We use privacy-friendly product analytics (no session recording, PII masked) to improve OpenStem. Load analytics? Privacy Policy
Explore STEM Content
Search the community's STEM library — free to study, yours to make your own.
Physics
Mechanics, electromagnetism and quantum on openstem — flashcards, notes, quizzes, plots and sketches shared by the community. Study free, or clone anything into your library.
Stretchy or not Some things stretch easily: a rubber band, a spring, an elastic waistband. Pull them and they get longer, then snap back once you let go. A rock, a pencil or a spoon barely move however hard you push. What elastic actually m
Curve the surface, change the reflection A flat mirror bounces light back evenly, so your reflection is the same size and the right way up. Curve the surface and the rays get pulled together or pushed apart instead. Concave: curving inward
One law, three centuries of orbits Gravitational potential energy Circular orbits Gravity supplies precisely the centripetal force the circle demands. Set them equal: Escape velocity Set total mechanical energy to zero: just enough kinetic
Stars shouldn't burn, classically The Sun's core sits near 10⁷ K, giving thermal energies around 1 keV. The Coulomb barrier between two protons is measured in MeV. Classically, nothing fuses. It happens anyway, by tunnelling. The Gamow peak
Physics
Physics · L5 · Nuclear Astrophysics: How Stars Build the Elements
Some materials let heat rush through, some don't Heat is always moving from warmer things to cooler ones. But materials differ enormously in how fast they let it through. Why metal feels cold Trapping warmth Using both on purpose A cooking
Reflection: one rule Angle of incidence equals angle of reflection, both measured from the NORMAL, not from the surface. Refractive index Snell's law Worked: air into water at 40°. Total internal reflection Going the other way, from dense t
Physics
Physics · L3 · Reflection, Refraction & Snell's Law
The sum of currents entering a node equals the sum of currents leaving it — charge cannot accumulate at a node in a steady circuit. It is a direct statement of conservation of charge.
Gravity isn't a force here In GR, spacetime is a four-dimensional manifold carrying a metric tensor g_μν. Mass and energy curve it. Free particles then move as straight as they can through the curved geometry, and you call the result gravit
Physics
Physics · L5 · General Relativity: Metric, Geodesics, and the Line Element