HD 222582
From Wikipedia, the free encyclopedia
| Observation data Epoch J2000 |
|
|---|---|
| Constellation (pronunciation) |
Aquarius |
| Right ascension | 23h 41m 51.5299s |
| Declination | -05° 59′ 08.726″ |
| Apparent magnitude (V) | 7.7 |
| Characteristics | |
| Spectral type | G5 |
| Astrometry | |
| Radial velocity (Rv) | 11.5 km/s |
| Proper motion (μ) | RA: -145.41 mas/yr Dec.: -111.1 mas/yr |
| Parallax (π) | 23.84 ± 1.11 mas |
| Distance | 137 ± 6 ly (42 ± 2 pc) |
| Absolute magnitude (MV) | 8.3 |
| Details | |
| Mass | 1 M☉ |
| Radius | 1.17 R☉ |
| Temperature | 5770 K |
| Metallicity | ? |
| Rotation | ? |
| Age | 10,000 million years |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Planet | |
| Database references | |
| SIMBAD | data |
HD 222582 is a magnitude 7.7 star in the constellation Aquarius. In 1999, the superjovian planet was announced orbiting the star by Steven Vogt.
[edit] HD 222582 b
| Orbital elements | ||
|---|---|---|
| Semi-major axis a: | 1.35 AU | |
| Eccentricity e: | 0.76 | |
| Orbital period P: | 572 d | |
| Inclination i: | ?° | |
| Angular distance θ: | 32 mas | |
| Longitude of periastron ω: |
293° | |
| Time of periastron τ: | 2,450,174.8 JD | |
| Semi-amplitude K: | 276.6 m/s | |
| Physical characteristics | ||
| Mass: | >5.4 MJ | |
| Radius: | ? RJ | |
| Density: | ? kg/m³ | |
| Gravity: | ? g | |
| Temperature: | ? K | |
| Discovery | ||
| Discovery date: | 1999 | |
| Discovery site: | ||
| Detection method(s): | radial velocity | |
| Discoverer(s): | Vogt et al. | |
| Other catalogue | ||
HD 222582 b is a massive planet orbiting the star HD 222582. The orbital period is 572 days and orbits at a semimajor axis of 1.35 AU in one of the most eccentric orbits of any known planet.
[edit] References
- Gimenez A. (2000). "ubvy Photometry of stars with planets" 356: 213.
- HAN I., BLACK D. & GATEWOOD G. (2000). "Preliminary astrometric masses for proposed exrasolar planetary companions" ([dead link] – Scholar search) 548: L57.
- Vogt et al. (2000). "Six New Planets from the Keck Precision Velocity Survey". The Astrophysical Journal 536 (2): 902 – 914. doi:.


