Delta Pavonis

Delta Pavonis, Latinized from δ Pavonis, is a single star in the southern constellation of Pavo. It has an apparent visual magnitude of 3.56, making it a fourth-magnitude star that is visible to the naked eye from the southern hemisphere. Parallax measurements yield an estimated distance of 19.89 light-years (6.10 parsecs) from Earth. This makes it one of the nearest bright stars to the Solar System. It is approaching the Sun with a radial velocity of −23.5 km/s, and is predicted to come as close as 17.8 light-years in around 49,200 years.

Delta Pavonis
Location of δ Pavonis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Pavo
Right ascension 20h 08m 43.60887s
Declination −66° 10 55.4428
Apparent magnitude (V) 3.56
Characteristics
Spectral type G8 IV
U−B color index 0.45
B−V color index 0.76
Variable type Suspected
Astrometry
Radial velocity (Rv)−23.52±0.81 km/s
Proper motion (μ) RA: +1,211.761 mas/yr
Dec.: –1,130.237 mas/yr
Parallax (π)163.9544 ± 0.1222 mas
Distance19.89 ± 0.01 ly
(6.099 ± 0.005 pc)
Absolute magnitude (MV)4.62
Details
Mass1.051±0.062 M
Radius1.197±0.016 R
Luminosity1.24±0.03 L
Surface gravity (log g)4.26±0.06 cgs
Temperature5,571±48 K
Metallicity [Fe/H]0.33±0.03 dex
Rotation21.4±9.3 d
Rotational velocity (v sin i)0.32 km/s
Age6.6–6.9 Gyr
9.3 Gyr
Other designations
δ Pav, NSV 12790, CD−66 2367, GJ 780, HD 190248, HIP 99240, HR 7665, SAO 254733, LFT 1520, LHS 485, LTT 7946, 2MASS J20084376-6610563
Database references
SIMBADdata
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