This topic necessitates a rigorous understanding of the solar system's structure, governed by gravitational forces that maintain circular and elliptical orbits. Candidates must analyze the life cycle of stars, detailing the equilibrium between gravitational collapse and radiation pressure from nuclear fusion, and differentiate evolutionary paths based on stellar mass (e.g., neutron stars vs. white dwarfs). Furthermore, the expansion of the universe must be evidenced through the analysis of red-shift and the Doppler effect, linking observed spectral data to the Big Bang theory. Mastery of this topic requires synthesizing mechanics (orbital motion) with nuclear physics (fusion) and cosmology.
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