HD 180902

HD 180902 is a star with two or more orbiting companions in the southern constellation of Sagittarius. This system is located at a distance of approximately 342 light years from the Sun based on parallax measurements, but is drifting closer with a radial velocity of −2.8 km/s. It has an absolute magnitude of 2.5, but at that distance the apparent visual magnitude of the system is 7.8, which is too faint to be seen with the naked eye.

HD 180902
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 19h 19m 17.708s
Declination −23° 33 29.36
Apparent magnitude (V) 7.785
Characteristics
Spectral type K0 III/IV
B−V color index +0.94
Astrometry
Radial velocity (Rv)−2.781±0.140 km/s
Proper motion (μ) RA: 37.832 mas/yr
Dec.: −20.334 mas/yr
Parallax (π)9.5339 ± 0.0521 mas
Distance342 ± 2 ly
(104.9 ± 0.6 pc)
Absolute magnitude (MV)2.5±0.3
Orbit
PrimaryHD 180902 A
CompanionHD 180902 B
Period (P)5880±440 d
Semi-major axis (a)7.15±0.69 AU
Eccentricity (e)0.335±0.025
Periastron epoch (T)2441100±1200 JD
Argument of periastron (ω)
(secondary)
73.3±1.6°
Semi-amplitude (K1)
(primary)
898±28 km/s
Details
HD 180902 A
Mass1.698±0.085 M
Radius4.247±0.212 R
Luminosity9.4±0.5 L
Temperature5,030±44 K
Metallicity [Fe/H]0.04±0.03 dex
Age2.8±0.7 Gyr
HD 180902 B
Mass44.53+12.91
5.88
 MJup
Other designations
CD−23° 15276, HD 180902, HIP 94951, SAO 187961, PPM 269620
Database references
SIMBADdata

The spectrum of the primary, component A, presents as an evolving subgiant star with a stellar classification of K0 III/IV. It is an estimated 2.8 billion years old with 1.7 times the mass of the Sun. The star has expanded to 4.2 times the radius of the Sun and is radiating 9.4 times the Sun's luminosity from an enlarged photosphere at an effective temperature of 5,030 K.

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