Stellar Dynamics and Earth's Spheres: A Cosmic Connection
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Stellar Dynamics: From Formation to Evolution
Stellar Composition and Formation
Stars are celestial bodies primarily formed by hydrogen and helium atoms. The simplest atoms are formed from a small number of more complex elemental particles. These particles contain large amounts of elementary matter. As the universe expanded and cooled, elementary particles began to combine, forming atoms. Inside a star, hydrogen density is so high that pressures and temperatures reach intense conditions.
Nuclear Fusion in Stars
Under these extreme conditions, nuclear fusion reactions occur. In these reactions, hydrogen atoms combine to produce more complex atoms, such as helium, releasing a high amount of energy. This process is the fundamental energy source for... Continue reading "Stellar Dynamics and Earth's Spheres: A Cosmic Connection" »