Iota Draconis b
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Extrasolar planet | List of extrasolar planets | |
---|---|---|
Orbital elements | ||
Semimajor axis | (a) | 1.275 ± 0.074 AU |
Eccentricity | (e) | 0.7124 ± 0.0039 |
Orbital period | (P) | 511.098 ± 0.089 d (1.4 y) |
Angular distance | (θ) | 40.476 mas |
Longitude of periastron |
(ω) | 91.58 ± 0.81° |
Time of periastron | (T0) | 2,452,014.59 ± 0.30 JD |
Semi-amplitude | (K) | 307.6 ± 2.3 m/s |
Physical characteristics | ||
Mass | (m) | >8.82 ± 0.72 MJ |
Discovery information | ||
Discovery date | 2001 | |
Discoverer(s) | Frink et al. | |
Detection method | Doppler Spectroscopy | |
Discovery status | Confirmed |
Iota Draconis b was discovered in 2001 during a radial velocity study of K-class giant stars and was the first planet discovered orbiting a giant star. It is in an eccentric orbit, which aided its detection as giant stars have pulsations which can mimic the presence of a planet.[2]
[edit] See also
[edit] References
- ^ Butler et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646: 505 – 522. doi: . (web Preprint)
- ^ Frink et al. (2002). "Discovery of a Substellar Companion to the K2 III Giant Iota Draconis". The Astrophysical Journal 576 (1): 478 – 484. doi: .