Gamma Ophiuchi
| |
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Ophiuchus |
Right ascension | 17h 47m 53.57s |
Declination | +02° 42′ 26.9″ |
Apparent magnitude (V) | +3.75 |
Characteristics | |
Spectral type | A0 V[1] |
Astrometry | |
Distance | 95 ly (29.14 pc) |
Absolute magnitude (MV) | +1.43 |
Details | |
Mass | 2.9[1] M☉ |
Radius | 1.8[2] R☉ |
Luminosity | 29[1] L☉ |
Temperature | 9506[1] K |
Rotational velocity (v sin i) | 220[3] km/s |
Age | +93 −134 184[3] Myr |
Other designations | |
Gamma Ophiuchi (γ Oph, γ Ophiuchi) is a fourth-magnitude star in the constellation Ophiuchus. It is located about 95 light-years from Earth. The system has an age of roughly 184 million years.[1]
This is an A-type main sequence star with a stellar classification of A0 V.[1] It has nearly three times the mass of the Sun and 1.8 times the Sun's radius.[2] The star shines with 29[1] times the luminosity of the Sun, which is being emitted from its outer atmosphere at an effective temperature of K. 9506[1] It is radiating an excess emission of infrared, suggesting the presence of a circumstellar disk of dust at an orbital radius of 64 AU from the host star.[1]
References
- 1 2 3 4 5 6 7 8 9 Wyatt, M. C.; et al. (July 2007), "Steady State Evolution of Debris Disks around A Stars", The Astrophysical Journal, 663 (1): 365–382, arXiv:astro-ph/0703608, Bibcode:2007ApJ...663..365W, doi:10.1086/518404
- 1 2 Malagnini, M. L.; Morossi, C. (November 1990), "Accurate absolute luminosities, effective temperatures, radii, masses and surface gravities for a selected sample of field stars", Astronomy and Astrophysics Supplement Series, 85 (3): 1015–1019, Bibcode:1990A&AS...85.1015M
- 1 2 Song, Inseok; et al. (February 2001), "Ages of A-Type Vega-like Stars from uvbyβ Photometry", The Astrophysical Journal, 546 (1): 352–357, arXiv:astro-ph/0010102, Bibcode:2001ApJ...546..352S, doi:10.1086/318269
- ↑ "HD 161868 -- Star", SIMBAD Astronomical Database, retrieved 2007-01-20
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