description 61 Virginis d Overview
61 Virginis d is the outermost member of the three-planet system reported around the nearby Sun-like star 61 Virginis. It was identified through the radial-velocity method and has an orbital period of about 123 days. Its minimum mass is approximately 22.9 times that of Earth, placing it in the Neptune-mass or super-Earth range, although the true mass depends on the inclination of its orbit.
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