Lambda Scorpii

Triple star system in the constellation Scorpius From Wikipedia, the free encyclopedia

Lambda Scorpii is a triple star system and the second-brightest object in the constellation of Scorpius. It is formally named Shaula; Lambda Scorpii is its Bayer designation, which is Latinised from λ Scorpii and abbreviated Lambda Sco or λ Sco. With an apparent visual magnitude of 1.63, 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 /ˈʃɔːlə/[1][2]
Right ascension 17h 33m 36.520s[3]
Declination −37° 06 13.76[3]
Apparent magnitude (V) 1.63[4]
Characteristics
Evolutionary stage Main sequence (A and B)[5] + pre-main sequence (a)[6]
Spectral type B1.5IV + B2IV[5][7]
U−B color index −0.880[8]
B−V color index −0.240[8]
Variable type Beta Cephei (Aa1)[6] + Algol (Aa1/2) [9]
Astrometry
Radial velocity (Rv)−3.00[10] km/s
Proper motion (μ) RA: −8.90[3] mas/yr[3]
Dec.: −29.95 mas/yr[3]
Parallax (π)5.71±0.90 mas[3]
Distanceapprox. 570 ly
(approx. 180 pc)
Absolute magnitude (MV)−3.70[11]
Orbit[12]
PrimaryAa
NameAb
Period (P)2.8825 yr
Semi-major axis (a)49.3 mas
Eccentricity (e)0.121
Inclination (i)77.2°
Orbit[12]
PrimaryAa1
NameAa2
Period (P)5.9520 d
Eccentricity (e)0.26
Semi-amplitude (K1)
(primary)
39.3 km/s
Details
λ Sco Aa1 (A)
Mass10.4[5] M
Radius8.8±1.2[6] R
Luminosity36,300[6] L
Surface gravity (log g)3.8[7] cgs
Temperature25,000±1,000[6] K
Rotation3.4±0.5[6] days
Rotational velocity (v sin i)150[6] km/s
λ Sco Aa2 (a)
Mass2.0±0.2[6] M
Radius1.5±0.2[6] R
λ Sco Ab (B)
Mass8.1[5] M
Radius4.7±1.0[6] R
Surface gravity (log g)4.0[7] cgs
Temperature25,000±1,000[6] K
Other designations
Shaula, 35 Scorpii, 35 Sco, CD−37 11673, FK5 652, HD 158926, HIP 85927, HR 6527, SAO 208954, CCDM J17336-3706A
Database references
SIMBADdata
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Nomenclature

λ Scorpii (Latinised to Lambda Scorpii) is the star system's Bayer designation.

It bore the traditional name Shaula, which comes from the Arabic الشولاء al-šawlā´ meaning 'the raised [tail]', as it is found in the tail of Scorpius, the scorpion. In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[13] to catalog and standardize proper names for stars. The WGSN's first bulletin of July 2016[14] included a table of the first two batches of names approved by the WGSN, which included Shaula for the star λ Scorpii Aa1.

In Indian astronomy, it is part of the asterism Mula with other stars in the tail of Scorpius. Mūla ("root") (Devanagari मूल/मूळ) (Tamil: மூலம்) is the 19th nakshatra or "lunar mansion" in Vedic astrology. The symbol of Mula is a bunch of roots tied together (reticulated roots) or an 'elephant goad' (ankusha).[15]

In Chinese, 尾宿 (Wěi Xiù), meaning Tail, refers to an asterism consisting of λ Scorpii, ε Scorpii, ζ1 Scorpii, ζ2 Scorpii, η Scorpii, θ Scorpii, ι1 Scorpii, ι2 Scorpii, κ Scorpii, μ1 Scorpii, and υ Scorpii.[16] Consequently, the Chinese name for λ Scorpii itself is 尾宿八 (Wěi Xiù bā), "the Eighth Star of Tail".[17]

Together with υ Scorpii (Lesath), Shaula is listed in the Babylonian compendium MUL.APIN as dSharur4 u dShargaz, meaning "Sharur and Shargaz".[18] In Coptic, these two stars were called Minamref.[19]

The indigenous Boorong people of northwestern Victoria (Australia) named it (together with Upsilon Scorpii) Karik Karik,[20] "the Falcons".[21]

Properties

A light curve for Lambda Scorpii, plotted from TESS data.[22] The large dips in brightness are eclipses, and the rapid oscillations show the Beta Cephei variability.

Lambda Scorpii is located approximately 570 light-years away from the Sun.

Spectroscopic and interferometric observations have shown that it is actually a triple star system consisting of two B-type stars and a pre-main-sequence star.[6] The primary star is a Beta Cephei variable star with rapid brightness changes of about a hundredth of a magnitude.[7][5] The pre-main-sequence star has an orbital period of 6 days and the B-type companion has a period of 1,053 days. The three stars lie in the same orbital plane, strongly suggesting that they were formed at the same time. The masses of the primary, pre-main-sequence star and the B-type companion are 14.5, 2.0 and 10.6 solar masses, respectively. The age of the system is estimated to be in the range 10–13 million years. Shaula Aa1 has sufficient mass to explode as a supernova.[23]

A 15th-magnitude star has a separation of 42 arcseconds, whereas a 12th-magnitude star is 95 arcseconds away. It is not known whether or not these components are physically associated with Lambda Scorpii. If they both were, the first would have a projected linear separation of approximately 7,500 astronomical units (AU) and the second approximately 17,000 AU (0.27 light-years) away. Gaia Data Release 3 reports that the fainter of these two stars is a little larger and brighter than the sun and about 420 light years away,[24] while the brighter star is a background object.[25]

In culture

Shaula appears on the flag of Brazil, symbolizing the state of Rio Grande do Norte.

USS Shaula (AK-118) was a U.S. Navy Crater-class cargo ship named after the star.

Shaula is the namesake of a character in Re:Zero, a Japanese web/light novel series by Tappei Nagatsuki.

References

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