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Gravity darkening, also referred to as gravity brightening, is an astronomical phenomenon where the poles of a star are brighter than the equator, due to rapid rotation and oblate shape. When a star is oblate, it has a larger radius at its equator than it does at its poles. As a result, the poles have a higher surface gravity, and thus higher temperature…
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star gravity poles centrifugal force equator rotation oblate pressure darkening surface thus temperature resulting displaystyle mass case rho axis equatorial
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