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94 Ceti b
Extrasolar planet in the constellation Cetus
Extrasolar planet in the constellation Cetus
| Field | Value |
|---|---|
| name | 94 Ceti b |
| image | 94 Ceti b.jpg |
| caption | Simulated view of the 94 Ceti binary system |
| discoverer | Mayor et al. |
| discovered | August 7, 2000 |
| discovery_method | Doppler Spectroscopy |
| apsis | astron |
| semimajor | 1.427 AU |
| eccentricity | 0.30±0.04 |
| period | 535.7±3.1 d |
| inclination | 65 or 115 ±3 |
| time_periastron | 2,450,944±12 |
| arg_peri | 41±8 |
| semi-amplitude | 36.2±1.9 |
| star | 94 Ceti |
| mass | 1.855±0.045 |
| semi-amplitude = 36.2±1.9 94 Ceti b or 94 Ceti Ab to distinguish it from the distant red dwarf companion, is an extrasolar planet orbiting its star once every 1.2 years. It was discovered on August 7, 2000 by a team led by Michel Mayor.
It is most stable if its inclination is about 65 or 115, yielding a mass of about 1.85 that of Jupiter.
References
References
- (2013). "Analysis of the motion of an extrasolar planet in a binary system". The Astronomical Journal.
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