Moon Bell: How Gravitational Waves Unveil Lunar Secrets ✎ express

Original: "Gravitational-wave Tomography of the Moon: Constraining Lunar Structure with Calibrated Gravitational Waves"
· Han Yan, Jan Harms
arXiv:2605.13960 · 2026-05-13 · arXiv non-exclusive · independent analysis · 1 min
The Moon's tremors from gravitational waves let us 'see' its interior.

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Back in the 1960s, physicist Joseph Weber tried to catch gravitational waves using aluminum cylinders: they were supposed to tremble like tuning forks from the ripples of spacetime. Modern detectors like LIGO, built with the involvement of Rainer Weiss, register such vibrations from black hole mergers. But what if we turned the whole Moon into an antenna? When a wave passes through the satellite, it starts ringing like a bell. By analyzing the frequencies and amplitude of this ringing, much like spectroscopy uses the color of light to determine the composition of stars, geophysicists reconstruct the internal structure: where the dense rocks are and where, perhaps, a molten core hides. The precision of this 'eavesdropping' increases tenfold compared to conventional seismology. And to make the Moon ring, no explosions are needed, just cosmic cataclysms billions of light-years away.

Lunar rocks lack moisture, which on Earth quickly dampens vibrations, so moonquakes last from ten minutes to several hours, an ideal environment for 'eavesdropping' on faint gravitational-wave signals.

Scientists
Bernhard RiemannJoseph WeberKarl SchwarzschildKip ThorneRainer WeissAlbert Einstein
Concepts
lunar gravitational wave detector Moon gravitational wave spectroscopy lunar formation giant impact gravimeter weighted mean signal strength seismometer microwave resonator gw170817 waveform Jeans instability gigahertz taiji quadrupole radiation formula template membrane interferometry gravitational wave parameter estimation lisa