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HD 149026 b image

HD 149026 b

World type: gas_giant
Discovery method: Radial Velocity
Discovery year: 2005
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HD 149026 b, known by its proper name Smertrios, is a fascinating exoplanet orbiting the star HD 149026. Discovered in 2005 using the radial velocity method by the HDS Spectrograph at the Subaru Telescope, this intriguing world sparks curiosity with its unique characteristics. Smertrios is a hot Jupiter, sizzling close to its star, and it boasts a surprisingly dense core, making it a standout among gas giants. Its close orbit creates a dramatic dance with its host star, bathing the planet in intense stellar energy. While we don’t have its exact distance from Earth here, Smertrios represents a remarkable find in our ongoing quest to explore diverse planetary systems beyond our own solar neighborhood. This exoplanet truly invites wonder and awe among cosmic explorers.