description HD 34445 b Overview
HD 34445 b is a giant exoplanet orbiting HD 34445, a Sun-like star about 152 light-years from Earth. It was discovered through radial-velocity observations made with the Keck Observatory and reported in 2009. The planet has a long orbital period compared with hot Jupiters, so it is commonly grouped with cold or long-period giant exoplanets. Its detection comes from the gravitational motion it induces in the host star, rather than from a recorded transit across the star's disk.
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