A protoplanetary disk as observed by ALMA (left), and a protoplanetary disk during planetary migration, as obtained from the ATERUI II simulation (right). The dashed line in the simulation represents the orbit of a planet, and the gray area indicates a region not covered by the computational domain of the simulation. CREDIT: Kazuhiro Kanagawa, ALMA(ESO/NAOJ/NRAO)

Simulations Provide Clue To Missing Planets Mystery

Forming planets are one possible explanation for the rings and gaps observed in disks of gas and dust around young … Continue reading Simulations Provide Clue To Missing Planets Mystery

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