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M-class stars take significantly longer to reach the main sequence compared to solar-type stars. While solar-type stars (like our Sun) typically take about 10 million years to reach the main sequence, M-class stars can take anywhere from tens of millions to over a hundred million years, depending on their mass. This extended duration is due to their lower mass and slower rates of nuclear fusion, resulting in a prolonged period of contraction before they achieve stable hydrogen burning.

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