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Rigel

Rigel, Beta Ori Rigel is the lower right star in the rectangle of bright stars in Orion. Observation data Epoch J2000.0      Equinox J2000.0 Constellation Orion Pronunciation /'ra?d??l, -g?l/ Right ascension 05h 14m 32.27210s Declination -08° 12' 05.8981? Apparent magnitude (V) 0.12 Characteristics Spectral type B8 Iae: U-B color index -0.66 B-V color index -0.03 Variable type Slightly irregular Astrometry Radial velocity (Rv) 20.7 km/s Proper motion (µ) RA: +1.31 mas/yr Dec.: +0.50 mas/yr Parallax (p) 3.78 ± 0.34 mas Distance 860 ± 80 ly (260 ± 20 pc) Absolute magnitude (MV) –7.84 ± 0.2 Details Mass 24 ± 3 M? Radius 71 R? Luminosity (bolometric) 96,456 L? Surface gravity (log g) 1.75 ± 0.10 Temperature 12,130 K Metallicity –0.06 ± 0.10 dex Rotational velocity (v sin i) 40 km/s Age (8 ± 1) × 106 years Other designations Database references SIMBAD data Computer generated image of Rigel compared to the Sun (to scale) Rigel (ß Ori, ß Orionis, Beta Orionis) is the brightest star in the constellation Orion and the sixth brightest star in the sky, with visual magnitude 0.18. Although it has the Bayer designation "beta", it is almost always brighter than Alpha Orionis (Betelgeuse). Since 1943, the spectrum of this star has served as one of the stable anchor points by which other stars are classified. Cite error: There are tags on this page, but the references will not show without a {{Reflist}} template or a tag; see the help page.
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