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BD+49 828 b image

BD+49 828 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2015
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Welcome to the intriguing world of BD+49 828 b, a distant exoplanet orbiting the star BD+49 828! Discovered in 2015 using the clever radial velocity technique at the McDonald Observatory with their High Resolution Spectrograph, this planet is a cosmic dance partner never seen directly but known by the star’s subtle wobble. While it doesn’t have a flashy proper name yet, BD+49 828 b sparks curiosity as a celestial neighbor in the vast expanse. Imagine a world circling a star far beyond our Sun, silently orbiting through the dark, detected by astronomers’ patient measurements from Earth. It’s a reminder of the many hidden gems waiting to be unveiled in our galaxy’s grand treasure hunt!