Я купил новый микрофон и звук стал на порядок лучше, мне прямо нравится даже в наушниках. Всё-таки техника очень сильно определяет результат, тут прям как с фотографами, ха-ха )
Выпуск получился длиннее обычного, но сокращать на монтаже не стал. Затронул важный и даже несколько болезненный для меня вопрос: как выходит, что унылые мобильные игры без геймплея и сюжета зарабатывают в десятки раз больше, чем крутые высокобюджетные блокбастеры на консолях и ПК.
И у меня очень давно зрела в голове гипотеза на эту тему. Лично я прям очень верю в неё, хотя кому-то может показаться фантастикой.
#podcast
P.S. На Яндекс.Музыке как обычно с опозданием в несколько часов, скорее всего утром, пока всё синхронизируется.
🪐 The mysterious "dark flow" observed in the movement of galaxy clusters like Abell 3627 suggests that something unseen—possibly related to dark matter or dark energy—is pulling vast regions of the universe in the same direction. This large-scale motion, detected using X-rays from hot gas in clusters, remains unexplained by normal gravity and hints at the hidden forces shaping the cosmos beyond what we can directly observe. ✨
#darkmatter⚡#universe⚡#galaxyclusters⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#cosmos⚡#space
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🪐 Deep in the Coma Cluster, a packed group of over 1,000 galaxies, astronomers have measured how dark energy—a mysterious force causing the universe to expand faster over time—stretches the space between galaxies. Observations show that the distance between massive galaxies in the Coma Cluster grows not just from their own motion, but because dark energy is steadily pushing the entire cosmic structure apart. ✨
#darkenergy⚡#galaxyclusters⚡#cosmology⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The Bullet Cluster, found in the constellation Carina, provides some of the clearest real-world evidence for dark matter—a mysterious, invisible substance making up most of the universe’s mass. When two galaxy clusters crashed together, X-ray images showed that most of the visible matter stayed at the center, but gravity maps revealed most of the mass had moved ahead, proving something unseen—dark matter—was driving the collision's aftermath. ✨
#darkmatter⚡#galaxyclusters⚡#carina⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The cosmic microwave background holds a hidden fingerprint—tiny temperature fluctuations mapped in exquisite detail by satellites like Planck reveal how the first stars and galaxies, such as those in the ancient cluster Abell 2744, grew from initial small ripples in the early universe. These faint variations, just millionths of a degree, became the seeds around which all the cosmic structures we see today first assembled. ✨
#cosmicmicrowavebackground⚡#earlyuniverse⚡#galaxyclusters⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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🪐 The cosmic microwave background contains faint "Sunyaev-Zel’dovich effects," which happen when the ancient microwave light passes through hot gas in galaxy clusters like the Bullet Cluster. This process boosts the energy of some photons (light particles), leaving tiny shadows in the background glow—allowing astronomers to map both distant galaxy clusters and the hot plasma between galaxies by studying these subtle marks in the oldest light in the universe. ✨
#microwave⚡#background⚡#galaxyclusters⚡#plasma⚡#nasa⚡#galaxy⚡#stars⚡#astronomy⚡#universe⚡#cosmos⚡#space
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