KELT-2 (also called HD 42176) is a binary star located about 439 light-years away in the constellation Auriga. The apparent magnitude of the system is 8.68, which means it is not visible to the naked eye but can be seen with binoculars. The system is moving towards the Sun at over 40 km/s.
Description KELT-2A is the primary star in the common-proper-motion binary star system KELT-2 (HD 42176). It is an F-type main sequence star about 1.314 times as massive as the sun. It has about 1.84 times the Sun's radius and radiates 3.5 times the Sun's luminosity at a temperature of about 6148 K. It is 3.97 billion years old and has a rotational velocity of around 9 km/s. KELT-2B is an early K dwarf approximately 295 AU away, which was discovered simultaneously with the planet KELT-2Ab in 2012. It has 78% of the Sun's mass, 70% of its radius, and an effective temperature of 4850±150 K.
Planetary system This star has one known planet, the extrasolar planet KELT-2Ab, a hot jupiter orbiting the star at an average distance of 0.05504±0.00086 AU with an orbital period of 4.11379±0.00001 days.
See also KELT
References
External links KELT-North survey website Archived 2019-01-24 at the Wayback Machine "Planet KELT-2A b". Extrasolar Planets Encyclopaedia. Archived from the original on 2012-10-19. Retrieved 2012-07-30.
