HR 6902

Star system in the constellation Ophiuchus From Wikipedia, the free encyclopedia

HR 6902 (also designated V2291 Oph) is a binary system located 880 light years away from the Sun in the Ophiuchus constellation. The system includes an orange bright giant star and a B-type main sequence star, forming an eclipsing binary of Zeta Aurigae type. The system is also surrounded by a warm circumstellar envelope and the spectra show silicon and carbon absorption up to a distance of 3.3 giant radii.[4]

Quick facts Observation data Epoch J2000 Equinox J2000, Constellation ...
HR 6902

Visible, blue and ultraviolet light curves for an eclipse of V2291 Ophiuchi, adapted from Griffin et al. (1995)[1]
Observation data
Epoch J2000      Equinox J2000
Constellation Ophiuchus
Right ascension 18h 25m 38.799s[2]
Declination +08° 01 55.23[2]
Apparent magnitude (V) +5.64[3]
Characteristics
Spectral type G9IIb / B8V
Variable type Zeta Aurigae-type
Astrometry
Proper motion (μ) RA: −3.920[2] mas/yr
Dec.: −6.549[2] mas/yr
Parallax (π)3.7061±0.1604 mas[2]
Distance880 ± 40 ly
(270 ± 10 pc)
Absolute magnitude (MV)–1.33[3]
Orbit
Period (P)1.055[4] yr
Semi-major axis (a)1.96[4] AU
Eccentricity (e)0.311[4]
Inclination (i)87[4]°
Details
Mass3.86/2.95[4] M
Radius33/3[4] R
Luminosity562/146 L
Temperature4,900/11,600[4] K
Other designations
V2291 Oph, GSC 01023-02454, HD 169690, HD 169689, 2MASS J18253880+0801551, BD+07 3682, FK5 1478, PPM 165790, HIP 90313, SAO 123462
Database references
SIMBADdata
Close

References

Related Articles

Wikiwand AI