HD 114386 b
HD 114386 b is an exoplanet orbiting the star HD 114386. The planet orbits the star in a rather eccentric orbit. Mean distance from the star is 1.62 AU, somewhat more than distance between Mars and the Sun. At periastron, the planet comes almost as close as Earth orbits the Sun, and at apoastron, the distance is twice as much.[1]
| Discovery | |
|---|---|
| Discovered by | Mayor et al. |
| Discovery site | La Silla Observatory, Chile |
| Discovery date | 10 February 2004 |
| Radial velocity (CORALIE) | |
| Orbital characteristics | |
| Apastron | 2.03 AU (304,000,000 km) |
| Periastron | 1.27 AU (190,000,000 km) |
| 1.65 AU (247,000,000 km) | |
| Eccentricity | 0.23 ± 0.03 |
| 937.7 ± 15.6 d 2.567 y | |
Average orbital speed | 19.2 |
| 2,450,454 ± 43 | |
| 273° ± 14 | |
| Semi-amplitude | 34.3 ± 1.6 |
| Star | HD 114386 |
| Physical characteristics | |
| Mass | >1.24 MJ (>394 M⊕) |
See also
References
- Mayor, M.; et al. (2004). "The CORALIE survey for southern extra-solar planets XII. Orbital solutions for 16 extra-solar planets discovered with CORALIE". Astronomy and Astrophysics. 415 (1): 391–402. arXiv:astro-ph/0310316. Bibcode:2004A&A...415..391M. doi:10.1051/0004-6361:20034250.
External links
- "HD 114386". Exoplanets. Archived from the original on 2012-10-25. Retrieved 2008-10-31.
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