HD 330075 b
HD 330075 b is an extrasolar planet approximately 164 light-years away in the constellation of Norma. This planet orbits the star HD 330075. It was discovered by the Geneva Extrasolar Planet Search team at ESO's La Silla Observatory using the HARPS spectrograph.[1]
| Discovery | |
|---|---|
| Discovered by | Pepe et al. |
| Discovery site | La Silla Observatory, Chile |
| Discovery date | February 10, 2004 |
| Radial velocity | |
| Orbital characteristics | |
| Apastron | 0.043 AU (6,400,000 km) |
| Periastron | 0.043 AU (6,400,000 km) |
| 0.043 AU (6,400,000 km) | |
| Eccentricity | 0 |
| 3.369 ± 0.004 d 0.009224 y | |
| 2,452,878.698 ± 0.032 | |
| 0 | |
| Semi-amplitude | 107 ± 0.7 |
| Star | HD 330075 |
The planet has a mass about three quarters that of Jupiter. Its orbital distance from the star is less than 1/23rd Earth's distance from the Sun, which makes HD 330075 b an example of a hot Jupiter. One orbit around the star takes a little more than 3 Earth days to complete, as compared to one year for the Earth around the Sun.[1]
References
- Pepe, F.; et al. (2004). "The HARPS search for southern extra-solar planets I. HD 330075 b: A new "hot Jupiter"". Astronomy and Astrophysics. 423 (1): 385–389. arXiv:astro-ph/0405252. Bibcode:2004A&A...423..385P. doi:10.1051/0004-6361:20040389.
External links
- "HD 330075". Exoplanets. Archived from the original on 2009-11-25. Retrieved 2008-08-16.
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