description HD 13908 b Overview
HD 13908 b is a gas-giant exoplanet orbiting the solar-type star HD 13908. Astronomers detected it through the radial-velocity method, using repeated measurements of the star's Doppler shifts to infer the presence of a companion. The planet belongs to a multi-planet system and represents the type of Jupiter-mass object found by long-running Doppler surveys of nearby stars.
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