Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Vulpecula |
Right ascension | 20h 11m 47.9738s[1] |
Declination | 26° 48′ 32.3736″[1] |
Apparent magnitude (V) | 5.40[2] |
Characteristics | |
Spectral type | K2 IIIa[3] |
B−V color index | 1.40[4] |
Astrometry | |
Radial velocity (Rv) | −19.33±0.11[4] km/s |
Proper motion (μ) | RA: 1.619±0.119[1] mas/yr Dec.: −10.600±0.122[1] mas/yr |
Parallax (π) | 1.9328 ± 0.0779 mas[1] |
Distance | 1,690 ± 70 ly (520 ± 20 pc) |
Absolute magnitude (MV) | −2.60[5] |
Details | |
Mass | 4.94±0.53[6] M☉ |
Radius | 100.3+1.7 −3.0[1] R☉ |
Luminosity | 2,889±145[1] L☉ |
Surface gravity (log g) | 1.40[7] cgs |
Temperature | 4,200[7] K |
Metallicity [Fe/H] | −0.01[7] dex |
Rotational velocity (v sin i) | < 3.4[8] km/s |
Other designations | |
Database references | |
SIMBAD | data |
19 Vulpeculae is star located approximately 1,690[1] light years from Earth in the northern constellation of Vulpecula.[9] It is a probable member of the open cluster NGC 6882.[4] This object is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 5.40.[2] It is moving closer to the Earth with a heliocentric radial velocity of −19 km/s.[4]
This is an aging giant star with a stellar classification of K2 IIIa,[3] having already consumed the hydrogen at its core and evolved away from the main sequence. It has nearly five[6] times the mass of the Sun but has expanded to around 100[1] times the Sun's radius. The star is radiating 2,889[1] times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,200 K.[7]
Gaia DR2
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