Also known as KOI-4878 b
KOI-4878.01 is an exoplanet candidate that orbits the G-type main-sequence star KOI-4878. It is distant from Earth. The features of the planet are very similar to that of Earth, and if it is confirmed, it would be one of the most Earth-like planets found. The orbital period of the exoplanet is around 449 days. It is located within the habitable zone of its parent stara region where water can exist at liquid state.
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Discovered by embedding cosine similarity (sentence-transformers MiniLM, 384-dim).