Zeta Sagittae
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Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
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Constellation | Sagitta |
Right ascension | 19h 48m 58.65978s[1] |
Declination | +19° 08′ 31.3516″[1] |
Apparent magnitude (V) | +5.00[2] (5.64 + 6.04 + 9.01)[3] |
Characteristics | |
Spectral type | A3 Vnn[4] (A1 V + A3 V)[5] |
U−B color index | +0.06[2] |
B−V color index | +0.10[2] |
Astrometry | |
Proper motion (μ) | RA: +17.63[1] mas/yr Dec.: +26.27[1] mas/yr |
Parallax (π) | 12.79 ± 0.67[1] mas |
Distance | 260 ± 10 ly (78 ± 4 pc) |
Orbit[6] | |
Period (P) | 487.9±4.9 d 8 |
Semi-major axis (a) | 05±0.00044″ 0.136 |
Eccentricity (e) | ±0.0019 0.7948 |
Inclination (i) | ±0.41 132.33° |
Longitude of the node (Ω) | ±0.68 340.97° |
Periastron epoch (T) | 44199.6 ± 5.9 HMJD |
Argument of periastron (ω) (secondary) | ±1.0 355.3° |
Details | |
ζ Sge A | |
Mass | 1.80[7] M☉ |
Radius | 1.7[8] R☉ |
Luminosity | 46[9] L☉ |
Surface gravity (log g) | 3.89[7] cgs |
Temperature | ±286 8,422[7] K |
Rotational velocity (v sin i) | 240[10] km/s |
Age | 347[7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Zeta Sagittae (ζ Sagittae) is triple star[3] system in the northern constellation of Sagitta. It is visible to the naked eye, having a combined apparent visual magnitude of +5.00.[2] Based upon an annual parallax shift of 12.79 mas,[1] the distance to this star is approximately 260 light years.
The inner pair is a visual binary system consisting of two A-type main-sequence stars with an orbital period of 23.2 years (8,487.9 d), a semimajor axis of 0.136 arc seconds, and an eccentricity of 0.79.[6] The primary, component A, has a visual magnitude of 5.64[3] with a stellar classification of A3 Vnn,[4] where the 'nn' suffix indicates "nebulous" lines due to rotation. It is spinning rapidly with a projected rotational velocity of 240 km/s. This is giving the star an oblate shape with an equatorial bulge that is 14% larger than the polar radius.[10]
The secondary member, component B, is a magnitude 6.04 star, while the more distant component C is magnitude 9.01 and lies at an angular separation of 8.330 arc seconds from the other two.[3]
Naming
In Chinese, 左旗 (Zuǒ Qí), meaning Left Flag, refers to an asterism consisting of ζ Sagittae, α Sagittae, β Sagittae, δ Sagittae, γ Sagittae, 13 Sagittae, 11 Sagittae, 14 Sagittae and ρ Aquilae. Consequently, ζ Sagittae itself is known as 左旗四 (Zuǒ Qí sì, English: the Fourth Star of Left Flag.)[12]
References
- 1 2 3 4 5 6 van Leeuwen, F. (2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics, 474 (2): 653–664, Bibcode:2007A&A...474..653V, arXiv:0708.1752 , doi:10.1051/0004-6361:20078357.
- 1 2 3 4 Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99), Bibcode:1966CoLPL...4...99J.
- 1 2 3 4 Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society, 389 (2): 869–879, Bibcode:2008MNRAS.389..869E, arXiv:0806.2878 , doi:10.1111/j.1365-2966.2008.13596.x.
- 1 2 Cowley, A.; et al. (April 1969), "A study of the bright A stars. I. A catalogue of spectral classifications", Astronomical Journal, 74: 375–406, Bibcode:1969AJ.....74..375C, doi:10.1086/110819.
- ↑ Christy, James W.; Walker, R. L., Jr. (October 1969), "MK Classification of 142 Visual Binaries", Publications of the Astronomical Society of the Pacific, 81 (482): 643, Bibcode:1969PASP...81..643C, doi:10.1086/128831.
- 1 2 Muterspaugh, Matthew W.; et al. (December 2010), "The Phases Differential Astrometry Data Archive. II. Updated Binary Star Orbits and a Long Period Eclipsing Binary", The Astronomical Journal, 140 (6): 1623−1630, Bibcode:2010AJ....140.1623M, arXiv:1010.4043 , doi:10.1088/0004-6256/140/6/1623.
- 1 2 3 4 David, Trevor J.; Hillenbrand, Lynne A. (2015), "The Ages of Early-Type Stars: Strömgren Photometric Methods Calibrated, Validated, Tested, and Applied to Hosts and Prospective Hosts of Directly Imaged Exoplanets", The Astrophysical Journal, 804 (2): 146, Bibcode:2015ApJ...804..146D, arXiv:1501.03154 , doi:10.1088/0004-637X/804/2/146.
- ↑ Pasinetti Fracassini, L. E.; et al. (February 2001), "Catalogue of Apparent Diameters and Absolute Radii of Stars (CADARS)", Astronomy and Astrophysics (Third ed.), 367: 521–524, Bibcode:2001A&A...367..521P, arXiv:astro-ph/0012289 , doi:10.1051/0004-6361:20000451.
- ↑ McDonald, I.; et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society, 427 (1): 343–57, Bibcode:2012MNRAS.427..343M, arXiv:1208.2037 , doi:10.1111/j.1365-2966.2012.21873.x.
- 1 2 Belle, G. T. (2012), "Interferometric observations of rapidly rotating stars", The Astronomy and Astrophysics Review, 20: 51, Bibcode:2012A&ARv..20...51V, arXiv:1204.2572 , doi:10.1007/s00159-012-0051-2.
- ↑ "zet Sge". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2017-07-11.
- ↑ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 3 日
External links
- Kaler, James B. (August 3, 2012), "Zeta Sagittae", stars, University of Illinois, retrieved 2017-07-13.