Kepler-25 [SEP] constellation
Kepler-25
Kepler-25 is a star in the northern constellation of Lyra. It is located at the celestial coordinates: 
Right Ascension Declination . With an apparent visual magnitude of 10.7, this star is too faint to be seen with the naked eye.
In 2012, two planets were found transiting the star. These planets were confirmed through transit-timing variation method. A third planet was discovered through follow-up radial velocity measurements which was confirmed in January 2014.
Kepler-25b
Kepler-25b is an extrasolar planet orbiting the star Kepler-25, located in the constellation Cygnus. It was discovered by the Kepler Space Telescope in 2012. Kepler-25b is one of the most massive planets ever found. if it had the equivalent of 1 extra Saturn mass, it would be considered a brown dwarf, as it has ≈12,7 Jupiter Masses. ≥13 Jupiter Masses is required for deuterium fusion.