10 Lacertae

Star in the constellation Lacerta From Wikipedia, the free encyclopedia

10 Lacertae (10 Lac) is a star in the constellation Lacerta. With an apparent magnitude of 4.9, it is located around 550 parsecs (1,800 ly) distant in the small Lacerta OB1 association. It is a hot blue main-sequence star of spectral type O9V, a massive star that is currently fusing its core hydrogen. It is a suspected Beta Cephei variable star.

Right ascension22h 39m 15.67804s[1]
Declination+39° 03 00.9724[1]
Quick facts Constellation, Right ascension ...
10 Lacertae
Location of 10 Lac (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Lacerta
Right ascension 22h 39m 15.67804s[1]
Declination +39° 03 00.9724[1]
Apparent magnitude (V) 4.880[2]
Characteristics
Spectral type O9V[3]
U−B color index 1.010[2]
B−V color index 0.210[2]
Variable type β Cep?[4]
Astrometry
Radial velocity (Rv)10.10[5] km/s
Proper motion (μ) RA: −1.274 mas/yr[1]
Dec.: −5.605 mas/yr[1]
Parallax (π)2.192±0.131 mas[1]
Distance1,800±100 ly
(552±32 pc)[6]
Absolute magnitude (MV)−4.17±0.12[6]
Details[6]
Mass21.6±0.5 M
Radius7.4±0.5 R
Luminosity69,200+8,440
−7,520
 L
Surface gravity (log g)4.04±0.05 cgs
Temperature34,550±300 K
Rotational velocity (v sin i)14±1 km/s
Age3.55+0.72
−0.60
 Myr
Other designations
10 Lac, HR 8622, BD+38°4826, HD 214680, SAO 72575, HIP 111841, NSV 25932, WDS J22393+3903
Database references
SIMBADdata
Close

It was one of the first O-type stars (along with S Monocerotis) to be defined as an anchor point for the MKK spectral classification; since the early twentieth century it has served as such a point. Specifically, the star is representative of O9V stars, meaning relatively cool O-type stars on the main-sequence.[7]

It is the star with the smallest angular diameter measured by the CHARA array as of 2018, at 0.11±0.02 milliarcseconds.[8]

10 Lacertae has an 8th magnitude companion about one arc-minute away.[9]

References

Related Articles

Wikiwand AI