Heliocentric distance, Ξ(t), and change in magnitude of the specific angular momentum, δL(t) ≡ L(t)−L(0), as a function of time, t, for 100 Monte Carlo test particles initialised with a = 10 kau, and q uniformly distributed on the interval (15,100) au. The top row represents an output of the Milgromian simulation, the bottom row, the Newtonian simulation. In MD simulation, the follow up time, T_rev, is set to 0.26 Myr (see top left quarter of the figure for motivation), in Newtonian simulation T_rev is set to be the Keplerian period T_Kep(a = 10 kau) ≈1 Myr.