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HD 109271 b image

HD 109271 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2013
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HD 109271 b is a charming little world orbiting the star HD 109271, discovered back in 2013 using the trusty HARPS Spectrograph at La Silla Observatory. This exoplanet was spotted through the radial velocity method, which essentially means astronomers detected the gentle wobble of its host star caused by the planet’s gravitational tug. While it’s not flashy with a proper name, HD 109271 b holds its own as an intriguing member of our galactic neighborhood. Hovering far beyond our solar system, it gives us a glimpse into the diverse variety of planets that exist in the universe. Imagine the cosmic dance between this planet and its star happening silently, millions of miles away from Earth—an invitation to dream about the unknown worlds out there.