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We lack detailed models of dust evolution in protoplanetary disks.

open Global / Unspecified, Global WS01841
Dust growth, fragmentation, and migration shape planet formation but are complex. Combined observation and modeling efforts are needed.
Added by: Ian Patel
Created at: 2026-07-22T15:14:00Z
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WS01841 | World Solve | https://www.worldsolve.org/index.php?view=problem&id=1841

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