description HD 190360 b Overview
HD 190360 b is a gas-giant exoplanet orbiting the nearby star HD 190360, a G-type subgiant in the constellation Lyra. Its orbit has a period of roughly eight years, placing it much farther from its star than the short-period giants found in many early exoplanet surveys. The planet was detected through the radial-velocity method, which measures the star's motion caused by the planet's gravity. It is used as an example of a long-period giant planet around a Sun-like star.
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