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Moon contraction study reveals thousands of fracture edges

A new study published in The Planetary Science Journal reveals that the Moon is slowly contracting, a process that creates seismic risks for future lunar missions. Led by planetary scientist Thomas R. Watters, the research utilized high-resolution imagery from the Lunar Reconnaissance Orbiter Camera (LROC) to map approximately 8,900 fracture edges in the lunar highlands and over 2,600 small ridges in the dark mare plains.

These fracture edges, characterized by an asymmetrical profile with a steep front and a gentle slope, form when the lunar crust shifts during contraction. The study estimates the Moon's radius has decreased by approximately 45 meters (with calculations ranging between 42 and 46 meters). This shrinkage occurs at an extremely slow rate of roughly 6 to 11 centimeters per million years, or about 0.1 micrometers per year.

The findings present a scientific mystery, as classical thermal cooling models predict a much more significant contraction of between 750 meters and 1.1 kilometers. The researchers noted that the absence of older, heavily weathered fracture edges in the highlands contradicts theories suggesting a much longer period of contraction.

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Lunar Reconnaissance Orbiter Camera · Moon · The Planetary Science Journal · Thomas R. Watters

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