What if a red dwarf star with 0.12 solar masses plunged through the outer Solar System on an unbound hyperbolic trajectory, passing the Sun at a closest distance of 40 AU? All eight planets, every major dwarf planet from Ceres to Eris, and the largest scattered-disc objects share their real January 2025 configuration as the interloper sweeps past. Scholz's Star actually grazed the Solar System about 70,000 years ago at 0.8 light-years, but a closer 40 AU passage would gravitationally roil the Oort Cloud, injecting comets into the inner system and potentially destabilising the outer planets' orbits over millions of years.