HD 130322 b
(Redirected from Eiger (planet))
| Discovery | |
|---|---|
| Discovered by | Udry, Mayor, Pepe et al. |
| Discovery site | La Silla Observatory |
| Discovery date | 4 May 2000 |
| Doppler spectroscopy (CORALIE) | |
| Orbital characteristics | |
| 0.088 AU (13,200,000 km) | |
| Eccentricity | 0.029±0.016[1] |
| 10.70871±0.00018[1] d | |
| 2453996.4±1.1[1] | |
| 193±36[1] | |
| Semi-amplitude | 112.5±2.4[1] |
| Star | HD 130322 |
HD 130322 b, officially named Eiger, is an exoplanet with a minimum mass slightly more than that of Jupiter. It orbits the star in a very close orbit distance being only a quarter that of Mercury from the Sun. It is thus a so-called "hot Jupiter". The planet orbits the star every 10 days 17 hours in a very circular orbit.[2]
Naming
[edit]The planet HD 130322 b is named Eiger. The name was selected in the NameExoWorlds campaign by Switzerland, during the 100th anniversary of the IAU. Eiger is one of the prominent peaks of the Bernese Alps.[3][4]
See also
[edit]References
[edit]- ^ a b c d e Hinkel, Natalie R.; et al. (2015). "Refined Properties of the Hd 130322 Planetary System". The Astrophysical Journal. 803 (1). 8. arXiv:1502.03441. Bibcode:2015ApJ...803....8H. doi:10.1088/0004-637X/803/1/8. S2CID 12657851.
- ^ Udry, S.; et al. (2000). "The CORALIE survey for southern extra-solar planets II. The short-period planetary companions to HD 75289 and HD 130322". Astronomy and Astrophysics. 356 (2): 590–598. Bibcode:2000A&A.....356590U. Archived from the original on 2012-02-04. Retrieved 2008-10-31.
- ^ "Approved names". NameExoworlds. Retrieved 2020-01-02.
- ^ "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
External links
[edit]- "HD 130322". Exoplanets. Archived from the original on 2012-02-19. Retrieved 2008-10-31.
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