HD 154857

HD 154857
Observation data
Epoch J2000      Equinox J2000
Constellation Ara
Right ascension 17h 11m 15.72205s
Declination −56° 40 50.8712
Apparent magnitude (V) 7.25
Characteristics
Evolutionary stage subgiant
Spectral type G5IV-V
B−V color index 0.699±0.001
Variable type Constant
Astrometry
Radial velocity (Rv)+28.10±0.12 km/s
Proper motion (μ) RA: +87.442 mas/yr
Dec.: −55.861 mas/yr
Parallax (π)15.8176±0.0197 mas
Distance206.2 ± 0.3 ly
(63.22 ± 0.08 pc)
Absolute magnitude (MV)3.07
Details
Mass1.718+0.03
−0.022
 M
Radius2.1±0.1 R
Luminosity4.4±0.3 L
Surface gravity (log g)3.83±0.03 cgs
Temperature5,740±46 K
Metallicity [Fe/H]−0.26±0.01 dex
Rotational velocity (v sin i)1.44±0.50 km/s
Age5.8±0.5 Gyr
Other designations
CD−56°6717, CPD−56°8059, GC 23146, HD 154857, HIP 84069, SAO 244491, PPM 345752, TYC 8735-1682-1, GSC 08735-01682
Database references
SIMBADdata

HD 154857 is a star with two exoplanetary companions in the southern constellation of Ara. It is too dim to be visible with the naked eye having an apparent visual magnitude of 7.25. The star is located at a distance of 206 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +28 km/s.

This is a G-type star with a stellar classification of G5IV-V. The absolute magnitude of this star is two magnitudes above the main sequence, which suggests that the star is evolving toward the subgiant stage. It is a metal-poor thin disk star approximately six billion years old and is chromopherically quiet although not in a Maunder Minimum state. The star is larger, more massive, and more luminous than the Sun. It is spinning with a projected rotational velocity of 1.4 km/s.