HD 30177

HD 30177 is a single star with a pair of orbiting exoplanets in the southern constellation Dorado. Based on parallax measurements, it is located at a distance of 181 light years from the Sun. It has an absolute magnitude of 4.72, but at that distance the star is too faint to be viewed by the naked eye with an apparent visual magnitude of 8.41. The star is drifting further away with a radial velocity of 62.7 km/s.

HD 30177
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Dorado
Right ascension 04h 41m 54.374s
Declination −58° 01 14.73
Apparent magnitude (V) 8.41
Characteristics
Evolutionary stage main sequence
Spectral type G8V
B−V color index 0.773±0.015
Astrometry
Radial velocity (Rv)62.697±0.0013 km/s
Proper motion (μ) RA: 66.303±0.023 mas/yr
Dec.: −11.795±0.024 mas/yr
Parallax (π)18.0190 ± 0.0195 mas
Distance181.0 ± 0.2 ly
(55.50 ± 0.06 pc)
Absolute magnitude (MV)4.72±0.09
Details
Mass1.053±0.023 M
Radius1.019±0.034 R
Luminosity1.04±0.01 L
Surface gravity (log g)4.417±0.034 cgs
Temperature5,607±47 K
Metallicity [Fe/H]0.39±0.05 dex
Rotation~45 d
Rotational velocity (v sin i)2.96±0.50 km/s
Age4.8±1.5 Gyr
2.525±1.954 Gyr
Other designations
CD−58°984, HD 30177, HIP 21850, SAO 233633, 2MASS J04415438-5801146
Database references
SIMBADdata

The spectrum of HD 30177 matches a late G-type main-sequence star with a stellar classification of G8V. It is a yellow dwarf with a mass and radius similar to the Sun that is fusing hydrogen in its core. The chromosphere shows a negligible level of magnetic activity. The abundance of iron, an indicator of the star's metallicity, is more than double the Sun's. It is radiating a similar luminosity to the Sun from its photosphere at an effective temperature of 5,607 K.

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