description HD 108874 b Overview
HD 108874 b is a gas-giant exoplanet orbiting the G-type star HD 108874. It was discovered through the radial-velocity method and has an orbital period of about 394 days, placing it near the distance from its star associated with the outer part of the habitable-zone region in some system models. The system also contains a second known planet farther out. The object is studied as a long-period giant around a star broadly comparable to the Sun.
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