This is a spectroscopic binary star system with a companion a mere 0.2 AU from the primary, assuming a distance of 71 parsecs, with an orbital period of 230 days.

TODO

Look at the following paper and confirm the distance is 0.2 AU. Other sources give a larger distance. See desigation HIP 50801. https://iopscience.iop.org/article/10.1088/0004-6256/145/3/81

binary star of

Tania Australis

citation

Wikipedia contributors. (2024, July 21). Mu Ursae Majoris. In Wikipedia, The Free Encyclopedia. Retrieved August 2, 2024, from https://en.wikipedia.org/w/index.php?title=Mu_Ursae_Majoris&oldid=1235876804

note

This is closer to the star than Mercury is to the Sun (the semi-major axis of Mercury is 0.387098 AU)

random

In a short interview with Lanny Poffo, he stated that the movie meant so much to André that he made his wrestling pals watch an advanced copy of the VHS with him over and over again while supplying dinner, drinks, and sweetly asking each time, “Did you like my performance?”

see also

Mercury (Wikipedia)

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Mu Ursae Majoris (Wikipedia) Mu Ursae Majoris (μ Ursae Majoris, abbreviated Mu UMa, μ UMa), formally named Tania Australis /ˈteɪniə ɔːˈstreɪlɪs/, is a binary star in the constellation of Ursa Major. An apparent visual magnitude of +3.06 places it among the brighter members of the constellation.

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