The SUN Should Have Died Billions of Years Ago — Feynman's Proof скачать в хорошем качестве

The SUN Should Have Died Billions of Years Ago — Feynman's Proof

The Sun burns 400 million tons of hydrogen every second. By every 19th-century calculation, it should've run out of fuel before the dinosaurs even existed. Lord Kelvin himself declared the Sun couldn't be more than 30 million years old — and his math was flawless. So what was he missing? In this video, we trace a puzzle that consumed physicists for over a century: why does the Sun still shine? Drawing from Richard Feynman's treatments of nuclear physics, quantum tunneling, and stellar energy in The Feynman Lectures on Physics and The Character of Physical Law, this lecture reconstructs the mystery step by step — from the failure of chemical energy, through Lord Kelvin's gravitational bet, to the shocking quantum accident that makes sunshine possible. 📚 SOURCES: Richard Feynman, The Feynman Lectures on Physics, Volume I, Chapter 3: "The Relation of Physics to Other Sciences" (1963) Richard Feynman, The Character of Physical Law, Chapter 2: "The Relation of Mathematics to Physics" (1965) Richard Feynman, QED: The Strange Theory of Light and Matter, Princeton University Press (1985) George Gamow, The Birth and Death of the Sun, Viking Press (1940) Arthur Eddington, The Internal Constitution of the Stars, Cambridge University Press (1926) John Gribbin, Stardust: Supernovae and Life, Yale University Press (2000) 🎙️ CREDITS: Script: AI-generated in the teaching style of Richard Feynman Narration: Synthetic TTS voice Production: The Physics Confessional TIMESTAMPS: 00:00 – A star that should already be dead 02:18 – What if the Sun were made of coal? 05:45 – Lord Kelvin's gravitational contraction theory 09:30 – Geologists vs. physicists: the 19th-century showdown 12:10 – Radioactivity blindsides Lord Kelvin 14:50 – Nuclear fusion and Einstein's missing mass 17:40 – The Coulomb barrier problem 20:25 – Why the Sun's core isn't hot enough 23:00 – Quantum tunneling saves the Sun 25:30 – A billion years of failure per proton 27:45 – What Kelvin couldn't have known — and what we might be missing What surprises you more — that the Sun almost shouldn't work, or that its survival depends on a quantum accident happening trillions of times per second? ⚠️ WARNING: [This video is AI-generated (synthetic voice and visuals). It is an original, fictional lecture inspired by Richard Feynman's teaching style and public ideas, and is not an authentic recording, endorsement, or statement by Richard Feynman or his estate. Any resemblance is for educational/creative purposes]