Spiral galaxies, with their majestic arms and luminous cores, are some of the most captivating and beautiful structures in the universe. These cosmic wonders, which include our own Milky Way, are characterized by their flat, rotating disk of stars, gas, and dust, along with a central bulge of older stars and a halo containing globular clusters Spiral Galaxies Spiral galaxies are distinguished by their distinct components: 1. The Disk: The most recognizable feature of a spiral galaxy is its disk, which contains spiral arms extending from the center. These arms are sites of active star formation and are composed of young, hot stars that give them a bright, bluish appearance. 2. The Bulge: At the heart of a spiral galaxy lies the central bulge, a densely packed region of older stars. The bulge can vary in size and shape, from nearly spherical to more elongated structures. 3. The Halo: Surrounding the disk and bulge is the halo, a spherical region containing older stars, globular clus
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