Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Lacerta |
Right ascension | 22h 47m 43.42677s [1] |
Declination | +55° 09′ 30.3036″ [1] |
Apparent magnitude (V) | 9.40 [2] |
Characteristics | |
Spectral type | M4epIab + B [3] |
U−B color index | +1.46 [2] |
B−V color index | +2.34 [2] |
Variable type | SRc [3] |
Astrometry | |
Radial velocity (Rv) | −68 [4] km/s |
Proper motion (μ) | RA: −3.207 [5] mas/yr Dec.: −3.150 [5] mas/yr |
Parallax (π) | 0.3519±0.0708 mas [5] |
Distance | 2,750 [6] pc |
Absolute magnitude (MV) | −5.6 [7] |
Details | |
Mass | 22 [7] M☉ |
Radius | 1,013 [8] R☉ |
Luminosity | 152,000 [8] L☉ |
Temperature | 3,535 [8] K |
Other designations | |
U Lac, HIP 112545, PPM 411, GSC 03988-01641, IRC+50446, TYC 3988-1641-1, BD+54°2863, HD 215924, 2MASS J22474341+5509303, AAVSO 2243+54 | |
Database references | |
SIMBAD | data |
U Lacertae is a spectroscopic binary star in the constellation Lacerta.
Despite being in the constellation of Lacerta, U Lacertae is considered to be a member of the Cepheus OB1 association. [9] It has been listed as a member of the open cluster ASCC 123. [10]
U Lacertae is a binary star consisting of a red supergiant and a small hot companion, similar to VV Cephei. The companion has been identified from a high excitation component in the spectrum and from radial velocity variations, but the orbit is unknown. [11]
In 1894, T. H. E. C. Espin announced that the star, then called BD +54° 2863, might be a variable star. [13] T. W. Blackhouse confirmed its variability in 1897. [14] It was listed with its variable star designation, U Lacertae, in Annie Jump Cannon's 1907 work Second Catalog of Variable Stars. [15] U Lacertae is classified as a semiregular variable. [3] The periodicity is uncertain but a main period of 150 days and a long secondary period of 550 – 690 days have been suggested. [16] A study of Hipparcos satellite photometry found an amplitude of 0.77 magnitudes and found no periodicity. [17] The General Catalogue of Variable Stars lists an amplitude of 2.7 magnitudes. [3]
Water masers have been detected around U Lacertae, common in the extended atmospheres of very luminous cool stars. [18]