Gravitational Collapse
Gravitational collapse is the process by which an object is pulled inward due to its own gravity to form a more massive object. In space and astronautical engineering, gravitational collapse is a fundamental process that governs the formation of celestial bodies such as stars, planets, and black holes. The process begins with a cloud of gas and dust that collapses under its own gravity, forming a protostar. As the protostar continues to collapse, it heats up and eventually reaches a temperature at which nuclear fusion can occur, leading to the formation of a star. In the case of a massive star, the core will eventually collapse under its own gravity, leading to a supernova explosion and the formation of a neutron star or black hole.
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