The sun gives tremendous energy because when two hydrogen atoms meet them energy is formed and one helium atom is form
Gravity compresses the Sun up to a point at which it has a high temperature and pressure in its center. This causes the nuclear fusion, which is the source of energy of the Sun.
A star is a body of gas that gives off tremendous amounts of radiant energy in the form of light and heat through nuclear fusion reactions in its core.
Nuclear fusion in the sun's core causes it to give off light and heat. This process involves the merging of hydrogen atoms to form helium, releasing a tremendous amount of energy in the form of light and heat.
Stars give off heat and light through the process of nuclear fusion in their cores. During this process, hydrogen atoms fuse to form helium, releasing a tremendous amount of energy in the form of heat and light. This energy is what sustains a star and allows it to shine brightly.
Yes! The energy they give off have an equivalent mass, and this mass is lost to the star. This follows from (a) the equivalence between mass and energy, and (b) conservation of mass. As an example, our Sun, which gives off tremendous amounts of light, loses 4 million tonnes a second, just through the light that leaves the Sun - that is, apart from any solar wind.
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Hydrogen bombs give off a tremendous amount of energy in the form of heat, light, and radiation when they detonate. This energy release is the result of the nuclear fusion process that occurs in the bomb's core.
Uranium-235 and plutonium-239 are the primary fuels used in nuclear reactors to generate energy through atomic fission. When these fuels undergo fission, a tremendous amount of energy is released in the form of heat, which is used to produce electricity.
Gravity compresses the Sun up to a point at which it has a high temperature and pressure in its center. This causes the nuclear fusion, which is the source of energy of the Sun.
A star is a body of gas that gives off tremendous amounts of radiant energy in the form of light and heat through nuclear fusion reactions in its core.
The Sun fuses hydrogen to create helium which makes tremendous amounts of energy. Thus producing sunlight.
To "eat their heads off" means to eat a tremendous amount of food.
Nuclear fusion in the sun's core causes it to give off light and heat. This process involves the merging of hydrogen atoms to form helium, releasing a tremendous amount of energy in the form of light and heat.
Stars give off heat and light through the process of nuclear fusion in their cores. During this process, hydrogen atoms fuse to form helium, releasing a tremendous amount of energy in the form of heat and light. This energy is what sustains a star and allows it to shine brightly.
True! Im pretty sure!
Yes! The energy they give off have an equivalent mass, and this mass is lost to the star. This follows from (a) the equivalence between mass and energy, and (b) conservation of mass. As an example, our Sun, which gives off tremendous amounts of light, loses 4 million tonnes a second, just through the light that leaves the Sun - that is, apart from any solar wind.
Infrared light doesn't "give off" energy; in this case, it IS the energy.