Synopsis

The universe knows no stillness. Within the Milky Way, countless stars trace paths around the galactic core. Some, like our sun, maintain a steady course, remaining roughly 30,000 light-years from the center and completing a revolution in 230 million years. This celestial choreography is far from graceful; it resembles a chaotic swirl, akin to toddlers on roller skates. This inherent disorder renders the galaxy a perilous place. Our solar neighborhood is in perpetual flux, with stars shifting hu