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In astronomy, accretion discs are structures formed by diffuse material in orbital motion around a central body, such as a star or a black hole.
In physics, accretion discs are used as models to study fluid dynamics, magnetohydrodynamics, and other physical processes in rotating systems.
In astrophysics, accretion discs play a crucial role in the process of mass transfer between celestial bodies, providing insights into the dynamics of cosmic systems.
In cosmology, accretion discs are studied to understand the formation and evolution of galaxies, as well as the distribution of matter in the universe.
In planetary science, accretion discs are relevant to the formation of planets and moons in protoplanetary disks around young stars.
Astronomers study accretion discs around stars and black holes to understand the process of matter falling into these objects.
Physicists use accretion discs as a model to study the transfer of angular momentum and energy in astrophysical systems.
Astrophysicists research accretion discs to investigate the formation of planets and stars in various cosmic environments.
Engineers may study accretion discs to design systems that efficiently transfer materials and energy in industrial processes.