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.
The sun gives tremendous energy because when two hydrogen atoms meet them energy is formed and one helium atom is form
Yes the sun does give off solar energy. It also gives off heat and light energy.
The ability to live
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.
solar and maybe ultraviolet -.-
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The sun gives tremendous energy because when two hydrogen atoms meet them energy is formed and one helium atom is form
Yes the sun does give off solar energy. It also gives off heat and light energy.
Solar Energy, by definition, is energy from the Sun.
Photosynthesis uses the solar energy directly when it recieves it. It does not give the solar energy to anything else.
The ability to live
Solar panels produce electrical energy when sunlight falls directly on them. The power of sunlight is about 1400 watts in every square metre and a solar panel converts some of that into volts and amps. Solar panels need direct sunlight falling face-on to produce a significant amount of electrical power. They also produce a very small amount of power when turned towards a bright sky without direct sunlight, and an even smaller amount on a cloudy day.
About 1,000 watts per square meter of solar panel
Radioactive and solar energy (or light and heat).
The firefighters made a tremendous effort to stop the fire from spreading.Defrauding a competition is a tremendous blow to the honest participants.With a tremendous force, the moon collided with the planet and shattered into smithereens.
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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