QS Virginis

QS Virginis

Visual band light curves for QS Virginis, adapted from O’Donoghue et al. (2003). The lowest plot shows two pre-eclipse dips.
Observation data
Epoch J2000      Equinox J2000
Constellation Virgo
Right ascension 13h 49m 52.0032s
Declination −13° 13 37.002
Apparent magnitude (V) +14.8
Characteristics
Spectral type DAm / M3.5V
Astrometry
Proper motion (μ) RA: 41.618±0.108 mas/yr
Dec.: 17.984±0.097 mas/yr
Parallax (π)19.9632±0.0584 mas
Distance163.4 ± 0.5 ly
(50.1 ± 0.1 pc)
Absolute magnitude (MV)11.74 + 11.82
Orbit
Period (P)217.092 min
Semi-major axis (a)0.0056 AU
Eccentricity (e)0.0
Inclination (i)60°
Details
White dwarf
Mass0.78 M
Radius0.011 R
Luminosity0.0044 L
Surface gravity (log g)8.34 cgs
Temperature14,200 K
Rotational velocity (v sin i)400 km/s
Red dwarf
Mass0.43 M
Radius0.42 R
Luminosity0.015 L
Temperature3,100 K
Rotational velocity (v sin i)140 km/s
Other designations
GSC 05559-00143, 1RXS J134951.0-131338, WD 1347-129, EC 13471-1258, SBC9 1944
Database references
SIMBADdata

QS Virginis (abbreviated QS Vir) is an eclipsing binary system approximately 163 light-years away from the Sun, forming a cataclysmic variable. The system comprises an eclipsing white dwarf and red dwarf that orbit each other every 3.62 hours.