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Qicheng Zhang
cometary.org
did:plc:5esj7kfblmwhoajcamfz6xv5
The previous figure in the exact same paper (arxiv.org/pdf/2508.02934) clearly shows the inner coma closely following a 1/rho profile just like a normal comet with steady dust loss. It rolls off farther out as normal, usually from activity beginning recently + radiation pressure + dust evolution.
https://arxiv.org/pdf/2508.02934
2025-08-18T05:28:52.705Z