TOI-2257 b I

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Proxima Centauri c is a candidate exoplanet which signals were previously detected through radial velocity method in 2020. However, follow-up studies in 2022 later cast doubt on the accuracy of its supposed signals, which was initially attributed to a ring system around the planet, but this doesn't rule out its existence completely

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Отваряне в „Celestia“ (препоръчително) или Изтегляне

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