HD 180902

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HD 180902
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Sagittarius
Right ascension 19h 19m 17.708s[1]
Declination −23° 33′ 29.36″[1]
Apparent magnitude (V) 7.785[2]
Characteristics
Spectral type K0 III/IV[3]
B−V color index +0.94[4]
Distance
342 ± 2 ly
(104.9 ± 0.6 pc)
Absolute magnitude (MV)2.5±0.3[4]
Semi-amplitude
(K1)
(primary)
898±28 km/s
Details
HD 180902 A
Gyr
HD 180902 B
Mass44.53+12.91
−5.88
[2] MJup
PPM 269620[6]
Database references
SIMBADdata

HD 180902 is a

apparent visual magnitude of the system is 7.8,[2]
which is too faint to be seen with the naked eye.

The

subgiant star[5] with a stellar classification of K0 III/IV.[3] It is an estimated 2.8[4] 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[2] and is radiating 9.4 times the Sun's luminosity from an enlarged photosphere at an effective temperature of 5,030 K.[4]

Companions

HD 180902 b was discovered using the Doppler spectroscopy method with observations taken at the W. M. Keck Observatory.[4] The radial velocities showed a long term linear trend in the data indicating an additional companion of unknown nature with a longer orbital period.[4] This was subsequently shown to be due to an orbiting brown dwarf or low mass stellar companion, designated component B.[5]

There is a second unconfirmed planet, HD 180902 c, with a mass at least twice that of Neptune and an orbital period of 15 days.[5]

The HD 180902 planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥1.685±0.041 MJ 1.40±0.11 510.9±1.5 0.107±0.022
c (unconfirmed) ≥0.099±0.014 MJ 0.139±0.011 15.9058±0.0055 0.28±0.13

References