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The discovery of the past of the solar system has emerged and has become an interesting issue since the 18th and 19th centuries, with many controversies. The study of the origin of the solar system with its planets, satellites, asteroids, asteroids, asteroids, requires answering many questions about the structure as well as the physiological properties that we know, why the planets have the same orbital plane, and why they rotate in the same direction. What factors cause the rotation of the sun and the planets? Or what is the cause of the distribution of mass from the sun to the planets around it? The effort to answer these questions has led to many different ideas and theories about the formation of our planet system. The formation and evolution of the solar system began about 4.6 billion years ago, with the attractive decay of a small part of a giant cluster of asteroids. Most of the decay continues in the center, creating the sun, while the rest is removed to form a cluster of dust clouds before the planet, gradually evolving into planets, moons, asteroids, and other celestial bodies in the solar system. Ideas related to the origin and destiny of the world originate from ancient writings, but the idea of the solar system as a planet system, according to modern observations, has only recently appeared. The first step towards a theory of the formation and development of the solar system is the recognition of the Sun-Jupiter theory, looking at the sun in the center and the Earth revolving around it. This idea has been passed down for thousands of years. Aristarchus of Samos has been talking about it since about 250 BC, but this theory has only been widely accepted since the 17th century. The first writing on the term solar system appeared in 1704. The current theory of the formation of the solar system, the Venus theory, has gone through many ups and downs since it appeared in the 18th century with Immanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace, and was sometimes almost rejected. The most noteworthy criticism of this theory is that it seems unsatisfactory that the sun has relatively little momentum compared to the planets. However, since the early 1980s, research on young stars has shown that they also have planets and dust around them, just like the Venus theory, which has recently been recognized by most scientists. How does the solar system continue to develop? This is a question of its energy origin. Arthur Stanley Eddington's confirmation of Einstein's relativistic theory has made him realize that solar energy arises from the internal thermal reaction. In 1935, Eddington went even further, proposing that other heavier elements could also form inside the stars. Fred Hoy developed this theme by arguing that stars have evolved, called red giant stars, to create many elements heavier than helium and helium in their core. When a red giant star separates the outer layers, these elements can return to form new star systems. The Venus theory has been widely accepted by Immanuel Swedenborg, Immanuel Kant, and Pierre-Simon Laplace since the 18th century. The theory of the formation of the sun has developed continuously thanks to the results of progress in many different fields, including astronomy, physics, geophysics, and planetary science. Since the dawn of space exploration, this model has faced many challenges, and it has been adjusted many times to adapt to new discoveries. The solar system has evolved significantly from its original form. Many moons are formed from gas and dust plates orbiting the planets, while some others are born independently, and some others, like the Earth's moon, may be the result of massive collisions. Collisions occur frequently to this day and play a central role in the evolution of the solar system. The positions of the planets change frequently, and this planet-transition phenomenon is considered essential in the initial stage of the evolution of the solar system. The classical theories were first written by Immanuel Kant and completed by Laplace at the end of the 18th century. The sun is a real star in the true sense of the word, that is, it can radiate itself thanks to the nuclear reactions in its core. About 4.6 billion years ago, a cluster of dust and gas between the stars began to form. When the core of this cluster became dust, it would not allow light to pass through. The process of gas extraction took place until the gas was compressed to the extent that its surface temperature was pushed up to 1,000 Kelvin. At that time, it would radiate in space like a star. At this time, scientists say it has entered the phase of the sun. According to poet Paul M. Sutter, we are here 4.5 billion years ago in the lifetime of the sun, with a series of smaller planets and objects revolving around it. The formation of the solar system is a challenging challenge for modern astronomy. In the beginning, there was nothing much in the universe. There were only stars formed from the collapse of the Milky Way. They were faint clouds and dust. Astronomers called it the Milky Way of the Sun and, of course, it does not exist today. But a star cannot collapse to form a solar system without something to push it to move. Therefore, there was a supernova explosion. A shock wave tore the star cluster in front of the sun, making it begin to shrink. The supernova released a large amount of certain radioactive elements. Then the process of transition from star to the solar system. For millions of years, this star cluster was shrinking. Finally, it reached the point where a solar system is surrounded by a thin layer of gas and dust, spinning fast. 4.5 billion years ago, our sun was not as bright as it is today. It was small and very hot. Although it was very hot, the sun had not reached the necessary density and temperature to maintain the reaction of the nuclear complex in the core. In this phase of evolution, planets began to form in a slow process. The closer to the sun, the hotter and brighter it was, nothing could be kept but rocks. Rocks began to erupt, evaporate, and vaporize like helium and helium. The remaining rocks slowly connect, bind together, and form large clusters. When the sun's mirror is measured by the sun's mirror and its brightness is 0.8 times that of today's sun, the reactions of the nuclear complexes begin. The sun has become the sun as we know it. At this time, the sun will be relatively stable and not shrink any more. This is called the 9th phase of its life. The 9th phase will last about 10 billion years before the sun passes the age period. During the 9th phase, in addition to balancing the crystal, it also achieves thermal balance. Energy from the center of the sun is transmitted out to the surface and completely discharged into space. Compared to the pre-sun period, its brightness has increased by 30%, as we see now. This ensures the evolution process and maintains life on Earth. If this number is larger or smaller, we may not exist, or the world will fall into an abyss. Finally, over time, the clusters have joined, forming planets. The Earth was hit by something about the size of a star, and the fragments from that collision finally became our moon today. At first, people thought that the planets formed near their current orbit. However, this view has changed dramatically in the late 20th and early 21st centuries. Today, people believe that the solar system looks very different from its original shape. Some of the heaviest objects, including asteroids, once appeared in the solar system. The outer surface was much smaller today, and Vandyakubra was much closer to the sun. Astronomers speculate that the four giant planets in the solar system — Jupiter, Saturn, Uranus, and Neptune — originally formed much closer than they do today, and the collisions with other objects around them have changed their orbits. In the first script, Jupiter and Saturn move inwards, towards the sun. This causes Uranus and Neptune to move outwards. In the second script, the worlds outside the solar system collide with another giant planet, and finally, they are pushed out completely. In the final script, Jupiter wanders near the orbit of Saturn before jumping out, breaking the other peaceful orbits of the other worlds. Astronomers believe that the exoplanets have created a period with strong impact of asteroids and small planets in the solar system about 4 billion years ago. The movement of giant worlds disrupts all the other objects in the solar system, bringing them to a safe place in the cold outer space, or returning to the inside to cause trouble for the asteroids. Different asteroids are created from the atmosphere of the sun, collecting the remaining gas and dust after the sun is formed. The way the asteroids are formed is accepted by the scientific community as an accretion. In this accretion, the asteroids start from the dust revolving around the stars. When they collide, the asteroids are joined into 200-meter diameter blocks. When it's their turn, these blocks collide to form larger objects, called planetesimals, about 10 kilometers in diameter. These objects continue to grow through collision, with a speed of a few centimeters a few million years later. These objects are very rare in space, with only 0.6% of their mass, so the asteroids can't grow much. The asteroids' pre-planetary objects grow up to 0.05 times the Earth's mass and stop collecting matter about 100,000 years after the sun is formed. The collisions and combinations of these objects allow them to grow to their current size. When the asteroids are formed, they still sink into the dust. The gas is affected by the pressure and doesn't revolve around the sun as fast as the asteroids. The collision creates a momentum that makes the asteroids gradually move into new orbits. The asteroids move inwards as the planets dissipate until they form a stable orbit like today. The giant asteroids — Jupiter, Saturn, Uranus, and Neptune — form a frost line between the orbit of Jupiter and Jupiter, where the temperature of the objects is low enough for the asteroids to be formed. The solar plexus continues to rotate fast. A part of the object receives enough centrifugal force to penetrate into the plexus and separate from the sun into rings. In each ring, the attraction plays the role of combining objects into large plexuses, which are the planets. The rotation of the plexus makes the objects into smaller plexuses, which are stopped when centrifugal force is generated due to the rotation of the plexus is not large enough to win the attraction of the plexus. This theory does not explain the factors of the abundance of planets and how they move near the sun causing the appearance of the planets. The theory of collision by Chamberlain and Merton in the early 20th century suggests that there was a star passing by and may have collided with the sun. This collision is called an elliptical collision. Air and dust combine on each plexus to form plexuses. The plexuses gradually become stable. These plexuses become planets. In 1918, James Jeans and Harold Jeffries proposed the elliptical theory, another variation of the collision theory. The attraction of this star is that air and dust form plexuses with different sizes on elliptical orbits. These plexuses form planets like today. This theory does not explain the abundance of planets. The modern theory suggests that the abundance of planets is due to the abundance of air and dust. This theory is similar to the one proposed by Gerard Cooper. In this theory, dust forms an unstable orbit. These plexuses form planets. Of course, Cooper's theory does not explain the difference in the physics of planets. The modern theory is proposed by another scientist, H.C.Urey. This theory suggests that planets are formed by dust. It is large enough to maintain the activity of gases like hydrogen or helium, but also small enough not to heat up metals like iron or silicon. Under the influence of attraction, dust on orbits come together and form planets. At this time, the temperature of gases is lower than the temperature of metals. With distant planets, gases like methane and ammonia are pushed down to a very low temperature. They freeze and block the access of heavy gases. Such planets become large planets known as giant planets. They exist in a region where the temperature of gases decreases and the orbits are longer, making it difficult to form them. Instead, these two planets are said to have formed in orbits near Jupiter and Saturn known as The movement of exoplanets is also necessary to assess the existence and nature of the outer regions of the solar system. Outside the Milky Way, the solar system is connected by the Kuiper Belt, the Planetary Plane, and the Oort Clouds, three small clusters of objects where most of the observable stars are born. After the formation of the solar system, the planetary plane was formed by interaction with a large number of other exoplanets. After about 500-600 million years, about 4 billion years ago, Jupiter and Saturn fell into the phenomenon of the 2-1 interaction between Jupiter's orbit and Saturn's orbit. This interaction created an attractive push between Jupiter's orbit and Saturn's orbit. In 1995, the first human study of an exoplanet outside the Kuiper Belt was conducted on Jupiter's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The study was conducted on Jupiter's orbit and Saturn's orbit. The sun will gradually cool down and expand many times its current size or become a giant red star before its outer layer separates and becomes a star cluster and leaves behind a white star. In the distant future, attraction from comets will gradually erase the planets of the sun. Some will be destroyed. Some others will separate and go into interstellar space.