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an early proposed hypothesis for the formation of the solar system is a disk of material...

an early proposed hypothesis for the formation of the solar system is a disk of material whose outer layers become the planets and asteroids as it collapses and all remaining material must be within the sun. Given the mass of the sun is many times larger than the total mass of everything else in the solar system, what could we observe, measure, and calculate to determine if this hypothesis is true? we may assume the conservation of angular momentum.

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