Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Sculptor |
Right ascension | 00h 53m 00.71555s[1] |
Declination | −30° 21′ 25.1677″[1] |
Apparent magnitude (V) | +7.3029[1] |
Characteristics | |
Spectral type | K2.5 V (k)[2] |
B−V color index | 0.936[1] |
Astrometry | |
Radial velocity (Rv) | −13.021±0.0064[3] km/s |
Proper motion (μ) | RA: +620.35[1] mas/yr Dec.: +30.26[1] mas/yr |
Parallax (π) | 71.5472 ± 0.0573 mas[4] |
Distance | 45.59 ± 0.04 ly (13.98 ± 0.01 pc) |
Absolute magnitude (MV) | +6.39[5] |
Details | |
Radius | 0.660[6] R☉ |
Luminosity | 0.29[5] L☉ |
Surface gravity (log g) | 4.55[2] cgs |
Temperature | 4,822[2] K |
Metallicity [Fe/H] | −0.21[2] dex |
Rotational velocity (v sin i) | 1.8[7] km/s |
Age | 6.67±4.74[8] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Gliese 42 is a star in the southern constellation of Sculptor. It is too faint to be seen with the naked eye, having an apparent visual magnitude of +7.3.[1] The annual parallax shift of 70.56 mas provides a distance estimate of 46 light years. It has a relatively high proper motion, advancing 0.62[10] arcseconds across the sky per annum, and is moving closer to the Sun with a radial velocity of −13 km/s.[3]
The spectrum of the star matches a stellar classification of K2.5 V (k),[2] indicating it is an ordinary K-type main-sequence star that is generating energy through hydrogen fusion at its core. It is radiating 29%[5] of the Sun's luminosity from its photosphere at an effective temperature of 4,822 K.[2] The star has 66%[6] of the Sun's radius.
vanLeeuwen2007
was invoked but never defined (see the help page).Gray2006
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was invoked but never defined (see the help page).GaiaDR2
was invoked but never defined (see the help page).Anderson2012
was invoked but never defined (see the help page).Cotten2016
was invoked but never defined (see the help page).Pace2013
was invoked but never defined (see the help page).apjss141_1_187
was invoked but never defined (see the help page).