Overview of the Planetesimal Hypothesis of Chamberlin (1905), detailing the theory's introduction, core concepts, and outcomes. Learn about the interaction between the Proto-Sun and an Intruding Star, and how this hypothesis explains the origin of the Earth, its structure, atmosphere, and the formation of continents and ocean basins.
When the Intruding Star came very close to the Proto-Sun, an infinite number of small particles were detached from the outer surface of the Proto-Sun due to the massive gravitational pull exerted by the giant Intruding Star.
This matter, composed of dust, gases, and rock fragments, eventually accreted, forming planets and other celestial bodies that revolve around the Proto-Sun.
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