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Season 1 Episode
- Season 1 Motion in a Straight Line
- Season 1 Derivatives
- Season 1 Integrals
- Season 1 Vectors and 2D Motion
- Season 1 Newton's Laws
- Season 1 Friction
- Season 1 Uniform Circular Motion
- Season 1 Newtonian Gravity
- Season 1 Work, Energy, and Power
- Season 1 Collisions
- Season 1 Rotational Motion
- Season 1 Torque
- Season 1 Statics
- Season 1 Fluids at Rest
- Season 1 Fluids in Motion
- Season 1 Simple Harmonic Motion
- Season 1 Traveling Waves
- Season 1 Sound
- Season 1 The Physics of Music
- Season 1 Temperature
- Season 1 Kinetic Theory and Phase Changes
- Season 1 The Physics of Heat
- Season 1 Thermodynamics
- Season 1 Engines
- Season 1 Electric Charge
- Season 1 Electric Fields
- Season 1 Voltage, Electric Energy, and Capacitors
- Season 1 Electric Current
- Season 1 DC Resistors & Batteries
- Season 1 Circuit Analysis
- Season 1 Capacitors and Kirchhoff
- Season 1 Magnetism
- Season 1 Ampère's Law
- Season 1 Induction - An Introduction
- Season 1 How Power Gets to Your Home
- Season 1 AC Circuits
- Season 1 Maxwell's Equations
- Season 1 Geometric Optics
- Season 1 Light Is Waves
- Season 1 Spectra Interference
- Season 1 Optical Instruments
- Season 1 Special Relativity
- Season 1 Quantum Mechanics - Part 1
- Season 1 Quantum Mechanics - Part 2
- Season 1 Nuclear Physics
- Season 1 Astrophysics and Cosmology
Crash Course Physics - Season 1 Episode 45 Nuclear Physics
0.00 10 minutes It's time for our second to final Physics episode. So, let's talk about Einstein and nuclear physics. What does E=MC2 actually mean? Why is it so useful to us as physicists and humans? In this episode of Crash Course Physics, Shini sits down to go over the basics of it all.
