Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Puppis |
Right ascension | 08h 21m 28.13685s[1] |
Declination | −39° 42′ 19.4843″[1] |
Apparent magnitude (V) | +7.17[2] |
Characteristics | |
Spectral type | G6V CN+0.5[3] |
B−V color index | 0.692±0.022[2] |
Astrometry | |
Radial velocity (Rv) | +49.31±0.12[1] km/s |
Proper motion (μ) | RA: −201.729 mas/yr[1] Dec.: 225.102 mas/yr[1] |
Parallax (π) | 34.1478 ± 0.0154 mas[1] |
Distance | 95.51 ± 0.04 ly (29.28 ± 0.01 pc) |
Absolute magnitude (MV) | +4.93[2] |
Details | |
Mass | 1.04±0.02[4] M☉ |
Radius | 0.97±0.01[4] R☉ |
Luminosity | 0.917±0.004[4] L☉ |
Surface gravity (log g) | 4.47±0.02[4] cgs |
Temperature | 5732±23[4] K |
Metallicity [Fe/H] | +0.17±0.04[5] dex |
Rotational velocity (v sin i) | 1.57[6] km/s |
Age | 1.9±1.1 Gyr[4] 3.8±2.6[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
ARICNS | data |
HD 70642 is a star with an exoplanetary companion in the southern constellation of Puppis. It has an apparent visual magnitude of +7.17,[2] which is too dim to be readily visible to the naked eye. The system is located at a distance of 95.5 light-years (29.3 parsecs) from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +49.3 km/s.[1] It came to within 55.3 ly of the Solar System some 329,000 years ago.[2]
This may be considered to be a solar analog star, being similar in physical properties to the Sun.[5] It is a G-type main-sequence star with a stellar classification of G6V CN+0.5.[3] It is comparable to the age of the Sun, estimated to be in the range of 2–6 billion years old. Although chromospherically inactive a magnetic field has been detected.[5] This star has about the same mass and radius as the Sun, is slightly cooler and less luminous,[4] and is richer in abundance of iron relative to hydrogen.[5] It is spinning at a leisurely rate, showing a projected rotational velocity of 1.6 km/s.[6]
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