Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Draco |
Right ascension | 18h 25m 59.13696s[1] |
Declination | +65° 33′ 48.5313″[1] |
Apparent magnitude (V) | 4.82[2] |
Characteristics | |
Spectral type | K1.5 III[2] |
B−V color index | 1.187 |
Astrometry | |
Radial velocity (Rv) | 31.75±0.12[1] km/s |
Proper motion (μ) | RA: +105.816 mas/yr[1] Dec.: −26.846 mas/yr[1] |
Parallax (π) | 11.056 ± 0.0841 mas[1] |
Distance | 295 ± 2 ly (90.4 ± 0.7 pc) |
Absolute magnitude (MV) | –0.108 |
Details | |
Mass | 0.879±0.050[2] M☉ |
Radius | 21.25+0.41 −0.43[3] R☉ |
Luminosity | 142.55±5.77[2] L☉ |
Surface gravity (log g) | 1.86±0.04[4] cgs |
Temperature | 4,367±46[4] K |
Metallicity [Fe/H] | −0.45±0.02[4] dex |
Age | 13.19±1.92[2] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
42 Draconis (abbreviated 42 Dra), formally named Fafnir (/ˈfɑːvnər/ or /ˈfɑːfnɪər/),[5][6] is a 5th magnitude K-type giant star located approximately 295 light years away in the constellation of Draco. As of 2009, an extrasolar planet (designated 42 Draconis b, later named Orbitar) is thought to be orbiting the star.
Of spectral type K1.5III, the star has a mass similar to the Sun but with a radius 22 times greater. It is a metal-poor star with metallicity as low as 35% that of the Sun and its age is 9.49 billion years. It is the northern pole star of Venus.[7]
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