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We do not have complete models of planetary formation from protoplanetary disks.

open Global / Unspecified, Global WS01834
Observed exoplanet diversity challenges simple core-accretion models. High-resolution imaging of disks and improved simulations are needed.
Added by: Ian Patel
Created at: 2026-07-22T15:14:00Z
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WS01834 | World Solve | https://worldsolve.org/index.php?view=problem&id=1834

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