Visual band light curves for QS Virginis, adapted from O’Donoghue et al. (2003).[1] The lowest plot shows two pre-eclipse dips. | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 13h 49m 52.0032s[2] |
Declination | −13° 13′ 37.0019″[2] |
Apparent magnitude (V) | +14.8 |
Characteristics | |
Spectral type | DAm / M3.5V |
Astrometry | |
Proper motion (μ) | RA: 41.618±0.108[2] mas/yr Dec.: 17.984±0.097[2] mas/yr |
Parallax (π) | 19.9632 ± 0.0584 mas[2] |
Distance | 163.4 ± 0.5 ly (50.1 ± 0.1 pc) |
Absolute magnitude (MV) | 11.74 + 11.82[1] |
Orbit | |
Period (P) | 217.092 min[1] |
Semi-major axis (a) | 0.0056 AU |
Eccentricity (e) | 0.0 |
Inclination (i) | 60[1]° |
Details[1] | |
White dwarf | |
Mass | 0.78 M☉ |
Radius | 0.011 R☉ |
Luminosity | 0.0044[3] L☉ |
Surface gravity (log g) | 8.34 cgs |
Temperature | 14,200 K |
Rotational velocity (v sin i) | 400 km/s |
Red dwarf | |
Mass | 0.43 M☉ |
Radius | 0.42 R☉ |
Luminosity | 0.015[3] L☉ |
Temperature | 3,100 K |
Rotational velocity (v sin i) | 140 km/s |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
QS Virginis (abbreviated QS Vir) is an eclipsing binary system approximately 163 light-years away from the Sun,[1][2] forming a cataclysmic variable. The system comprises an eclipsing white dwarf and red dwarf that orbit each other every 3.37 hours.[1]
Gaia DR2
was invoked but never defined (see the help page).Simbad
was invoked but never defined (see the help page).