A light curve for V377 Geminorum, plotted from TESS data,[1] with the 6.46 day rotation period shown in red, | |
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Gemini[a] |
Right ascension | 07h 49m 55.05s[2] |
Declination | 27° 21′ 47.45″[2] |
Apparent magnitude (V) | 6.92[3] |
Characteristics | |
Evolutionary stage | Main sequence[4] |
Spectral type | G5V[4] |
Variable type | BY Draconis[5][6] |
Astrometry | |
Radial velocity (Rv) | −16.07±0.13[3] km/s |
Proper motion (μ) | RA: −10.0268±0.0846 mas/yr[3] Dec.: −11.3143±0.0487 mas/yr[3] |
Parallax (π) | 44.6848 mas[7] |
Distance | 73.035±0.073 ly (22.4035±0.0225 pc)[3] |
Absolute magnitude (MV) | 5.19[8] |
Details[9] | |
Mass | 0.99±0.03 M☉ |
Radius | 0.912±0.034 R☉ |
Luminosity | 0.753±0.026 L☉ |
Surface gravity (log g) | 4.52±0.05[4] cgs |
Temperature | 5640±74 K |
Metallicity [Fe/H] | 0.03±0.05[4] dex |
Rotation | 6.45±0.05 d |
Rotational velocity (v sin i) | 7.3±0.3 km/s |
Age | 414±23 Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 63433 (TOI-1726, V377 Geminorum) is a G-type main sequence star located 73 light-years from Earth in the zodiacal constellation Gemini,[9][a] visually close to the star Pollux.[7] It has nearly the same radius and mass of the Sun, hence being classified as a Sun-like star.[9] However, it is much younger than the Sun, less than one tenth as old with an age of about 400 million years.[9][b] With an apparent magnitude of 6.9, it is not visible to the naked eye, but can be seen with a small telescope[11] or binoculars.[12] Based on its kinematic, rotational and lithium abundance properties, it is part of the Ursa Major Moving Group.[9] There are three exoplanets orbiting it, one is classified as an Earth-sized planet, while the two others are mini-Neptunes.[4]
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