Roche lobe overflow during gas giant destruction aligns stellar spins with orbits within tens of degrees regardless of starting conditions, offering an observable to differentiate this mechanism from high-eccentricity migration.
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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.
Stellar spindown cannot trigger secular resonance crossings in regular peas-in-a-pod systems, requiring inner-planet migration instead, and resonance crossing times vary across stellar evolution tracks.
citing papers explorer
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Revealing the Origin of Desert Dwellers via Stellar Obliquities
Roche lobe overflow during gas giant destruction aligns stellar spins with orbits within tens of degrees regardless of starting conditions, offering an observable to differentiate this mechanism from high-eccentricity migration.
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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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Peas and USPs: Can Stellar Spindown and Peas in a Pod Replicate Ultra-Short-Period Planet Characteristics?
Stellar spindown cannot trigger secular resonance crossings in regular peas-in-a-pod systems, requiring inner-planet migration instead, and resonance crossing times vary across stellar evolution tracks.