Lambda Scorpii is a triple star system and the second-brightest object in the constellation of Scorpius. It is also called Shaula. Lambda Scorpii is its Bayer designation, which is translated from λ Scorpii and abbreviated Lambda Sco or λ Sco. With an apparent visual magnitude of 1.62, it is one of the brightest stars in the night sky.
Quick facts Constellation, Pronunciation ...
λ Scorpii
Location of λ Scorpii (circled) |
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Scorpius |
Pronunciation |
[1][2] |
Right ascension |
17h 33m 36.520s[3] |
Declination |
−37° 06′ 13.76″[3] |
Apparent magnitude (V) |
1.62 + 14.9 + 12.0[3][4] |
Characteristics |
Spectral type |
B1.5IV + B2IV[5][6] |
U−B color index |
−0.880[7] |
B−V color index |
−0.240[7] |
Variable type |
Beta Cephei (A)[8] |
Astrometry |
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|
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Radial velocity (Rv) | −3.00[9] km/s |
Proper motion (μ) | RA: −8.90[3][3] mas/yr Dec.: −29.95[3] mas/yr |
Parallax (π) | 5.71 ± 0.90[3] mas |
Distance | approx. 570 ly (approx. 180 pc) |
Absolute magnitude (MV) | −3.70[10] |
|
Orbit[11] |
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Primary | A |
Companion | B |
Period (P) | 2.8825 yr |
Semi-major axis (a) | 49.3 mas |
Eccentricity (e) | 0.121 |
Inclination (i) | 77.2° |
Orbit[11] |
---|
Primary | Aa |
Companion | Ab |
Period (P) | 5.9520 d |
Eccentricity (e) | 0.26 |
Semi-amplitude (K1) (primary) | 39.3 km/s |
Details |
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λ Sco Aa |
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Mass | 10.4[5] M☉ |
Radius | 8.8±1.2[8] R☉ |
Luminosity | 36,300[8] L☉ |
Surface gravity (log g) | 3.8[6] cgs |
Temperature | 25,000±1,000[8] K |
Rotation | 3.4±0.5 d[8] |
Rotational velocity (v sin i) | 150[8] km/s |
λ Sco B |
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Mass | 8.1[5] M☉ |
Radius | 4.7±1.0[8] R☉ |
Surface gravity (log g) | 4.0[6] cgs |
Temperature | 25,000±1,000[8] K |
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λ Sco Ab |
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Mass | 1.8[5] M☉ |
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Other designations |
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Shaula, 35 Scorpii, 35 Sco, CD−37 11673, FK5 652, HD 158926, HIP 85927, HR 6527, SAO 208954, CCDM J17336-3706A/B/C |
Database references |
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SIMBAD | data |
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