1 Scorpii

Star in the constellation Scorpius From Wikipedia, the free encyclopedia

1 Scorpii, or b Scorpii, is a single[9] star in the southern zodiac constellation of Scorpius. It has an apparent magnitude of 4.63,[1] which is bright enough to be faintly visible to the naked eye on a dark night. The star shows an annual parallax shift of 6.59 mas from Earth's orbit, which equates to a distance of roughly 490 light years. It is a probable (89% chance) member of the Sco OB2 moving group.[10][9]

Quick facts Observation data Epoch J2000.0 Equinox J2000.0, Constellation ...
1 Scorpii
Location of 1 Scorpii (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Scorpius[1]
Right ascension 15h 50m 58.74452s[2]
Declination −25° 45 04.6649[2]
Apparent magnitude (V) 4.63[1]
Characteristics
Spectral type B1.5 Vn[3]
B−V color index −0.072±0.003[1]
Astrometry
Radial velocity (Rv)−3.0±4.7[4] km/s
Proper motion (μ) RA: −14.20[2] mas/yr
Dec.: −25.12[2] mas/yr
Parallax (π)6.59±0.27 mas[2]
Distance490 ± 20 ly
(152 ± 6 pc)
Absolute magnitude (MV)−1.27[1]
Details
Mass8.3±0.2[5] M
Radius3.7[6] R
Luminosity3,890[6] L
Temperature24,000[6] K
Rotational velocity (v sin i)310[7] km/s
Age10.3±5.3[5] Myr
Other designations
b Sco, 1 Sco, CD−25°11131, HD 141637, HIP 77635, HR 5885, SAO 183854[8]
Database references
SIMBADdata
Close

This is a B-type main-sequence star with a stellar classification of B1.5 Vn,[3] where the 'n' suffix indicates "nebulous" absorption lines being induced by rapid rotation. It has a projected rotational velocity of 310 km/s, which is giving the star an oblate shape with an equatorial bulge that is 13% wider than the polar radius.[7] There is some weak evidence that this is a Be star with a gaseous disk that is being viewed edge-on.[11]

1 Scorpii is a young star at around 10[5] million years old, with 8.3[5] times the mass of the Sun and 3.7 times the Sun's radius.[6] The star is radiating 3,890 times the Sun's luminosity from its photosphere at an effective temperature of about 24,000 K.[6]

References

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