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水位增六

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水位增六(巨蟹座Mu2
觀測資料
曆元 J2000.0
星座 巨蟹座
星官
赤經 08h 07m 45.85574s[1]
赤緯 +21° 34′ 54.5441″[1]
視星等(V) +5.30[2]
特性
光谱分类G2 IV[3]
U−B 色指数+0.21[2]
B−V 色指数+0.63[2]
天体测定
徑向速度 (Rv)−36.0±0.1[4] km/s
自行 (μ) 赤经:+23.00[1] mas/yr
赤纬:−66.42[1] mas/yr
视差 (π)42.94 ± 0.30[1] mas
距离76.0 ± 0.5 ly
(23.3 ± 0.2 pc)
绝对星等 (MV)+3.46[5]
詳細資料
質量1.192+0.017
−0.016
[6] M
半徑1.82[7] R
表面重力 (log g)3.97±0.02[6]
亮度3.45[8] L
溫度5,809±59[6] K
金属量 [Fe/H]0.11[6] dex
自轉速度 (v sin i)3.7±0.3[5] km/s
年齡5.64+0.35
−0.14
[6] Gyr
其他命名
μ Cnc、​10 Cancri、​BD+22° 1862、​FK5 2630、​HD 67228、​HIP 39780、​HR 3176、​SAO 79959[9]
參考資料庫
SIMBAD资料

水位增六巨蟹座Mu2)是一顆單獨的黃色恆星[10],位置在黃道星座巨蟹座內。它是肉眼可見的恆星,視星等+5.30等[2],依據從地球測得的周年視差42.94毫角秒[1],這顆恆星與太陽的距離是76光年。水位增六將在60萬年後,以最接近的4.9 pc(16 ly)距離掠過太陽[11]

估計它的年齡是56億年,它已演化G型次巨星類型為C2IV。[3]。它的質量是1.2倍太陽質量[6],和1.8倍的太陽半徑 [7]。 水位增六有相對較高的金屬量 – 天文學家所謂的金屬是除了氫和氦之外的其他元素,比太陽的豐度高出29% [6]。它的輻射量 太陽亮度的3.45倍3.45[8],表面的有效溫度是5,809k[6]

參考資料

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  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 Johnson, H. L.; et al, UBVRIJKL photometry of the bright stars, Communications of the Lunar and Planetary Laboratory, 1966, 4 (99), Bibcode:1966CoLPL...4...99J. 
  3. ^ 3.0 3.1 Gray, R. O.; et al, Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 parsecs: The Northern Sample I, The Astronomical Journal, July 2006, 132 (1): 161–170, Bibcode:2006AJ....132..161G, arXiv:astro-ph/0603770可免费查阅, doi:10.1086/504637. 
  4. ^ de Bruijne, J. H. J.; Eilers, A.-C., Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project, Astronomy & Astrophysics, October 2012, 546: 14, Bibcode:2012A&A...546A..61D, arXiv:1208.3048可免费查阅, doi:10.1051/0004-6361/201219219, A61. 
  5. ^ 5.0 5.1 Ammler-von Eiff, M.; Reiners, A., New measurements of rotation and differential rotation in A-F stars: are there two populations of differentially rotating stars?, Astronomy & Astrophysics, June 2012, 542: 31, Bibcode:2012A&A...542A.116A, arXiv:1204.2459可免费查阅, doi:10.1051/0004-6361/201118724, A116. 
  6. ^ 6.0 6.1 6.2 6.3 6.4 6.5 6.6 6.7 Ramírez, I.; et al, Oxygen abundances in nearby FGK stars and the galactic chemical evolution of the local disk and halo, The Astrophysical Journal, February 2013, 764 (1): 78, Bibcode:2013ApJ...764...78R, arXiv:1301.1582可免费查阅, doi:10.1088/0004-637X/764/1/78. 
  7. ^ 7.0 7.1 Takeda, Genya; et al, Structure and Evolution of Nearby Stars with Planets. II. Physical Properties of ~1000 Cool Stars from the SPOCS Catalog, The Astrophysical Journal Supplement Series, February 2007, 168 (2): 297–318, Bibcode:2007ApJS..168..297T, arXiv:astro-ph/0607235可免费查阅, doi:10.1086/509763. 
  8. ^ 8.0 8.1 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. 
  9. ^ mu.02 Cnc. SIMBAD. 斯特拉斯堡天文資料中心. [2017-06-17]. 
  10. ^ 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. ^ Bailer-Jones, C. A. L., Close encounters of the stellar kind, Astronomy & Astrophysics, March 2015, 575: 13, Bibcode:2015A&A...575A..35B, arXiv:1412.3648可免费查阅, doi:10.1051/0004-6361/201425221, A35.