Newton’s Laws of Motion — All 3 Laws Explained Simply (2026) Classical Mechanics · 10 min read Newton’s laws of motion — the three rules behind every push and pull Newton’s three laws of motion describe exactly how forces change the way objects move. Published in 1687, they’re still the foundation of classical mechanics —…
What Is Energy in Physics? Types, Formulas & Examples (2026) Energy & Work · 8 min read What is energy — and why it’s the one quantity that ties all of physics together Energy is the capacity to do work or cause change, and it shows up in more forms than almost any other physics…
The Work-Energy Theorem — W = ΔKE Explained (2026) Classical Mechanics · 9 min read The work-energy theorem — how pushing on something changes its energy The work-energy theorem connects two ideas you already know separately: force applied over a distance (work) and the energy of motion (kinetic energy). This guide breaks down the formula…
Gravitational Potential Energy — PE = mgh Explained (2026) Energy & Work · 8 min read Gravitational potential energy — the energy an object has because of its height Gravitational potential energy is stored energy an object has because of its position above the ground. This guide breaks down the formula PE = mgh, shows…
Momentum and Impulse — p = mv and J = FΔt Explained (2026) Classical Mechanics · 9 min read Momentum and impulse — why mass in motion is so hard to stop Momentum measures how much motion an object carries, and impulse measures how much that motion changes when a force acts over time. This…
Pressure in Fluids — P = ρgh Explained Simply (2026) Fluid Dynamics · 8 min read Pressure in fluids — P = ρgh, and why deep water pushes back harder Pressure in a fluid describes how the weight of a liquid or gas presses on anything submerged within it, and it grows deeper the further…
Heat Transfer Explained — Conduction, Convection & Radiation (2026) Thermodynamics · 9 min read Heat transfer — conduction, convection and radiation explained Heat transfer describes how thermal energy moves from a hotter object or region to a colder one, and it always happens in one of three ways: conduction, convection, or radiation. This guide breaks…
E = mc² — Mass-Energy Equivalence Explained Simply (2026) Nuclear & Modern Physics · 9 min read E = mc² — why mass and energy are the same thing Mass-energy equivalence is the idea that mass and energy are interchangeable, expressed in Einstein’s famous 1905 formula E = mc². This guide breaks down what each…
