N-body simulations show gas drag prevents efficient outward scattering of CM-like planetesimals beyond 15 au during Saturn's growth, yielding at most 0.02-0.04 Earth masses of CM material in the outer ring and negligible CI contamination.
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2 Pith papers cite this work. Polarity classification is still indexing.
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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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Shaken, not stirred: inefficient mixing of CM- and CI-like materials
N-body simulations show gas drag prevents efficient outward scattering of CM-like planetesimals beyond 15 au during Saturn's growth, yielding at most 0.02-0.04 Earth masses of CM material in the outer ring and negligible CI contamination.
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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.