天球赤道座標星圖 13h 16m 51.051430s,+17° 01′ 01.840901″

HD 115404 是一個位於后髮座附近的雙星系統。依巴谷卫星進行的視差測量將系統置於 36 光年或 11 秒差距之外[11]視星等分別為 6.66 和 9.50[2]

HD 115404
观测数据
曆元 J2000      分點 J2000
星座 后髮座
HD 115404 A
赤經 13h 16m 51.051430s[1]
赤緯 +17° 01′ 01.840901″[1]
視星等 (V) 6.66[2]
HD 115404 B
赤經 13h 16m 51.554014s[3]
赤緯 +17° 00′ 59.892133″[3]
視星等 (V) 9.50[2]
特性
U−B 色指数+0.64[4]
B−V 色指数+0.92[4]
特性
光谱分类K2 V[5]
天体测定
HD 115404 A
徑向速度 (Rv)7.62 ± 0.09[6] km/s
自行 (μ) 赤经:636.285±0.028 mas/yr
赤纬:−264.678±0.031 mas/yr
视差 (π)91.0176 ± 0.0236[1] mas
距离35.834 ± 0.009 ly
(10.987 ± 0.003 pc)
HD 115404 B
徑向速度 (Rv)5.95±0.13[3] km/s
自行 (μ) 赤经:649.666±0.031 mas/yr
赤纬:−263.937±0.026 mas/yr
视差 (π)90.9475 ± 0.0232[3] mas
距离35.862 ± 0.009 ly
(10.995 ± 0.003 pc)
軌道[7]
繞行週期 (P)770.0 yr
半長軸 (a)8.06"
偏心率 (e)0.12
倾斜角 (i)93.41°
升交点黃經 (Ω)104.66°
近心点 曆元 (T)B 1875.0
近心點幅角 (ω)
(secondary)
276.99°
詳細資料
HD 115404 A
質量0.70 ± 0.09[8] M
半徑0.76 ± 0.02[8] R
表面重力 (log g)4.58 ± 0.03[8]
亮度3.1[8] L
溫度4976[8] K
金属量 [Fe/H]−0.08[8] dex
自轉速度 (v sin i)2.8[8] km/s
年齡10.2 (5.4–13.5)[8] Gyr
HD 115404 B
質量0.542[9] M
半徑0.550[9] R
其他命名
BD+17° 2611、​GJ 505、​HD 115404、​HIP 64797、​SAO 100491、​LHS 2713[10]
參考資料庫
SIMBADA
B
ARICNSA
B

主星A是一顆K型主序星[5]。它的質量大約是太陽的70%,半徑是太陽的0.76倍[8]。它的伴星是一顆紅矮星(M0.5 V)[12]。它的質量是太陽的54.2%,半徑是太陽的0.55 倍[9]。這兩顆恆星每770年繞軌道運行一次[7]。該系統被認為相當古老,有5.4到135億年的歷史[8]

參考資料 编辑

  1. ^ 1.0 1.1 1.2 Vallenari, A.; et al. Gaia Data Release 3. Summary of the content and survey properties. Astronomy & Astrophysics. 2022. arXiv:2208.00211 . doi:10.1051/0004-6361/202243940 .  已忽略未知参数|collaboration= (帮助) Gaia DR3 record for this source at VizieR.
  2. ^ 2.0 2.1 2.2 Fabricius, C.; Høg, E.; Makarov, V. V.; Mason, B. D.; Wycoff, G. L.; Urban, S. E. The Tycho double star catalogue. Astronomy and Astrophysics. 2002, 384: 180–189. Bibcode:2002A&A...384..180F. doi:10.1051/0004-6361:20011822 . 
  3. ^ 3.0 3.1 3.2 3.3 Vallenari, A.; et al. Gaia Data Release 3. Summary of the content and survey properties. Astronomy & Astrophysics. 2022. arXiv:2208.00211 . doi:10.1051/0004-6361/202243940 .  已忽略未知参数|collaboration= (帮助) Gaia DR3 record for this source at VizieR.
  4. ^ 4.0 4.1 Cowley, A. P.; Hiltner, W. A.; Witt, A. N. Spectral classification and photometry of high proper motion stars. The Astronomical Journal. 1967, 72: 1334. Bibcode:1967AJ.....72.1334C. doi:10.1086/110413. 
  5. ^ 5.0 5.1 White, Russel J.; Gabor, Jared M.; Hillenbrand, Lynne A. High-Dispersion Optical Spectra of Nearby Stars Younger Than the Sun. The Astronomical Journal. 2007, 133 (6): 2524. Bibcode:2007AJ....133.2524W. S2CID 122854. arXiv:0706.0542 . doi:10.1086/514336. 
  6. ^ Maldonado, J.; Martínez-Arnáiz, R. M.; Eiroa, C.; Montes, D.; Montesinos, B. A spectroscopy study of nearby late-type stars, possible members of stellar kinematic groups. Astronomy and Astrophysics. 2010, 521: A12. Bibcode:2010A&A...521A..12M. S2CID 119209183. arXiv:1007.1132 . doi:10.1051/0004-6361/201014948. 
  7. ^ 7.0 7.1 Sixth Catalog of Orbits of Visual Binary Stars. United States Naval Observatory. [11 August 2017]. (原始内容存档于2017-08-01). 
  8. ^ 8.00 8.01 8.02 8.03 8.04 8.05 8.06 8.07 8.08 8.09 Brewer, John M.; Fischer, Debra A.; Valenti, Jeff A.; Piskunov, Nikolai. Spectral Properties of Cool Stars: Extended Abundance Analysis of 1,617 Planet-Search Stars. The Astrophysical Journal Supplement Series. 2016, 225 (2): 32. Bibcode:2016ApJS..225...32B. S2CID 118507965. arXiv:1606.07929 . doi:10.3847/0067-0049/225/2/32. 
  9. ^ 9.0 9.1 9.2 Newton, Elisabeth R.; Irwin, Jonathan; Charbonneau, David; Berlind, Perry; Calkins, Michael L.; Mink, Jessica. The Hα emission of nearby M dwarfs and its relation to stellar rotation. The Astrophysical Journal. 2017, 834 (1): 85. Bibcode:2017ApJ...834...85N. S2CID 55000202. arXiv:1611.03509 . doi:10.3847/1538-4357/834/1/85. 
  10. ^ HD 115404. SIMBAD. 斯特拉斯堡天文資料中心. 
  11. ^ van Leeuwen, F. Validation of the new Hipparcos reduction. Astronomy and Astrophysics. 2007, 474 (2): 653–664 [2023-04-19]. Bibcode:2007A&A...474..653V. S2CID 18759600. arXiv:0708.1752 . doi:10.1051/0004-6361:20078357. (原始内容存档于2016-04-02).  Vizier catalog entry 页面存档备份,存于互联网档案馆
  12. ^ Alonso-Floriano, F. J.; Morales, J. C.; Caballero, J. A.; Montes, D.; Klutsch, A.; Mundt, R.; Cortés-Contreras, M.; Ribas, I.; Reiners, Ansgar; Amado, P. J.; Quirrenbach, A.; Jeffers, S. V. CARMENES input catalogue of M dwarfs (PDF). Astronomy & Astrophysics. 2015, 577: A128. S2CID 53135130. arXiv:1502.07580 . doi:10.1051/0004-6361/201525803. [失效連結]