces observed longitudinal inclination anomaly variations, while elevated chemical driving reduces longitudinal structures and promotes polar radial field minima.
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The Barnard's Star Planetary System: Stability, Composition, and Evolution of Four Sub-Earth Exoplanets
Barnard's Star planets have masses 0.19-0.84 M_earth, are tidally locked, unlikely to retain primary atmospheres, and possess mantles rich in ferropericlase with less than half Earth's water capacity and radiogenic heating.