Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Ara[1] |
Right ascension | 16h 53m 05.755s[2] |
Declination | –46° 19′ 58.64″[2] |
Apparent magnitude (V) | 9.18[1] |
Characteristics | |
Spectral type | G6V[3] |
Apparent magnitude (B) | 9.891[1] |
Apparent magnitude (J) | 7.984±0.021[1] |
Apparent magnitude (H) | 7.656±0.031[1] |
Apparent magnitude (K) | 7.634±0.021[1] |
B−V color index | 0.711±0.025[1] |
Astrometry | |
Radial velocity (Rv) | −21.338±0.0007[4] km/s |
Proper motion (μ) | RA: −107.358 mas/yr[2] Dec.: −93.597 mas/yr[2] |
Parallax (π) | 11.3545 ± 0.0142 mas[2] |
Distance | 287.2 ± 0.4 ly (88.1 ± 0.1 pc) |
Absolute magnitude (MV) | 4.62[1] |
Details | |
Mass | 1.147±0.030[5] M☉ |
Radius | 1.128±0.074[5] R☉ |
Luminosity | 1.443[6] L☉ |
Surface gravity (log g) | 4.365±0.054[5] cgs |
Temperature | 5,907±52[5] K |
Metallicity [Fe/H] | 0.29±0.07[5] dex |
Rotational velocity (v sin i) | 2.6[6] km/s |
Age | 6.2 Gyr[6] 1.622±1.369[5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HD 152079 is a star with an orbiting exoplanet in the southern constellation of Ara. It is located at a distance of 287 light years from the Sun based on parallax measurements,[2] but is drifting closer with a radial velocity of −21 km/s.[4] At that distance the star is much too faint to be visible with the naked eye, having an apparent visual magnitude of 9.18.[1]
This is a G-type main-sequence star[8] with a stellar classification of G6V.[3] Age estimates range from 1.6[5] to 6.2[6] billion years. It has 1.15 times the mass of the Sun and 1.13 times the Sun's girth. This is a metal-rich star, having a higher iron abundance than in the Sun.[5] The star is radiating 1.44[6] times the luminosity of the Sun from its photosphere at an effective temperature of 5,907 K.[5]
Anderson_Francis_2012
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