Gamma Cephei Ab
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Extrasolar planet | List of extrasolar planets | |
---|---|---|
Parent star | ||
Star | Gamma Cephei A | |
Constellation | Cepheus | |
Right ascension | (α) | 23h 39m 20.8s |
Declination | (δ) | +77° 37′ 56″ |
Distance | 45 ± 0.3 ly (13.81 ± 0.1 pc) | |
Spectral type | K1IVe | |
Orbital elements | ||
Semimajor axis | (a) | 2.044 AU |
Eccentricity | (e) | 0.115 ± 0.069 |
Orbital period | (P) | 902.96 ± 6 d (2.47 y) |
Angular distance | (θ) | 173.22 mas |
Longitude of periastron |
(ω) | 75.6 ± 18.8° |
Time of periastron | (T0) | 2,453,156.8 ± 52.4 JD |
Semi-amplitude | (K) | 27.5 ± 1.5 m/s |
Physical characteristics | ||
Mass | (m) | >1.59 MJ |
Discovery information | ||
Discovery date | July 13, 1988 and confirmed on Sept 24, 2002 |
|
Discoverer(s) | Campbell, Walker, Yang et al. | |
Detection method | Doppler Spectroscopy | |
Discovery status | Confirmed |
Gamma Cephei Ab is an extrasolar planet orbiting Gamma Cephei A every two years.
Contents |
[edit] Discovery
A planet orbiting Gamma Cephei A was tentatively identified by a Canadian team of Bruce Campbell, Gordon Walker, and Stephenson Yang in July 1988. Its existence was also announced by Anthony Lawton and P. Wright in 1989. This would have been the first confirmed extrasolar planet, and it was hypothesized based on the same radial velocity technique later used successfully by others. However, the claim was retracted in 1992 due to the quality of the data not being good enough to make a solid discovery. But on September 24, 2002, Gamma Cephei Ab was finally confirmed. The team of astronomers (including William D. Cochran, Artie P. Hatzes... etc.) at the Planetary Systems and their Formation Workshop announced the preliminary confirmation of a long-suspected planet Gamma Cephei Ab with a minimum mass of 1.59 times that of Jupiter.
[edit] Orbit and mass
Gamma Cephei moves between 1.81 and 2.28 AUs in orbital distance around Gamma Cephei A, with an average separation of around 2.044 AUs, which would be placed beyond the orbit of Mars in the solar system. Its orbit has an eccentricity of 0.115 and takes 2.47 years to complete.
[edit] See also
[edit] References
- Hatzes et al. (2003). "A Planetary Companion to Gamma Cephei A". The Astrophysical Journal 599 (2): 1383 – 1394. doi: .
[edit] External links
- McDonald Observatory: Planet Search finds first planet orbiting close-in binary star
- A Planetary Companion to the Binary Star Gamma Cephei
- SolStation: Errai 2
- Extrasolar Planets Encyclopaedia: Gamma Cephei b
- Extrasolar Visions: Gamma Cephei Ab