QS Virginis
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 | |
Absolute magnitude (MV) | 11.74 + 11.82[1] | |
Inclination (i) 60[1]° | | |
Details Rotational velocity (v sin i)140 km/s | | |
Database references | ||
Exoplanet Archive | data |
QS Virginis (abbreviated QS Vir) is an
Variability
The eclipsing binary nature of QS Virginis was discovered in 1997 during the Edinburgh-Cape Blue Object Survey for blue stellar objects in the southern hemisphere.[5]
Possible third body
In 2009 the discovery of an extrasolar planet in orbit around the binary star was announced, detected by variations in the timings of the eclipses of the two stars.
Subsequent observations revealed that the timings were not following the pattern predicted by the planetary model. While the observed variations in eclipse times may be caused by a third body, the best fit model orbit is for an object with minimum mass 0.05 solar masses (about 50 times the mass of Jupiter) in a highly eccentric 14-year orbit.[7]
See also
- Algol
- HW Virginis
- NN Serpentis
- CM Draconis
- DP Leonis
- NSVS 14256825
- List of extrasolar planets
References