Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.
Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.
Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.
Nuclear fusion. Most stars (the so-called "main sequence" stars) convert hydrogen-1 into helium-4.
Stars produce energy from the fusion of hydrogen into helium during the main sequence stage of their life cycle. This is when a star is stable and balanced, and the fusion of hydrogen into helium in its core generates the energy that makes the star shine.
The two competing forces in a star are gravity, which tries to collapse the star under its own weight, and nuclear fusion, which generates energy and causes the star to expand outward. These forces balance each other to maintain a stable, long-lived star.
A very bright object that generates far more energy than a typical star is a quasar. Quasars are supermassive black holes at the centers of distant galaxies, surrounded by accreting material that emits enormous amounts of energy, often outshining entire galaxies. This energy is produced as matter falls into the black hole, heating up and emitting radiation across the electromagnetic spectrum. Their extreme luminosity makes them some of the brightest objects in the universe.
In a star, energy changes primarily occur through nuclear fusion, where hydrogen nuclei fuse to form helium, releasing vast amounts of energy in the form of light and heat. This process generates the energy that powers the star and creates pressure to counteract gravitational collapse. As the star ages, it undergoes changes in fusion processes, eventually fusing heavier elements, which alters its energy output and leads to different stages of stellar evolution, such as red giants or supernovae. Ultimately, energy changes in a star reflect its life cycle and the transformations within its core.
This could be a star, such as our sun, which generates energy through nuclear fusion in its core. Stars are composed mostly of hydrogen and helium gases. When hydrogen atoms combine under immense pressure and heat, they release energy in the form of light and heat.
A star.
A protostar generates energy by friction whereas a main sequence star generates energy by fusion.
Hydrogen
A protostar generates energy by friction whereas a main sequence star generates energy by fusion.
A supernova explosion releases greatly more energy than our Sun in its entire lifetime.
Nuclear fusion is the primary process in stars that generates energy by fusing lighter elements into heavier ones. Gravitational contraction is another process where a star generates energy by converting gravitational potential energy into thermal energy. Both processes contribute to maintaining the star's internal thermal pressure.
A large ball of gas that generates its own energy is called a star. Stars achieve this by undergoing nuclear fusion reactions in their cores, converting hydrogen into helium and releasing tremendous amounts of energy in the process.
Generator generates electrical energy. It uses mechanical energy and transforms it.
A Horizontal Branch star generates energy through the fusion of helium into carbon and oxygen in its core. This fusion process releases energy in the form of light and heat, which provides the necessary support to balance the star against gravitational collapse.
No, the sun is not a planet. It is a star, specifically a medium-sized main sequence star that generates energy through nuclear fusion in its core. Planets orbit stars, including our sun.
By nuclear fusion - converting hydrogen-1 into helium-4.
It shines (it generates light).