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47 UMa d image

47 UMa d

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2009
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Meet 47 Ursae Majoris d, the mysterious outer sibling in the 47 Ursae Majoris star system, discovered back in 2009 using the trusty radial velocity method at California’s Lick Observatory. This giant planet orbits a sun-like star not too far from our cosmic neighborhood, making it a fascinating target for curious stargazers. Although it doesn’t have a snappy proper name yet, 47 UMa d holds its own as part of a family that has intrigued astronomers for decades. While you can’t visit just yet, imagining this distant world sailing through space, quietly orbiting its star, brings a touch of wonder to anyone who dreams about the vastness beyond our solar system. Keep your eyes—and telescopes—on the skies!