15 Boötis
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15 Boötis is a binary star[3] system in the northern constellation of Boötes,[8] located approximately 260 light years away from the Sun.[2] It is visible to the naked eye as a dim, orange-hued star with an apparent visual magnitude of 5.45.[3] The system has a relatively high proper motion, traversing the celestial sphere at the rate of 0.166 arc seconds per annum.[9] It is moving away from the Earth with a heliocentric radial velocity of +16.8 km/s.[1]
The magnitude 5.51[3] primary, designated component A, is an aging K-type giant star with a stellar classification of K1 III.[5] It is a red clump giant,[4] which indicates it is on the horizontal branch and is generating energy through helium fusion at its core. It is around two[6] billion years old with 1.5[6] times the mass of the Sun and has expanded to 10[7] times the Sun's radius. The star is radiating 61[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,845 K.[6]
Its companion, component B, is a magnitude +8.53 star[3] was located at an angular separation of Script error: No such module "val". along a position angle of 111° from the primary, as of 2015. This is the same separation it had when the system was discovered in 1936.[10]
References
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