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Theta Muscae

Theta Muscae
Musca constellation map.svg
Red circle.svg

Location of θ Mus (circled)
Observation data
Epoch 2000      Equinox 2000
Constellation Musca
Right ascension 13h 08m 07.15286s
Declination −65° 18′ 21.6819″
Apparent magnitude (V) 5.53(5.662 + 7.555)
Characteristics
θ Mus A
Spectral type WC5/6 + O6/7V + O9.5/B0Iab
U−B color index −0.91
B−V color index −0.43
Variable type Eclipsing + WR
B
Spectral type O9III
U−B color index −0.90
B−V color index −0.055
Astrometry
Radial velocity (Rv) −28.4 km/s
Proper motion (μ) RA: -2.10 mas/yr
Dec.: −11.52 mas/yr
Parallax (π) 0.26 ± 0.48mas
Distance 7,400ly
(2,270pc)
Absolute magnitude (MV) −6.2
Details
WR
Mass <11.5 M
Luminosity 230,000 L
Other designations
Theta Muscae, CD−64° 699, HR 4952, HD 113904, HIP 64094, GSC 08997-02337, SAO 252162, PPM 359890, GC 17788, UCAC3 50-186265, IRAS 15465+2818, WR 48
Database references
SIMBAD data

Theta Muscae (θ Mus) is a multiple star system in the southern constellation Musca ("the Fly") with an apparent magnitude of 5.5. It is the second brightest Wolf–Rayet star in the sky, although much of the visual brightness comes from the massive companions and it is not one of the closest of its type.

Theta Muscae is a remote triple star system, the primary component of which is a carbon-sequence Wolf–Rayet star. This is a variety of highly-luminous hot blue star that has blown off its hydrogen envelope and is emitting heavier elements, in this case carbon, amid a strong stellar wind. Theta Muscae is the second-brightest such star in the sky after Gamma Velorum in Vela. θ Mus is beyond the current reach of useful visual parallax measurements, but has been estimated as around 7,400 light-years (460 million astronomical units) from Earth. While cataloging the stars in the far-southern sky, French explorer and astronomer Nicolas Louis de Lacaille gave the star its Bayer designation in 1756.

To small telescopes, Theta Muscae appears as a double star, with a blue-cream brighter star and an O9III companion of magnitude 7.3 some 5.3 arcseconds away. The primary θ Muscae A is a massive triple star system.


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Wikipedia

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