The Milky Way is the galaxy that houses our solar system. It is a barred spiral galaxy featuring a distinct structure with several key components.
- The Disk: This is a flattened region containing most of the galaxy's stars, including our Sun, gas, and dust.
- The Bulge: A densely packed region of stars and dust located at the center of the galaxy.
- The Halo: This spherical component surrounds the disk and bulge and contains older stars and many globular clusters.
Due to its spiral nature, the Milky Way has several spiral arms emanating from the center and wrapping around the galaxy. These arms are places of active star formation.
When considering the distribution of objects like globular clusters in the Milky Way, it becomes evident that these clusters tend to gather around the galactic center, revealing the galaxy's gravitational influence and structure.