
Kepler-1649 is a red dwarf star of spectral type M5V with a radius , a mass , and a metallicity of -0.15 [Fe/H].
Kepler-1649 is a red dwarf star of spectral type M5V with a radius , a mass , and a metallicity of -0.15 [Fe/H].
==Planetary system== thumb|left|Artist's impression and size comparison of the two planets in the Kepler-1649 system with Earth Two confirmed planets orbit the star: Kepler-1649b and Kepler-1649c. Kepler-1649b is similar to Venus, whereas Kepler-1649c is a potentially habitable exoplanet similar to Earth.
Discovered by embedding cosine similarity (sentence-transformers MiniLM, 384-dim).