"We are particularly interested in the phase when the distance between the Earth and the Moon was about one-third of today's distance," said Prof. Dr. Francis Nimmo of the University of California, Santa Cruz, the study's lead author. During this period, changes in the Moon's orbit caused intense tidal forces that generated significant internal heating. A similar phenomenon is observed on Jupiter's moon Io, the Solar System's most volcanically active body. Researchers believe Earth's early Moon underwent similar extreme volcanic activity.
This volcanic activity reset the geological clock of most lunar rocks. As Prof. Dr. Thorsten Kleine of the Max Planck Institute for Solar System Research explained, "Lunar rock samples don't reveal their original age but only when they were last strongly heated." However, heat-resistant zircon crystals avoided this reset in regions untouched by magma, preserving evidence of the Moon's earliest history.
The findings also address the apparent scarcity of lunar craters. "Lava from the Moon's interior could have filled the early impact basins, making them unrecognizable," said co-author Prof. Dr. Alessandro Morbidelli of the College de France. Additionally, differences between the compositions of the Moon's mantle and Earth's mantle may stem from a second melting event, which allowed some elements to escape into the Moon's iron core.
"The new results mean that all the pieces of the puzzle that previously didn't fit together now form a coherent overall picture of the Moon's formation," Kleine added.
Research Report:Tidally Driven Remelting Around 4.35 Billion Years Ago Indicates the Moon is Old
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