Mu Ursae Majoris
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. Parallax measurements give an estimated distance of roughly 230 light-years (71 parsecs) from the Sun, with a margin of error of 4%.
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 |
Distance | 183 ± 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 | |
Mass | 6.3 M☉ |
Radius | 75 R☉ |
Luminosity | 977–1,200 L☉ |
Surface gravity (log g) | 1.0 cgs |
Temperature | 3,899 K |
Metallicity [Fe/H] | +0.00 dex |
Rotational velocity (v sin i) | 7.5 km/s |
companion | |
Mass | 0.96 M☉ |
Other designations | |
Database references | |
SIMBAD | data |
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