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39 Draconis

39 Draconis
Observation data
Epoch J2000      Equinox J2000
Constellation Draco
Right ascension 18h 23m 54.60641s
Declination +58° 48′ 02.6446″
Apparent magnitude (V) 5.034
(5.06 + 8.07)
Characteristics
Spectral type A1V + F5V
U−B color index +0.06
B−V color index +0.10
Astrometry
Radial velocity (Rv) -24.53 ± 0.23 km/s
Proper motion (μ) RA: -37.82 mas/yr
Dec.: 61.60 mas/yr
Parallax (π) 17.71 ± 0.35mas
Distance 184 ± 4 ly
(56 ± 1 pc)
Absolute magnitude (MV) 1.31 / 4.32
Orbit
Period (P) 3962.50 ± 209.26 yr
Semi-major axis (a) 6.621 ± 0.325″
Eccentricity (e) 0.553 ± 0.005
Inclination (i) 107.7 ± 0.12°
Longitude of the node (Ω) 179.9 ± 0.10°
Periastron epoch (T) 5671.40 ± 12.08
Argument of periastron (ω)
(secondary)
128.0 ± 2.18°
Details
39 Dra A
Mass 2.12 M
Radius 2.3 R
Surface gravity (log g) 4.05 ± 0.07 cgs
Temperature 8710 K
39 Dra B
Mass 1.18 M
Other designations
BD+58° 1809, HD 170073, HIP 90156, HR 6923, SAO 30949
Database references
SIMBAD 39 Dra
39 Dra A
39 Dra B

39 Draconis, also known as b Draconis, is a wide binary star in the constellation Draco. Its apparent magnitude is 5.034. Parallax measurements made by the Hipparcos spacecraft put it at a distance of 184 light-years, or 56 parsecs away.

The two components of 39 Draconis are separated by 6.621″ and take almost 4,000 years to orbit each other. The primary star is an early A-type main-sequence star, 2.12 times the mass of the Sun. The secondary star is an F-type main-sequence star, and is 1.18 times the mass of the Sun.



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