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The Moon Assembled from a Swarm of Earth's Fragments ⚡ экспресс

Original: "Formation of the Moon and Binary Asteroids"
· Nick Gorkavyi
arXiv:2512.22375 · 2025-12-26 · CC BY 4.0 · ⏱ 1 min · Exoplanets
The Moon, Charon, and binary asteroids may have formed from many small impacts, not one giant one.
Abstract

It turns out that the Moon may have been born not from one monstrous collision, but from many small 'splashes.' The early Earth was bombarded by asteroids, ejecting chunks of its mantle. Those that flew in the direction of the protolunar cloud's rotation stuck to it, like snowflakes to a snowball, while the ones going the opposite way fell back. This explains why the Moon is poor in iron and more similar to Earth's crust.

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When countless asteroids pummeled the young Earth, they tore chunks from its mantle. These fragments spiraled in a cosmic disk around the planet and, like a snowball in a blizzard, fused into the Moon.

The mantle contains little iron—so the Moon lacks it too, contrary to the expectations of the classic hypothesis where a monstrous impact supposedly mixed everything.

The same scenario applies to Pluto's moon Charon and hundreds of binary asteroids in the Solar System. Importantly, fragments moving in the same direction as the disk's rotation stayed in orbit and contributed to growth, while those coming the opposite way fell back. Thus, some material destined for the Moon scattered over Earth: we walk on rocks that once traveled through space.

🎯 The Moon is iron-poor, which long didn't fit the single-impact hypothesis: such a collision would have mixed crust and mantle material, enriching the satellite. The new multi-impact model naturally solves this puzzle.

Scientists
Emmy NoetherLudwig BoltzmannWolfgang PauliEnrico FermiPaul DiracJames Jeans
Tags
cosmic dust Standard Model Sun
Laws
Noether's theoremStefan–Boltzmann lawspin–statistics theoremFermi's golden ruleJeans instabilityCPT theorem
Original: arXiv:2512.22375 · CC BY 4.0 · bridge42worlds