轸宿二
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| 观测资料 历元 J2000 | |
|---|---|
| 星座 | 乌鸦座 |
| 星官 | |
| 赤经 | 12h 10m 07.48058s[1] |
| 赤纬 | –22° 37′ 11.1620″[1] |
| 视星等(V) | +3.024[2] |
| 特性 | |
| 光谱分类 | K2 III[3] |
| U−B 色指数 | +1.458[2] |
| B−V 色指数 | +1.318[2] |
| 天体测定 | |
| 径向速度 (Rv) | +4.9[4] km/s |
| 自行 (μ) | 赤经:–71.74 mas/yr 赤纬:+10.25 mas/yr |
| 视差 (π) | 10.26 ± 0.16[1] mas |
| 距离 | 318 ± 5 ly (97 ± 2 pc) |
| 绝对星等 (MV) | −1.82+0.15 −0.14[5] |
| 详细资料 | |
| 质量 | 3.2[6] M☉ |
| 半径 | 52[7] R☉ |
| 表面重力 (log g) | 2.16[8] |
| 温度 | 4320[8] K |
| 金属量 [Fe/H] | –0.13[8] dex |
| 自转速度 (v sin i) | 1.0[6] km/s |
| 其他命名 | |
| 参考数据库 | |
| SIMBAD | 资料 |
轸宿二(Epsilon Corvi,ε Crv,ε Corvi)是在南天星座乌鸦座的一颗恒星,它的固有名称Minkar /ˈmɪŋkɑːr/,源自阿拉伯语的 منقار “minqar”,意思是“乌鸦的喙”[10]。它的视星等为+3.0[2], 位于距离地球318光年(97秒差距)之处[1]。
轸宿二是一颗红巨星,其恒星分类为K2III。它已经耗尽了核心的氢,在演化上易经远离主序列。它的质量约为太阳的3倍[6]。以干涉测量术量测得到这颗恒星的角直径大约为4.99 毫角秒[13],以其估计的距离,它的真实半径大约相当于太阳半径的52倍[7]。表面的有效温度是4320 K[8],使其具有K型恒星特有的橙色色调[14]。它的质量大约是太阳的4倍,在其生命的大部分时间里都是光谱类型为B5V的主序星[15]。
参考资料[编辑]
- ↑ 1.0 1.1 1.2 1.3 van Leeuwen, F., Validation of the new Hipparcos reduction, Astronomy and Astrophysics, November 2007, 474 (2): 653–664, Bibcode:2007A&A...474..653V, S2CID 18759600, arXiv:0708.1752 可免费查阅, doi:10.1051/0004-6361:20078357
- ↑ 2.0 2.1 2.2 2.3 Celis S., L., Photoelectric photometry of late-type variable stars, Astronomy and Astrophysics Supplement Series, October 1975, 22: 9–17, Bibcode:1975A&AS...22....9C
- ↑ Houk, Nancy, Michigan catalogue of two-dimensional spectral types for the HD stars 4, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, 1979, Bibcode:1988mcts.book.....H
- ↑ Wielen, R.; et al, Sixth Catalogue of Fundamental Stars (FK6). Part I. Basic fundamental stars with direct solutions, Veroeffentlichungen des Astronomischen Rechen-Instituts Heidelberg (Astronomisches Rechen-Institut Heidelberg), 1999, 35 (35): 1, Bibcode:1999VeARI..35....1W
- ↑ Carney, Bruce W.; et al, Rotation and Macroturbulence in Metal-Poor Field Red Giant and Red Horizontal Branch Stars, The Astronomical Journal, March 2008, 135 (3): 892–906, Bibcode:2008AJ....135..892C, S2CID 2756572, arXiv:0711.4984 可免费查阅, doi:10.1088/0004-6256/135/3/892
- ↑ 6.0 6.1 6.2 Melo, C. H. F.; et al, On the nature of lithium-rich giant stars. Constraints from beryllium abundances, Astronomy and Astrophysics, August 2005, 439 (1): 227–235, Bibcode:2005A&A...439..227M, S2CID 10580797, arXiv:astro-ph/0504133 可免费查阅, doi:10.1051/0004-6361:20041805
- ↑ 7.0 7.1 Lang, Kenneth R., Astrophysical formulae, Astronomy and astrophysics library 1 3rd, Birkhäuser, 2006 [2024-04-02], ISBN 3-540-29692-1, (原始内容存档于2023-07-28). The radius (R*) is given by:
- <math>\begin{align} 2\cdot R_*
- ↑ 8.0 8.1 8.2 8.3 McWilliam, Andrew, High-resolution spectroscopic survey of 671 GK giants. I - Stellar atmosphere parameters and abundances, Astrophysical Journal Supplement Series, December 1990, 74: 1075–1128, Bibcode:1990ApJS...74.1075M, doi:10.1086/191527 可免费查阅
- ↑ MINKAR -- Variable Star, SIMBAD (Centre de Données astronomiques de Strasbourg), [2012-01-23], (原始内容存档于2024-04-11)
- ↑ Al-Sufi, Book Of Fixed Stars, Constellation: The Crow. [2024-04-02]. (原始内容存档于2020-10-03).
- ↑ (中文) 中国星座神话, written by 陈久金. Published by 台湾书房出版有限公司, 2005, ISBN 978-986-7332-25-7.
- ↑ (中文) 香港太空馆 - 研究资源 - 亮星中英对照表 互联网档案馆的存档,存档日期January 30, 2011,., Hong Kong Space Museum. Accessed on line November 23, 2010.
- ↑ Richichi, A.; Percheron, I.; Khristoforova, M., 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 可免费查阅
- ↑ The Colour of Stars, Australia Telescope, Outreach and Education (Commonwealth Scientific and Industrial Research Organisation), December 21, 2004 [2012-01-16], (原始内容存档于2012-03-18)
- ↑ Kaler, James B. (Jim), Minkar, Stars (University of Illinois), [12 July 2015], (原始内容存档于2021-04-15)