HW Virginis

HW Virginis

The HW Virginis system in Celestia.
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 12h 44m 20.2387s
Declination −08° 40 16.849
Apparent magnitude (V) 10.69
Characteristics
Spectral type sdB / dM
Variable type eclipsing binary
Astrometry
Proper motion (μ) RA: 8.969±0.175 mas/yr
Dec.: −15.677±0.107 mas/yr
Parallax (π)5.7972±0.0849 mas
Distance563 ± 8 ly
(172 ± 3 pc)
Absolute magnitude (MV)4.22 (sdB) + 15.59 (dM)
Absolute bolometric
magnitude
 (Mbol)
1.46 (sdB) + 11.20 (dM)
Orbit
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
sdB
Mass0.485 ± 0.013 M
Radius0.183 ± 0.026 R
Luminosity19.7 ± 5.6 L
Temperature28488 ± 208 K
dM
Mass0.142 ± 0.004 M
Radius0.175 ± 0.026 R
Luminosity0.003 ± 0.001 L
Temperature3084 ± 889 K
Other designations
BD−07 3477, HIP 62157, 2MASS J12442024-0840168
Database references
SIMBADdata

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, 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.