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Luminance 69-62 is a red dwarf star located approximately seventy-eight light years from Earth. It is classified as a spectral class M0V star with a mass around twenty-five percent of the Sun. At this time, there are no known exoplanets within this star system. The star is also recognized for its high proper motion.
This star, with a notable spectral classification, offers unique insights into stellar evolution and the dynamics of distant celestial bodies.
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