HD 88133 b

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HD 88133 b is an exoplanet that the sub-giant HD 88133 every 3.416 days orbits.

It was developed by Debra Fischer et al. Discovered in 2004 using the radial velocity method. The major semi-axis of the exoplanet's orbit measures approx. 0.05 astronomical units , its eccentricity is 0.13. The object has a minimum mass of approx. 0.29 Jupiter masses (approx. 95 earth masses ).

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