Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Circinus |
Right ascension | 14h 46m 03.06521s[1] |
Declination | –68° 45′ 45.8797″[1] |
Apparent magnitude (V) | 8.80[2] |
Characteristics | |
Spectral type | G6 V[3] |
Apparent magnitude (B) | 9.556[2] |
Apparent magnitude (J) | 7.531±0.023[2] |
Apparent magnitude (H) | 7.243±0.027[2] |
Apparent magnitude (K) | 7.167±0.026[2] |
B−V color index | 0.756±0.002[2] |
Astrometry | |
Radial velocity (Rv) | +8.56±0.13[1] km/s |
Proper motion (μ) | RA: –197.892 mas/yr[1] Dec.: –57.069 mas/yr[1] |
Parallax (π) | 14.9136 ± 0.0147 mas[1] |
Distance | 218.7 ± 0.2 ly (67.05 ± 0.07 pc) |
Absolute magnitude (MV) | 4.73[2] |
Details[4] | |
Mass | 1.06+0.03 −0.05 M☉ |
Radius | 1.18±0.01[5] R☉ |
Luminosity | 1.229+0.005 −0.004[5] L☉ |
Surface gravity (log g) | 4.39±0.08 cgs |
Temperature | 5,605+21 −34[5] K |
Metallicity [Fe/H] | 0.36±0.10 dex |
Rotational velocity (v sin i) | 1.4[6] km/s |
Age | 4.94+3.77 −2.04 Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HD 129445 (HIP 72203; LTT 5856) is a star located in the southern constellation Circinus. It has an apparent magnitude of 8.80,[2] making it faintly visble in binoculars but not to the naked eye. The object is located relatively close at a distance of 219 light-years based on Gaia DR3 parallax measurements but it is drifting away with a spectroscopic radial velocity of 8.56 km/s.[1] It has an absolute magnitude of +4.73,[2] which is similar to the Sun's absolute magnitude of 4.83.
GaiaDR3
was invoked but never defined (see the help page).Anderson_Francis_2012
was invoked but never defined (see the help page).Houk1979
was invoked but never defined (see the help page).AguileraGómez_et_al_2018
was invoked but never defined (see the help page).GaiaDR2
was invoked but never defined (see the help page).Jenkins_et_al_2011
was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).