天门二
| 观测资料 历元 J2000.0 | |
|---|---|
| 星座 | 室女座 |
| 星官 | 天门 （角宿） |
| 赤经 | 13h 27m 27.16348s[1] |
| 赤纬 | −15° 58′ 24.8980″[1] |
| 视星等（V） | 4.76[2] |
| 特性 | |
| 演化阶段 | 水平分支 |
| 光谱分类 | K0 III-IIIb CN1.5 CH0.5[3] |
| U−B 色指数 | +1.06[4] |
| B−V 色指数 | +1.09[4] |
| 天体测定 | |
| 径向速度 (Rv) | −12.9±0.5[5] km/s |
| 自行 (μ) | 赤经：−121.016[1] mas/yr 赤纬：+21.197[1] mas/yr |
| 视差 (π) | 12.5871 ± 0.2367[1] mas |
| 距离 | 259 ± 5 ly (79 ± 1 pc) |
| 绝对星等 (MV) | 0.09[2] |
| 详细资料 [6] | |
| 质量 | 3.51±0.94 M☉ |
| 半径 | 15[7] R☉ |
| 表面重力 (log g) | 2.70±0.11 |
| 亮度 | 87.1[7] L☉ |
| 温度 | 4,909±92 K |
| 金属量 [Fe/H] | 0.11[8] dex |
| 自转速度 (v sin i) | 4.3[7] km/s |
| 年龄 | 288+343 −156 Myr |
| 其他命名 | |
| 参考数据库 | |
| SIMBAD | 资料 |
天门二（室女座69，69 Virginis）是室女座的一颗[10]恒星，距离地球约259光年。它可以用肉眼看见，是微弱的橙色恒星，视星等 4.76，[2]但它疑似是变星，视星等从4.75到4.79之间变化。[11]天门二以 -13 km/s 的日心径向速度向地球靠近。[5]由于宇宙尘埃，天门二发出的光受到偏振。[12]
天门二是演化了的K型巨星，恒星分类为K0 III-IIIb CN1.5 CH0.5，[3]显示其恒星光谱中有过多的CN和CH分子。它是一个红群聚巨星，表明它在水平分支的核心通过氦聚变产生能量。[13]天门二的年龄约2.88亿年，质量是太阳的3.5倍[6]，半径是太阳的15倍[7]。它从扩大的光球辐射出的光是太阳的87倍[7]，有效温度 4,909 K。[6]
参考资料
[编辑]- ^ 1.0 1.1 1.2 1.3 1.4 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中此天体在盖亚望远镜第二批数据发布的记录
- ^ 2.0 2.1 2.2 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.
- ^ 3.0 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.
- ^ 4.0 4.1 Hoffleit, Dorrit; Jaschek, Carlos, The Bright star catalogue, New Haven, 1991, Bibcode:1991bsc..book.....H
- ^ 5.0 5.1 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, S2CID 59451347, arXiv:1208.3048 , doi:10.1051/0004-6361/201219219, A61.
- ^ 6.0 6.1 6.2 Feuillet, Diane K.; et al, Determining Ages of APOGEE Giants with Known Distances, The Astrophysical Journal, 2016, 817 (1): 40, Bibcode:2016ApJ...817...40F, S2CID 118675933, arXiv:1511.04088 , doi:10.3847/0004-637x/817/1/40.
- ^ 7.0 7.1 7.2 7.3 7.4 Massarotti, Alessandro; et al, Rotational and Radial Velocities for a Sample of 761 HIPPARCOS Giants and the Role of Binarity, The Astronomical Journal, January 2008, 135 (1): 209–231, Bibcode:2008AJ....135..209M, doi:10.1088/0004-6256/135/1/209.
- ^ Meléndez, J.; et al, Chemical similarities between Galactic bulge and local thick disk red giant stars, Astronomy and Astrophysics, June 2008, 484 (3): L21–L25, Bibcode:2008A&A...484L..21M, S2CID 3201679, arXiv:0804.4124 , doi:10.1051/0004-6361:200809398.
- ^ 69 Vir. SIMBAD. 斯特拉斯堡天文资料中心.
- ^ 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.
- ^ Samus, N. N.; et al, General Catalogue of Variable Stars, Astronomy Reports, 5.1, 2017, 61 (1): 80–88, Bibcode:2017ARep...61...80S, S2CID 125853869, doi:10.1134/s1063772917010085.
- ^ Leroy, J. L., A Polarimetric Investigation on Interstellar Dust Within 50-PARSECS from the Sun, Astronomy and Astrophysics, July 1993, 274 (1): 203, Bibcode:1993A&A...274..203L.
- ^ Alves, David R., K-Band Calibration of the Red Clump Luminosity, The Astrophysical Journal, August 2000, 539 (2): 732–741, Bibcode:2000ApJ...539..732A, S2CID 16673121, arXiv:astro-ph/0003329 , doi:10.1086/309278.
