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Binary star system in the constellation Ursa Major From Wikipedia, the free encyclopedia
78 Ursae Majoris is a binary star system in the northern circumpolar constellation of Ursa Major. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.93.[13] Parallax estimates by Hipparcos put it at a distance of 83 light-years (25 pc),[1] but it is drifting closer with a radial velocity of −5 km/s.[2] The system is a candidate member of the Ursa Major Moving Group.[14]
The binary nature of this system was announced by S. W. Burnham in 1894.[15] The pair orbit each other with a period of 105 years and an eccentricity of 0.39. Their semimajor axis has an angular size of 1.2″ and the orbital plane is inclined by 47°.[8]
The primary member, designated component A, has a magnitude of 5.02[3] and is an F-type main-sequence star with a stellar classification of F2V.[4] It is 785[9] million years old and is spinning with a projected rotational velocity of 92 km/s.[12] The star has 1.34[9] times the mass of the Sun and is radiating 5.75[2] times the Sun's luminosity from its photosphere at an effective temperature of 6,908 K.[9]
The secondary, designated component B, has a visual magnitude of 7.88.[3] It is a G-type main-sequence star with a class of G6V.[5] The star is a suspected variable.[16]
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