The Moon Is Older Than Its Rocks: Why 4.35 Billion Years? ✎ express

Original: "Tidal Heating of the Lunar Magma Ocean: Reconciling an Old Moon with a Young Solidification"
arXiv:2511.19946 · 2025-11-25 · arXiv non-exclusive · independent analysis · 1 min
Tidal heating from Earth hid the Moon's true birth date — now we know why lunar samples are 4.35 billion years old.

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Lunar rocks brought a puzzle: their age is 4.35 billion years, but the Moon itself should have appeared 150 million years earlier. The missing time is hidden in tidal heating. When the Moon hung closer to Earth, Earth's gravity acted like tireless hands: it constantly kneaded and bent the satellite. From this, heat was generated inside — just like in a rapidly bending wire. The nature of these forces was unraveled by Isaac Newton. For a full 150 million years, the lunar ocean of magma would not solidify, kept warm by this cosmic workout. But as soon as the magma began to thicken, tidal heating weakened, and the last drops of liquid rock snapped into solid in an instant. That is the moment we mistakenly consider the Moon's birth. In reality, lunar rocks merely recorded the final exhalation of its internal heat. This also explains the difference between the near and far sides of the Moon: cooling happened unevenly. And today, the same hellish heating melts the interior of Io — Jupiter's moon, making it the most volcanic body in the system.

The two sides of the Moon are like two different worlds: the near side has smooth dark 'seas', while the far side is a chaos of mountains and craters. It turns out tidal heating is to blame: it made the magma solidify unevenly.

Scientists
Albert EinsteinRobert H. DickeJosef LenseWilliam UnruhEdward WittenJuan Maldacena
Concepts
lunar formation giant impact magma ocean tidal heating tidally locked Atlantic multidecadal oscillation solidification titan oxidation tidal migration europa age of the universe red giant young star metals stellar age marine heatwave Pacific decadal oscillation planetary embryo early universe star formation metallicity in stellar evolution