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Scientists Uncover Critical Reaction Behind Unique Lunar Rock Formation

The discovery, involving the exchange of iron in magma with magnesium in surrounding rocks, explains the presence of titanium-rich 'high-Ti basalts' on the moon's surface.

  • Scientists have discovered a critical reaction that occurred deep within the moon 3.5 billion years ago, leading to the creation of a unique rock type distributed across the lunar surface.
  • The reaction involved the exchange of iron in magma with magnesium in surrounding rocks, changing chemical and physical properties in one of the three components of magma.
  • High concentrations of titanium (Ti) on certain parts of the lunar surface have been recognized since the NASA Apollo missions, and these 'high-Ti basalts' are widespread across the moon.
  • Until now, models have been unable to recreate magma compositions that match essential chemical and physical characteristics of the high-Ti basalts, particularly their low density.
  • The team used high-temperature laboratory experiments and spectroscopic examinations of actual high-Ti basalts returned from the moon to solve this puzzle.
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