Omicron Sagittarii

ο Sagittarii

ο Sagittarii's position in Sagittarius
(rendered in Celestia)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 19h 04m 40.98s [1]
Declination 21° 44 29.4 [1]
Apparent magnitude (V) +3.76
Characteristics
Spectral type K0III
Astrometry
Proper motion (μ) RA: 76.35 ± 0.31 [1] mas/yr
Dec.: 58.12 ± 0.18 [1] mas/yr
Parallax (π)22.96 ± 0.24[1] mas
Distance142 ± 1 ly
(43.6 ± 0.5 pc)
Absolute magnitude (MV)0.61
Other designations
Manubrij, ο Sagittarii, ο Sgr, Omicron Sgr, 39 Sagittarii, BD-21 5237, CCDM J19047-2144A, GC 26224, HD 177241, HIP 93683, HR 7217, IDS 18587-2153, PPM 269274, SAO 187643, ADS 11996, WDS J19047-2144A.

Omicron Sagittarii (Omicron Sgr, ο Sagittarii, ο Sgr) is a binary star in the constellation Sagittarius. ο Sagittarii is located 142 light years from Earth[1] and is a spectral type K0 orange giant with an apparent magnitude of +3.77. It has a faint, 13th magnitude companion, ο Sagittarii B, 36 arc seconds away.

Because it is close to the ecliptic, ο Sagittarii can be occulted by the Moon and very rarely by planets. The last occultation of ο Sagittarii by a planet took place on 24 December 1937, when it was occulted by Mercury.

Name and etymology

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 van Leeuwen, F. (2007). "HIP 93683". Hipparcos, the New Reduction. Retrieved 2009-12-04.
  2. MANUBRIUM
  3. (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 5 月 11 日