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.
via Wikipedia infobox
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.
== Host star == KOI-4878 is a G-type main-sequence star, more precisely of spectral class G4V. It has an apparent magnitude of 12.37 and is located in the constellation of Draco. The star has a mass of , a radius of and an effective temperature of . Its age is estimated at billion years, older than the Solar System.
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Discovered by embedding cosine similarity (sentence-transformers MiniLM, 384-dim).