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Welcome back to JEE Unfudged — where Physics finally clicks. In this lecture, we take the next big leap in Rotational Motion and enter one of the most powerful ideas in all of Physics — Angular Momentum and its Conservation. Torque told us how rotation changes. Angular momentum tells us what keeps rotating — and conservation explains why some motions look almost magical. Why does a spinning skater pull in their arms and suddenly rotate faster? Why does a planet keep orbiting without any engine? And why does JEE love asking questions where nothing changes… yet everything speeds up? 📚 In this session, we cover: 🔹 Angular Momentum (𝐋): – What angular momentum really represents – Particle vs rigid body angular momentum – Direction, vector nature & right-hand rule (no blind mugging) – Relation between torque and angular momentum (the real meaning of τ = dL/dt) 🔹 Conservation of Angular Momentum: – When and why angular momentum is conserved – Internal vs external torque (the deal-breaker concept) – Classic applications: skaters, planets, collapsing stars – High-yield JEE/NEET numericals with clean logic ⚡ You’ll also learn: – Why angular momentum is often easier than torque (if you think right) – How JEE hides conservation laws in scary-looking problems – Shortcuts to instantly spot L-conservation situations ✅ Perfect for: Class 11 students transitioning from torque to full rotational dynamics, and JEE aspirants who want to think like the examiner rather than fight equations. 🧠 Focus: Conceptual clarity. Physical meaning. Zero rote learning. By the end, angular momentum won’t feel like a formula — it’ll feel like a law of nature you can predict motion with. 🔔 Subscribe & stay tuned — rolling motion, collisions in rotation, and some beautiful problem-solving ahead. 💬 Drop your doubts below — if angular momentum ever felt mysterious, this lecture ends that mystery.