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Openai/691a2d9f-c044-8012-bccf-942bfce6334d
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===== - Comet orbits are typically highly eccentric, bound to the Sun or hyperbolic (escaping) β mostly Solar System-centric. Wikipedia<ref>{{cite web|title=Wikipedia|url=https://en.wikipedia.org/wiki/Comet|publisher=en.wikipedia.org|access-date=2025-11-17}}</ref> ===== * Even long-period comets have orbits of tens of thousands to hundreds of thousands of years within the Solar System, not full stellar transfers. For example: C/1996 B2 (Hyakutake) has an outbound period ~70,000 years. Wikipedia<ref>{{cite web|title=Wikipedia|url=https://en.wikipedia.org/wiki/Comet_Hyakutake|publisher=en.wikipedia.org|access-date=2025-11-17}}</ref> * An orbit that reaches another star system would likely be hyperbolic, unbound, or extremely perturbed; we have very weak data for those. * Interstellar transfer has enormous delta-v, changes in direction, and is far beyond the typical natural comet trajectory.
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