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In the Chandrasekhar–Eddington dispute of the early 20th century, English astronomer Arthur Eddington and Indian astronomer Subrahmanyan Chandrasekhar disagreed over the correct theory to describe the final stages of a star's lifecycle. During the dispute, Chandrasekhar was at the beginning of his career and Eddington was a renowned physicist of the time. Chandrasekhar had proposed a limit, now known as the Chandrasekhar limit, to the mass of a white dwarf star. In a series of conferences and encounters Eddington advocated for an alternative theory, openly criticizing and mocking Chandrasekhar's models.
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