Multi-planet systems reach local pairwise tidal equilibria with equal masses and regular spacing, matching observations but not a global energy minimum, and implying a steep surface density profile.
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Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.
citing papers explorer
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Pairwise Tidal Equilibrium States and the Architecture of Extrasolar Planetary Systems
Multi-planet systems reach local pairwise tidal equilibria with equal masses and regular spacing, matching observations but not a global energy minimum, and implying a steep surface density profile.
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The role of inner disk edges in shaping ultra-short-period planet systems around late M dwarfs
Ultra-short-period planet formation around late M dwarfs occurs only in fixed close-in or inward-evolving inner disk edge scenarios, as planets follow the edge movement in simulations.