Lunar Heating: How Tides Prolonged Earth's Magma Ocean express

Original: "Onset of habitable conditions on the Hadean Earth set by feedback between tides and greenhouse forcing"
arXiv:2511.00952 · 2025-11-02 · CC BY 4.0 · 1 min
Lunar tidal heat stretched the life of the molten rock ocean to half a billion years, altering Earth's early atmosphere.

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After the Moon's birth, Earth resembled a sizzling lump of dough: a continuous liquid magma and a dense shroud of gases. The Moon acted like a giant spoon, constantly kneading this lump with its gravity. Friction generated heat, delaying cooling. Scientists calculated: depending on tidal strength and oxygen content inside, the ocean of molten rock lasted from 30 to 500 million years. When oxygen was scarce, carbon turned into carbon monoxide. With an excess, water vapor enveloped the planet like a kitchen towel, holding in the heat. Weak tides added gases rich in hydrogen — ammonia and hydrogen sulfide. Eventually, Earth, like dough on a table, reached equilibrium: as much energy came in as went out. Such periods lasted up to 320 million years. If tidal friction had been weaker, the ocean would have solidified in 30 million years, and solid crust would have appeared half a billion years earlier: this could have changed the planet's entire history.

Earth's magma ocean existed longer than the time from the first dinosaurs to today — nearly half a billion years.

Scientists
Daniel BernoulliLeonhard EulerArchimedesJames Jeans
Concepts
tidal heating magma ocean lunar formation giant impact hydrogen atmosphere marine heatwave seasonal forcing tidal migration greenhouse effect Indian Ocean Dipole global warming climate Atlantic multidecadal oscillation oxidation habitability annual cycle monsoon titan europa wind stress tropical cyclone