HD 132406 b
From Wikipedia, the free encyclopedia
Extrasolar planet | List of extrasolar planets | |
---|---|---|
Orbital elements | ||
Semimajor axis | (a) | 1.98 AU |
Eccentricity | (e) | 0.34 ± 0.09 |
Orbital period | (P) | 974 ± 39 d |
Angular distance | (θ) | 4.408 mas |
Longitude of periastron |
(ω) | 214 ± 19° |
Time of periastron | (T0) | 2453474 ± 44 JD |
Semi-amplitude | (K) | 72.06 m/s |
Physical characteristics | ||
Mass | (m) | >5.61 MJ |
Discovery information | ||
Discovery date | 2007 | |
Discoverer(s) | Da Silva et al. | |
Detection method | Radial velocity | |
Discovery site | Geneva observatory | |
Discovery status | Accepted |
HD 132406 b is a long period massive gas giant extrasolar planet orbiting the Sun-like star HD 132406 at a distance of 71 parsecs.
HD 132406 b is a superjovian planet >5.61 times the mass of Jupiter. The orbital distance from the star is almost twice that of from Earth to the Sun. The orbital period is 2.7 years. Its surface gravity is very strong. About 13-15 times more than Earth. [1]
[edit] References
- Da Silva R., Udry S., Bouchy F., Moutou C., Mayor M., Beuzit J.-L., Bonfils X., Delfosse X., Desort M., Forveille T., Galland F., Hebrard G., Lagrange A.-M., Loeillet B., Lovis C., Pepe F., Perrier C., Pont F., Queloz D., Santos N., Segresan D., Sivan J.-P., Vidal-Madjar A. (2007). "Elodie metallicity-biased search for transiting Hot Jupiters. IV. Intermediate period planets orbiting the stars HD43691 and HD132406". Astron & Astrophys.
[edit] External links
- ^ Star : HD 132406. Extrasolar Planets Encyclopedia. Retrieved on 2007-07-07.