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玉夫座ι

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玉夫座ι
玉夫座ι的位置(紅圈中心,被星座連線的綠線覆蓋)。
觀測資料
曆元 J2000
星座 玉夫座
星官
赤經 00h 21m 31.19799s[1]
赤緯 -28° 58′ 53.2957″[1]
視星等(V) 5.18[2]
特性
光谱分类K0III[3]
U−B 色指数+0.84[4]
B−V 色指数+1.00[5]
天体测定
徑向速度 (Rv)+20.60[6] km/s
自行 (μ) 赤经:+33.263[1] mas/yr
赤纬:-72.065[1] mas/yr
视差 (π)9.7081 ± 0.1287[1] mas
距离336 ± 4 ly
(103 ± 1 pc)
绝对星等 (MV)0.16[2]
詳細資料
質量2.94[7] M
半徑12.28[7] R
表面重力 (log g)2.48[8]
亮度97[7] L
溫度5,020[7] K
金属量 [Fe/H]+0.09[2] dex
自轉速度 (v sin i)3.1[9] km/s
其他命名
ι Scl、​CD−29°86、​GC 433、​HD 1737、​HIP 1708、​HR 84、​SAO 166207、​GSC 06419-01055[10]
參考資料庫
SIMBAD资料

玉夫座ι拉丁化Iota Sculptoris,縮寫為ι Scl,是在南天星座玉夫座的一顆孤獨的恆星[11]。它是一個昏暗的橙色光點,視星等為5.18,肉眼可見[2]。根據視差,這顆恒星距離太陽約336光年[1],並且正以+21公里/秒的徑向速度遠離中[6]

這是一顆衰老的巨星,其恒星分類為K0III[3],現時位於赫羅圖紅巨星分支[7]。它的質量是太陽質量的2.9倍,並且已經膨脹到太陽半徑的12倍。這顆恆星在5020 K的有效溫度下,從其擴大的光球層輻射出97倍於太陽的光度[7]。這顆恆星的座標位置是 X射線發射的來源,因此最有可能(99.4%的幾率)是X射線的發射源[12]

參考資料

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  1. ^ 1.0 1.1 1.2 1.3 1.4 1.5 Brown, A. G. A.; Vallenari, A.; Prusti, T.; de Bruijne, J. H. J.; et al. Gaia Data Release 2. Summary of the contents and survey properties. Astronomy & Astrophysics. 2018. Bibcode:2018A&A...616A...1G. arXiv:1804.09365可免费查阅. doi:10.1051/0004-6361/201833051.  VizieR中此天体在盖亚望远镜第二批数据发布的记录
  2. ^ 2.0 2.1 2.2 2.3 Anderson, E.; Francis, Ch. XHIP: An extended hipparcos compilation. Astronomy Letters. 2012, 38 (5): 331. Bibcode:2012AstL...38..331A. S2CID 119257644. arXiv:1108.4971可免费查阅. doi:10.1134/S1063773712050015.  Vizier catalog entry
  3. ^ 3.0 3.1 Houk, N. Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0. Michigan Catalogue of Two-dimensional Spectral Types for the HD stars. Volume_3. Declinations -40_ƒ0 to -26_ƒ0. 1982. Bibcode:1982mcts.book.....H. 
  4. ^ Mermilliod, J. C. VizieR Online Data Catalog: Homogeneous Means in the UBV System (Mermilliod 1991). VizieR On-line Data Catalog: II/168. Originally Published in: Institut d'Astronomie. 2006, 2168. Bibcode:2006yCat.2168....0M. Vizier catalog entry
  5. ^ Mallama, A. Sloan Magnitudes for the Brightest Stars. The Journal of the American Association of Variable Star Observers. 2014, 42 (2): 443. Bibcode:2014JAVSO..42..443M. Vizier catalog entry
  6. ^ 6.0 6.1 Wilson, R. E. General Catalogue of Stellar Radial Velocities. Carnegie Institute Washington D.C. Publication (Carnegie Institution for Science). 1953. Bibcode:1953GCRV..C......0W. LCCN 54001336. 
  7. ^ 7.0 7.1 7.2 7.3 7.4 7.5 Jones, M. I.; Jenkins, J. S.; Rojo, P.; Melo, C. H. F. Study of the impact of the post-MS evolution of the host star on the orbits of close-in planets. Astronomy & Astrophysics. 2011, 536: A71. Bibcode:2011A&A...536A..71J. S2CID 55769003. arXiv:1110.6459可免费查阅. doi:10.1051/0004-6361/201117887.  Vizier catalog entry
  8. ^ Allende Prieto, C.; Lambert, D. L. Fundamental parameters of nearby stars from the comparison with evolutionary calculations: Masses, radii and effective temperatures. Astronomy and Astrophysics. 1999, 352: 555–562. Bibcode:1999A&A...352..555A. arXiv:astro-ph/9911002可免费查阅.  Vizier catalog entry
  9. ^ De Medeiros, J. R.; Alves, S.; Udry, S.; Andersen, J.; Nordström, B.; Mayor, M. A catalog of rotational and radial velocities for evolved stars. Astronomy & Astrophysics. 2014, 561: A126. Bibcode:2014A&A...561A.126D. S2CID 54046583. arXiv:1312.3474可免费查阅. doi:10.1051/0004-6361/201220762.  Vizier catalog entry
  10. ^ iot Scl. SIMBAD. 斯特拉斯堡天文資料中心. 
  11. ^ Eggleton, P. P.; Tokovinin, A. A. A catalogue of multiplicity among bright stellar systems. Monthly Notices of the Royal Astronomical Society. September 2008, 389 (2): 869–879. Bibcode:2008MNRAS.389..869E. S2CID 14878976. arXiv:0806.2878可免费查阅. doi:10.1111/j.1365-2966.2008.13596.x可免费查阅. 
  12. ^ Haakonsen, Christian Bernt; Rutledge, Robert E. XID II: Statistical Cross-Association of ROSAT Bright Source Catalog X-ray Sources with 2MASS Point Source Catalog Near-Infrared Sources. The Astrophysical Journal Supplement. September 2009, 184 (1): 138–151. Bibcode:2009ApJS..184..138H. S2CID 119267456. arXiv:0910.3229可免费查阅. doi:10.1088/0067-0049/184/1/138.