HD 134606

HD 134606 is a yellow-hued star with a planetary system, positioned in the southern constellation of Apus. It is below the nominal limit for visibility with the naked eye, having an apparent visual magnitude of 6.86. Based upon an annual parallax shift of 37.3 mas, it is located 87.44 light-years away. The star appears to be moving further from the Earth with a heliocentric radial velocity of +1.9 km/s.

HD 134606
Observation data
Epoch J2000      Equinox J2000
Constellation Apus
Right ascension 15h 15m 15.04464s
Declination −70° 31 10.6449
Apparent magnitude (V) 6.86
Characteristics
Spectral type G6 IV
B−V color index 0.740±0.001
Astrometry
Radial velocity (Rv)+1.94±0.12 km/s
Proper motion (μ) RA: −177.871 mas/yr
Dec.: −164.709 mas/yr
Parallax (π)37.3020 ± 0.0182 mas
Distance87.44 ± 0.04 ly
(26.81 ± 0.01 pc)
Absolute magnitude (MV)4.74
Details
Mass1.046+0.070
−0.059
 M
Radius1.158+0.039
−0.036
 R
Luminosity1.161+0.071
−0.049
 L
Surface gravity (log g)4.330+0.044
−0.041
 cgs
Temperature5,576+86
−85
 K
Metallicity [Fe/H]+0.343+0.081
−0.084
 dex
Rotation42.0±3.9 d
Age7.3+3.6
−3.4
 Gyr
Other designations
CD−70° 1258, GC 20455, HD 134606, HIP 74653, SAO 257257, LTT 6064, 2MASS J15151504-7031105
Database references
SIMBADdata

This is an evolving G-type subgiant star with a stellar classification of G6 IV and is not considered active, having a chromospheric activity index of −5.04. It has about the same mass as the Sun but is 25% more luminous. The photosphere is radiating energy at an effective temperature of 5,614 K. It has a higher than solar metallicity – a term astronomers use to describe the abundance of elements other than hydrogen and helium.

There is a red dwarf companion star of spectral type M3V at a separation of ~1500 AU, designated L 72-1.

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