
Ultra-Low-Acceleration Gravity: New Study Sparks MOND Possibilities
A Gaia-based study of 26,500 wide binary stars within 650 light-years finds that at ultra-low accelerations (~0.1 nm/s^2) observed accelerations exceed Newton-Einstein predictions by about 30–40%, while at higher accelerations (~10 nm/s^2) the data align with standard gravity. The results could be explained by Modified Newtonian Dynamics (MOND) and the AQUAL formulation, offering potential evidence for gravity behavior beyond the classical model, though MOND remains a theory and further observations are needed amid ongoing dark-matter explanations.









