Recent measurements from the Chandrayaan-3 mission reveal surprising variations in surface temperature on the moon's poles.The surface temperature discrepancies are attributed to factors like topography, thermal conductivity, and sunlight exposure.The moon's surface is covered with a 'fluff layer' that hinders heat conductivity, leading to significant temperature variations.Subsurface temperature plays a crucial role in the accumulation and retention of water on the moon.The Chandrayaan-3 data suggests that water ice might also be present outside the lunar poles due to suitable topographical features.This new study highlights the complexity of water accumulation and storage on the moon.Improved models for understanding water-ice migration and stability are being developed based on Chandrayaan-3 mission data.The research emphasizes the importance of firsthand data collection to enhance our knowledge of lunar water distribution.The presence of water under the moon's poles and surrounding regions signifies potential implications for future lunar exploration and research.Further investigations are essential to determine the exact amount and distribution of water ice on the moon.