Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Gemini |
Right ascension | 06h 11m 49.0763s[1] |
Declination | +22° 49′ 32.686″[1] |
Apparent magnitude (V) | 11.51 |
Astrometry | |
Proper motion (μ) | RA: -0.067[1] mas/yr Dec.: -1.889[1] mas/yr |
Parallax (π) | 0.4403 ± 0.0856 mas[1] |
Distance | approx. 7,000 ly (approx. 2,300 pc) |
Orbit[2] | |
Period (P) | 78.80±0.01 d |
Eccentricity (e) | 0.0±0.01 |
Semi-amplitude (K1) (primary) | 52.9±0.1 km/s |
Semi-amplitude (K2) (secondary) | 11.2±1.0 km/s |
Details[2] | |
stripped helium star | |
Mass | 1.5±0.4 M☉ |
Luminosity | 630 L☉ |
Surface gravity (log g) | 3.0±0.2 cgs |
Temperature | 12700±500 K |
Be star | |
Mass | 7±2 M☉ |
Luminosity | 1,260 L☉ |
Surface gravity (log g) | 4.0±0.3 cgs |
Temperature | 18000±2000 K |
Database references | |
SIMBAD | data |
LB-1 is a binary star system in the constellation Gemini. In 2019 a paper in Nature proposed the system contained an unusually massive stellar black hole outside of ordinary single stellar evolution parameters.[3] However, analyses in 2020 found the original 2019 conclusion to be incorrect. Some researchers now believe the system consists of a stripped B-type star and a massive rapidly rotating Be star.[2][4]
Shenar_etal_2020
was invoked but never defined (see the help page).