Fools are easier to control.
And if you think that most of today's mandatory education schools educate you, you are mistaken. They are trying to raise obedient sheep out of you. They tell you what you can learn even without these schools, but they tell you in a way that discourages you from wishing to learn it and from, most importantly – actually learning. And if you don't believe me, then try to answer the question:
Why don't they let you get enough sleep before they start teaching you? Maybe when you are sleepy, you are more capable of learning? Why do classes start at eight o'clock instead of ten?
You need to take knowledge everywhere: both in school and outside the school. You should only count on yourself.
And this is the first thing about the Universe that you should firmly grasp.
We will begin our consideration of the issue by looking at the Sun and its energy. Why? The Sun is the closest particular star to us, and the entire Universe is a collection of structures consisting of stars and stellar systems. But we will see that all the differences with the official science in what I am going to tell you begin precisely with the Sun.
The energy that the Earth receives comes from two sources. From inside the Earth and from the Sun. We will talk about the energy that comes from inside the Earth later, but for now a few words about the Sun and about the stars in general.
When scientific officials learned what a thermonuclear reaction is, they immediately seized on it, like an unreasonable child at a toy, and began to say that the sun is shining because thermonuclear reactions occur in it.
Thermonuclear reactions on stars might be happening, but perhaps not as intensely as it is commonly believed, otherwise the stars would have already either exploded or burned out.
Because a thermonuclear reaction is a chain reaction.
The main thing that the fans of that the main energy of the sun is thermonuclear opinion rely on, fusion of four protons into a helium nucleus is a neutrino. As two neutrons decay, two negative antineutrinos should be released. These neutrinos are caught. But just a neutron in a free state decays in 880.1 ± 1.1 seconds. The consequences are the same. Negative antineutrino.
It is claimed, that the Sun emits 1.2 · 1034 joules annually. But does this mean that its mass should decrease? M = E/C2 And its composition must change. The amount of helium should increase, and the amount of hydrogen should decrease accordingly. However, it is rather difficult to calculate the exact composition, and even according to the models that are used today, these are very approximate numbers. These observations began not so long ago. In a hundred years, we may be able to ask them to explain whether the composition of the Sun has changed in accordance with the existing theory or not. But we could already notice the decrease in mass today. The fact that certain Ptolemy calculated the orbits of planetary motion. He took part in his research in Alexandria of Egypt in the period 127-151 ah.