With evidence mounting against the standard model of cosmology, Modified Newtonian Dynamics, or MOND, is the strongest contender. But in a recent iai News article, Idranil Banik argued that new research into wide binary stars falsifies MOND. Here, Pavel Kroupa and Jan Pflamm-Altenburg argue that data around wide binary stars are beset by uncertainty, bringing into question what, if anything, can be determined from them at the present – and ask whether a single test, even if carried out to the highest confidence, is sufficient to falsify an otherwise successful theory.
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