HR 6902

HR 6902

Visible, blue and ultraviolet light curves for an eclipse of V2291 Ophiuchi, adapted from Griffin et al. (1995)
Observation data
Epoch J2000      Equinox ICRS
Constellation Ophiuchus
Right ascension 18h 25m 38.799s
Declination +08° 01′ 55.23″
Apparent magnitude (V) +5.64
Characteristics
Spectral type G9IIb / B8V[citation needed]
Variable type Zeta Aurigae-type[citation needed]
Astrometry
Proper motion (μ) RA: −3.920 mas/yr
Dec.: −6.549 mas/yr
Parallax (π)3.7061±0.1604 mas
Distance880 ± 40 ly
(270 ± 10 pc)
Absolute magnitude (MV)–1.33
Orbit
Period (P)1.055 yr
Semi-major axis (a)1.96 AU
Eccentricity (e)0.311
Inclination (i)87°
Details
Mass3.86/2.95 M☉
Radius33/3 R☉
Luminosity562/146 L☉
Temperature4,900/11,600 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

HR 6902 (also designated V2291 Oph) is a binary system located 880 light years away from the Sun in the constellation Ophiuchus. 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.

References

  1. ↑ Griffin, R. E. M.; Marshall, K. P.; Griffin, R. F.; Schroeder, K. P. (September 1995). "Optical spectra of ζ Aurigae binary systems. VII. The 1987 and 1989 eclipses of HR 6902". Astronomy and Astrophysics. 301: 217–230. Bibcode:1995A&A...301..217G.
  2. ↑ Roman, Nancy G. (1987). "Identification of a constellation from a position". Publications of the Astronomical Society of the Pacific. 99 (617): 695. Bibcode:1987PASP...99..695R. doi:10.1086/132034. Constellation record for this object at VizieR.
  3. 1 2 3 4 5 Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
  4. 1 2 Jasniewicz, G.; et al. (February 1999). "Late-type giants with infrared excess. I. Lithium abundances". Astronomy and Astrophysics. 342: 831–838. Bibcode:1999A&A...342..831J.
  5. 1 2 3 4 5 6 7 8 Kirsch; Baade, R.; Reimers, D. (2001). "The warm circumstellar envelope and wind of the G9 IIb star HR 6902". Astronomy and Astrophysics. 379 (3): 925–935. arXiv:astro-ph/0008378. Bibcode:2001A&A...379..925K. doi:10.1051/0004-6361:20011117. S2CID 12157488.