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] |
Astrometry | |
Radial velocity (Rv) | −2.781±0.140 [2] km/s |
Proper motion (μ) |
RA: 37.832
mas/
yr
[1] Dec.: −20.334 mas/ yr [1] |
Parallax (π) | 9.5339 ± 0.0521 mas [1] |
Distance | 342 ± 2
ly (104.9 ± 0.6 pc) |
Absolute magnitude (MV) | 2.5±0.3 [4] |
Orbit [5] | |
Primary | HD 180902 A |
Companion | HD 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 | |
Mass | 1.698±0.085 [2] M☉ |
Radius | 4.247±0.212 [2] R☉ |
Luminosity | 9.4±0.5 [4] L☉ |
Temperature | 5,030±44 [4] K |
Metallicity [Fe/H] | 0.04±0.03 [4] dex |
Age | 2.8±0.7 [4] Gyr |
HD 180902 B | |
Mass | 44.53+12.91 −5.88 [2] MJup |
Other designations | |
Database references | |
SIMBAD | data |
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. [2] It has an absolute magnitude of 2.5, [4] but at that distance the apparent visual magnitude of the system is 7.8, [2] which is too faint to be seen with the naked eye.
The spectrum of the primary, component A, presents as an evolving 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]
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]
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 | — | — |