Loss of Mass and Stability of Galaxies in Mond

The self-binding energy and stability of a galaxy in MOND-based gravity are curiously decreasing functions of its center of mass acceleration (of the order of 10 10m/s) towards neighbouring mass concentrations. A tentative indication of this breaking of the Strong Equivalence Principle in field galaxies is the RAVE-observed escape speed in the Milky Way. Another consequence is that satellites of field galaxies will move on nearly Keplerian orbits at large radii (100 500 kpc), with a declining speed below the asymptotically constant naive MOND prediction. But conseqences of an environment-sensitive gravity are even more severe in clusters, where member galaxies accelerate fast: no more Dark-Halo-like potential is present to support galaxies, meaning that extended axisymmetric disks of gas and stars are likely unstable. These predicted reappearance of asymptotic Keplerian velocity curves and disappearance of “stereotypic galaxies” in clusters are falsifiable with targeted surveys. Subject headings: gravitation dark matter galaxies: structure galaxies: kinematics and dynamics