MOND predicts a number of laws that galactic systems should obey irrespective of their complicated, haphazard, and mostly unknowable histories -as Kepler's laws are obeyed by planetary systems. The main purpose of this work is to show how, and to what extent, these MOND laws follow from only the paradigm's basic tenets: departure from standard dynamics at accelerations a a 0 , and space-time scale invariance in the limit a ≪ a 0 . Such predictions will be shared by all MOND theories that embody these premises. This is important because we do not know which of the existing MOND theories, if any, is a step in the right direction. In the Newtonian-dynamics-plus-darkmatter paradigm, the validity of such clear-cut laws -which tightly constrain baryons, 'dark matter', and their mutual relations -is contrary to expectations.
Subject headings:1 Here, and in many other instances, when I refer to 'accelerations' in comparison with a0, I mean 'all quantities with the dimensions of acceleration'. This is analogous to relativity reducing to ND when all quantities with the dimensions of velocity are much smaller than the speed of light (not only velocities, but also, e.g. the square root of the gravitational potential).