15 Lyncis

15 Lyncis
Observation data
Epoch J2000      Equinox J2000
Constellation Lynx
Right ascension 06h 57m 16.60526s
Declination +58° 25 21.9404
Apparent magnitude (V) 4.35 (4.7 / 5.8)
Characteristics
Spectral type G8III + F8V
U−B color index +0.51
B−V color index +0.85
Astrometry
Radial velocity (Rv)1.86±0.28 km/s
Proper motion (μ) RA: 6.08 mas/yr
Dec.: -122.83 mas/yr
Parallax (π)18.29±0.25 mas
Distance178 ± 2 ly
(54.7 ± 0.7 pc)
Orbit
Period (P)262.0 yr
Semi-major axis (a)1.19″
Eccentricity (e)0.74
Inclination (i)78.0°
Longitude of the node (Ω)43.4°
Periastron epoch (T)B 1992.68
Argument of periastron (ω)
(secondary)
98.0°
Details
15 Lyn A
Radius8 R
Luminosity40 L
Surface gravity (log g)3.0 cgs
Temperature5,164±5 K
Metallicity [Fe/H]0.05 dex
Other designations
15 Lyn, BD+58° 982, HD 50522, HIP 33449, HR 2560, SAO 26051
Database references
SIMBADdata

15 Lyncis is a binary star system in the northern constellation of Lynx. It is visible to the naked eye as a faint point of light with a combined apparent visual magnitude of 4.35. Based on the system's parallax, it is located 178 light-years (54.7 parsecs) away. The pair are moving away from the Earth with a heliocentric radial velocity of +2 km/s.

A telescope reveals it is formed by two yellowish stars of magnitudes 4.7 and 5.8 that are 0.9 arcseconds apart. The two stars orbit each other every 262 years and the orbital eccentricity is 0.74. The components are a magnitude 4.7 evolved giant star of spectral type G8III, and a magnitude 5.8 F-type main-sequence star of spectral type F8V. The former has exhausted the hydrogen at its core, causing it to expand to 8 times the Sun's radius. It is radiating 40 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 5,164 K.