HD 63433

HD 63433

A light curve for V377 Geminorum, plotted from TESS data, with the 6.46 day rotation period shown in red,
Observation data
Epoch J2000      Equinox J2000
Constellation Gemini
Right ascension 07h 49m 55.061s
Declination +27° 21 47.46
Apparent magnitude (V) 6.92
Characteristics
Evolutionary stage Main sequence
Spectral type G5V
Variable type BY Draconis
Astrometry
Radial velocity (Rv)−16.07±0.13 km/s
Proper motion (μ) RA: −10.220 mas/yr
Dec.: −11.235 mas/yr
Parallax (π)44.6848±0.0228 mas
Distance72.99 ± 0.04 ly
(22.38 ± 0.01 pc)
Absolute magnitude (MV)5.19
Details
Mass0.99±0.03 M
Radius0.912±0.034 R
Luminosity0.753±0.026 L
Surface gravity (log g)4.52±0.05 cgs
Temperature5,640±74 K
Metallicity [Fe/H]0.03±0.05 dex
Rotation6.45±0.05 d
Rotational velocity (v sin i)7.3±0.3 km/s
Age414±23 Myr
Other designations
V377 Gem, BD+27°1490, HD 63433, HIP 38228, SAO 79729, PPM 98012, TOI-1726, TYC 1933-747-1, GSC 01933-00747, 2MASS J07495506+2721473
Database references
SIMBADdata

HD 63433 (TOI-1726, V377 Geminorum) is a G-type main sequence star located 73 light-years from Earth in the zodiacal constellation Gemini, visually close to the star Pollux. With an apparent magnitude of 6.9, it is not visible to the naked eye, but can be seen with a small telescope or binoculars. It is part of the Ursa Major Moving Group.

HD 63433 has nearly the same radius and mass as the Sun, hence is classified as a Sun-like star. However, it is much younger than the Sun, less than one tenth as old at about 400 million years. There are three exoplanets orbiting it: one is classified as an Earth-sized planet, while the other two are mini-Neptunes.