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.
F., Tsiganis, K., & Gomes, R
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Simulations of solar analogues in stellar clusters demonstrate that extended debris disks perturbed by stellar encounters form Oort cloud-like structures and interstellar comets, while compact disks produce Kuiper-belt analogues.
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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Implications for the formation of Oort cloud-like structures and interstellar comets in dense environments
Simulations of solar analogues in stellar clusters demonstrate that extended debris disks perturbed by stellar encounters form Oort cloud-like structures and interstellar comets, while compact disks produce Kuiper-belt analogues.