σ Boötis
Observation data Epoch J2000 Equinox J2000 |
Constellation |
Boötes |
Right ascension |
14h 34m 40.8171s |
Declination |
+29° 44′ 42.468″ |
Apparent magnitude (V) | 4.46 |
Characteristics |
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Spectral type | F2V |
U−B color index | -0.08 |
B−V color index | 0.36 |
R−I color index | 0.19 |
Variable type | Variable star |
Astrometry |
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Radial velocity (Rv) | 0.2 km/s |
Proper motion (μ) | RA: 188.32 mas/yr Dec.: 132.72 mas/yr |
Parallax (π) | 64.66 ± 0.72 mas |
Distance | 50.4 ± 0.6 ly (15.5 ± 0.2 pc) |
Absolute magnitude (MV) | 4.82 |
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Details |
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Radius | 1.431 ± 0.023[1] R☉ |
Luminosity | 3.461 ± 0.042[1] L☉ |
Temperature | 6,594 ± 55[1] K |
Age | 1.7[2] Gyr |
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Other designations |
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28 Boötis, HR 5447, HD 128167, Gl 557, BD+30°2536, FK5 1380, HIP 71284, SAO 83416, GC 19659, CCDM 14347+2945. |
Database references |
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SIMBAD | data |
Data sources: |
Hipparcos Catalogue, CCDM (2002), Bright Star Catalogue (5th rev. ed.) |
Database references |
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SIMBAD | data |
Sigma Boötis (σ Boo, σ Boötis) is a star in the constellation Boötes.
Sigma Boötis is a yellow-white F-type main sequence dwarf with an apparent magnitude of +4.47. It is approximately 50.4 light years from Earth.
In Chinese, 梗河 (Gěng Hé), meaning Celestial Lance, refers to an asterism consisting of σ Boötis, ε Boötis and ρ Boötis.[3] Consequently, σ Boötis itself is known as 梗河二 (Gěng Hé èr, English: the Second Star of Celestial Lance.)[4]
Located to the southeast of Rho Boötis, the fusing dwarf Sigma may at first appear as a naked-eye double, but the angular proximity with Rho is merely line-of-sight. Like many of its spectral class, Sigma is apparently a variable of the Delta Scuti variety, which vary subtly with multiple periods of hours.
References
- ↑ 1.0 1.1 1.2 Boyajian, Tabetha S. et al. (February 2012), "Stellar Diameters and Temperatures. I. Main-sequence A, F, and G Stars", The Astrophysical Journal 746 (1): 101, arXiv:1112.3316, Bibcode:2012ApJ...746..101B, doi:10.1088/0004-637X/746/1/101 . See Table 10.
- ↑ Decin, G. et al. (November 2003), "Age Dependence of the Vega Phenomenon: Observations", The Astrophysical Journal 598 (1): 636–644, arXiv:astro-ph/0308294, Bibcode:2003ApJ...598..636D, doi:10.1086/378800
- ↑ (Chinese) 中國星座神話, written by 陳久金. Published by 台灣書房出版有限公司, 2005, ISBN 978-986-7332-25-7.
- ↑ (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 29 日
External links
← Star systems within 50–55 light-years → |
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- Castor (51.6 ± 1.0 ly; 6 stars)
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- 51 Pegasi (50.1 ± 0.6 ly; 1 star, 1 planet: b «Bellerophon»)
- GJ 3233 (50.2+6.0
−4.9 ly; 1 star)
- Gliese 758 (50.5 ± 0.5 ly; 1 star, 1 brown dwarf: B)
- HD 38858 (50.8 ± 0.9 ly; 1 star, 1 planet: b)
- HR 8323 (51.0 ± 0.6 ly; 1 star)
- 104 Tauri (51.8 ± 0.8 ly; 2 stars)
- Gliese 777 (51.8 ± 0.5 ly; 3 stars, 2 planets: c
- b)
- GJ 3781 (52.3 ± 1.2 ly; 2 stars)
- HR 3138 (52.8 ± 0.4 ly; 3 stars)
- 9 Puppis (53.4 ± 0.8 ly; 2 stars)
- Psi⁵ Aurigae (53.9 ± 0.6 ly; 1 star)
- HD 53705/53706/53680 (53.9 ± 0.9 ly; 4 stars)
- HR 5273 (54.1 ± 0.7 ly; 2 stars)
- HR 2225 (54.5 ± 0.7 ly; 1 star)
- 39 Tauri (54.6 ± 0.8 ly; 2 stars)
- Gliese 295 (54.8 ± 0.7 ly; 1 star)
- HR 2721 (55.0 ± 0.6 ly; 1 star)
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- HR 159 (50.2 ± 0.8 ly; 2 stars)
- Gliese 156 (50.3 ± 0.9 ly; 1 star)
- Gliese 862 (50.4 ± 0.8 ly; 1 star)
- Gliese 227 (50.4 ± 0.7 ly; 1 star)
- HD 135599 (50.8 ± 0.8 ly; 1 star)
- Gliese 778 (50.8 ± 0.7 ly; 1 star)
- GJ 1175 (50.9 ± 0.6 ly; 1 star)
- Gliese 782 (51.1 ± 1.2 ly; 1 star)
- Gliese 397 (51.1 ± 1.0 ly; 1 star)
- HD 113538 (51.2 ± 1.1 ly; 1 star, 2 planets: b
- c)
- HD 139763 (51.3 ± 1.1 ly; 1 star)
- Gliese 157 (51.4 ± 1.7 ly; 3 stars)
- Gliese 619 (51.9 ± 0.7 ly; 1 star)
- Gliese 112.1 (51.9 ± 1.3 ly; 1 star)
- Gliese 156.2 (52.1 ± 0.7 ly; 1 star)
- Gliese 462 (52.2 ± 1.1 ly; 1 star)
- Gliese 3 (52.2 ± 0.7 ly; 1 star)
- Gliese 32 (52.3 ± 1.4 ly; 2 stars)
- Gliese 472 (52.8 ± 0.5 ly; 1 star)
- Gliese 824 (52.8 ± 0.9 ly; 1 star)
- Gliese 152 (52.9 ± 0.6 ly; 1 star)
- Gliese 143 (53.4 ± 1.3 ly; 1 star)
- GJ 1177 (53.4 ± 2.7 ly; 2 stars)
- Gliese 826.1 (53.4 ± 1.2 ly; 1 star)
- Gliese 247 (53.5 ± 1.2 ly; 1 star)
- BY Draconis (53.6 ± 0.6 ly; 1 star)
- Gliese 531 (53.6 ± 0.8 ly; 1 star)
- Gliese 322 (53.8 ± 1.3 ly; 1 star)
- Gliese 553 (53.9 ± 1.4 ly; 1 star)
- HD 128311 (54.0 ± 0.9 ly; 1 star, 2 planets: b
- c)
- Gliese 795 (54.5 ± 2.0 ly; 2 stars)
- A 2329 (54.6 ± 1.1 ly; 2 stars)
- GJ 1181 (54.8 ± 2.5 ly; 2 stars)
- Gliese 786 (54.8 ± 0.7 ly; 1 star)
- HD 7924 (54.9 ± 0.5 ly; 1 star, 1 planet: b)
- Gliese 895.4 (55.0 ± 0.6 ly; 1 star)
- Gliese 200 (55.0 ± 1.6 ly; 2 stars)
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- GJ 3685/3686 (50.7+11.8
−8.0 ly; 2 stars)
- GJ 1062 (52.3 ± 2.9 ly; 1 star)
- HD 179930 (52.5 ± 1.7 ly; 2 stars)
- GJ 1264 (52.6 ± 2.1 ly; 1 star)
- Gliese 676 (53.7 ± 1.5 ly; 2 stars, 4 planets: Ad
- Ae
- Ab
- Ac)
- GJ 1049 (53.9 ± 1.2 ly; 1 star)
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T |
- WISE 0614+3912 (~50.2 ly; 1 brown dwarf)
- WISE 1617+1807 (~50.2 ly; 1 brown dwarf)
- WISE 1627+3255 (~50.2 ly; 1 brown dwarf)
- WISE 0542-1628 (~50.6 ly; 1 brown dwarf)
- WISE 1124-0421 (~50.6 ly; 1 brown dwarf)
- WISE 2015+6646 (~50.6 ly; 1 brown dwarf)
- WISE 1519+7009 (~50.9 ly; 1 brown dwarf)
- WISE 0325-3854 (~51.2 ly; 1 brown dwarf)
- WISE 2342+0856 (~51.2 ly; 1 brown dwarf)
- WISE 0614+0951 (~51.5 ly; 1 brown dwarf)
- WISE 0750+2725 (~51.5 ly; 1 brown dwarf)
- WISE 0906+4735 (~51.5 ly; 1 brown dwarf)
- WISE 1906+4508 (~51.5 ly; 1 brown dwarf)
- WISE 1457+5815 (~52.2 ly; 1 brown dwarf)
- WISE 2319-1844 (~52.2 ly; 1 brown dwarf)
- WISE 1622-0959 (52.2 ± 6.5 ly; 1 brown dwarf)
- WISE 1042-3842 (~53.2 ly; 1 brown dwarf)
- WISE 2237-0614 (~53.5 ly; 1 brown dwarf)
- WISE 0241-3653 (~53.8 ly; 1 brown dwarf)
- WISE 0656+4205 (~54.1 ly; 1 brown dwarf)
- WISE 2348-1028 (~54.1 ly; 1 brown dwarf)
- WISE 1804+3117 (54.4+12.2
−8.4 ly; 1 brown dwarf)
- WISE 0148+7202 (54.4+19.8
−11.4 ly; 1 brown dwarf)
- WISE 0333-5856 (~54.8 ly; 1 brown dwarf)
- WISE 2357+1227 (~54.8 ly; 1 brown dwarf)
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In left column are stellar classes of primary members of star systems. Bold are systems containing at least one component with absolute magnitude of +8.5 or brighter. Italic are systems without known trigonometric parallax. |
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