Group of lunar meteorites throw light on the origin of basalts on the Moon: ISRO

GS Paper 1

 Syllabus: Geography/ Awareness in space.

 

Source: The Print

 Context: A team of scientists from Ahmedabad-based Physical Research Laboratory (PRL), the United States, and Japan has found a unique group of ancient lunar basaltic meteorites, suggesting a new scenario for the origin of lunar basalts.

 

More about the findings:

  • The Apollo, Luna, and Chang’E-5 missions have brought to Earth an extensive collection of mare basalts.
    • Mare basalts are formed by the partial melting of the lunar mantle, made of mostly pyroxene and olivine
  • Apollo mare basalts are highly rich in potassium, rare earth elements, and phosphorous known as Procellarum KREEP Terrane (PKT).
  • KREEP is the acronym for a place that has deposits of potassium (chemical symbol – K), rare earth elements (REE), and phosphorus (chemical symbol – P).
  • These are rich in radioactive elements that provide the heat to melt rocks resulting in KREEP-rich basalts.

  • ISRO stated that the result shows that these basalts must be a result of low-pressure melting on the Moon, similar to those in other terrestrial bodies, such as Earth and Mars.
  • They also reveal that these basalts originated from a cool, shallow, and compositionally distinct part of the lunar interior.