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Protostars surrounded by protoplanetary disks support the nebular theory by indicating the potential formation of protoplanets. Observations of circumstellar disks around young stars suggest a common occurrence in star formation. These disks mirror processes hypothesized in our solar system's early stages, showcasing key aspects of stellar and planetary formation.
Protostars surrounded by disk-shaped planes of gas and dust, known as protoplanetary disks, provide evidence in support of the nebular theory, indicating the potential formation of protoplanets within these disks.
Observations of circumstellar disks around young stars, such as those seen in the Orion Nebula, suggest a common occurrence in star formation where planets could originate from this disk material as they cool and coalesce.
These disks, ranging in size and mass, often containing enough material to potentially form a planetary system, mirror the processes hypothesized to have occurred in our own solar system's early stages, demonstrating a key aspect of stellar and planetary formation.
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