59 Arietis

Star in the constellation Aries From Wikipedia, the free encyclopedia

59 Arietis is a star in the northern constellation of Aries. 59 Arietis is the Flamsteed designation. It is dimly visible to the naked eye with an apparent visual magnitude of 5.91.[2] Based upon an annual parallax shift of 15.40±0.06 mas,[1] it is located approximately 212 light-years (65 parsecs) distant from the Sun. The star is moving closer to the Earth with a heliocentric radial velocity of −4.7 km/s.[1]

Right ascension03h 19m 55.79556s[1]
Declination+27° 04 16.0661[1]
Quick facts Constellation, Right ascension ...
59 Arietis
Observation data
Epoch J2000      Equinox ICRS
Constellation Aries
Right ascension 03h 19m 55.79556s[1]
Declination +27° 04 16.0661[1]
Apparent magnitude (V) 5.91[2]
Characteristics
Spectral type G7 IV[3]
B−V color index 0.860±0.015[2]
Astrometry
Radial velocity (Rv)−4.67±0.14[1] km/s
Proper motion (μ) RA: −25.853[1] mas/yr
Dec.: −72.813[1] mas/yr
Parallax (π)15.3970±0.0621 mas[1]
Distance211.8 ± 0.9 ly
(64.9 ± 0.3 pc)
Absolute magnitude (MV)1.78[2]
Details[4]
Mass1.96±0.30 M
Radius5.76±0.27 R
Luminosity19.5+1.9
−3.6
 L
Surface gravity (log g)3.21 cgs
Temperature5,044 K
Metallicity [Fe/H]−0.06 dex
Rotational velocity (v sin i)1.8 km/s
Age1.7+0.4
−0.3
 Gyr
Other designations
59 Ari, BD+26°540, HD 20618, HIP 15514, HR 995, SAO 75863[5]
Database references
SIMBADdata
Close

The spectrum of this object is that of a subgiant star with a stellar classification of G7 IV,[3] which would suggest it has exhausted the supply of hydrogen at its core and has begun to evolve into a giant star. It is around 1.7 billion years old with a projected rotational velocity of 1.8 km/s. The star has nearly double the mass of the Sun and almost six times the Sun's radius. It is radiating 20 times the luminosity of the Sun from its photosphere at an effective temperature of 5,044 K.[4]

References

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