V.3 No 1

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Chapter 2. Hypothesis of origin of planetary system (part 1)

Some aspects of the Earth evolution

Sergey B. Karavashkin and Olga N. Karavashkina

Special Laboratory for Fundamental Elaboration SELF

187 apt., 38 bldg., Prospect Gagarina, 38, Kharkov 61140, Ukraine

Phone: +38 (057) 7370624; e-mail: selftrans@yandex.ru , selflab@mail.ru

Chapter 2. Hypothesis of origin of planetary system (part I)

I.S. Shklovsky [1]

Among the versatile hypotheses which we have considered in [2], many contain impressively convincing elements, but no one can be recognised accomplished and more or less harmoniously explaining the origin of planetary system. In this chapter we will endeavour to synthesise the achievements of considered hypotheses, when possible - to lift the layered discrepancies, to add omitted chains and to seek out the answer, how the planets origin.

The existent hypotheses are incomplete not occasionally, since our possibility to observe in details the processes occurring far from the Earth is too young, whilst the issues of evolution make a huge complex depending on many factors which can essentially vary in the course of evolution. This is why in 20th century, with the "burst" of observation scope, there happened the "burst" of hypotheses of evolution. Many of them are now impetuously developed, transformed either decay, if they appeared discrepant with the newest observational data. Hypotheses that lately dominated are revised; other that recently were severe criticised as unproved and contradicting to the conventional ideas suddenly appear in agreement with the last observed data and become leading.

To be able to understand this maelstrom, to sort out the trustworthy facts and convincing approaches and to construct a correct sequence of regularities and processes making the amount of protoplanet and planet evolution, we will have to touch first a broad spectrum of closely related issues that precede the issues of planets origin. They are:

• why, how, of what, under affection of which forces a star originates and which is its structure;

• where from and how the star accumulates complex nuclei of chemical elements, while the interstellar medium consists almost exceptionally of hydrogen;

• what makes versatile kinds of stars, spectra and magnetic fields;

• where from and how the star accumulates the energy that reveals in its radiation;

• why stars burst, and do they have necessarily to burst;

• on what factors the gauge of burst depends;

• which is the mechanism of redistribution of the substance and energy in the burst;

• what is the part of burst in the star evolution.

We will just touch these subjects slightly, as each is extremely wide and has been enlightened in a tremendous bibliography, while we have to follow the thread principal for our investigation - how the planetary system originates. Only having tracked the entire course of evolution, we possibly will be able to grasp, with which result this consideration will come to the last point - i.e., which amount of regularities and conditions will determine the process final for this chapter. With it we will see, how the hypotheses of different authors inosculate and, complementing each other, merge into the harmonic non-contradictive pattern - hopefully, able to stand the check by observations.