Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
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2026 2verdicts
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Statistical analysis of 1155 protoplanetary disks shows only 1.2% are formally gravitationally unstable, likely because observations underestimate their masses.
citing papers explorer
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Dust distribution in circumstellar disks harboring multi-planet systems. II. Super-thermal mass planets
Multi-planet systems produce size-dependent dust traps, asymmetric structures, and eccentric orbits that can hide gaps in synthetic ALMA images and limit grain growth.
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Investigation of gravitational stability of protoplanetary disks based on statistical analysis of their masses
Statistical analysis of 1155 protoplanetary disks shows only 1.2% are formally gravitationally unstable, likely because observations underestimate their masses.