In GCSE Physics you study nuclear fusion, where light nuclei join together and release enormous energy, similar to the reactions powering our Sun and other stars.
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You can find more about this topic by visiting BBC Bitesize - Nuclear fusion
The process requires large amounts of energy to start. When it has started, the energy released from the fusion reaction is more than enough to keep it going - it is a chain reaction. Overall, it is highly exothermic
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Stars are excellent examples of the process of nuclear fusion. They burn vast quantities of fuel every second, and reach incredibly hot temperatures
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Anything that has mass has a gravitational attraction, however small
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It is the simplest element
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It is in supernova explosions that the naturally-occurring elements with atomic numbers greater than that of iron are formed
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The gravitational pull of the weight of the star is in equilibrium with the outward radiation pressure generated by the burning of the fuel within the core of the star
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Stars containing the most mass burn the brightest and have the shortest lifespan. Without these super-massive stars, only the elements up to and including iron would exist naturally
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The material in a white dwarf is extremely dense as there is no more radiation pressure from nuclear fusion to balance the inward pull of gravity
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No one has ever seen a black hole directly, but we know they are there because of the gravitational effect they have on other objects within their vicinity
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The Sun is about four and a half thousand million years old. This is about half way through its life cycle
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