Stellar Clusters
Stellar clusters are captivating astronomical phenomena, comprising groups of stars held together by gravitational forces within a relatively small region of space. These clusters offer astronomers invaluable insights into stellar evolution, formation, and dynamics. Classified into two main types—globular and open clusters—each presents distinct characteristics and behaviors. Globular clusters, with their densely packed arrangement of ancient stars, provide crucial data for understanding the universe's age and structure. On the other hand, open clusters, often containing younger stars, offer a glimpse into ongoing star formation processes. Studying stellar clusters unveils the complexities of galactic environments and sheds light on the fundamental principles governing celestial bodies.
- What are globular clusters?
- In globular clusters, what type of stars will be the brightest?
- How did globular clusters form?
- How big are globular clusters?
- What is the difference between open clusters and globular clusters?
- Why are stars generally several light years apart except in binary star system, etc.?