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An accretion disk may form a variety of celestial objects, primarily through the gravitational attraction of material falling toward a central mass, such as a star or a black hole. As this material spirals inward, it loses angular momentum and heats up, emitting radiation. This process can lead to the formation of a new star, a planet, or even a binary star system, depending on the mass and dynamics involved. Additionally, in the case of black holes, the accretion disk can contribute to the growth of the black hole itself.

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