V3903 Sagittarii

V3903 Sagittarii

A red-light light curve for V3903 Sagittarii, adapted from Wraight et al. (2011)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 18h 09m 17.6999s
Declination −23° 59 18.2312
Apparent magnitude (V) 7.00–7.45
Characteristics
Spectral type O7V(n)z + B0:V:
U−B color index −0.82
B−V color index +0.16
Variable type Algol
Astrometry
Proper motion (μ) RA: +0.87±0.67 mas/yr
Dec.: −0.66±0.42 mas/yr
Parallax (π)0.8368±0.0258 mas
Distance3,900 ± 100 ly
(1,200 ± 40 pc)
Absolute magnitude (MV)−4.59 + −3.69
Orbit
Period (P)1.744204 days
Eccentricity (e)0
Inclination (i)65.20°
Semi-amplitude (K1)
(primary)
236.6 km/s
Semi-amplitude (K2)
(secondary)
339.4 km/s
Details
A
Mass27.27 M
Radius8.088 R
Luminosity122,000 L
Surface gravity (log g)4.058 cgs
Temperature38,000 K
Rotational velocity (v sin i)230 km/s
B
Mass19.01 M
Radius6.125 R
Luminosity45,500 L
Surface gravity (log g)4.143 cgs
Temperature34,100 K
Rotational velocity (v sin i)170 km/s
Age1.6 Myr
Other designations
V3903 Sgr, CD−24°13962, HD 165921, HIP 88943, SAO 186366
Database references
SIMBADdata

V3903 Sagittarii (also known as 11 Sagittarii, or its abbreviation 11 Sgr) is an eclipsing binary star system in the constellation Sagittiarus. It creates an H II region LBN 29 (Sh 2-29) 1,070 parsecs (3,500 light-years) away from the Sun.

John Flamsteed designated this star the Flamsteed designation 11 Sagittarii, although the designation 11 Sgr is now more often used to refer to the star he designated 1 Sagittarii.