Iota Draconis b[1]
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]
See also
* Iota Draconis
References
- ^ Butler et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal 646: 505 – 522. (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.
Links
SIMBAD: HD 137759 b
SolStation: Edasich/Iota Draconis
The Extrasolar Planet Encyclopaedia: Notes for planet HIP 75458 b
Extrasolar Visions: Iota Draconis b