格利泽829

格利泽829 是位于飞马座中由两颗红矮星组成的双星系统。[6] 基于视差测量,距离太阳约为22光年[1] 该系统将在大约91,000年后最接近太阳,届时它的近日点距离将达到17.65光年﹙5.41秒差距﹚。[4]

Gliese 829
观测资料
历元 J2000.0
星座 飞马座
星官
赤经 21h 29m 36.81225s[1]
赤纬 +17° 38′ 35.8542″[1]
视星等(V) 10.35[2]
特性
光谱分类M3.0Ve[3]
U−B 色指数+1.31[2]
B−V 色指数+1.61[2]
天体测定
径向速度 (Rv)−25.0[4] km/s
自行 (μ) 赤经:+1007.13[1] mas/yr
赤纬:+377.27[1] mas/yr
视差 (π)147.4958 ± 0.0257[5] mas
距离22.113 ± 0.004 ly
(6.780 ± 0.001 pc)
轨道[6]
绕行周期 (P)53.221±0.004 d
偏心率 (e)0.374±0.004
近心点 历元 (T)48980.2±0.2 JD
近心点幅角 (ω)
(secondary)
300±1°
半振幅 (K1)
(primary)
18.7±0.1 km/s
半振幅 (K2)
(secondary)
18.7±0.1 km/s
详细资料
表面重力 (log g)5.0[3]
温度3,400[3] K
金属量 [Fe/H]−0.13[7] dex
其他命名
HIP 106106, Ross 775.[8]
参考数据库
SIMBAD资料
ARICNS资料

特性

主星的温度为3400K。它的光谱分类为M3.0Ve,B-V 颜色指数为1.61,也称为Ross 775。它的视星等为10.35。

参考

  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 Ianna, P. A.; Whitman, W. R., Parallaxes and proper motions from the McCormick Observatory List 45, Astronomical Journal, April 1984, 89: 568–570, Bibcode:1984AJ.....89..568I, doi:10.1086/113550. 
  3. ^ 3.0 3.1 3.2 Lépine, Sébastien; et al, A Spectroscopic Catalog of the Brightest (J < 9) M Dwarfs in the Northern Sky, The Astronomical Journal, 2013, 145 (4): 102, Bibcode:2013AJ....145..102L, S2CID 117144290, arXiv:1206.5991 , doi:10.1088/0004-6256/145/4/102. 
  4. ^ 4.0 4.1 Bailer-Jones, C. A. L., Close encounters of the stellar kind, Astronomy & Astrophysics, March 2015, 575: 13, Bibcode:2015A&A...575A..35B, S2CID 59039482, arXiv:1412.3648 , doi:10.1051/0004-6361/201425221, A35. 
  5. ^ Brown, A. G. A.; et al. Gaia Early Data Release 3: Summary of the contents and survey properties. Astronomy & Astrophysics. 2021, 649: A1. Bibcode:2021A&A...649A...1G. S2CID 227254300. arXiv:2012.01533 . doi:10.1051/0004-6361/202039657 .  已忽略未知参数|collaboration= (帮助) (勘误: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
  6. ^ 6.0 6.1 Delfosse, Xavier; et al, New neighbours. I. 13 new companions to nearby M dwarfs, Astronomy and Astrophysics, April 1999, 344: 897–910, Bibcode:1999A&A...344..897D, arXiv:astro-ph/9812008 . 
  7. ^ Rojas-Ayala, Bárbara; et al. Metallicity and Temperature Indicators in M Dwarf K-band Spectra: Testing New and Updated Calibrations with Observations of 133 Solar Neighborhood M Dwarfs (PDF). The Astrophysical Journal. April 2012, 748 (2): 93 [2023-03-23]. Bibcode:2012ApJ...748...93R. S2CID 41902340. arXiv:1112.4567 . doi:10.1088/0004-637X/748/2/93. (原始内容存档 (PDF)于2021-01-29). 
  8. ^ Ross 775. SIMBAD. 斯特拉斯堡天文资料中心. [2016-10-25].