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Nu2 Canis Majoris

ν2 Canis Majoris
Canis Major constellation map.svg
link=ν2 CMa

Location of ν2 Canis Majoris (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Canis Major
Right ascension 06h 36m 41.038s
Declination −19° 15′ 21.17″
Apparent magnitude (V) 3.96
Characteristics
Spectral type K1 III
Astrometry
Radial velocity (Rv) 5.39 km/s
Proper motion (μ) RA: 62.57 ± 0.15 mas/yr
Dec.: −69.97 ± 0.16 mas/yr
Parallax (π) 50.63 ± 0.23mas
Distance 64.4 ± 0.3 ly
(19.75 ± 0.09 pc)
Absolute magnitude (MV) −0.05
Details
Mass 1.3±0.1 M
Radius 4.9±0.1 R
Luminosity 11.3±0.1 L
Surface gravity (log g) 3.18±0.03 cgs
Temperature 4,790±27 K
Metallicity [Fe/H] 0.21±0.10 dex
Rotational velocity (v sin i) 1.15 km/s
Age 4.6±0.7 Gyr
Other designations
7 Canis Majoris, HR 2429, HD 47205, Gl 239.1, BD −19° 1502, FK5 2510, HIP 31592, SAO 151702, GC 8624
Database references
SIMBAD data

Nu2 Canis Majoris2 CMa, ν2 Canis Majoris) is a star in the constellation Canis Major. It is an evolved K-type giant approximately 65 light years away, seen below Sirius. Around 1.5 times as massive as the Sun, it has expanded to around 2.3 times the Sun's diameter and 11 times its luminosity. In 2011, it was discovered to have a planet.

In Chinese astronomy, ν2 Canis Majoris is called 野雞, Pinyin: Yějī, meaning Wild Cockerel, because this star is marking itself and stand alone in Wild Cockerel asterism, Well mansion (see : Chinese constellation). 野雞 (Yějī), westernized into Ya Ke. According to R.H. Allen opinion, the name Ya Ke is asterism consisting ο1 Canis Majoris and π Canis Majoris, with other small stars in the body of the Dog



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Wikipedia

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