Alpha Lyncis

Alpha Lyncis (α Lyn, α Lyncis) is the brightest star in the northern constellation of Lynx with an apparent magnitude of +3.13. Unusually, it is the only star in the constellation that has a Bayer designation. Based upon parallax measurements, this star is located about 203 light-years (62 parsecs) from the Earth.

α Lyncis
Location of α Lyncis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Lynx
Right ascension 09h 21m 03.30074s
Declination +34° 23 33.2245
Apparent magnitude (V) +3.14
Characteristics
Spectral type K7 III
U−B color index +1.95
B−V color index +1.55
Astrometry
Radial velocity (Rv)37.15 km/s
Proper motion (μ) RA: –223.63 mas/yr
Dec.: 15.18 mas/yr
Parallax (π)16.06 ± 0.17 mas
Distance203 ± 2 ly
(62.3 ± 0.7 pc)
Absolute bolometric
magnitude
 (Mbol)
–2.32 ± 0.13
Details
Mass~2 M
Radius54.50 ± 3.02 R
Luminosity673 ± 83 L
Surface gravity (log g)1.5 cgs
Temperature3,882 K
Metallicity [Fe/H]–0.26 dex
Rotational velocity (v sin i)6.4 km/s
Age1.4 Gyr
Other designations
40 Lyncis, HR 3705, HD 80493, BD +35 1979, HIP 45860, SAO 61414, FK5 352, NSV 4456, GC 12880.
Database references
SIMBADdata

This is a giant star that has exhausted the hydrogen at its core and has evolved away from the main sequence. It has expanded to about 55 times the Sun's radius and it is emitting roughly 673 times the luminosity of the Sun. The estimated effective temperature of the star's outer envelope is 3,882 K, which is lower than the Sun's effective temperature of 5,778 K, and is giving Alpha Lyncis an orange hue that is characteristic of K-type stars.

Alpha Lyncis is a suspected small-amplitude red variable star that changes apparent magnitude from +3.17 up to +3.12. This variability pattern typically occurs in stars that have developed an inert carbon core surrounded by a helium-fusing shell, and suggests that Alpha Lyncis is starting to evolve into a Mira-type variable.

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