Modified Newtonian Dynamics (MOND) is a theoretical framework that adjusts Newton's laws of motion and gravity to account for the observed discrepancies in the motion of galaxies and galactic clusters without invoking dark matter. This approach proposes that at very low accelerations, the force of gravity behaves differently than predicted by traditional Newtonian physics. MOND aims to explain phenomena such as the flat rotation curves of galaxies, which cannot be fully accounted for by the presence of visible matter alone.
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