Omicron Velorum

ο Velorum


Location of ο Velorum (circled)

Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Vela
Right ascension 08h 40m 17.58553s[1]
Declination –52° 55 18.8002[1]
Apparent magnitude (V) +3.60[2] (3.57 - 3.63[3])
Characteristics
Spectral type B3 IV[4]
U−B color index –0.62[2]
B−V color index –0.18[2]
Variable type SPB[3]
Astrometry
Proper motion (μ) RA: –24.42[1] mas/yr
Dec.: +34.44[1] mas/yr
Parallax (π)6.61 ± 0.35[1] mas
Distance490 ± 30 ly
(151 ± 8 pc)
Details
Mass5.5 ± 0.4[4] M
Radius4.3 ± 0.7[4] R
Luminosity1,000[4] L
Surface gravity (log g)3.91 ± 0.20[4] cgs
Temperature16,200 ± 700[4] K
Rotational velocity (v sin i)9 ± 5[4] km/s
Other designations
CP-52 1583, FK5 1227, HD 74195, HIP 42536, HR 3447, SAO 236164.

Omicron Velorum (ο Vel, ο Velorum) is a star in the constellation Vela. It is the brightest member of the loose naked eye open cluster IC 2391, also known as the ο Velorum Cluster.

Omicron Velorum is a blue-white B-type subgiant with a mean apparent magnitude of +3.60. It is approximately 495 light years from Earth. A slowly pulsating B star, it ranges between magnitudes 3.57 and 3.63 over 2.8 days.[3]

References

  1. 1 2 3 4 5 van Leeuwen, F. (November 2007), "Validation of the new Hipparcos reduction", Astronomy and Astrophysics 474 (2): 653–664, arXiv:0708.1752, Bibcode:2007A&A...474..653V, doi:10.1051/0004-6361:20078357
  2. 1 2 3 Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99), Bibcode:1966CoLPL...4...99J
  3. 1 2 3 Samus, N. N.; Durlevich, O. V.; et al. (2009). "VizieR Online Data Catalog: General Catalogue of Variable Stars (Samus+ 2007-2013)". VizieR On-line Data Catalog: B/gcvs. Originally published in: 2009yCat....102025S 1. Bibcode:2009yCat....102025S.
  4. 1 2 3 4 5 6 7 Hubrig, S.; et al. (January 2009), "New magnetic field measurements of beta Cephei stars and Slowly Pulsating B stars", Astronomische Nachrichten 330 (4): 317, arXiv:0902.1314, Bibcode:2009AN....330..317H, doi:10.1002/asna.200811187
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