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Chandrayaans ChaSTE takes the moon’s temperature

Overview of ChaSTE Experiment

  • Chandras Surface Thermophysical Experiment (ChaSTE) is the first instrument to measure temperatures in situ near the moon’s south pole.
  • Part of the Vikram lander on Chandrayaan-3, which successfully landed on August 23, 2023.
  • A thermal probe that penetrates the lunar soil and records temperature variations.
  • Findings suggest water ice is more prevalent on the moon than previously expected.

Relevance : GS 3(Science and Technology)

ChaSTE’s Mechanism and Functioning

  • The probe is equipped with 10 temperature sensors spaced 1 cm apart along its length.
  • Uses a rotation-based deployment mechanism, different from previous hammering-based probes.
  • Once deployed, the probe measures temperature variations at different depths.
  • Penetrated up to 10 cm into the lunar soil, recording data until September 2, 2023.

Previous Failed Missions for Similar Objectives

  • Philae Lander (ESA, 2014, Comet 67P):
    • Attempted to deploy MUPUS (Multi-Purpose Sensors for Surface and Subsurface Science).
    • Failed due to bouncing on landing, preventing deployment.
  • InSight Lander (NASA, 2018, Mars):
    • Carried Heat Flow and Physical Properties Package (HP3) with a self-hammering probe (“The Mole”).
    • Low soil friction prevented it from reaching the target depth of 5 m.
    • Despite a year-long effort, temperature sensors failed to gather meaningful data.

Why ChaSTE Succeeded Where Others Failed

  • Instead of a hammering mechanism like MUPUS and HP3, ChaSTE used a rotating device to push into the soil.
  • Rotation-based deployment provided better soil penetration.
  • Successfully measured in situ lunar temperature, a feat no previous mission accomplished.

Scientific and Future Implications

  • Validates the presence of water ice in the lunar south pole region.
  • Data will be crucial for future lunar missions, especially those planning human colonization.
  • Success strengthens Indias lunar exploration capabilities and provides insights into planetary thermophysical properties.
  • May influence future deep-space exploration technologies, improving probe deployment mechanisms.

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