У нас вы можете посмотреть бесплатно Feynman Explain That the Universe Is Full of Stars but Why Is It Dark? или скачать в максимальном доступном качестве, видео которое было загружено на ютуб. Для загрузки выберите вариант из формы ниже:
Если кнопки скачивания не
загрузились
НАЖМИТЕ ЗДЕСЬ или обновите страницу
Если возникают проблемы со скачиванием видео, пожалуйста напишите в поддержку по адресу внизу
страницы.
Спасибо за использование сервиса ClipSaver.ru
#feynman #universe #space #cosmology #astrophysics #science #physics #olbersparadox #spacemystery #learnscience Why is the night sky dark? It sounds like the simplest question in the world… but answering it forces us to tear apart everything we think we know about the universe, time, and the Big Bang itself. In this video, we step into the shoes (and the legendary storytelling voice) of Richard Feynman to unravel Olbers' Paradox. Here’s the mind-blowing puzzle: If the universe is infinite and packed with infinite stars in every direction, then every line of sight should eventually hit a star. The night sky should be blazing as bright as the surface of the Sun. So why isn’t the whole sky on fire? Why aren’t we cooked right now? We’ll explore: The strange geometry of an infinite forest vs. an infinite universe Why cosmic “dust” doesn’t save the day (thanks to thermodynamics — it would just heat up and glow back at us) The killer clue: the finite age of the universe How the expansion of space stretches light and causes redshift The faint afterglow we actually do see: the Cosmic Microwave Background — the cooled-down leftover “fire” of the Big Bang Drawn directly from Feynman’s own lectures: A. Onion-shell geometry & the inverse-square law – The Feynman Lectures on Physics, Vol. I, Chapter 13 (same logic he uses for Newton’s shell theorem and gravity) B. Thermodynamics and equilibrium – Vol. I, Chapter 44 (the famous ratchet-and-pawl argument: you can’t extract work from a uniform-temperature system; dust would eventually shine as brightly as it absorbs) C. Expansion & redshift – Feynman Lectures on Gravitation (Lectures 15–16) D. The deep philosophical punchline: why we need a cold, dark sky – The Character of Physical Law (life runs on the gradient between hot Sun and cold empty space; if the whole sky were 5000°C, entropy would be maxed out and no ordered life could exist) Disclaimer: This audio is AI-generated in the persona and teaching style of Professor Richard Feynman. It is a loving tribute to his way of explaining deep physics — not an actual historical recording. Purely for education and wonder.