HD 29399

HD 29399
Location of HD 29399 (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Reticulum
Right ascension 04h 33m 33.949s
Declination −62° 49 25.24
Apparent magnitude (V) 5.780
Characteristics
Evolutionary stage Red-giant branch
Spectral type K1III
U−B color index +2.111
B−V color index +0.332
Astrometry
Radial velocity (Rv)31.56±0.13 km/s
Proper motion (μ) RA: −117.58±0.04 mas/yr
Dec.: −18.73±0.04 mas/yr
Parallax (π)22.7240±0.0339 mas
Distance143.5 ± 0.2 ly
(44.01 ± 0.07 pc)
Details
Mass1.361±0.057 M
Radius4.845±0.082 R
Luminosity11.7+0.6
−0.7
 L
Surface gravity (log g)3.202±0.023 cgs
Temperature4,845±52 K
Metallicity [Fe/H]0.14±0.03 dex
Rotational velocity (v sin i)2.48 km/s
Age6.20±0.5 Gyr
Other designations
CD−63°153, HD 29399, HIP 21253, HR 1475, SAO 249054
Database references
SIMBADdata

HD 29399 is a binary star in the constellation Reticulum. Its main component is a red giant with an apparent magnitude of +5.78 which hosts an exoplanet. The secondary is a magnitude 9.2 star that is 31.9" distant from the primary. This system is only visible to the naked eye under dark skies far from light pollution. From its parallax measured by the Gaia spacecraft, it is located at a distance of 144 light-years (44 parsecs) from Earth.