Sigma Boötis
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Boötes
|
Right ascension | 14h 34m 40.81718s[1] |
Declination | +29° 44′ 42.4637″[1] |
Apparent magnitude (V) | 4.46[2] |
Characteristics | |
Spectral type | F4VkF2mF1[3] |
U−B color index | −0.084[2] |
B−V color index | +0.366[2] |
Variable type | Suspected[4] |
Absolute magnitude (MV) | 3.52[6] |
Details | |
Gyr | |
Database references | |
SIMBAD | data |
Sigma Boötis, its name
The
Sigma Boötis is a solar-type star but is larger and more massive than the Sun. It has an estimated age of around two
Infrared surveys with the Spitzer and Herschel space telescopes failed to detect an infrared excess around this star at wavelengths up to 160 μm. However, the HOSTS Survey with the Large Binocular Telescope reported a detection of an excess in the far infrared, indicating the presence of exozodiacal dust near the habitable zone of the star.[21]
Nomenclature
Sigma Boötis is known by several different names, including σ Boo, 28 Boötis, BD+30°2536, GC 19659, GJ 557, HD 128167, HIP 71284, HR 5447, SAO 83416, and CCDM 14347+2945.[14]
Chinese name
In
References
- ^ .
- ^ hdl:2152/34447.
- ^ doi:10.1086/319956.
- S2CID 125853869.
- S2CID 51814894.
- ^ S2CID 56332289, A67.
- S2CID 33401607.
- ^ S2CID 125765376, 111.
- ^ S2CID 18993744.. See Table 10.
- S2CID 118786105.
- ^ S2CID 43455849.
- ^ S2CID 16751327.
- ^ S2CID 693296.
- ^ a b "sig Boo", SIMBAD, Centre de données astronomiques de Strasbourg, retrieved 2021-01-26.
- S2CID 14878976.
- S2CID 119237891.
- S2CID 2603568.
- Bibcode:2009ssc..book.....G.
- .
- S2CID 119267456.
- S2CID 52227431, 194.
- ISBN 978-986-7332-25-7.
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 6 月 29 日