Lambda Scorpii
Template:Location mark Location of λ Scorpii (circled) | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Scorpius |
| Pronunciation | Script error: No such module "IPAc-en".[1][2] |
| Right ascension | Template:RA[3] |
| Declination | Template:DEC[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 Template:Engvar | −0.880[8] |
| B−V Template:Engvar | −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] |
| Distance | approx. Template:Rnd ly (approx. Template:Rnd pc) |
| Absolute magnitude (MV) | −3.70[11] |
| Orbit[12] | |
| Primary | Aa |
| Companion | Ab |
| Period (P) | 2.8825 yr |
| Semi-major axis (a) | Script error: No such module "val". |
| Eccentricity (e) | 0.121 |
| Inclination (i) | 77.2° |
| Orbit[12] | |
| Primary | Aa1 |
| Companion | Aa2 |
| Period (P) | Script error: No such module "val". |
| Eccentricity (e) | 0.26 |
| Semi-amplitude (K1) (primary) | 39.3 km/s |
| Details | |
| λ Sco Aa1 (A) | |
| Mass | 10.4[5] Template:Solar mass |
| Radius | Script error: No such module "val".[6] Template:Solar radius |
| Luminosity | 36,300[6] Template:Solar luminosity |
| Surface gravity (log g) | 3.8[7] cgs |
| Temperature | Script error: No such module "val".[6] K |
| Rotation | Script error: No such module "val".[6] days |
| Rotational velocity (v sin i) | 150[6] km/s |
| λ Sco Aa2 (a) | |
| Mass | Script error: No such module "val".[6] Template:Solar mass |
| Radius | Script error: No such module "val".[6] Template:Solar radius |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| λ Sco Ab (B) | |
| Mass | 8.1[5] Template:Solar mass |
| Radius | Script error: No such module "val".[6] Template:Solar radius |
| Surface gravity (log g) | 4.0[7] cgs |
| Temperature | Script error: No such module "val".[6] K |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| Template:Odlist | |
| Database references | |
| SIMBAD | data |
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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.
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, Script error: No such module "Lang". (Script error: No such module "Lang".), 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 Script error: No such module "Lang". (Script error: No such module "Lang".), "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
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.
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,[23] while the brighter star is a background object.[24]
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.
References
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- ↑ Template:In lang 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, Template:ISBN.
- ↑ Template:In lang 香港太空館 - 研究資源 - 亮星中英對照表 Script error: No such module "webarchive"., Hong Kong Space Museum. Accessed on line November 23, 2010.
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