Omicron Sagittarii
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Sagittarius |
Right ascension | 19h 04m 40.98177s[1] |
Declination | −21° 44′ 29.3845″[1] |
Apparent magnitude (V) | +3.771[2] |
Characteristics | |
Evolutionary stage | horizontal branch[3] |
Spectral type | G9IIIb[4] |
B−V color index | +1.012±0.008[5] |
Absolute magnitude (MV) | 0.625[2] |
Details | |
Gyr | |
Database references | |
SIMBAD | data |
ο Sagittarii, Latinized as Omicron Sagittarii, is a single
This object is position 0.86 degrees north of the ecliptic, so ο Sagittarii can be occulted by the Moon and very rarely by planets. The last occultation by a planet took place on 24 December 1937, when it was occulted by Mercury.[citation needed] It was almost eclipsed by the sun, which occupies a mean, rounded, half of one degree of the sky, on 5 January.[10] Thus the star can be viewed the whole night, crossing the sky, in early July.
This is an aging
It has a faint, magnitude 13.8 companion, designated component B and positioned 38.4
Name and etymology
- In Chinese name for ο Sagittarii itself is 建二 (Jiàn èr, English: the Second Star of Establishment.)[12]
References
- ^ S2CID 18759600.
- ^ .
- ^ S2CID 16673121.
- ^ doi:10.1086/191373.
- ^ S2CID 119257644.
- ^ S2CID 118505114.
- ^ .
- ^ "omi Sgr". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2019-10-09.
- S2CID 14878976.
- ^ In the Sky Earth astronomy reference utility showing the ecliptic and relevant date as at J2000 - present
- doi:10.1086/323920.
- ^ (in Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 11 日