Chandrayaan-2 identifies ‘possible presence’ of ice in lunar south pole

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1. At a Glance

2. Why in the News

3. Background & Evolution

4. Core Static Facts

Item Detail
Mission Chandrayaan-2 (launched 2019)
Implementing agency ISRO (Department of Space)
Instrument used Dual Frequency Synthetic Aperture Radar (DFSAR) — L-band & S-band, fully polarimetric [S1]
Research institute Physical Research Laboratory (PRL), Ahmedabad — autonomous institute under Dept. of Space [S1][S3]
Publication npj Space Exploration (Nature portfolio journal) [S1]
Target region Lunar South Polar Region, focus on "doubly shadowed craters" inside Permanently Shadowed Regions (PSRs) [S3]
Key crater Crater of 1.1 km diameter within Faustini crater — strongest ice evidence [S1][S3]
Temperature in PSRs As low as ~-25K (extremely cold, favouring long-term ice preservation) [S3]
Number of craters studied Four doubly shadowed craters showed radar signatures consistent with possible sub-surface ice [S3]
Detection method Radar polarimetric analysis using CPR + DOP criteria [S1]

5. Multi-Dimensional Analysis

6. Recent Developments (last 12-18 months)

7. Prelims Hooks

8. Mains Relevance

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10. Common Errors / Trap Areas

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