Why Does The Sun SHINE If It Isn't Burning? What I Found Will Change How You See The Sky

🔗 https://oxadow.com/?v=HgdXsIG-5yU — The Physics of Everything: gravity, light, time, quantum mechanics and the invisible world of electromagnetism, explained step by step. Explore all three illustrated PDF books in The Complete Library.Uploaded 17-10-26🔗 https://oxadow.com/mail/?v=HgdXsIG-5yU — The Physics Letter: interesting physics news, remarkable discoveries and clear explanations, delivered to your inbox. Free to join.The Sun has no flames and no oxygen to burn, yet it has shone for 4.5 billion years. The smartest scientists of the 1800s tried to explain it and were wrong by a factor of a million. The real answer involves missing weight, a "forbidden" quantum trick, and a ghost particle that's passing through your body right now. By the end, you'll never look at sunlight the same way.00:00 The Sun is not on fire, so what is it eating? 02:01 The secret inside a burning match 09:12 The clue nobody expected: atoms that weigh too little 16:35 Why protons refuse to touch 19:54 The ball that goes through the hill 30:44 Why the Sun isn't a hydrogen bomb 33:49 Sunlight older than farming 37:04 The ghost passing through your thumb 43:36 The Sun loses 4 million tonnes every second 45:00 You are made of dead starsSOURCESRichard P. Feynman, Robert B. Leighton, Matthew Sands, The Feynman Lectures on Physics, Vol. I (1963), Chapter 3 "The Relation of Physics to Other Sciences" (Section 3-4, Astronomy) and Chapter 4 "Conservation of Energy"The Feynman Lectures on Physics, Vol. III (1965), Chapter 1 "Quantum Behavior"Richard P. Feynman, The Character of Physical Law (1965), Chapter 6 "Probability and Uncertainty: The Quantum Mechanical View of Nature"William Thomson (Lord Kelvin), "On the Age of the Sun's Heat," Macmillan's Magazine (1862)Albert Einstein, "Does the Inertia of a Body Depend Upon Its Energy Content?" Annalen der Physik 18 (1905)Arthur S. Eddington, The Internal Constitution of the Stars (1926), chapter on the source of stellar energyCecilia H. Payne, Stellar Atmospheres, Harvard Observatory Monographs No. 1 (1925)George Gamow, "Zur Quantentheorie des Atomkernes," Zeitschrift für Physik 51 (1928)Robert d'E. Atkinson and Fritz G. Houtermans, Zeitschrift für Physik 54 (1929)Hans A. Bethe and Charles L. Critchfield, "The Formation of Deuterons by Proton Combination," Physical Review 54 (1938)Hans A. Bethe, "Energy Production in Stars," Physical Review 55 (1939)Raymond Davis Jr., Don S. Harmer, Kenneth C. Hoffman, "Search for Neutrinos from the Sun," Physical Review Letters 20 (1968)John N. Bahcall, Neutrino Astrophysics (1989), Cambridge University Press⚠️ 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]
Learn more about your ad choices. Visit megaphone.fm/adchoices