HR 6902
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Ophiuchus |
| Right ascension | 18h 25m 38.799s[1] |
| Declination | +08° 01′ 55.23″[1] |
| Apparent magnitude (V) | +5.64[2] |
| Characteristics | |
| Spectral type | G9IIb / B8V |
| Variable type | Zeta Aurigae-type |
| Astrometry | |
| Proper motion (μ) | RA: -4.07 ± 0.54[1] mas/yr Dec.: -6.34 ± 0.31[1] mas/yr |
| Parallax (π) | 4.14 ± 0.41[1] mas |
| Distance | 790 ± 80 ly (240 ± 20 pc) |
| Absolute magnitude (MV) | –1.33[2] |
| Details | |
| Mass | 3.86/2.95[3] M☉ |
| Radius | 33/3[3] R☉ |
| Luminosity | 562/146 L☉ |
| Temperature | 4900/11600[3] K |
| Orbit | |
| Period (P) | 1.055[3] yr |
| Semi-major axis (a) | 1.96[3] Astronomical Units" |
| Eccentricity (e) | 0.311[3] |
| Inclination (i) | 87[3]° |
| Other designations | |
| Database references | |
| SIMBAD | data |
HR 6902 (also designated V2291 Oph) is a binary system located 790 light years away[1] 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.[3]
References
- 1 2 3 4 5 6 van Leeuwen, F. (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. Vizier catalog entry
- 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
- 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.
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