Australe Basin & Chandrayaan-1 [Prelims Bits]

15 Sep 2026

Tags: Prelims   Current events of national and international importance

Source: The Indian Express

  • Physical Research Laboratory (PRL), Ahmedabad researchers identified the Australe Basin on the Moon using mineralogical data from Chandrayaan-1.
  • It may be older than the South Pole–Aitken (SPA) Basin, currently regarded as the largest and oldest known lunar impact basin.

Australe Basin

  • Located in the southeastern hemisphere of the Moon, near the South Polar region.
  • Ancient basin became difficult to detect because of erosion of its rims.
  • Shows distinctive morphological, gravity and mineralogical signatures.
  • Contains 248 small basalt ponds arranged in a circular pattern.
  • Its basalts are relatively low in calcium and high in magnesium, unlike most lunar basalts.

Impact Basins

  • Formed by major asteroid/meteorite impacts on the lunar surface.
  • Much larger than ordinary impact craters; may extend hundreds of kilometres.
  • Often possess outer rims and impact-related ejecta, and may subsequently contain volcanic/basaltic deposits.
  • Around 300 impact basins are estimated on the Moon, but only about 74 had been identified according to the study cited.

South Pole–Aitken Basin

  • Located on the far side of the Moon, spanning the southern polar region.
  • Largest and oldest known lunar impact basin, formed over 4 billion years ago.
  • Its enormous age makes it important for understanding the early history of the Moon and Solar System.

Chandrayaan-1 & Moon Mineralogy Mapper

  • Chandrayaan-1: India's first lunar mission; launched in 2008.
  • Carried 11 scientific payloads, including 6 from international space agencies.
  • Moon Mineralogy Mapper (M³): imaging spectrometer contributed by NASA, used to map lunar surface mineralogy.
  • Operated in the 405–3000 nanometre wavelength range.
  • Detects mineral signatures through characteristic spectral absorption bands.

Significance

  • Material excavated by the Australe impact may have been transported towards the lunar South Pole.
  • Helps interpret the geological evolution of South Polar regions and identify potentially valuable sites for future lunar sample-return missions.
  • Relevant to proposed Chandrayaan-4 and future international lunar exploration.
  • Basalt is a dark, fine-grained volcanic rock formed from rapidly cooled lava; lunar maria are largely composed of basaltic plains.
  • Olivine, pyroxene and plagioclase are major minerals used to study the composition and geological evolution of the Moon.

Prelims Question

Q1. With reference to lunar impact basins and the Australe Basin, consider the following statements:

  1. The identification of an ancient impact basin on the Moon can rely on a combination of morphological, gravity and mineralogical signatures.
  2. Basaltic deposits within an impact basin necessarily imply that the basalt was produced by the impact event itself.
  3. The unusual magnesium-rich and relatively calcium-poor composition of Australe Basin basalts can provide clues about the Moon’s geological evolution.

Which of the statements given above are correct?

(a) 1 and 3 only
(b) 2 and 3 only
(c) 1 and 2 only
(d) 1, 2 and 3

Answer: (a) 1 and 3 only

Explanation:

  • Statement 1 is correct: Australe Basin was identified through a combination of morphological, gravity and mineralogical signatures, particularly useful where basin rims have been degraded.
  • Statement 2 is incorrect: Impact basins may subsequently contain volcanic/basaltic deposits; the presence of basalt does not mean the impact itself produced the basalt.
  • Statement 3 is correct: The relatively low-calcium, high-magnesium composition of Australe basalts is distinctive and can help reconstruct lunar geological history.