Structure
Spiral galaxies consist of four distinct components:
- A flat, rotating disc of (mostly newly created) stars and interstellar matter
- A central stellar bulge of mainly older stars, which resembles an elliptical galaxy
- A near-spherical halo of stars, including many in globular clusters
- A supermassive black hole at the very center of the central bulge
The relative importance, in terms of mass, brightness and size, of the different components varies from galaxy to galaxy.
Read more about this topic: Spiral Galaxy
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—Karl Wilhelm Von Humboldt (1767–1835)
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—Friedrich Nietzsche (1844–1900)