Fusion: Harnessing the Power of the Sun

History From the beginning of this century the sun has become a source of great power This is a well-known fact. In 1929 scientists initially speculated that energy production in the stars was produced by nuclear fusion: nuclear reaction involves the formation of heavier elements by light element reaction. In the late 1930's, H. Bethe analyzed most of our sun's nuclear fusion cycle. Helium and neon (two hydrogen isotopes) react (in the presence of large amounts of heat) to form helium, energy, and additional neutrons cause solar fusion.

Fusion power is the process of driving the sun and other stars. It creates a great deal of heat by merging the nuclei of hydrogen or helium isotopes that may come from sea water. In theory, you can generate electricity using heat. Maintaining the temperature and pressure necessary for nuclear fusion is a process that is very difficult to control. In theory, integration can supply a lot of energy, contamination is relatively small. According to the report, the United States, the European Union and other countries support nuclear fusion research (such as investing in ITER facilities), but the progress of inadequate research in the past two decades has led to progress in nuclear fusion research It hampered.

In the process called nuclear fusion, nuclear fusion creates stars and produces almost all elements. The sun is the main sequence star, hence energy is generated by the sequential condensation of hydrogen nuclei. Its core is that the sun melts 620 million tons of hydrogen and produces 606 million tons of helium per second. The fusion of lighter elements in the star releases energy and is always accompanied by its mass. For example, if two hydrogen nuclei fuse together to form helium, 0.7% of the mass is carried away in the form of alpha particle kinetic energy or other forms of energy such as electromagnetic radiation.

Fusion is the process of moving the sun and stars. It is a reaction in which two hydrogen atoms are bonded or fused together to form a ruthenium atom. In this process, part of the hydrogen is converted into energy. The most common nuclear fusion reaction is to combine hydrazine (or "heavy hydrogen") with hydrazine (or "heavy heavy hydrogen") to produce hydrazine and neutrons. Hello, there are plenty of normal water Niobium can be produced by combining fusion neutrons and abundant light metal lithium. Therefore, consolidation may become an inexhaustible energy source.