Central Idea
- As Chandrayaan-3 succeeded on its lunar soft landing, its six-wheeled rover begins a journey to unravel the mysteries of the Moon.
- With its payloads and instruments, the mission aims to build on the knowledge gained from its predecessors, investigating lunar quakes, mineral compositions, and water-ice presence.
Chandrayaan-3 Mission: Journey post soft landing
- Rover’s Arrival: The 26-kg rover, launched from the Chandrayaan-3 lander, is poised to cover up to 500 meters, commencing its lunar exploration.
- Duration: The lander and rover, equipped with six payloads, are primed to collect valuable data during the single lunar day (equivalent to 14 Earth days) of operation.
- Studying Lunar Quakes: The Chandrayaan-3 mission seeks to deepen insights into lunar quakes, expanding on the knowledge gained from its predecessors.
- Mineral Composition: The rover’s endeavors include examining the mineral compositions of the Moon’s surface, shedding light on its geological history.
- Electrons and Ions Study: The Radio Anatomy of Moon Bound Hypersensitive ionosphere and Atmosphere (RAMBHA) payload aims to study the behavior of electrons and ions near the lunar surface over time.
- Thermal Properties: Chandra’s Surface Thermo physical Experiment (ChaSTE) will explore the thermal characteristics of the Moon’s Polar Regions.
- Lunar Seismic Activity: The Instrument for Lunar Seismic Activity (ILSA) endeavors to measure lunar quakes and study the Moon’s crust and mantle composition.
- Laser Retroreflector Array: A passive experiment by NASA, the LASER Retroreflector Array (LRA), will serve as a target for precise laser measurements in future missions.
- Chemical Insights: The LASER Induced Breakdown Spectroscope (LIBS) aboard the rover is designed to identify the chemical and mineral composition of the lunar surface.
- Elemental Analysis: The Alpha Particle X-ray Spectrometer (APXS) aims to analyze elements such as magnesium, aluminium, silicon, potassium, calcium, titanium, and iron in lunar soil and rocks.
- Mineral Mapping: The CLASS X-ray Fluorescence experiment, covering nearly 95% of the lunar surface, offers detailed mineral mapping. Oxygen-rich minerals hold potential for future missions as fuel resources.
Earlier Chandrayaan: Pioneering discoveries
- Water Unveiled: Chandrayaan-1 played a pivotal role in uncovering the presence of water and hydroxyl molecules in the Moon’s atmosphere and surface, particularly in its southern polar regions.
- Subsurface Water-Ice: Payloads like mini-SAR and Moon Mineralogy Mapper (M3) detected subsurface water-ice deposits within craters near the lunar South Pole.
- Lava Tubes for Habitability: Terrain mapping on Chandrayaan-1 unveiled buried lava tubes that could provide protective habitats for humans, shielding against radiation and extreme lunar conditions.
- Magma Ocean Hypothesis: M3 payload data suggested the possibility of a past magma ocean on the Moon, pointing to its formation and evolution.
- Active Moon: Contrary to previous notions of lunar inactivity, Chandrayaan-1 revealed dynamic lunar processes, including volcanic activity evidenced by lava channels and vents less than 100 million years old.
- Surface-Exosphere Interaction: Measurements indicated that the lunar surface interacts with the exosphere, evident in the emission of carbon dioxide and other gases.
- Solar Mysteries: The Solar X-Ray Monitor on Chandrayaan-2’s orbiter observed solar microflares outside active regions, providing insights into coronal heating mysteries.
Conclusion
- Chandrayaan-3’s scientific journey exemplifies India’s dedication to unraveling the Moon’s mysterious nature.
- As data pours in from its payloads and instruments, the mission builds upon its predecessors, propelling our understanding of lunar geology, composition, and mysteries.
