Mu Ursae Majoris

Mu Ursae Majoris (μ Ursae Majoris, abbreviated Mu UMa, μ UMa), formally named Tania Australis /ˈtniə ɔːˈstrlɪs/, 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. Parallax measurements give an estimated distance of roughly 230 light-years (71 parsecs) from the Sun, with a margin of error of 4%.

Mu Ursae Majoris

Location of μ Ursae Majoris (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Ursa Major
Right ascension 10h 22m 19.73976s
Declination +41° 29 58.2691
Apparent magnitude (V) +3.06
Characteristics
Evolutionary stage AGB
Spectral type M0 IIIab
U−B color index +1.90
B−V color index +1.59
Variable type suspected
Astrometry
Radial velocity (Rv)−21.30±1.66 km/s
Proper motion (μ) RA: –81.47 mas/yr
Dec.: +35.34 mas/yr
Parallax (π)17.7987 ± 0.3933 mas
Distance183 ± 4 ly
(56 ± 1 pc)
Absolute magnitude (MV)−1.11±0.083
Orbit
Period (P)230.089 days
Semi-major axis (a)0.0028″
Eccentricity (e)0.061
Inclination (i)13.6°
Periastron epoch (T)2425577.030 JD
Argument of periastron (ω)
(secondary)
236.4°
Semi-amplitude (K1)
(primary)
7.40 km/s
Details
Mass6.3 M
Radius75 R
Luminosity977–1,200 L
Surface gravity (log g)1.0 cgs
Temperature3,899 K
Metallicity [Fe/H]+0.00 dex
Rotational velocity (v sin i)7.5 km/s
companion
Mass0.96 M
Other designations
Tania Australis, Alkafzah al Thaniyah, μ Ursae Majoris, μ UMa, Mu UMa, 34 Ursae Majoris, BD+42 2115, FK5 386, GC 14232, HD 89758, HIP 50801, HR 4069, PPM 51850, SAO 43310
Database references
SIMBADdata
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