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Secrets of the Lunar Garden: How Meteorites Mix Cosmic Dust ⚡ экспресс

Original: "Gardening on the Moon: An Advection-Diffusion Model to Guide the Search for Supernova Debris in the Lunar Regolith"
arXiv:2604.09524 · 2026-04-10 · CC BY 4.0 · ⏱ 1 min · Exoplanets High Energy Instrumentation
Meteorites churn the Moon like gardeners, and a new model shows how stardust from ancient explosions gets scattered in the process.
Abstract

The vertical redistribution of matter in the lunar regolith—from continuously forming products of space weathering to episodic influx of isotopes from supernovae or kilonovae—remains a fundamental challenge. We propose a unified stochastic model of regolith gardening driven by a flux of impacts. The model, treating mixing as a competition between advection and diffusion, reproduces the maturity profiles of Apollo drill cores over timescales from 1.4×10⁷ to 4.5×10⁸ years. It accurately describes depth profiles of live Fe⁶⁰, pointing to an independence of supernova dust capture from native iron content and a uniform influx across the Apollo landing latitudes. The model is extended to predict lunar signals of live r-process isotopes: Pu²⁴⁴, tied to terrestrial detections, as well as I¹²⁹, Hf¹⁸², and Cm²⁴⁷ based on calculations. The Pu²⁴⁴/Fe⁶⁰ profile can help clarify the origin of Pu²⁴⁴, motivating searches in regolith samples from the Artemis mission at depths on the order of 100 cm.

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Lunar soil is a garden that meteorite impacts constantly dig over. Instead of a shovel, asteroids shake up the surface, scattering cosmic dust and bringing deep layers to the top. This cosmic “tending of the bed” goes on for millions of years, creating a uniform layer.

Scientists call this “gardening” of the lunar soil.

A new computer model has, for the first time, combined two effects of impacts: the transport and mixing of particles. Testing it with data from the Apollo missions, researchers saw how the content of iron-60—alien atoms that came from supernova explosions (studied by Zwicky)—changes with depth. It turned out that stardust is distributed evenly, without mixing with local iron. The lunar garden works so thoroughly that the soil in different spots on the planet is identical—as if it’s constantly sifted through a giant sieve. Now the model predicts where to look for traces of even rarer events—for example, plutonium-244, born in the merger of neutron stars.

By reading the depth at which such atoms lie, like the rings of a tree, we can read the history of cosmic catastrophes.

🎯 The mixed layer reaches several meters—as if a gardener dug a bed to the depth of a three-story building.

🎬 Arthur C. Clarke, in *A Fall of Moondust*, described mining rare resources on the Moon. Perhaps in the future, we’ll go there for traces of supernovae and other cosmic catastrophes.

Scientists
Enrico FermiPaul DiracSubrahmanyan ChandrasekharJames JeansAugustin-Louis CauchyChristiaan Huygens
Tags
supernova neutron star cosmic dust
Laws
Fermi–Dirac statisticsChandrasekhar limitFermi accelerationJeans instabilitylaw of conservation of momentumquadrupole radiation formula
Original: arXiv:2604.09524 · CC BY 4.0 · bridge42worlds