跳转到内容

狗国增二

维基百科,自由的百科全书
狗国增二(人马座θ2
Diagram showing star positions and boundaries of the Sagittarius constellation and its surroundings
狗国增二的位置(红圈)Location of θ2 Sagittarii (circled)
观测资料
历元 J2000.0
星座 人马座
星官
赤经 19h 59m 51.35684s[1]
赤纬 −34° 41′ 52.0797″[1]
视星等(V) +5.30[2]
特性
光谱分类A4/A5 IV[3]
U−B 色指数+0.06[2]
B−V 色指数+0.17[2]
天体测定
径向速度 (Rv)−17.60[4] km/s
自行 (μ) 赤经:+108.23[1] mas/yr
赤纬:−69.51[1] mas/yr
视差 (π)20.62 ± 0.28[1] mas
距离158 ± 2 ly
(48.5 ± 0.7 pc)
绝对星等 (MV)+1.87[5]
详细资料
质量1.93[6] M
表面重力 (log g)4.07±0.14[6]
亮度14[7] L
温度8,113±276[6] K
自转速度 (v sin i)45.2±0.5[8] km/s
年龄809[6] Myr
其他命名
θ2 Sgr、​CPD−35° 8701、​HD 189118、​HIP 98421、​HR 7624、​SAO 211717、​WDS J19599-3442[9]
参考资料库
SIMBAD资料

狗国增二人马座θ2)是黄道星座人马座中一颗单独的恒星 [10]。它的视星等为 +5.30等[2],在足够黑暗的场所肉眼隐约可见。这颗恒星正以每秒17.60公里的径向速度朝向太阳接近[4]。根据从地球测得年周视差20.62mas的数值[1],它与太阳的距离是158光年

狗国增二光谱类型是A4/A5IV[3],估计它的年龄为8亿900万年[6],是一颗演化至[A-型星|A型]]的次巨星。它被怀疑是一颗Am星,因为至少在1992年的观测周期上,经光度测量是颗变星[11]。估计它的质量是太阳的1.93倍[6],辐射是太阳的14倍[7],来自光球有效温度是8,113K[6]。它自转的投影自转速度是每秒45.2公里[8]

狗国增二有一对目视伴星。伴星B的视星等11.3等,在2000年的角距离为32.8弧秒位置角165°;伴星C在1965年与B的距离为1.5弧秒,位置角104度[12]。但这两者与狗国增二都没有物理上的实质关系[10]

参考资料

  1. ^ 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F., Validation of the new Hipparcos reduction, Astronomy and Astrophysics, 2007, 474 (2): 653–664, Bibcode:2007A&A...474..653V, arXiv:0708.1752可免费查阅, doi:10.1051/0004-6361:20078357. 
  2. ^ 2.0 2.1 2.2 2.3 Mendoza, E. E.; et al, UBVRI photometry of 225 AM stars, Astronomical Journal, June 1978, 83: 606–614, Bibcode:1978AJ.....83..606M, doi:10.1086/112242. 
  3. ^ 3.0 3.1 Houk, Nancy, Michigan catalogue of two-dimensional spectral types for the HD stars 3, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, 1979, Bibcode:1982mcts.book.....H. 
  4. ^ 4.0 4.1 Gontcharov, G. A., Pulkovo Compilation of Radial Velocities for 35495 Hipparcos stars in a common system, Astronomy Letters, November 2006, 32 (11): 759–771, Bibcode:2006AstL...32..759G, arXiv:1606.08053可免费查阅, doi:10.1134/S1063773706110065. 
  5. ^ Anderson, E.; Francis, Ch., XHIP: An extended hipparcos compilation, Astronomy Letters, 2012, 38 (5): 331, Bibcode:2012AstL...38..331A, arXiv:1108.4971可免费查阅, doi:10.1134/S1063773712050015. 
  6. ^ 6.0 6.1 6.2 6.3 6.4 6.5 6.6 David, Trevor J.; Hillenbrand, Lynne A., 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, 2015, 804 (2): 146, Bibcode:2015ApJ...804..146D, arXiv:1501.03154可免费查阅, doi:10.1088/0004-637X/804/2/146. 
  7. ^ 7.0 7.1 McDonald, I.; et al, Fundamental Parameters and Infrared Excesses of Hipparcos Stars, Monthly Notices of the Royal Astronomical Society, 2012, 427 (1): 343–57, Bibcode:2012MNRAS.427..343M, arXiv:1208.2037可免费查阅, doi:10.1111/j.1365-2966.2012.21873.x. 
  8. ^ 8.0 8.1 Díaz, C. G.; et al, Accurate stellar rotational velocities using the Fourier transform of the cross correlation maximum, Astronomy & Astrophysics, July 2011, 531: A143, Bibcode:2011A&A...531A.143D, arXiv:1012.4858可免费查阅, doi:10.1051/0004-6361/201016386. 
  9. ^ tet02 Sgr. SIMBAD. 斯特拉斯堡天文资料中心. [2017-07-07]. 
  10. ^ 10.0 10.1 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, arXiv:0806.2878可免费查阅, doi:10.1111/j.1365-2966.2008.13596.x. 
  11. ^ Anders, G. J., Theta2 Sgr: Serendipitous Discovery of Variability in an Am Star?, Information Bulletin on Variable Stars, September 1992, 3768: 1, Bibcode:1992IBVS.3768....1A. 
  12. ^ Mason, B. D.; et al, The Washington Visual Double Star Catalog, 2014 [2015-07-22], Bibcode:2001AJ....122.3466M, doi:10.1086/323920可免费查阅, (原始内容存档于2019-07-04).