I keep running simulations of the local galaxies on Universe Sandbox, and every time a large magellanic cloud (a relatively small irregular gassy galaxy near the Milky Way) collides with the core of the Milky way in just under 300 million years, the simulations differ, but most of the time it predicts a catastrophic collision of the cores, the shock of which knocks the core of the Milky Way off it's current course at a relatively fast speed that leaves half the stars (mostly middle and outer stars) out of orbit of the Milky Way completely! The effect is similar to a diamond ring, an expanding ring of dust and stars with the core of the Milky way expanding at one end. Could this really happen?