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HD 34445 c image

HD 34445 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2017
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HD 34445 c is an intriguing exoplanet orbiting the star HD 34445, discovered in 2017 through the clever technique of radial velocity. This method, which detects the gentle wobble of a star caused by an orbiting planet, was employed using multiple instruments at various ground-based observatories. While the exact details of HD 34445 c’s size and orbit might remain a cosmic mystery for now, its discovery adds another piece to the puzzle of planetary systems beyond our own. Imagine a world circling a distant star, quietly tracing its path as astronomers on Earth piece together its story from afar — a subtle yet remarkable dance millions of miles away in the vast theater of space.