Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ophiuchus[1] |
Right ascension | 17h 28m 41.09661s[2] |
Declination | −00° 34′ 51.5234″[2] |
Characteristics | |
Sun-like star | |
Evolutionary stage | Main sequence |
Spectral type | G[3] |
Apparent magnitude (G) | 13.77[3] |
Black hole | |
Evolutionary stage | Stellar black hole |
Astrometry | |
Radial velocity (Rv) | 23.03±2.63[2] km/s |
Proper motion (μ) | RA: −7.70±0.020 mas/yr[3] Dec.: −25.85±0.027 mas/yr[3] |
Parallax (π) | 2.09 ± 0.02 mas[3] |
Distance | 1,560 ± 10 ly (478 ± 5 pc) |
Orbit[3] | |
Period (P) | 185.59±0.05 d |
Semi-major axis (a) | 1.40±0.01 AU |
Eccentricity (e) | 0.451±0.005 |
Inclination (i) | 126.6±0.4° |
Longitude of the node (Ω) | 97.8±1.0° |
Periastron epoch (T) | 2457387.9±0.7 |
Argument of periastron (ω) (secondary) | 12.8±1.1° |
Details[3] | |
Sun-like star | |
Mass | 0.93±0.05 M☉ |
Radius | 0.99±0.05 R☉ |
Luminosity (bolometric) | 1.06±0.04 L☉ |
Surface gravity (log g) | 4.55±0.16 cgs |
Temperature | 5850±50 K |
Metallicity [Fe/H] | −0.2±0.05 dex |
Rotational velocity (v sin i) | <3.5 km/s |
Black hole | |
Mass | 9.62±0.18 M☉ |
Other designations | |
Database references | |
SIMBAD | data |
Gaia BH1 (Gaia DR3 4373465352415301632) is a binary system consisting of a G-type main-sequence star and a likely stellar-mass black hole, located about 1,560 light-years (478 pc) away from the Solar System in the constellation of Ophiuchus.[4] As of May 2024[update], it is the nearest known system that astronomers are reasonably confident contains a black hole, followed by Gaia BH3, Gaia BH2 and A0620-00.[3][5]
GaiaDR3
was invoked but never defined (see the help page).El-Badry2022
was invoked but never defined (see the help page).NOIRLab2227
was invoked but never defined (see the help page).