Omega1 Cygni

B-type subgiant star in the constellation Cygnus From Wikipedia, the free encyclopedia

Omega1 Cygni, Latinized from ω1 Cygni, is the Bayer designation for a solitary[13] star in the northern constellation of Cygnus. It is visible to the naked eye with an apparent visual magnitude of 4.94.[4] Based upon an annual parallax shift of 2.59 mas,[7] it is estimated to lie roughly 1,260 light years from the Sun. Relative to its neighbors, this star has a peculiar velocity of 25.7±2.2 km/s.[6]

A light curve for V2014 Cygni, plotted from TESS data[14]
Right ascension20h 30m 03.54116s[1]
Declination+48° 57 05.6446[1]
Apparentmagnitude(V)+4.93 - 4.96[2]
Quick facts Constellation, Right ascension ...
Omega1 Cygni
Location of ω1 Cygni (circled in red)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cygnus
Right ascension 20h 30m 03.54116s[1]
Declination +48° 57 05.6446[1]
Apparent magnitude (V) +4.93 - 4.96[2]
Characteristics
Spectral type B2.5 IV[3]
U−B color index −0.68[4]
B−V color index −0.09[4]
Variable type β Cep[5] (λ Eri[2])
Astrometry
Radial velocity (Rv)−21.9±2.0[6] km/s
Proper motion (μ) RA: +10.883[7] mas/yr
Dec.: +7.057[7] mas/yr
Parallax (π)2.5878±0.1637 mas[7]
Distance1,260 ± 80 ly
(390 ± 20 pc)
Absolute magnitude (MV)−2.65[8]
Details
Mass8.1±0.2[3] M
Radius4.55[9][a] R
Luminosity1,549[9] L
Surface gravity (log g)2.312[10] cgs
Temperature16,982[9] K
Metallicity [Fe/H]0.0[8] dex
Rotational velocity (v sin i)145[11] km/s
Age33.2±4.5[3] Myr
Other designations
ω1 Cyg, 45 Cygni, BD+48°3142, FK5 3641, HD 195556, HIP 101138, HR 7844, SAO 49712, V2014 Cygni[12]
Database references
SIMBADdata
Close

This is a somewhat evolved B-type subgiant star with a stellar classification of B2.5 IV.[3] Telting and colleagues report it as a Beta Cephei variable with a high degree of confidence as they found regular pulsations in its spectrum in a high-resolution spectroscopy study published in 2006.[5] Its brightness varies irregularly by 0.034 magnitude every 1.137 days.[15]

Notes

  1. Calculated, using the Stefan-Boltzmann law and the star's effective temperature and luminosity, with respect to the solar nominal effective temperature of 5,772 K:

References

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