it was born with a name PRECIOUS
The energy in a star is generated by nuclear fusion.
The main source of a star's light is nuclear fusion in its core. This process involves the conversion of hydrogen into helium, releasing energy in the form of light and heat. The energy generated by nuclear fusion is what makes stars shine brightly.
A star gets its energy from nuclear fusion reactions that occur in its core. These reactions fuse lighter elements, such as hydrogen, into heavier elements, releasing energy in the process. This energy is what fuels a star's brightness and heat.
The outward force in a star is caused by the pressure generated from the energy released during nuclear fusion in its core. This pressure counteracts the force of gravity pulling inward, creating a stable equilibrium that allows the star to maintain its shape and balance.
Thermonuclear fusion in the core of the star heats the material of the star. A series of complex energy transfer mechanisms transport the heat from the core to the photosphere of the star. The photosphere then emits electromagnetic radiation.
Energy in a star's core is generated through nuclear fusion, where hydrogen atoms combine to form helium releasing a massive amount of energy in the process. The extreme temperature and pressure in the core of a star make this fusion process possible, sustaining the star's energy output.
The energy in a star is generated by nuclear fusion.
In the Sun's core.
Heat energy.
In the Sun's core.
At the core where the fuel is burning
The main source of a star's light is nuclear fusion in its core. This process involves the conversion of hydrogen into helium, releasing energy in the form of light and heat. The energy generated by nuclear fusion is what makes stars shine brightly.
The sun's energy is generated at its core through the process of nuclear fusion, where hydrogen atoms fuse together to form helium, releasing immense amounts of energy in the form of heat and light. This energy then travels through the sun's layers before being emitted as sunlight into space.
Yes.
In a star, energy from fusion moves outward from the core through radiation and convection. In the core, where fusion takes place, high-energy photons are generated and slowly diffuse outwards. In the outer layers, energy is carried by convection, where hot plasma rises and cooler plasma sinks, creating a cycle that transports energy towards the surface of the star.
The convection zone in a star like the Sun is located just beneath the photosphere. It is the layer where energy generated in the star's core is transported to the surface via convection currents, providing the energy needed for the star to shine.
In a star, energy is primarily transferred through radiation in the outer layers and through convection in the inner layers. In the core, where nuclear fusion occurs, energy is generated and eventually travels outward through the layers by radiation, heating up the outer layers.