A galaxy is a massive, gravitationally bound system that consists of stars, stellar remnants, interstellar medium, dust, and dark matter.
A galaxy consists of various components, including:
Galaxies are thought to have formed from the gravitational collapse of primordial gas and dust, eventually giving rise to stars and other celestial bodies. Over time, galaxies evolve through interactions with other galaxies, mergers, and star formation processes.
Galaxies are classified based on their visual appearance, as well as their spectral characteristics. This classification system helps astronomers categorize and study different types of galaxies.
The Milky Way, the galaxy in which Earth is located, is a barred spiral galaxy.
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