A star is a celestial body that produces its own light through nuclear reactions occurring in its core. The Sun is the closest and most familiar example, but there are billions of other stars in our galaxy, each with its own physical characteristics and evolutionary history.
The closest star to us, Proxima Centauri, is a small red dwarf located about 4 light-years away, which is nearly 250,000 times farther than the Sun. Other remarkable stars populate our sky, such as Sirius, a binary system composed of Sirius A and Sirius B, or Betelgeuse, a massive red supergiant with a radius about 900 times that of the Sun.
Observing stars means exploring a diversity of sizes, colors, temperatures, and evolutionary stages. Some are young and massive, while others are old and nearing the end of their lives. Studying them helps us understand the formation of galaxies, the evolution of matter, and the fundamental mechanisms that shape the universe. Each star tells part of the cosmic story.
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