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This lecture covers the concept of curvilinear motion, focusing on cylindrical and spherical coordinates, as well as the Frenet frame. It explains the tangential and normal accelerations in curvilinear motion, emphasizing their significance in trajectory analysis. The use of spherical coordinates for orbital movements, such as satellites orbiting the Earth, is also discussed, along with practical applications like laser telemetry on satellites and the laser-moon distance experiment. The lecture delves into the mathematical expressions for accelerations in the Frenet frame and the definition of angles and unit vectors in spherical coordinates. It concludes with a detailed explanation of position, velocity, and acceleration in spherical coordinates, providing a comprehensive understanding of motion analysis in different coordinate systems.