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10 Lacertae
Star in the constellation Lacerta
Star in the constellation Lacerta
| b-v = −0.210 | u-b = −1.010
10 Lacertae (10 Lac) is a star in the constellation Lacerta. With an apparent magnitude of 4.9, it is located around 550 pc 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.
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.
It is the star with the smallest angular diameter measured by the CHARA array , at .
10 Lacertae has an 8th magnitude companion about one arc-minute away.
References
References
- (September 1993). "UBV photometry of stars whose positions are accurately known. VII". Astronomy and Astrophysics Supplement Series.
- (January 2009). "VizieR On-line Data Catalog: General Catalogue of Variable Stars". VizieR On-line Data Catalog.
- (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters.
- {{cite DR3. 1908095850396090880
- (2023-03-01). "Quantitative spectroscopy of late O-type main-sequence stars with a hybrid non-LTE method". Astronomy and Astrophysics.
- (1994). "A Hierarchy of Standards for the MK Process". [[Astronomical Society of the Pacific]].
- (December 2018). "Angular Sizes and Effective Temperatures of O-type Stars from Optical Interferometry with the CHARA Array". The Astrophysical Journal.
- (1994). "Catalogue of the Components of Double and Multiple stars (CCDM). First edition.". Communications de l'Observatoire Royal de Belgique.
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