Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Capricornus |
Right ascension | 20h 40m 02.94518s[1] |
Declination | −18° 08′ 19.1664″[1] |
Apparent magnitude (V) | 5.17[2] |
Characteristics | |
Spectral type | M1 III[3] |
B−V color index | +1.65[2] |
Astrometry | |
Radial velocity (Rv) | −12.3±1.6[4] km/s |
Proper motion (μ) | RA: −23.503[1] mas/yr Dec.: −22.157[1] mas/yr |
Parallax (π) | 4.4702 ± 0.2352 mas[1] |
Distance | 730 ± 40 ly (220 ± 10 pc) |
Absolute magnitude (MV) | −1.09[5] |
Details | |
Radius | 76.36+8.05 −14.16[1] R☉ |
Luminosity | 1,283.0±76.5[1] L☉ |
Temperature | 3,953+427 −193[1] K |
Metallicity [Fe/H] | −0.08[5] dex |
Other designations | |
Database references | |
SIMBAD | data |
Upsilon Capricorni, Latinized from υ Capricorni, is a solitary[7] star in the southern constellation of Capricornus. It has a reddish hue and is dimly visible to the naked eye with an apparent visual magnitude of 5.17.[2] The star is about 730 light years from the Sun based on parallax,[1] but is drifting closer with a radial velocity of −12 km/s.[4] It is 0.22 degree north of the ecliptic, so is subject to lunar occultations.[8][9]
This is an aging red giant star on the asymptotic giant branch[10] with a stellar classification of M1 III,[3] a star that has exhausted the supply of hydrogen at its core then cooled and expanded. At present it has 76[1] times the radius of the Sun. It is a suspected variable star of unknown type with a brightness that has been measured ranging from a peak of 5.19 down to 5.24.[11] The star is radiating 1,283[1] times the luminosity of the Sun from its swollen photosphere at an effective temperature of 3,953 K.[1]
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