Chang'e-6 Samples Point to Sideways Magma Flows Behind Moon's Two Faces
First-ever samples from the Moon's far side suggest tidal locking triggered a heat imbalance that pushed magnesium-rich magma sideways, building the far side's thicker crust, Nanjing University researchers propose.
Step by step
- 1
Magma ocean cools evenly on both sides
- 2
Moon becomes tidally locked to Earth
- 3
Near side receives more tidal heating
- 4
Hot magma flows sideways toward far side
- 5
Far side gains thicker, magnesium-rich crust
The Moon shows two very different faces. The side facing Earth is covered in dark volcanic plains, while the far side, never visible from Earth, has rugged, heavily cratered highlands, a much thicker , and far fewer volcanic plains. Scientists have long puzzled over why the Moon's near and far sides look, and are built, so differently.
New research on samples from China's Chang'e-6 mission may help explain the difference. In 2024, Chang'e-6 returned the first-ever samples collected from the Moon's far side. A team led by Professor Hejiu Hui of Nanjing University compared these far-side rocks with near-side material earlier returned by the Apollo missions and China's Chang'e-5 mission. The findings were published in the journal National Science Review.
The comparison suggests the Moon's , the thick rock layer beneath the crust, is broadly similar on both sides: chemical signatures in far-side rocks matched those in near-side Apollo samples, the researchers reported. Far-side anorthosite rocks contained more magnesium than similar near-side samples, showing the far side's crust is more magnesium-rich than the near side's. The near side, by contrast, holds higher concentrations of potassium, rare earth elements and phosphorus.
The researchers propose that this split emerged after the Moon became to Earth, meaning the same side always faces it. Before that, they suggest, the Moon's early ocean of molten rock cooled evenly on both sides. Once tidal locking set in, the model proposes, the near side received more tidal heating than the far side, creating a temperature difference between the hemispheres. That gradient, the team suggests, may have driven hot magma sideways from the near side toward the far side, carrying magnesium-rich material and building the far side's thicker crust.
According to the model, this sideways flow would also have pushed residual melted rock toward the near side, leaving the far side with only thin layers of the potassium-, rare-earth- and phosphorus-rich material, the researchers reported.
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The story so far
- China Achieves Two-Way Laser Communication With a Satellite in Lunar Orbit
- NASA Funds 'Slingshot' Concept to Scout Minerals on Moon, Asteroids and Phobos
- Moon May Have Formed in Just Five Hours After Giant Impact, Simulations Suggest
- The Moon Will Hide Jupiter in Broad Daylight Today, Here's How to Watch
- China Postpones Chang'e-7 Moon Mission After Rocket Was Already on the Pad
- NASA's Artemis II Commander and Pilot Move to Emeritus Status
- Chang'e-6 Samples Point to Sideways Magma Flows Behind Moon's Two Faces
