These are hot, high-mass stars that burn intensely—over 20,000 times brighter than our Sun—and are expected to eventually end their lives as supernovas.
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A third, smaller B-type companion star that orbits the central binary pair at a much greater distance, with an estimated orbital period of roughly 225 to 288 years . Key Characteristics These are hot, high-mass stars that burn intensely—over
The Centauri system has garnered significant attention for several reasons: These are hot
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