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NASA’s GRAIL Mission


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NASA’s Gravity Recovery and Interior Laboratory (GRAIL) mission has uncovered key structural and thermal contrasts between the near side and far side of the Moon, explaining its asymmetrical appearance and volcanic history.


About GRAIL Mission

AspectDetails
Mission NameGravity Recovery and Interior Laboratory (GRAIL)
Conducted ByNASA (launched in 2011)
Spacecraft NamesTwin spacecraft: Ebb and Flow
ObjectiveMap lunar gravity variations to understand Moon’s internal structure
TechniqueMeasured changes in the distance between twin orbiters due to gravity
OutcomeProduced highest-resolution gravity map of the Moon

Key Findings of GRAIL Mission

ParameterNear Side (Facing Earth)Far Side (Hidden from Earth)
Tidal LockingAlways visible from Earth due to synchronous rotationPermanently turned away from Earth
Crust ThicknessThinner and more porousThicker, which restricts volcanic activity
TemperatureWarmer (100–200°C higher)Colder
Volcanic FeaturesDominated by dark lava plains (maria)Fewer lava flows; heavily cratered
Surface TextureSmoother due to ancient molten activityBright, rugged, heavily cratered
Thermal AsymmetrySupported by differences in historical internal heatingInhibited by thick crust and limited magma flow

Significance of the Findings

DimensionInsights Gained
GeologicalValidates theories of asymmetric volcanic history
StructuralConfirms Moon’s porous and thinner crust
EvolutionaryExplains the Moon’s Janus-faced appearance (smooth vs cratered)
Planetary ScienceEnhances understanding of tidally locked celestial bodies

Implications for India

DimensionRelevance
ISRO MissionsOffers comparative data for Chandrayaan missions
Lunar ResearchAids in identifying potential landing zones based on crust and heat maps
Science EducationEnhances curriculum with real-world planetary science applications

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