29 Vulpeculae

29 Vulpeculae
Location of 29 Vulpeculae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Vulpecula
Right ascension 20h 38m 31.32904s
Declination 21° 12 04.3763
Apparent magnitude (V) 4.82
Characteristics
Spectral type A0V
U−B color index −0.07
B−V color index −0.02
Astrometry
Radial velocity (Rv)−17.10 km/s
Proper motion (μ) RA: +78.741 mas/yr
Dec.: −4.572 mas/yr
Parallax (π)15.6257±0.3374 mas
Distance209 ± 5 ly
(64 ± 1 pc)
Absolute magnitude (MV)0.56
Details
Mass2.67 M
Luminosity71 L
Surface gravity (log g)4.20 cgs
Temperature10,507 K
Metallicity [Fe/H]−0.15 dex
Rotational velocity (v sin i)52 km/s
Age254 Myr
Other designations
29 Vul, BD+20°4658, FK5 1539, HD 196724, HIP 101867, HR 7891, SAO 88944
Database references
SIMBADdata

29 Vulpeculae is a suspected astrometric binary star system in the northern constellation Vulpecula. It is visible to the naked eye as a faint, white-hued point of light with an apparent visual magnitude of 4.82. The system lies approximately 209 light years away from the Sun based on parallax, and is a member of the IC 2391 supercluster. It is moving closer to the Earth with a heliocentric radial velocity of −17 km/s.

Radial velocity measurements from High Accuracy Radial Velocity Planet Searcher with an amplitude of 4 km/s indicate that it is a spectroscopic binary of unknown period. The visible component is an A-type main-sequence star with a stellar classification of A0V, and has some slight abundance anomalies that resemble a weak Am star. It is catalogued as a shell star, showing spectral features of a cooler circumstellar jacket of gas, and may be a proto-shell star. The star is an estimated 254 million years old with a relatively low projected rotational velocity of 52 km/s. It has 2.67 times the mass of the Sun and is radiating 71 times the Sun's luminosity from its photosphere at an effective temperature of 10,507 K.