Star in the constellation Ophiuchus From Wikipedia, the free encyclopedia
μ Ophiuchi, Latinized as Mu Ophiuchi, is a solitary,[10] blue-white hued star in the equatorial constellation of Ophiuchus. It is visible to the naked as a faint point of light with an apparent visual magnitude of 4.62.[2] This object is located approximately 760 light years away from the Sun based on parallax,[5] but is drifting closer with a radial velocity of −18.5 km/s.[4]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ophiuchus |
Right ascension | 17h 37m 50.71308s[1] |
Declination | −8° 07′ 07.5749″[1] |
Apparent magnitude (V) | 4.62[2] |
Characteristics | |
Spectral type | B8II-IIIp:Mn[3] |
U−B color index | −0.20[2] |
B−V color index | +0.11[2] |
Astrometry | |
Radial velocity (Rv) | −18.50[4] km/s |
Proper motion (μ) | RA: −11.31[5] mas/yr Dec.: −20.47[5] mas/yr |
Parallax (π) | 4.32 ± 0.20 mas[5] |
Distance | 750 ± 30 ly (230 ± 10 pc) |
Absolute magnitude (MV) | -2.24[6] |
Details | |
Radius | 11.1+2.1 −0.6[1] R☉ |
Luminosity | 398.7±26.8[1] L☉ |
Temperature | 7,748+210 −651[1] K |
Metallicity [Fe/H] | +0.00[7] dex |
Rotational velocity (v sin i) | 95[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
This object has a stellar classification of B8II-IIIp:Mn,[3] showing a luminosity class with mixed traits of a giant or bright giant star. The suffix notation indicates it is a candidate chemically peculiar star with an overabundance of manganese in its spectrum. It may be a mercury-manganese star.[11] This object has 11 times the radius of the Sun and is radiating nearly 400 times the Sun's luminosity from its photosphere at an effective temperature of 7,748 K.[1] It is spinning with a projected rotational velocity of 95 km/s.[8]
In 2006, a new nearby star cluster, Mamajek 2 (/ˈmæmədʒɛk/), was discovered. Mu Ophiuchi is a candidate member.[12] The cluster has an estimated age of 120±25 million years.[13]
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