HD 169405

HD 169405
Observation data
Epoch J2000      Equinox J2000
Constellation Telescopium
Right ascension 18h 26m 54.01379s
Declination −48° 07 02.0638
Apparent magnitude (V) +5.44
Characteristics
Spectral type K0.5III + F/G
B−V color index 0.855±0.004
Astrometry
Radial velocity (Rv)+2.11±3.42 km/s
Proper motion (μ) RA: +3.041±0.182 mas/yr
Dec.: −54.895±0.169 mas/yr
Parallax (π)12.2045±0.2664 mas
Distance267 ± 6 ly
(82 ± 2 pc)
Absolute magnitude (MV)1.14
Details
Mass2.4 M
Radius9.8 R
Luminosity35 L
Surface gravity (log g)2.94 cgs
Temperature5,062 K
Metallicity [Fe/H]+0.04 dex
Rotational velocity (v sin i)2.7±1.7 km/s
Age557 Myr
Other designations
CD−48°12505, GC 25150, HD 169405, HIP 90414, HR 6894, SAO 229021
Database references
SIMBADdata

HD 169405 (HR 6894), is a suspected binary star system in the southern constellation Telescopium, about a degree to the north of Zeta Telescopii. It has an apparent magnitude of 5.44, making it faintly visible to the naked eye under ideal conditions. HD 169405 is located at a distance of 267 light years and is drifting away with a heliocentric radial velocity of 3.8 km/s.

The visible component has a spectral classification K0.5III which indicates that it is an evolved star between a K0 and K1 giant. It has expanded to ten times the Sun's radius, shines at 35 solar luminosities, and has an effective temperature of 5,062 K. This temperature gives it the yellowish-orange glow of a K-type star, and it spins slowly with a projected rotational velocity of 2.7 km/s.