Gamma2 Sagittarii
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Template:Location mark Location of γ2 Sagittarii (circled) | |
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Sagittarius |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | +2.96[2] |
| Characteristics | |
| Evolutionary stage | Red clump[3] |
| Spectral type | K0III[2] |
| U−B Template:Engvar | +0.77[4] |
| B−V Template:Engvar | +1.006[2] |
| Astrometry | |
| Radial velocity (Rv) | 22.0[5] km/s |
| Proper motion (μ) | RA: −48.839 mas/yr[1] Dec.: −204.86 mas/yr[1] |
| Parallax (π) | 30.6791±0.4451 mas[2] |
| Distance | Script error: No such module "val". ly (Script error: No such module "val". pc)[2] |
| Absolute magnitude (MV) | +0.395[2] |
| Details[2] | |
| Mass | Script error: No such module "val". Template:Solar mass |
| Radius | Script error: No such module "val". Template:Solar radius |
| Luminosity | Script error: No such module "val". Template:Solar luminosity |
| Surface gravity (log g) | Script error: No such module "val". cgs |
| Temperature | Script error: No such module "val". K |
| Metallicity [Fe/H] | Script error: No such module "val". dex |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| Alnasl, Nushaba,[6] Awal al Warida, γ Sagittarii, γ Sgr, Gamma2 Sgr, 10 Sagittarii, CPD−30 5241, FK5 679, GC 24632, HD 165135, HIP 88635, HR 6746, PPM 297231, SAO 209696[7] | |
| Database references | |
| SIMBAD | data |
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Gamma2 Sagittarii (γ2 Sagittarii, abbreviated Gamma2 Sgr, γ2 Sgr), formally named Alnasl Template:IPAc-en,[8] is a 3rd-magnitude star in the zodiac constellation of Sagittarius. The location of this star is in the handle of the Bow of Sagittarius the Centaur. It is approximately Script error: No such module "convert". from the Sun and has an apparent visual magnitude of +2.96,[2] making it the seventh-brightest star in the constellation.
It forms part of a double star along with a fainter optical companion designated Gamma1 Sagittarii located about 50 arcminutes north of this star. The latter is a magnitude 4.7 Cepheid variable star that also has the variable star designation W Sagittarii.[9][10]
Nomenclature
γ2 Sagittarii (Latinised to Gamma2 Sagittarii) is the star's Bayer designation.
It bore the traditional names Alnasl (alternatively Nasl, El Nasl, "al Nasl"), Nushaba (Nash) and Awal al Warida. Alnasl is derived from the Arabic النصل al-naşl and Nushaba is derived from the Arabic Zujj al-Nashshaba, both meaning "arrowhead".[11][12] In the catalogue of stars in the calendarium of al Achsasi al Mouakket, this star was designated Awal al Waridah, meaning "first [star] of the [ostrich] going down to the water", from the Arabic النعامة الواردة al Naʽāma al Wārida, the name of the asterism consisting of this star, Delta Sagittarii, Epsilon Sagittarii and Eta Sagittarii. This ostrich was thought of as going down to the river (the Milky Way) to drink, and another ostrich (σ, φ, τ, and ζ, al Sadira) was thought of as coming back up.[13][12]
In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN)[14] to catalogue and standardize proper names for stars. The WGSN approved the name Alnasl for this star on 21 August 2016 and it is now so included in the List of IAU-approved Star Names.[8]
Gamma2 Sagittarii, together with Delta Sagittarii, Epsilon Sagittarii, Zeta Sagittarii, Lambda Sagittarii, Sigma Sagittarii, Tau Sagittarii and Phi Sagittarii, comprise the Teapot asterism.[15]
Together with Delta Sagittarii and Epsilon Sagittarii, Gamma2 Sagittarii formed the Akkadian Sin-nun‑tu, or Si-nu-nu‑tum 'the Swallow'.[12]
In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Winnowing Basket, refers to an asterism consisting of Gamma Sagittarii, Delta Sagittarii, Epsilon Sagittarii and Eta Sagittarii. Consequently, Gamma2 Sagittarii itself is known as Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx.)[16]
Properties
A stellar classification of K0 III reveals that this is a giant star, having expanded to an estimated 12 times the Sun's radius.[2] This means it has exhausted the hydrogen in its core and evolved away from the main sequence. It is now fusing helium, being in the evolutionary stage known as the horizontal branch.[3] Gamma2 Sagittarii is two times more massive than the Sun and is emitting 73 times more luminosity.[2] The abundance of elements other than hydrogen and helium in this star, what astronomers term the star's metallicity, is lower than in the Sun.[2] Gamma2 Sagittarii has an effective temperature of 4,864 K,[2] compared to Script error: No such module "val". for the Sun. It is this lower temperature that gives Gamma2 Sagittarii the orange hue that is a characteristic of K-type stars.
References
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- ↑ a b c Template:Cite Gaia DR3
- ↑ a b c d e f g h i j k l Script error: No such module "citation/CS1". Alnasl's database entry at VizieR.
- ↑ a b Script error: No such module "citation/CS1".
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- ↑ a b Script error: No such module "citation/CS1".
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- ↑ a b c Script error: No such module "citation/CS1".
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- ↑ Script error: No such module "citation/CS1".
- ↑ Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 11 日 Template:Webarchive
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