Circumstellar Disks
Circumstellar disks are flat structures of gas and dust that surround a star and extend outward from its planetary system. These disks are formed during the star's early stages of formation and are believed to be the birthplace of planets. The disks are composed of small dust particles and gas, which can clump together to form larger bodies. The disks can also exhibit various features such as gaps, rings, and spiral arms, which can be caused by the gravitational influence of planets or other objects within the disk. Studying circumstellar disks can provide insights into the formation and evolution of planetary systems.
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