Difference in the position (panels a, c, and e) and velocity (b, d, and f) when the stellar trajectory is calculated as (i) a trajectory of uniformly moving object along a straight line and (ii) a trajectory of the object gravitationally perturbed by the Milky Way. Panels a and b: Maximum detected differences in the galactic coordinate frame. The maximum occurred as for the distance as velocity in the case of star No. 1475. Panels c and d: Differences in the heliocentric coordinate frame of this star. In this frame, the maximum was not detected for this star and, instead, the heliocentric distance maximum for star No. 2857 (e) and the heliocentric velocity maximum for star No. 5497 (f) were detected. The modified galactic coordinate system, with the x-axis oriented outward from the Galactic center, is adopted.