EVOLUTION OF THE UNIVERSE FROM THE BIG BANG BEFORE THE BIG RIP OR A BRIEF EXCURSION IN THE HISTORY OF COSMOLOGY AND SOLAR SYSTEM COSMOGONY: FROM ANCIENT TIMES TO THE PRESENT DAY. PART IV. COSMOGONY OF THE SOLAR SYSTEM

This work continues a series of four articles, which are a brief excursion into the history cosmology and
cosmogony of the Solar System, covering the time scale – from the most ancient times up to the present
day. The release of this cycle is dedicated to the 135-th anniversary of the birth of the world-famous Russian
scientist Fridman A. A., the founder of modern physical cosmology and the author of the first non-stationary
model of the Universe. This article is devoted to an overview of the most significant examples of cosmogonic
models of the Solar System (SS) of the XVIII-XXI centuries. In particular, the first nebular model of the
origin and evolution of the SS by Kant is considered. Its strengths and weaknesses, and the key ideas
embodied in modern cosmogonic models are noted. The nebular models of the hot primary nebula of Laplace
and the vortex SS of Faye are also presented. The work also pays attention to catastrophic models of the
origin and evolution of the SS: the planetesimal model of Moulton and Chamberlin, the tidal model of Jeans
and Jeffreys. Using modern astrophysical data, the main shortcomings of these models are clearly indicated,
and their unrealisticness is substantiated. A separate paragraph is devoted to the modern model of the
origin and evolution of the SS up to the present day. In particular, the chronology of the main stages of
the SS evolution in the past is presented. It also considers the current trends in the possible future of the
SS and its composition. The final part of the work presents brief conclusions in the form of an epilogue.