36 Arietis

36 Arietis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Aries
Right ascension 02h 44m 19.11285s
Declination +17° 45′ 50.1359″
Apparent magnitude (V) 6.40
Characteristics
Evolutionary stage red giant branch
Spectral type K2 III
B−V color index 1.143±0.008
Astrometry
Radial velocity (Rv)−34.29±0.29 km/s
Proper motion (μ) RA: +36.836 mas/yr
Dec.: −36.203 mas/yr
Parallax (π)8.7094±0.0252 mas
Distance374 ± 1 ly
(114.8 ± 0.3 pc)
Absolute magnitude (MV)1.45±0.11
Details
Mass1.06±0.30 M
Radius9.82+0.13
−0.47
 R
Luminosity44.16±0.29 L
Surface gravity (log g)2.59±0.11 cgs
Temperature4,749±92 K
Metallicity [Fe/H]0.24 dex
Age1.95+0.68
−0.50
 Gyr
Other designations
36 Ari, BD+17°426, FK5 2190, GC 3294, HD 17017, HIP 12784, HR 808, SAO 93081
Database references
SIMBADdata

36 Arietis is a star in the northern constellation of Aries. 36 Arietis is the Flamsteed designation. It is a dim, orange-hued star that is a challenge to view with the naked eye, having an apparent visual magnitude of 6.40. Based upon an annual parallax shift of 8.71±0.02 mas, this star is located 374 light-years (114.8 parsecs) away from the Sun. It is moving closer to the Earth with a heliocentric radial velocity of −34 km/s, and is a member of the Wolf 630 moving group of stars that share a common motion through space.

This object is an evolved giant star with a stellar classification of K2 III. It is around two million years old with a similar mass as the Sun. With the hydrogen at its core exhausted, the star has expanded to ten times the girth of the Sun. It has a higher than solar metallicity, showing a high abundance of iron in its spectrum. The star is radiating 44 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,749 K.