The HW Virginis system in Celestia. | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 12h 44m 20.2387s[1] |
Declination | −08° 40′ 16.8486″[1] |
Apparent magnitude (V) | 10.69[2] |
Characteristics | |
Spectral type | sdB / dM[3] |
Variable type | eclipsing binary |
Astrometry | |
Proper motion (μ) | RA: 8.969±0.175[1] mas/yr Dec.: −15.677±0.107[1] mas/yr |
Parallax (π) | 5.7972 ± 0.0849 mas[1] |
Distance | 563 ± 8 ly (172 ± 3 pc) |
Absolute magnitude (MV) | 4.22 (sdB) + 15.59 (dM)[4] |
Absolute bolometric magnitude (Mbol) | 1.46 (sdB) + 11.20 (dM)[4] |
Orbit[4] | |
Period (P) | 0.11671967 d |
Semi-major axis (a) | 0.860 ± 0.010 R☉ |
Eccentricity (e) | <0.0003 |
Inclination (i) | 80.98 ± 0.10° |
Details[4] | |
sdB | |
Mass | 0.485 ± 0.013 M☉ |
Radius | 0.183 ± 0.026 R☉ |
Luminosity | 19.7 ± 5.6 L☉ |
Temperature | 28488 ± 208 K |
dM | |
Mass | 0.142 ± 0.004 M☉ |
Radius | 0.175 ± 0.026 R☉ |
Luminosity | 0.003 ± 0.001 L☉ |
Temperature | 3084 ± 889 K |
Other designations | |
Database references | |
SIMBAD | data |
HW Virginis, abbreviated HW Vir, is an eclipsing binary system (of the Algol type), approximately 563 light-years away based on the parallax measured by the Gaia spacecraft,[1] in the constellation of Virgo. The system comprises an eclipsing B-type subdwarf star and red dwarf star. The two stars orbit each other every 0.116795 days.[6]
Gaia DR2
was invoked but never defined (see the help page).BrownSevilla
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).