Zeta Gruis

Zeta Gruis
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Grus
Right ascension 23h 00m 52.79777s
Declination −52° 45 14.8705
Apparent magnitude (V) 4.12
Characteristics
Spectral type K1 III Fe−1.2 CN−0.5
U−B color index +0.722
B−V color index +0.967
Astrometry
Radial velocity (Rv)−1.1±2.7 km/s
Proper motion (μ) RA: −57.911 mas/yr
Dec.: −13.371 mas/yr
Parallax (π)24.5452±0.5124 mas
Distance133 ± 3 ly
(40.7 ± 0.9 pc)
Absolute magnitude (MV)+1.49
Details
Mass1.44±0.06 M
Radius8.83±0.21 R
Luminosity39.4±1.7 L
Surface gravity (log g)2.759±0.077 cgs
Temperature4,865±22 K
Metallicity [Fe/H]−0.308±0.018 dex
Rotational velocity (v sin i)<1.3 km/s
Other designations
ζ Gru, CPD−53°10382, FK5 868, HD 217364, HIP 113638, HR 8747, SAO 247680
Database references
SIMBADdata

Zeta Gruis, Latinised from ζ Gruis, is a solitary star in the southern constellation of Grus. It is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 4.12. Based upon an annual parallax shift of 24.5 mas as seen from the Earth, the system is located about 133 light-years from the Sun.

This is an evolved K-type giant star with a stellar classification of K1 III Fe−1.2 CN−0.5, where the suffix notation indicates underabundances of iron and cyanogen in the spectrum. Having exhausted the supply of hydrogen at its core, the star has expanded and cooled; at present it has 9 times the girth of the Sun. The star is radiating 39 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,865 K.