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Chandrayaan-3 data says water ice easier to find on moon than believed

Chandrayaan-3’s data reveals that water ice on the Moon is more accessible than previously thought, with potential stability even in non-polar regions. Temperature variations at Shiv Shakti Point highlight extreme lunar conditions, influencing water ice distribution and its viability for future human missions.

Relevance : GS 3(Science and Technology)

  • Temperature Variations:
    • Surface temperature at Shiv Shakti Point recorded at 82°C.
    • Just a meter away, temperature dropped to 58°C, highlighting micro-scale thermal variations.
    • Nighttime temperature plummeted to -181°C, showcasing extreme lunar conditions.
  • Implications for Water Ice Stability:
    • Previously, water ice was thought to be stable only at polar regions.
    • New data suggests higher latitude regions could also support water ice at shallow depths.
    • Slopes facing away from the Sun with an inclination greater than 14° maintain lower temperatures, allowing ice to stabilize beneath the surface.

Significance for Lunar Exploration and Human Missions

  • Water as a Crucial Lunar Resource:
    • Essential for drinking and sanitation for astronauts.
    • Potential source of rocket fuel via electrolysis to separate hydrogen and oxygen.
    • Reduces dependence on Earth-based supply missions, making long-term lunar habitation feasible.
  • Advancements in Lunar Thermophysics Understanding:
    • First-ever in-situ temperature measurements in a high-latitude lunar region.
    • Challenges previous remote-sensing estimates from NASA’s Lunar Reconnaissance Orbiter (LRO).
    • Helps in refining 3D thermophysical models to predict water ice migration and stability.

Strategic Importance for India and Global Lunar Missions

  • Indias Lunar Science Leadership:
    • Enhances ISROs credibility in space exploration.
    • Positions India as a key contributor to international lunar resource utilization efforts.
  • Support for Future Moon Bases:
    • Identifying water-rich zones eases site selection for permanent lunar habitats.
    • Facilitates fuel depots for deep-space missions (e.g., Mars exploration).
  • Collaborations & Future Missions:
    • Findings can guide Artemis Accords nations (NASA-led coalition) and other global lunar projects.
    • India could leverage this data for Chandrayaan-4 and potential manned lunar missions.

Conclusion

  • Chandrayaan-3’s findings expand the scope of lunar water availability, challenging existing assumptions.
  • The discovery of temperature fluctuations and ice stability at non-polar locations enhances lunar resource planning for long-term human presence.
  • Future studies on lunar thermophysics will further refine water ice mapping, aiding sustainable moon colonization efforts.

March 2025
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