Lambda Cygni

Star in the constellation Cygnus From Wikipedia, the free encyclopedia

Lambda Cygni (λ Cyg) is a class B5V (blue main-sequence) star in the constellation Cygnus. Its apparent magnitude is 4.54[2] and it is approximately 770 light years away based on parallax.[1]

Right ascension20h 47m 24.53766s[1]
Declination+36° 29 26.5737[1]
Quick facts Constellation, Right ascension ...
Lambda Cygni
Location of λ Cygni (circled in red)
Observation data
Epoch J2000      Equinox J2000
Constellation Cygnus
Right ascension 20h 47m 24.53766s[1]
Declination +36° 29 26.5737[1]
Apparent magnitude (V) 4.54[2]
Characteristics
Spectral type B5Ve[3]
U−B color index −0.50 [2]
B−V color index −0.11 [2]
Variable type Be star[4]
Astrometry
Radial velocity (Rv)-23.20[5] km/s
Proper motion (μ) RA: +14.71[1] mas/yr
Dec.: −8.96[1] mas/yr
Parallax (π)4.24±0.43 mas[1]
Distanceapprox. 770 ly
(approx. 240 pc)
Details
λ Cyg Aa
Mass6.40[6] M
Radius3.56[7] R
Surface gravity (log g)3.195[8] cgs
Temperature13,925[8] K
Rotational velocity (v sin i)133[8] km/s
λ Cyg Ab
Mass6.40[6] M
λ Cyg B
Mass5.12[6] M
Other designations
54 Cygni, CCDM J20475+3629, GC 28994, HIP 102589, HR 7963, HD 198183, SAO 70505, WDS J20474+3629
Database references
SIMBADdata
Close

Lambda Cygni is a multiple star, with components A, B, and C observed in the 19th century; the main component, A, is a spectroscopic binary itself with two components Aa and Ab reported at magnitudes 5.4 and 5.8 orbiting with a period of 12 years.[9] Component B has type B7V, magnitude 6.26, and separation 0.77" (about 180 AU based on parallax).[9][10] Component C has reported type K2III-IV, apparent magnitude 9.65, and separation about 85".[11] Recent observations indicate the presence of additional smaller companions D (about 50" from A), E (about 8" from C), and F (about 40" from C) all around apparent magnitude 14.[11]

References

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