Epsilon Reticuli - Planetary System

Planetary System

On December 11, 2000, a team of astronomers announced the discovery of a planet Epsilon Reticuli b. With a minimum mass of 1.17 that of Jupiter and a similar radius, the planet moves around Epsilon Reticuli with an average separation of 1.16 AUs. The eccentricity of the planet is extremely low (at 0.06), and it completes an orbit every 418 days (or 1.13 years).

Stability analysis shows that the planet's Lagrangian points would be stable enough to host Earth-sized planets, though as yet no trojan planets have been detected in this system.

The Epsilon Reticuli system
Companion
Mass Semimajor axis
Orbital period
Eccentricity Radius
b >1.56 ± 0.14 MJ 1.271 ± 0.073 428.1 ± 1.1 0.060 ± 0.043

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