水位一小犬6 6 Canis Minoris)是赤道星座小犬座的一顆恆星,距離太陽大約570光年。它是一顆肉眼可見,黯淡的橙色恆星,視星等為+4.55等[2]。這顆恆星正以日心點運動學−16.3 km/s 徑向速度向地球靠近[4],它是屬於天狼星超星系團英語Sirius#Star cluster membership的大熊座星流周邊一個群的成員[9]

水位一
觀測資料
曆元 J2000.0 (ICRS)
星座 小犬座
星官 水位井宿
赤經 07h 29m 47.78172s[1]
赤緯 +12° 00′ 23.6347″[1]
視星等(V) +4.55[2]
特性
演化階段巨星
光譜分類K1 III[3]
B−V 色指數1.276±0.001[2]
天體測定
徑向速度 (Rv)−16.31±0.13[4] km/s
自行 (μ) 赤經:−0.57[1] mas/yr
赤緯:−18.85[1] mas/yr
視差 (π)5.70 ± 0.21[1] mas
距離570 ± 20 ly
(175 ± 6 pc)
絕對星等 (MV)−1.67[2]
詳細資料
質量4.0[5] M
半徑44[6] R
亮度761.44[2] L
溫度4,370[5] K
金屬量 [Fe/H]0.02[5] dex
自轉速度 (v sin i)1.7[7] km/s
其他命名
6 CMi、​BD+12°1567、​FK5 1193、​GC 10024、​HD 59294、​HIP 36425、​HR 2864、​SAO 96952[8]
參考資料庫
SIMBAD資料

這是一顆演化的巨星恆星分類為K1 III.[3]。它有輕度的鋇異常[10],這可能表明這是一顆有白矮星伴星的聯星系統[11]。對可見分量的干涉量測-量測的角直徑約為2.31±0.03 mas[12],估計其距離相當於約44倍太陽半徑的物理半徑[6]。質量約為4 太陽質量[5],在4,370k的有效溫度[5],其擴大光球的輻射為太陽的761倍[2]

參考資料

  1. ^ 1.0 1.1 1.2 1.3 1.4 van Leeuwen, F., Validation of the new Hipparcos reduction, Astronomy and Astrophysics, 2007, 474 (2): 653–664, Bibcode:2007A&A...474..653V, S2CID 18759600, arXiv:0708.1752 , doi:10.1051/0004-6361:20078357. 
  2. ^ 2.0 2.1 2.2 2.3 2.4 2.5 Anderson, E.; Francis, Ch., XHIP: An extended hipparcos compilation, Astronomy Letters, 2012, 38 (5): 331, Bibcode:2012AstL...38..331A, S2CID 119257644, arXiv:1108.4971 , doi:10.1134/S1063773712050015. 
  3. ^ 3.0 3.1 Keenan, Philip C.; McNeil, Raymond C., The Perkins catalog of revised MK types for the cooler stars, Astrophysical Journal Supplement Series, 1989, 71: 245, Bibcode:1989ApJS...71..245K, doi:10.1086/191373. 
  4. ^ 4.0 4.1 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 . doi:10.1051/0004-6361/201833051.  VizieR中此天體在蓋亞望遠鏡第二批數據發佈的記錄
  5. ^ 5.0 5.1 5.2 5.3 5.4 Gondoin, P., Evolution of X-ray activity and rotation on G-K giants, Astronomy and Astrophysics, December 1999, 352: 217–227, Bibcode:1999A&A...352..217G. 
  6. ^ 6.0 6.1 Lang, Kenneth R., Astrophysical formulae, Astronomy and astrophysics library 1 3rd, Birkhäuser, 2006 [2023-12-20], ISBN 3-540-29692-1, (原始內容存檔於2023-07-28).  The radius (R*) is given by:
     
  7. ^ De Medeiros, J. R.; et al, Rotation and lithium in single giant stars, Astronomy and Astrophysics, November 2000, 363: 239–243, Bibcode:2000A&A...363..239D, arXiv:astro-ph/0010273 . 
  8. ^ 6 CMi. SIMBAD. 斯特拉斯堡天文資料中心. 
  9. ^ Chupina, N. V.; et al, Kinematic structure of the corona of the Ursa Major flow found using proper motions and radial velocities of single stars, Astronomy and Astrophysics, June 2006, 451 (3): 909–916, Bibcode:2006A&A...451..909C, doi:10.1051/0004-6361:20054009 . 
  10. ^ Escorza, A.; et al, Hertzsprung-Russell diagram and mass distribution of barium stars, Astronomy & Astrophysics, December 2017, 608: 13, Bibcode:2017A&A...608A.100E, S2CID 119428276, arXiv:1710.02029 , doi:10.1051/0004-6361/201731832, A100. 
  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 , doi:10.1111/j.1365-2966.2008.13596.x. 
  12. ^ Richichi, A.; et al, CHARM2: An updated Catalog of High Angular Resolution Measurements, Astronomy and Astrophysics, February 2005, 431 (2): 773–777, Bibcode:2005A&A...431..773R, doi:10.1051/0004-6361:20042039