HIP 72217

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HIP 72217
Observation data
Epoch J2000      Equinox J2000
Constellation Libra[1]
AB
Right ascension 14h 46m 10.811s[2]
Declination −21° 10 35.05[2]
Apparent magnitude (V) 6.43±0.01[3]
(7.06 + 7.33)[1]
C
Right ascension 14h 46m 11.349s[4]
Declination −21° 10 36.04[4]
Apparent magnitude (V) 16.82[1]
Characteristics
Evolutionary stage subgiant + subgiant + main sequence[1]
Spectral type G1V[5]
B−V color index 0.603[1]
Astrometry
AB
Radial velocity (Rv)−1.9±0.4[6] km/s
Proper motion (μ) RA: −57.28 mas/yr[7]
Dec.: −101.60 mas/yr[7]
Parallax (π)24.24±0.63 mas[7]
Distance135 ± 3 ly
(41 ± 1 pc)
Absolute magnitude (MV)+3.35[8]
C
Proper motion (μ) RA: −71.95 mas/yr[4]
Dec.: −108.23 mas/yr[4]
Parallax (π)24.8360±0.1337 mas[4]
Distance131.3 ± 0.7 ly
(40.3 ± 0.2 pc)
Orbit[1]
PrimaryA
CompanionB
Period (P)12.9170±0.0012 years
Semi-major axis (a)0.1854±0.0003"
(7.65 au[a])
Eccentricity (e)0.6319±0.0012
Inclination (i)25.29±0.31°
Longitude of the node (Ω)277.42±0.96°
Periastron epoch (T)1995.2607±0.0022
Argument of periastron (ω)
(secondary)
44.42±0.91°
Semi-amplitude (K1)
(primary)
7.06±0.00 km/s
Semi-amplitude (K2)
(secondary)
7.32±0.00 km/s
Details[1]
A
Mass1.14±0.15 M
Radius1.47±0.04 R
Luminosity2.73±0.19 L
Habitable zone inner limit1.223 au
Habitable zone outer limit2.847 au
Surface gravity (log g)4.14±0.11 cgs
Temperature6,125±50 K
Age3.55±0.30 Gyr
B
Mass1.12±0.14 M
Radius1.39±0.03 R
Luminosity2.21±0.14 L
Habitable zone inner limit1.108 au
Habitable zone outer limit2.599 au
Surface gravity (log g)4.20±0.12 cgs
Temperature5,950±50 K
Age3.55±0.30 Gyr
C
Mass0.17±0.01 M
Radius0.28±0.01 R
Luminosity0.0070±0.0002 L
Surface gravity (log g)4.76±0.17 cgs
Temperature3,250±50 K
Age3.55±0.30 Gyr
Other designations
BD−20°4087, HD 129980, HIP 72217, HR 5504, TYC 6166-454-1[9]
Database references
SIMBADdata
C

HIP 72217 is a triple star system in the constellation Libra. With an apparent visual magnitude of 6.43, it is very close to the limit for naked eye vision, and thus can only be seen in dark skies. Based on parallax measurements, it lies at a distance of roughly 130 light-years (40 parsecs).

Notes

References

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