A galaxy is a massive, gravitationally bound system that consists of stars, stellar remnants, interstellar gas, dust, dark matter, and an important but poorly understood component tentatively dubbed dark energy. Galaxies contain varying amounts of star systems, star clusters, and types of interstellar clouds.
There are three main types of galaxies:
Galaxies are thought to have formed from the gravitational collapse of dense regions within the early universe. As galaxies evolve, they can interact and merge with other galaxies, leading to the formation of different types of galaxies and influencing their structures and properties.
Galaxies can be studied through various methods, including:
When studying galaxies, it's important to understand the following key concepts:
Additionally, familiarizing yourself with prominent galaxies, such as the Milky Way, Andromeda, and the Magellanic Clouds, can provide valuable context for understanding the diversity and complexity of galactic systems.
Remember to engage with visual aids, such as images and diagrams of galaxies, to reinforce your understanding of their structures and features.
Good luck with your studies!
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