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Protoplanetary disks are rotating disks of gas and dust around young stars in which planets can form.
supportedProtoplanetary disks are rotating disks of gas and dust around young stars in which planets can form. Disk physics links star formation to planet formation and helps explain why planetary composition varies with distance from a star.
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Protoplanetary disks are rotating disks of gas and dust around young stars in which planets can form.
supportedDust grains collide and sometimes stick, forming progressively larger aggregates.
supportedYoung stars are commonly observed with infrared excess emission produced by warm circumstellar dust.