The Milky Way has a complex structure characterized by a central bulge, spiral arms, a disk, and a halo. The central bulge contains older stars and a supermassive black hole at its core, while the spiral arms feature younger stars, gas, and dust. The disk is where most of the galaxy’s stars, including the Sun, reside, while the halo contains globular clusters and dark matter.
Come for the Scenery, Stay for the Stars