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HD 48265 b image

HD 48265 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2008
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Meet Naqaỹa, officially known as HD 48265 b, a fascinating giant exoplanet orbiting the star HD 48265. Discovered back in 2008 using the clever radial velocity method with the MIKE Spectrograph at Chile’s Las Campanas Observatory, Naqaỹa boasts a massive presence in its cosmic neighborhood. This gas giant doesn’t mess around, circling its host star with a gravitational grip strong enough to give astronomers a great thrill. While we can’t hop on a spaceship for a visit just yet, Naqaỹa’s discovery adds a sparkling gem to our galaxy’s treasure chest, reminding us how much there is to explore beyond our solar system!