Abstract
A review is given of a priori predictions made for the dynamics of rotating galaxies. One theory—MOND—has had many predictions corroborated by subsequent observations. While it is sometimes possible to offer post hoc explanations for these observations in terms of dark matter, it is seldom possible to use dark matter to predict the same phenomena.
Funder
National Aeronautics and Space Administration
National Science Foundation
Subject
Astronomy and Astrophysics
Cited by
52 articles.
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