๐ The energy Earth receives from the sun is a crucial factor in various phenomena and the existence of life.
๐ก The amount of energy Earth radiates back into space is less than the energy it receives from the sun.
โ๏ธ Sadi Carnot's study on steam engines aimed to improve the efficiency of converting thermal energy into mechanical work.
๐ Carnot's ideal heat engine is a fully reversible engine that converts heat into the energy of a flywheel.
โ๏ธ The efficiency of the engine can be calculated by dividing the energy of the flywheel by the heat input from the hot side.
๐ก๏ธ Lord Kelvin realizes that Carnot's engine concept could be used to create an absolute temperature scale, known as the Kelvin scale.
๐ The efficiency of an ideal heat engine depends on the temperatures of the hot and cold sides.
๐ To achieve 100% efficiency in a heat engine, either infinite temperature on the hot side or absolute zero on the cold side is required.
๐ Energy spreads out over time, resulting in a decrease in usable energy and an increase in entropy.
๐ Energy packets hop randomly between two bars, creating different configurations.
๐ Heat can flow from cold to hot, but it is unlikely due to the even distribution of energy.
๐ฆ Entropy can decrease in one place by increasing it elsewhere, maintaining the overall increase in entropy.
๐ Earth is not a closed system due to the sun's energy, allowing for the existence of life.
๐ The sun provides a concentrated source of low entropy energy, which is essential for life on Earth.
โ๏ธ The increase in entropy can be observed through the conversion of higher energy photons to lower energy photons in various processes on Earth.
๐ The early universe was hot, dense, and almost completely uniform, but gravity caused matter to clump together, resulting in low entropy.
โ๏ธ As the universe expanded and cooled, matter started to clump together, converting potential energy into kinetic energy and increasing entropy.
โฑ๏ธ Stephen Hawking's discovery of Hawking radiation confirmed that black holes have entropy, with the total entropy of all black holes exceeding that of the early universe.
๐ Entropy is the key concept that explains the arrow of time, going from unlikely to more likely states.
๐ฎ The heat death of the universe is expected to happen when the energy gets spread out completely and nothing interesting will happen anymore.
๐ก Complex structures appear and thrive in the middle ground between low and high entropy, where we find ourselves.