Alpha Lacertae

α Lacertae
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Lacerta
Right ascension 22h 31m 17.5010s[1]
Declination +50° 16 56.969[1]
Apparent magnitude (V) 3.777[1]
Characteristics
Spectral type A1 V[1]
U−B color index 0.00[2]
B−V color index +0.01[2]
R−I color index −0.03[2]
Astrometry
Radial velocity (Rv)−4.0 ± 2[1] km/s
Proper motion (μ) RA: 137.22[1] mas/yr
Dec.: 17.15[1] mas/yr
Parallax (π)31.86 ± 0.54[1] mas
Distance102 ± 2 ly
(31.4 ± 0.5 pc)
Absolute magnitude (MV)1.29[3]
Details
Mass2.194[4] M
Radius2.1432[4] R
Luminosity27.6750±0.2138[4] L
Luminosity (bolometric)27[5] L
Temperature9050±157[4] K
Rotational velocity (v sin i)146[2] km/s
Age400[4] Myr
Other designations
α Lac, Alpha Lacertae, Alpha Lac, 7 Lacertae, 7 Lac, ADS 16021 A, BD+49°3875, CCDM J22313+5017A, FK5 848, GC 31471, HD 213558, HIP 111169, HR 8585, SAO 34542, WDS 22131+5017A.[1][6]
Database references
SIMBADdata

Alpha Lacertae (Alpha Lac, α Lacertae, α Lac) is an A-type main sequence star in the constellation of Lacerta.[1] It is the brightest star in Lacerta and has an apparent visual magnitude of approximately 3.777.[1][5]

The star has a visual companion, CCDM J22313+5017B, of spectral type A and apparent visual magnitude 11.8, approximately 36 arcseconds away.[6] The companion is optical, a chance line-of-sight coincidence.[2]

Naming

In Chinese, 螣蛇 (Téng Shé), meaning Flying Serpent, refers to an asterism consisting of α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, λ Andromedae, κ Andromedae, ι Andromedae, and ψ Andromedae. Consequently, α Lacertae itself is known as 螣蛇一 (Téng Shé yī, English: the First Star of Flying Serpent)[7]

References

  1. 1 2 3 4 5 6 7 8 9 10 11 * alf Lac -- Star in double system, database entry, SIMBAD. Accessed on line September 3, 2008.
  2. 1 2 3 4 5 HR 8585, database entry, The Bright Star Catalogue, 5th Revised Ed. (Preliminary Version), D. Hoffleit and W. H. Warren, Jr., CDS ID V/50. Accessed on line September 3, 2008.
  3. From apparent magnitude and parallax.
  4. 1 2 3 4 5 Boyajian, Tabetha S.; et al. (July 2013), "Stellar Diameters and Temperatures. III. Main-sequence A, F, G, and K Stars: Additional High-precision Measurements and Empirical Relations", The Astrophysical Journal 771 (1): 31, arXiv:1306.2974, Bibcode:2013ApJ...771...40B, doi:10.1088/0004-637X/771/1/40, 40. See Table 3.
  5. 1 2 Alpha Lac, Jim Kaler, Stars. Accessed on line September 3, 2008.
  6. 1 2 Entry 22313+5017, discoverer code BU 703, The Washington Double Star Catalog, United States Naval Observatory. Accessed on line September 3, 2008.
  7. (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 7 日
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