On the Source of Energy of Stars

Avagyan Slavik, slavikavagyan@yahoo.com, State Engineering University of Armenia, Gyumri Campus

Abstract
It is considered that the universe has existed for more than 5 billion years in its current form. It is of the same age as the Sun. The fact that the number of neutrinos coming out of the Sun is too little dispels doubts that fusion reaction is the energy source of the Sun. Besides, in order to have thermonuclear reaction in stars, temperature of 20 million degrees is needed, whereas, for example, solar underground temperature is 6 million degrees. It is also known that, for example, the energy emitted from Mars and Saturn approximately equals to the Sun's energy. And there is no fusion reaction inside them. In this paper energy of the magnetic field of bodies is considered as source of energy of the bodies (including stars). As it is known, in each 1 cm3 there is one atom of hydrogen in average. The Sun, for example, attracts these particles belonging to its magnetic field and conveys them kinetic energy which was then converted into heat, when the particles fall on it. This is the endless source of energy that stars have. After using corresponding mathematical apparatus, estimates show that the energy acquired by the Sun equals to E=5,1.?10?^32 erg/s. As we know, the Sun emits Q=3,8.?10?^33 erg/s temperature to environment. Taking into account the influence of various factors, we can see that the correspondence is simply astounding. Depending on their weights, some stars become astronomical bodies, but the most important conclusion is that each body provides energy for its existence. Gaining energy, atoms act the same way. Eradiating energy by portions is explained by the fact that acquired energy is eradiated (“leaves the atom”) only when it reaches certain critical value. If the atom radiates energy then it loses energy. If it does not gain extra energy, then ceases to exist. In other words, Bor’s stationary orbits also do not save stars.