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Mysteries of the Sun and Solar system.doc

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Mysteries of the Sun and Solar system.doc

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Mysteries of the Sun and Solar system.doc

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文档介绍:Solar aspects of papers
Mysteries of the Sun and Solar system
Alexander M. Ilyanok
CJSC Consulting Center “Nanobiology”, Belarus, Minsk,
Every new fundamental step in science development was directly or indirectly connected with discoveries in astronomy. Thus, Newton created differential and integral calculus solving equations for s. New element, Helium, was discovered from the Solar spectra. High energy physics is directly connected with exploring cosmic rays. They was cosmic rays from that the antimatter – positron was discovered.
Nevertheless, the space is being discovered more the new mysteries and paradoxes are being brought by it. The closest of them to the humanity are mysteries of the energy origin and dynamics of the Sun and Solar system. They are, first of all:
Origin of the Sun and Solar system in a whole;
The incitement of the motion of s of the solar system;
Ecliptic motion of s;
The law of conservation of rotation energy in the solar system;
Observed value of squeezing the Sun;
Existence of helioseismic waves with the period of 160 min and 5 min observed on the surface of the sun;
Solar flares and sun-spots;
The temperature of the Sun photosphere.
Many of these problems were attempted to be solved separately one to each other. In this work the new model of the Sun and origin of the Solar system able to give a joint view on all problems listed above is proposed.
Models describing the origin of energy from stars, including the energy of the sun were created at each stage of formation of new concepts in physics. For example, in the 19th century H. Helmholtz considered pression to be the main power source of the solar energy1 puted the time of full illumination of the sun 33 millions of years.
However, further palaeontological investigations showed, that life on the Earth was not interrupted during the last 3 billion years and, consequently, the luminosity of the sun was relatively uniform. This scientific fact led to the first crisis