Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Canis Major |
Right ascension | 07h 16m 34.99315s[1] |
Declination | −27° 52′ 52.2453″[1] |
Apparent magnitude (V) | 4.66[2] |
Characteristics | |
Evolutionary stage | AGB[3] |
Spectral type | M2III[4] |
B−V color index | 1.589±0.028[2] |
Astrometry | |
Radial velocity (Rv) | +41.5±2.8[2] km/s |
Proper motion (μ) | RA: −13.479[1] mas/yr Dec.: +38.625[1] mas/yr |
Parallax (π) | 8.3189 ± 0.2874 mas[1] |
Distance | 390 ± 10 ly (120 ± 4 pc) |
Absolute magnitude (MV) | −0.80[2] |
Details | |
Radius | 61.1+7.3 −6.9[1] R☉ |
Luminosity | 699.7±27.3[1] L☉ |
Temperature | 3,797+233 −209[1] K |
Other designations | |
Database references | |
SIMBAD | data |
HD 56618 is a single[6] star in the southern constellation of Canis Major. It is a red-hued star that is faintly visible to the naked eye with an apparent visual magnitude of 4.66.[2] This object is located at a distance of approximately 390 light years from the Sun based on parallax measurements. It is drifting further away with a radial velocity of +41.5 km/s,[2] having come to within 203 light-years some 2.2 million years ago.[2] Olin J. Eggen listed it as a probable member of the Hyades supercluster.[7]
This is an aging red giant star currently on the asymptotic giant branch[3] with a stellar classification of M2III.[4] It is no longer undergoing core hydrogen fusion and has expanded to 61[1] times the radius of the Sun. The star is radiating 700[1] times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 3,797 K.[1]
GaiaDR2
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Eggen1992
was invoked but never defined (see the help page).houk1979
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Eggleton2008
was invoked but never defined (see the help page).Eggen1985
was invoked but never defined (see the help page).