HD 213240

HD 213240
Observation data
Epoch J2000      Equinox J2000
Constellation Grus
Right ascension 22h 31m 00.36634s
Declination −49° 25 59.7690
Apparent magnitude (V) 6.81
Characteristics
Spectral type G0/G1V + M5-5.5
B−V color index 0.603±0.005
Astrometry
Radial velocity (Rv)−0.37±0.12 km/s
Proper motion (μ) RA: −135.912 mas/yr
Dec.: −193.844 mas/yr
Parallax (π)24.4247±0.0208 mas
Distance133.5 ± 0.1 ly
(40.94 ± 0.03 pc)
Absolute magnitude (MV)3.77
Details
Mass1.57±0.02 M
Radius1.56+0.03
−0.04
 R
Luminosity2.687+0.007
−0.006
 L
Surface gravity (log g)4.17±0.02 cgs
Temperature5,921+70
−58
 K
Metallicity [Fe/H]0.14±0.01 dex
Rotational velocity (v sin i)3.5 km/s
Age4.6±0.6 Gyr
Other designations
CD−50° 13701, HD 213240, HIP 111143, SAO 231175, LTT 9047
Database references
SIMBADdata

HD 213240 is a possible binary star system in the constellation Grus. It has an apparent visual magnitude of 6.81, which lies below the limit of visibility for normal human sight. The system is located at a distance of 133.5 light years from the Sun based on parallax. The primary has an absolute magnitude of 3.77.

This is an ordinary G-type main-sequence star with a stellar classification of G0/G1V. It is a metal-rich star with an age that has been calculated as being anywhere from 2.7 to 4.6 billion years. The star has 1.6 times the mass of the Sun and 1.56 times the Sun's radius. It is spinning with a projected rotational velocity of 3.5 km/s. The star is radiating 2.69 times the luminosity of the Sun from its photosphere at an effective temperature of 5,921 K.

A red dwarf companion star was detected in 2005 with a projected separation of 3,898 AU.