HD 68402

HD 68402 is a solitary star located in the circumpolar constellation Volans. With an apparent magnitude of 9.09, it is invisible to the naked eye but can be seen with an amateur telescope. This star is located at a distance of 256 light years based on its parallax shift but is drifting away at a rate of 11.60 km/s.

HD 68402
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Volans
Right ascension 08h 05m 23.69129s
Declination −74° 24 37.4873
Apparent magnitude (V) 9.09 ± 0.02
Characteristics
Spectral type G5 IV/V
B−V color index +0.68
Astrometry
Radial velocity (Rv)11.60 ± 0.49 km/s
Proper motion (μ) RA: −78.195 mas/yr
Dec.: +78.973 mas/yr
Parallax (π)12.7204 ± 0.0101 mas
Distance256.4 ± 0.2 ly
(78.61 ± 0.06 pc)
Absolute magnitude (MV)+4.66
Details
Mass1.12 ± 0.05 M
Radius1.02 ± 0.05 R
Luminosity1.17+0.06
−0.07
 L
Surface gravity (log g)4.43 ± 0.04 cgs
Temperature5,907 ± 68 K
Metallicity [Fe/H]+0.29 ± 0.10 dex
Rotational velocity (v sin i)2.9 ± 0.2 km/s
Age1 ± 0.9 Gyr
Other designations
CD−74° 392, CPD−74° 486, HD 68402, HIP 39589
Database references
SIMBADdata
Exoplanet Archivedata

HD 68402 has a classification of G5 IV/V, which indicates that it is a G5 star with the characteristics of a subgiant and main-sequence star. Contrary to its classification, it is actually a G1 dwarf. At present it is slightly more massive than the Sun and has a similar radius to the latter. It radiates at 1.17 times the luminosity of the Sun from its photosphere at an effective temperature of 5,907 K, which gives it a yellow hue. At an age of 1 billion years HD 68402 has a projected rotational velocity of almost 3 km/s and is metal rich like most planetary hosts (1.94 times to be exact).

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