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HIP 67851 b image

HIP 67851 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2015
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Orbiting the bright star HIP 67851, HIP 67851 b is a giant exoplanet discovered in 2015 using the radial velocity method from ground-based observatories. This massive world is a gas giant, somewhat like a heavyweight cousin of Jupiter, swirling in its celestial dance far beyond our solar system. Although it doesn’t have a catchy nickname just yet, HIP 67851 b captivates astronomers with its impressive presence and the clues it holds about planetary formation around stars outside our own neighborhood. Thanks to careful observations from multiple instruments across various observatories, HIP 67851 b continues to be an intriguing cosmic companion in the vast expanse of the galaxy. It’s a fantastic target for those dreaming of distant worlds and extraterrestrial adventure!