Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Delphinus |
Right ascension | 20h 55m 38.5698s[1] |
Declination | +12° 34′ 06.8774″[1] |
Apparent magnitude (V) | 5.54±0.01[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | A5 V[4] |
U−B color index | +0.09[2] |
B−V color index | +0.11[2] |
Astrometry | |
Radial velocity (Rv) | 2.0±4.3[5] km/s |
Proper motion (μ) | RA: +39.558 mas/yr[1] Dec.: +27.772 mas/yr[1] |
Parallax (π) | 16.4866 ± 0.06 mas[1] |
Distance | 197.8 ± 0.7 ly (60.7 ± 0.2 pc) |
Absolute magnitude (MV) | +1.63[6] |
Details | |
Mass | 2.0±0.1[7] M☉ |
Radius | 1.9±0.1[8] R☉ |
Luminosity | 18.7[6] L☉ |
Surface gravity (log g) | 4.10±0.14[7] cgs |
Temperature | 9,093±309[7] K |
Metallicity [Fe/H] | −0.01[9] dex |
Rotational velocity (v sin i) | 159[10] km/s |
Age | 400+150 −215[7] Myr |
Other designations | |
Database references | |
SIMBAD | data |
16 Delphini is a star in the equatorial constellation Delphinus. It has an apparent magnitude of 5.54,[2] making it faintly visible to the naked eye. The star is relatively close at a distance of 198 light years[1] but is receding with a poorly constrained radial velocity of 2 km/s.[5]
16 Delphini is a chemically peculiar A-type main-sequence star with a stellar classification of A5 V. It has twice the Sun's mass,[7] 1.9 times it's radius,[8] and shines at 18.7 L☉.[6] This yields an effective temperature of 9,039 K,[7] giving it a white glow. 16 Del is 400 million years old[7] – 56.5% through its main sequence lifetime[3] – and spins rapidly with a projected rotational velocity of 159 km/s.[10]
16 Del has a companion that was first discovered by John Herschel and was even noted to be a spectroscopic binary.[11] It is now considered to be a single star. [12]
EDR3
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