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Gravitational binding of galaxies refers to the gravitational forces that hold a galaxy's stars, gas, dust, and dark matter together, preventing them from dispersing into space. This binding is primarily influenced by the mass of the galaxy and its components, with larger galaxies having stronger gravitational pulls. The interplay of gravitational attraction and the kinetic energy of stars and other matter plays a crucial role in the stability and structure of galaxies. Overall, gravitational binding ensures that galaxies remain cohesive entities within the cosmic landscape.

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