HD 114386 b
Discovery | |
---|---|
Discovered by | Mayor et al. |
Discovery site | La Silla Observatory, Chile |
Discovery date | 10 February 2004 |
Detection method | Radial velocity (CORALIE) |
Orbital characteristics | |
Apastron | 2.03 AU (304,000,000 km) |
Periastron | 1.27 AU (190,000,000 km) |
Semi-major axis | 1.65 AU (247,000,000 km) |
Eccentricity | 0.23 ± 0.03 |
Orbital period | 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 MEarth) |
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]
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.
Coordinates: 13h 10m 39.8231s, −35° 03′ 17.218″
Categories:
- Exoplanets discovered in 2004
- Giant planets
- Centaurus (constellation)
- Exoplanets detected by radial velocity
- Exoplanet stubs