An advection-diffusion model of impact-driven lunar regolith gardening explains Fe-60 depth profiles from supernovae and predicts locations for r-process isotopes like Pu-244.
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Gardening on the Moon: An Advection-Diffusion Model to Guide the Search for Supernova Debris in the Lunar Regolith
An advection-diffusion model of impact-driven lunar regolith gardening explains Fe-60 depth profiles from supernovae and predicts locations for r-process isotopes like Pu-244.