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Can the Moon have its own moon? ⚡ экспресс

Original: "A revision of the lifetime of submoons: tidal dynamics with the Euler-Lagrange equation"
arXiv:2510.10344 · 2025-10-11 · CC BY 4.0 · ⏱ 1 min · Exoplanets
Research shows: moons can have their own moons, and some of them could be habitable.
Abstract

Within a constant geometric lag model for tidal dissipation, the Euler-Lagrange equations were solved numerically, and the parameter space of star–planet–moon–submoon systems with submoons massive enough for life was explored. Earth could hold onto asteroid-mass submoons (~10^15 kg), while a submoon at the upper limit (~4.6·10^17 kg) would push the Moon ~30% farther from its current orbit. For the warm Jupiter Kepler-1625b: a submoon with ~10% of the moon's mass is stable if the moon is at a distance of 67 R_p (instead of 40 R_p). Giant submoons (1.8 M⊕) are stable with a wide moon orbit (>100 R_p). At a mass of 0.5 M⊕ (a condition for an atmosphere and tectonics), the number of stable configurations drops. A stability minimum is found at ~0.1 M⊕, explained by the balance of tidal forces and the Roche limit. If the formation of submoons in such systems tends toward intermediate masses, habitable submoons may be rare.

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The Moon can have its own tiny moon — like a nesting doll, but in space. The outer doll is a planet, the middle one is a moon, the inner one is a small moon-satellite, or submoon. Ньютон showed that all bodies attract each other, and gravity holds them together. But gravity is not uniform: on the near side of the satellite it's stronger than on the far side. This difference creates tidal forces that squeeze and stretch the object, like clay. If a submoon gets too close to the main moon, it gets torn apart — possibly just like the dusty ring around Saturn's moon Rhea was torn apart. искривление пространства-времени explains this as a deformation of space itself.

Calculations show: Earth could host an asteroid-sized submoon. If it were bigger, the Moon would move 30% farther away from us. For экзопланеты Kepler-1625b — a warm gas giant — submoons could be as large as Earth. For life to arise on such a moon, жидкая вода, an atmosphere, and plate tectonics are needed, meaning the mass should be about half of Earth's. But precisely at that 'half' mass the orbit becomes unstable — a paradox that might make habitable submoons extremely rare.

🎯 Saturn's moon Rhea may have once had a dusty ring — almost submoons.

Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Tags
exoplanet spacetime curvature Water
Laws
Doppler effectKepler's third lawKepler's first lawequivalence principleKepler's second lawLense–Thirring effect
Original: arXiv:2510.10344 · CC BY 4.0 · bridge42worlds