![]() ![]() Here, there is a smashing or colliding of hydrogen atoms that are comparatively lighter atoms together, which is followed by the generation of energy in any of its forms. It is one of the nuclear fusion examples. It is basically observed to be the prime source of power in the case of stars, even the sun. Image credits: Pixabay free images Stellar nucleosynthesis We can observe a release of kinetic energy possessed by the neutron, which results from the conversion of lost mass during the assembling of heavier isotopes. Basically, they are made to come together and recombine in order to bring helium along with a fast neutron into the picture in the form of component parts. Let us now aim to analyze the fusion reaction by combining deuterium and tritium together. Following is the reaction that depicts the above-mentioned nuclear fusion.ġH 2 + 1H 2 → 2He 4 + Energy Fusion o f deuterium and tritium This is under the governance of Einstein’s formula. The energy generated results from a mass transformation in the form of energy which is said to be lost during the process. It is also found that there is a large amount of energy (In the form of heat) that is excavated during this fusion. There is a formation of a helium nucleus by combining two nuclei of deuterium together. Fusion of deuteriumĭeuterium is also regarded as heavy hydrogen. ![]() Prior to and after the reaction, there is an observable difference in the nuclear binding energy, which in turn pave a way to a difference in the masses. At the same time, the helium formed due to the fusion of hydrogen isotopes is known to be the lightest element next to hydrogen. Hydrogen is known to be the lightest in the periodic table. This phenomenon is supported by the existence of very high pressure and temperature in the stars. There is a smashing or colliding of hydrogen atoms together that are comparatively lighter atoms, which is followed by the generation of energy in any of its forms. Hence, it is one of the nuclear fusion examples. On average, the hydrogen that converts into helium is about 600 million tons per unit second. There is a production of an incredibly large amount of heat, one of the forms of energy. Due to these conditions, helium is formed by combining two isotopes of hydrogen, deuterium and tritium. Celsius along with this incredibly high temperature, it also possesses very high pressure. It is found that at the sun’s core, the temperature is nearer to 15 million degrees. The best description of the fusion can be seen to be taking place in the sun’s core. In the upcoming section, let us focus on the nuclear fusion examples. In the atmosphere, we can observe a reaction that compasses any two atoms that stick or join together so that they end up forming different atomic nuclei, which are one or more in number, and also some subatomic particles, namely protons and neutrons. In the present article, we are focussing on discussing nuclear fusion examples and their detailed explanations. ![]()
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