HD 4203
From Wikipedia, the free encyclopedia
Observation data Epoch J2000.0 |
|
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Constellation (pronunciation) |
Pisces |
Right ascension | 00h 44m 41.2s |
Declination | +20° 26′ 56.1″ |
Apparent magnitude (V) | +8.68 |
Absolute magnitude (V) | +4.23 |
Distance | 253 ly (77.5 pc) |
Spectral type | G5 |
Other designations | |
BD+19º117, HIP 3502, SAO 74235
|
HD 4203 is a 9th magnitude star in the constellation Pisces. The star is yellow with spectral type G5. It is approximately 253 ly away. The star has evolved for 9.41 billion years. The star has a giant planet orbiting around +0.22 dex star.
[edit] HD 4203 b
Extrasolar planet | List of extrasolar planets | |
---|---|---|
Orbital elements | ||
Semimajor axis | (a) | 2.07±0.13 AU |
Eccentricity | (e) | 0.519±0.027 |
Orbital period | (P) | 431.88±0.85 d |
Angular distance | (θ) | 26.71 mas |
Longitude of periastron |
(ω) | 329.1±3.1° |
Time of periastron | (T0) | 2,451,918.9±2.7 JD |
Semi-amplitude | (K) | 60.3±2.2 m/s |
Physical characteristics | ||
Mass | (m) | >1.16 MJ |
Discovery information | ||
Discovery date | 2001 | |
Discoverer(s) | Vogt et al. | |
Detection method | radial velocity | |
Discovery site | Keck telescope | |
Discovery status | Published |
HD 4203 b is a planet more massive than Jupiter. It orbits two times further from the star than Earth to the Sun. The planet takes 1.1824 year to orbit the star very eccentrically from 1.00 AU to 3.14 AU. The planet was discovered by Steve Vogt using the Keck telescope.
[edit] References
- Vogt et al. (2002). "Ten Low-Mass Companions from the Keck Precision Velocity Survey". The Astrophysical Journal 568 (1): 352 – 362. doi: .
- Butler et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646 (1): 505 – 522. doi: . (web Preprint)