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HD 164922 c image

HD 164922 c

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2016
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HD 164922 c is a fascinating exoplanet orbiting the star HD 164922, discovered back in 2016 using the trusty radial velocity method from multiple ground-based observatories. This clever technique detects the tiny star wobbles caused by the planet’s gravitational tug, letting astronomers uncover worlds far beyond our solar system. While HD 164922 c remains a bit mysterious without a proper name to fancy it up, it’s part of a star system that invites curiosity and wonder. Imagine a world orbiting quietly around its sun in a cosmic dance, discovered by patient, precise instruments spread across multiple observatories. It’s an exciting reminder of the vast and varied planetary neighborhood that stretches far beyond our Earthly view.