Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Apus |
Right ascension | 15h 15m 15.04464s[1] |
Declination | −70° 31′ 10.6449″[1] |
Apparent magnitude (V) | 6.86[2] |
Characteristics | |
Spectral type | G6 IV[3] |
B−V color index | 0.740±0.001[2] |
Astrometry | |
Radial velocity (Rv) | +1.94±0.12[1] km/s |
Proper motion (μ) | RA: −177.871 mas/yr[1] Dec.: −164.709 mas/yr[1] |
Parallax (π) | 37.3020 ± 0.0182 mas[1] |
Distance | 87.44 ± 0.04 ly (26.81 ± 0.01 pc) |
Absolute magnitude (MV) | 4.74[2] |
Details[4] | |
Mass | 1.046+0.070 −0.059 M☉ |
Radius | 1.158+0.039 −0.036 R☉ |
Luminosity | 1.161+0.071 −0.049 L☉ |
Surface gravity (log g) | 4.330+0.044 −0.041 cgs |
Temperature | 5,576+86 −85 K |
Metallicity [Fe/H] | +0.343+0.081 −0.084 dex |
Rotation | 42.0±3.9 d |
Age | 7.3+3.6 −3.4 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
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.[2] 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.[1]
This is an evolving G-type subgiant star with a stellar classification of G6 IV[3] and is not considered active, having a chromospheric activity index of −5.04.[6] It has about the same[7] mass as the Sun but is 25% more luminous.[2] The photosphere is radiating energy at an effective temperature of 5,614 K.[7] It has a higher than solar metallicity – a term astronomers use to describe the abundance of elements other than hydrogen and helium.[7]
There is a companion star of spectral type M3V at a separation of ~1500 AU, designated L 72-1.[8][4] This companion presents a bimodal distribution of the Gaia DR3 G-band light-curve, indicating that it is a close binary.[9]
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