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Explore advanced theoretical models of solar system formation in this comprehensive lecture delivered by Alessandro Morbidelli during the RED Astrobiology training school. Delve into sophisticated computational and analytical frameworks that explain how our solar system evolved from a primordial disk of gas and dust into the complex planetary system we observe today. Examine the latest modeling approaches that address key questions about planetary migration, the formation of terrestrial and giant planets, the distribution of asteroids and comets, and the delivery of water and organic materials to Earth. Learn how these models reconcile observational data with theoretical predictions, including insights from exoplanetary systems that have revolutionized our understanding of planetary formation processes. Discover how numerical simulations and mathematical models help explain the unique architecture of our solar system, including the spacing of planets, the asteroid belt's structure, and the outer solar system's configuration. Gain insights into cutting-edge research methodologies used by planetary scientists to test and refine formation theories, and understand how these models contribute to our broader understanding of astrobiology and the potential for life in other planetary systems.
