The endless space that surrounds us is not just a huge airless space and emptiness. Here everything is subject to a single and strict order, everything has its own rules and obeys the laws of physics. Everything is in constant motion and is constantly interconnected with each other. This is a system in which each celestial body occupies its specific place. The center of the Universe is surrounded by galaxies, among which is our Milky Way. Our galaxy, in turn, is formed by stars around which large and small planets with their natural satellites revolve. The picture of a universal scale is complemented by wandering objects - comets and asteroids.
In this endless cluster of stars our Solar System is located - a tiny astrophysical object by cosmic standards, which includes our cosmic home - planet Earth. For us earthlings, the size of the solar system is colossal and difficult to perceive. In terms of the scale of the Universe, these are tiny numbers - only 180 astronomical units or 2.693e+10 km. Here, too, everything is subject to its own laws, has its own clearly defined place and sequence.
Brief characteristics and description
The interstellar medium and the stability of the Solar System are ensured by the location of the Sun. Its location is an interstellar cloud included in the Orion-Cygnus arm, which in turn is part of our galaxy. From a scientific point of view, our Sun is located on the periphery, 25 thousand light years from the center of the Milky Way, if we consider the galaxy in the diametrical plane. In turn, the movement of the solar system around the center of our galaxy is carried out in orbit. A complete revolution of the Sun around the center of the Milky Way is carried out in different ways, within 225-250 million years and is one galactic year. The orbit of the Solar System has an inclination of 600 to the galactic plane. Nearby, in the neighborhood of our system, other stars and other solar systems with their large and small planets are running around the center of the galaxy.
The approximate age of the Solar System is 4.5 billion years. Like most objects in the Universe, our star was formed as a result of the Big Bang. The origin of the Solar System is explained by the same laws that operated and continue to operate today in the fields of nuclear physics, thermodynamics and mechanics. First, a star was formed, around which, due to the ongoing centripetal and centrifugal processes, the formation of planets began. The Sun was formed from a dense accumulation of gases - a molecular cloud, which was the product of a colossal Explosion. As a result of centripetal processes, molecules of hydrogen, helium, oxygen, carbon, nitrogen and other elements were compressed into one continuous and dense mass.
The result of grandiose and such large-scale processes was the formation of a protostar, in the structure of which thermonuclear fusion began. We observe this long process, which began much earlier, today, looking at our Sun 4.5 billion years after its formation. The scale of the processes occurring during the formation of a star can be imagined by assessing the density, size and mass of our Sun:
- density is 1.409 g/cm3;
- the volume of the Sun is almost the same figure - 1.40927x1027 m3;
- star mass – 1.9885x1030 kg.
Today our Sun is an ordinary astrophysical object in the Universe, not the smallest star in our galaxy, but far from the largest. The Sun is in its mature age, being not only the center of the solar system, but also the main factor in the emergence and existence of life on our planet.
The final structure of the solar system falls on the same period, with a difference of plus or minus half a billion years. The mass of the entire system, where the Sun interacts with other celestial bodies of the Solar System, is 1.0014 M☉. In other words, all the planets, satellites and asteroids, cosmic dust and particles of gases revolving around the Sun, compared to the mass of our star, are a drop in the bucket.
The way we have an idea of our star and the planets revolving around the Sun is a simplified version. The first mechanical heliocentric model of the solar system with a clock mechanism was presented to the scientific community in 1704. It should be taken into account that the orbits of the planets of the solar system do not all lie in the same plane. They rotate around at a certain angle.
The model of the solar system was created on the basis of a simpler and more ancient mechanism - tellurium, with the help of which the position and movement of the Earth in relation to the Sun was simulated. With the help of tellurium, it was possible to explain the principle of the movement of our planet around the Sun and to calculate the duration of the earth's year.
The simplest model of the solar system is presented in school textbooks, where each of the planets and other celestial bodies occupies a certain place. It should be taken into account that the orbits of all objects revolving around the Sun are located at different angles to the central plane of the Solar System. The planets of the Solar System are located at different distances from the Sun, rotate at different speeds and rotate differently around their own axis.
A map - a diagram of the Solar System - is a drawing where all objects are located in the same plane. In this case, such an image gives an idea only of the sizes of celestial bodies and the distances between them. Thanks to this interpretation, it became possible to understand the location of our planet among other planets, to assess the scale of celestial bodies and to give an idea of the enormous distances that separate us from our celestial neighbors.
Planets and other objects of the solar system
Almost the entire universe is made up of myriads of stars, among which there are large and small solar systems. The presence of a star with its own satellite planets is a common occurrence in space. The laws of physics are the same everywhere and our solar system is no exception.
If you ask the question how many planets there were in the solar system and how many there are today, it is quite difficult to answer unequivocally. Currently, the exact location of 8 major planets is known. In addition, 5 small dwarf planets revolve around the Sun. The existence of a ninth planet is currently disputed in scientific circles.
The entire solar system is divided into groups of planets, which are arranged in the following order:
Terrestrial planets:
- Mercury;
- Venus;
- Mars.
Gas planets - giants:
- Jupiter;
- Saturn;
- Uranus;
- Neptune.
All planets presented in the list differ in structure and have different astrophysical parameters. Which planet is larger or smaller than the others? The sizes of the planets of the solar system are different. The first four objects, similar in structure to the Earth, have a solid rock surface and are endowed with an atmosphere. Mercury, Venus and Earth are the inner planets. Mars closes this group. Following it are the gas giants: Jupiter, Saturn, Uranus and Neptune - dense, spherical gas formations.
The process of life of the planets of the solar system does not stop for a second. Those planets that we see in the sky today are the arrangement of celestial bodies that the planetary system of our star has at the current moment. The state that existed at the dawn of the formation of the solar system is strikingly different from what has been studied today.
The astrophysical parameters of modern planets are indicated by the table, which also shows the distance of the planets of the Solar System to the Sun.
The existing planets of the solar system are approximately the same age, but there are theories that in the beginning there were more planets. This is evidenced by numerous ancient myths and legends that describe the presence of other astrophysical objects and disasters that led to the death of the planet. This is confirmed by the structure of our star system, where, along with planets, there are objects that are products of violent cosmic cataclysms.
A striking example of such activity is the asteroid belt, located between the orbits of Mars and Jupiter. Objects of extraterrestrial origin are concentrated here in huge numbers, mainly represented by asteroids and small planets. It is these irregularly shaped fragments that are considered in human culture to be the remains of the protoplanet Phaeton, which perished billions of years ago as a result of a large-scale cataclysm.
In fact, there is an opinion in scientific circles that the asteroid belt was formed as a result of the destruction of a comet. Astronomers have discovered the presence of water on the large asteroid Themis and on the small planets Ceres and Vesta, which are the largest objects in the asteroid belt. Ice found on the surface of asteroids may indicate the cometary nature of the formation of these cosmic bodies.
Previously one of the major planets, Pluto is not considered a full-fledged planet today.
Pluto, which was previously ranked among the large planets of the solar system, is today reduced to the size of dwarf celestial bodies revolving around the Sun. Pluto, along with Haumea and Makemake, the largest dwarf planets, is located in the Kuiper belt.
These dwarf planets of the solar system are located in the Kuiper belt. The region between the Kuiper belt and the Oort cloud is the most distant from the Sun, but space is not empty there either. In 2005, the most distant celestial body of our solar system, the dwarf planet Eris, was discovered there. The process of exploration of the most distant regions of our solar system continues. The Kuiper Belt and Oort Cloud are hypothetically the border regions of our star system, the visible boundary. This cloud of gas is located at a distance of one light year from the Sun and is the region where comets, the wandering satellites of our star, are born.
Characteristics of the planets of the solar system
The terrestrial group of planets is represented by the planets closest to the Sun - Mercury and Venus. These two cosmic bodies of the solar system, despite the similarity in physical structure with our planet, are a hostile environment for us. Mercury is the smallest planet in our star system and is closest to the Sun. The heat of our star literally incinerates the surface of the planet, practically destroying its atmosphere. The distance from the surface of the planet to the Sun is 57,910,000 km. In size, only 5 thousand km in diameter, Mercury is inferior to most large satellites, which are dominated by Jupiter and Saturn.
Saturn's satellite Titan has a diameter of over 5 thousand km, Jupiter's satellite Ganymede has a diameter of 5265 km. Both satellites are second in size only to Mars.
The very first planet rushes around our star at tremendous speed, making a full revolution around our star in 88 Earth days. It is almost impossible to notice this small and nimble planet in the starry sky due to the close presence of the solar disk. Among the terrestrial planets, it is on Mercury that the largest daily temperature differences are observed. While the surface of the planet facing the Sun heats up to 700 degrees Celsius, the back side of the planet is immersed in universal cold with temperatures up to -200 degrees.
The main difference between Mercury and all the planets in the solar system is its internal structure. Mercury has the largest iron-nickel inner core, which accounts for 83% of the mass of the entire planet. However, even this uncharacteristic quality did not allow Mercury to have its own natural satellites.
Next to Mercury is the closest planet to us - Venus. The distance from Earth to Venus is 38 million km, and it is very similar to our Earth. The planet has almost the same diameter and mass, slightly inferior in these parameters to our planet. However, in all other respects, our neighbor is fundamentally different from our cosmic home. The period of Venus' revolution around the Sun is 116 Earth days, and the planet rotates extremely slowly around its own axis. The average surface temperature of Venus rotating around its axis over 224 Earth days is 447 degrees Celsius.
Like its predecessor, Venus lacks the physical conditions conducive to the existence of known life forms. The planet is surrounded by a dense atmosphere consisting mainly of carbon dioxide and nitrogen. Both Mercury and Venus are the only planets in the solar system that do not have natural satellites.
Earth is the last of the inner planets of the solar system, located at a distance of approximately 150 million km from the Sun. Our planet makes one revolution around the Sun every 365 days. Rotates around its own axis in 23.94 hours. The Earth is the first of the celestial bodies located on the path from the Sun to the periphery, which has a natural satellite.
Digression: The astrophysical parameters of our planet are well studied and known. Earth is the largest and densest planet of all the other inner planets in the solar system. It is here that natural physical conditions have been preserved under which the existence of water is possible. Our planet has a stable magnetic field that holds the atmosphere. Earth is the most well studied planet. The subsequent study is mainly of not only theoretical interest, but also practical one.
Mars closes the parade of terrestrial planets. The subsequent study of this planet is mainly not only of theoretical interest, but also of practical interest, associated with human exploration of extraterrestrial worlds. Astrophysicists are attracted not only by the relative proximity of this planet to Earth (on average 225 million km), but also by the absence of difficult climatic conditions. The planet is surrounded by an atmosphere, although it is in an extremely rarefied state, has its own magnetic field, and temperature differences on the surface of Mars are not as critical as on Mercury and Venus.
Like Earth, Mars has two satellites - Phobos and Deimos, the natural nature of which has recently been questioned. Mars is the last fourth planet with a rocky surface in the solar system. Following the asteroid belt, which is a kind of inner boundary of the solar system, begins the kingdom of gas giants.
The largest cosmic celestial bodies of our solar system
The second group of planets that are part of the system of our star has bright and large representatives. These are the largest objects in our solar system, which are considered the outer planets. Jupiter, Saturn, Uranus and Neptune are the most distant from our star, huge by earthly standards and their astrophysical parameters. These celestial bodies are distinguished by their massiveness and composition, which is mainly gaseous in nature.
The main beauties of the solar system are Jupiter and Saturn. The total mass of this pair of giants would be enough to fit in it the mass of all known celestial bodies of the Solar System. So Jupiter, the largest planet in the solar system, weighs 1876.64328 1024 kg, and the mass of Saturn is 561.80376 1024 kg. These planets have the most natural satellites. Some of them, Titan, Ganymede, Callisto and Io, are the largest satellites of the Solar System and are comparable in size to the terrestrial planets.
The largest planet in the solar system, Jupiter, has a diameter of 140 thousand km. In many respects, Jupiter more closely resembles a failed star - a striking example of the existence of a small solar system. This is evidenced by the size of the planet and astrophysical parameters - Jupiter is only 10 times smaller than our star. The planet rotates around its own axis quite quickly - only 10 Earth hours. The number of satellites, of which 67 have been identified to date, is also striking. The behavior of Jupiter and its moons is very similar to the model of the solar system. Such a number of natural satellites for one planet raises a new question: how many planets were there in the Solar System at the early stage of its formation. It is assumed that Jupiter, having a powerful magnetic field, turned some planets into its natural satellites. Some of them - Titan, Ganymede, Callisto and Io - are the largest satellites of the solar system and are comparable in size to the terrestrial planets.
Slightly smaller in size than Jupiter is its smaller brother, the gas giant Saturn. This planet, like Jupiter, consists mainly of hydrogen and helium - gases that are the basis of our star. With its size, the diameter of the planet is 57 thousand km, Saturn also resembles a protostar that has stopped in its development. The number of satellites of Saturn is slightly inferior to the number of satellites of Jupiter - 62 versus 67. Saturn's satellite Titan, like Io, a satellite of Jupiter, has an atmosphere.
In other words, the largest planets Jupiter and Saturn with their systems of natural satellites strongly resemble small solar systems, with their clearly defined center and system of movement of celestial bodies.
Behind the two gas giants come the cold and dark worlds, the planets Uranus and Neptune. These celestial bodies are located at a distance of 2.8 billion km and 4.49 billion km. from the Sun, respectively. Due to their enormous distance from our planet, Uranus and Neptune were discovered relatively recently. Unlike the other two gas giants, Uranus and Neptune contain large quantities of frozen gases - hydrogen, ammonia and methane. These two planets are also called ice giants. Uranus is smaller in size than Jupiter and Saturn and ranks third in the solar system. The planet represents the pole of cold of our star system. The average temperature on the surface of Uranus is -224 degrees Celsius. Uranus differs from other celestial bodies revolving around the Sun by its strong tilt on its own axis. The planet seems to be rolling, revolving around our star.
Like Saturn, Uranus is surrounded by a hydrogen-helium atmosphere. Neptune, unlike Uranus, has a different composition. The presence of methane in the atmosphere is indicated by the blue color of the planet's spectrum.
Both planets move slowly and majestically around our star. Uranus orbits the Sun in 84 Earth years, and Neptune orbits our star twice as long - 164 Earth years.
Finally
Our Solar System is a huge mechanism in which each planet, all satellites of the Solar System, asteroids and other celestial bodies move along a clearly defined route. The laws of astrophysics apply here and have not changed for 4.5 billion years. Along the outer edges of our solar system, dwarf planets move in the Kuiper belt. Comets are frequent guests of our star system. These space objects visit the inner regions of the Solar System with a periodicity of 20-150 years, flying within visibility range of our planet.
If you have any questions, leave them in the comments below the article. We or our visitors will be happy to answer them
solar system is a system of celestial bodies welded together by forces of mutual attraction. It includes: the central star - the Sun, 8 large planets with their satellites, several thousand small planets, or asteroids, several hundred observed comets and countless meteoroids, dust, gas and small particles .
It was formed by gravitational compression gas and dust cloud approximately 4.57 billion years ago.
Sun
The Sun is the closest star to Earth; all the others are immeasurably further away from us. For example, the closest star to us is Proxima from the system a Centauri is 2500 times farther than the Sun. For the Earth, the Sun is a powerful source of cosmic energy. It provides the light and heat necessary for flora and fauna, and forms the most important properties of the Earth's atmosphere.. In general, the Sun determines the ecology of the planet. Without it, there would be no air necessary for life: it would turn into a liquid nitrogen ocean around frozen waters and icy land. For us earthlings, the most important feature of the Sun is that our planet arose near it and life appeared on it.
Merkur th
Mercury is the planet closest to the Sun.
The ancient Romans considered Mercury the patron of trade, travelers and thieves, as well as the messenger of the gods. It is not surprising that a small planet, quickly moving across the sky following the Sun, received his name. Mercury has been known since ancient times, but ancient astronomers did not immediately realize that they saw the same star in the morning and evening. Mercury is closer to the Sun than the Earth: the average distance from the Sun is 0.387 AU, and the distance to Earth ranges from 82 to 217 million km. The inclination of the orbit to the ecliptic i = 7° is one of the largest in the Solar System. Mercury's axis is almost perpendicular to the plane of its orbit, and the orbit itself is very elongated (eccentricity e = 0.206). The average speed of Mercury's orbit is 47.9 km/s. Due to the tidal influence of the Sun, Mercury fell into a resonant trap. The period of its revolution around the Sun (87.95 Earth days), measured in 1965, relates to the period of rotation around its axis (58.65 Earth days) as 3/2. Mercury completes three full revolutions around its axis in 176 days. During the same period, the planet makes two revolutions around the Sun. Thus, Mercury occupies the same position in orbit relative to the Sun, and the orientation of the planet remains the same. Mercury has no satellites. If they were, then during the formation of the planets they fell on protomercury. The mass of Mercury is almost 20 times less than the mass of the Earth (0.055M or 3.3 10 23 kg), and its density is almost the same as that of the Earth (5.43 g/cm3). The radius of the planet is 0.38R (2440 km). Mercury is smaller than some of the moons of Jupiter and Saturn.
Venus
The second planet from the Sun, has an almost circular orbit. It passes closer to Earth than any other planet.
But the dense, cloudy atmosphere does not allow you to directly see its surface. Atmosphere: CO 2 (97%), N2 (approx. 3%), H 2 O (0.05%), impurities CO, SO 2, HCl, HF. Thanks to the greenhouse effect, the surface temperature heats up to hundreds of degrees. The atmosphere, which is a thick blanket of carbon dioxide, traps heat coming from the Sun. This results in the temperature of the atmosphere being much higher than in the oven. Radar images show a very wide variety of craters, volcanoes and mountains. There are several very large volcanoes, up to 3 km high. and hundreds of kilometers wide. The outpouring of lava on Venus takes much longer than on Earth. The pressure at the surface is about 107 Pa. The surface rocks of Venus are similar in composition to terrestrial sedimentary rocks.
Finding Venus in the sky is easier than any other planet. Its dense clouds reflect sunlight well, making the planet bright in our sky. For a few weeks every seven months, Venus is the brightest object in the western sky in the evenings. Three and a half months later, it rises three hours earlier than the Sun, becoming the sparkling “morning star” of the eastern sky. Venus can be observed an hour after sunset or an hour before sunrise. Venus has no satellites.
Third from Sol 
ntsa planet. The speed of the Earth's revolution in an elliptical orbit around the Sun is 29.765 km/s. The inclination of the earth's axis to the ecliptic plane is 66 o 33 "22". The Earth has a natural satellite - the Moon. The Earth has a magnetic fieldIT and electric fields. The Earth was formed 4.7 billion years ago from gas dispersed in the protosolar system-dust substances. The composition of the Earth is dominated by: iron (34.6%), oxygen (29.5%), silicon (15.2%), magnesium (12.7%). The pressure in the center of the planet is 3.6 * 10 11 Pa, the density is about 12,500 kg/m 3, the temperature is 5000-6000 o C. Most of the timeThe surface is occupied by the World Ocean (361.1 million km 2; 70.8%); the land area is 149.1 million km 2 and forms six motherscoves and islands. It rises above the level of the world's oceans by an average of 875 meters (the highest altitude is 8848 meters - the city of Chomolungma). Mountains occupy 30% of the land, deserts cover about 20% of the land surface, savannas and woodlands - about 20%, forests - about 30%, glaciers - 10%. The average depth of the ocean is about 3800 meters, the greatest is 11022 meters (Mariana Trench in the Pacific Ocean), the volume of water is 1370 million km 3, the average salinity is 35 g/l. The Earth's atmosphere, the total mass of which is 5.15 * 10 15 tons, consists of air - a mixture of mainly nitrogen (78.1%) and oxygen (21%), the rest is water vapor, carbon dioxide, noble and other gases. About 3-3.5 billion years ago, as a result of the natural evolution of matter, life arose on Earth and the development of the biosphere began.
Mars
The fourth planet from the Sun, similar to Earth, but smaller and cooler. Mars has deep canyons
giant volcanoes and vast deserts. There are two small moons flying around the Red Planet, as Mars is also called: Phobos and Deimos. Mars is the next planet after the Earth, if you count from the Sun, and the only cosmic world besides the Moon that can already be reached with the help of modern rockets. For astronauts, this four-year journey could represent the next frontier in space exploration. Near the equator of Mars, in an area called Tharsis, there are volcanoes of colossal size. Tarsis is the name that astronomers gave to the hill, which has 400 km. wide and about 10 km. in height. There are four volcanoes on this plateau, each of which is simply gigantic compared to any terrestrial volcano. The largest volcano on Tharsis, Mount Olympus, rises 27 km above the surrounding area. About two-thirds of Mars' surface is mountainous, with many impact craters surrounded by rock debris. Near the volcanoes of Tharsis, a vast system of canyons snakes around the length of about a quarter of the equator. The Valles Marineris is 600 km wide, and its depth is such that Mount Everest would sink entirely to its bottom. Sheer cliffs rise thousands of meters, from the valley floor to the plateau above. In ancient times, there was a lot of water on Mars; large rivers flowed across the surface of this planet. There are ice caps at the South and North Poles of Mars. But this ice does not consist of water, but of frozen atmospheric carbon dioxide (freezes at a temperature of -100 o C). Scientists believe that surface water is stored in the form of ice blocks buried in the ground, especially in polar regions. Atmospheric composition: CO 2 (95%), N 2 (2.5%), Ar (1.5 - 2%), CO (0.06%), H 2 O (up to 0.1%); pressure at the surface is 5-7 hPa. In total, about 30 interplanetary space stations were sent to Mars.
Jupiter
The fifth planet from the Sun, the largest planet in the Solar System. Jupiter is not a rocky planet. Unlike the four rocky planets closest to the Sun, Jupiter is a gas ball. Atmospheric composition: H 2 (85%), CH 4, NH 3, He (14%). Jupiter's gas composition is very similar to the sun's. Jupiter is a powerful source of thermal radio emission. Jupiter has 16 satellites (Adrastea, Metis, Amalthea, Thebe, Io, Lysithea, Elara, Ananke, Karme, Pasiphae, Sinope, Europa, Ganymede, Callisto, Leda, Himalia), as well as a ring 20,000 km wide, almost closely adjacent to planet. Jupiter's rotation speed is so high that the planet bulges along the equator. In addition, this rapid rotation causes very strong winds in the upper atmosphere, where clouds stretch out into long, colorful ribbons. There are a very large number of vortex spots in the clouds of Jupiter. The largest of them, the so-called Great Red Spot, is larger than the Earth. The Great Red Spot is a huge storm in Jupiter's atmosphere that has been observed for 300 years. Inside the planet, under enormous pressure, hydrogen turns from a gas into a liquid, and then from a liquid into a solid. At a depth of 100 km. there is a boundless ocean of liquid hydrogen. Below 17,000 km. hydrogen is compressed so tightly that its atoms are destroyed. And then it begins to behave like metal; in this state it easily conducts electricity. The electric current flowing in metallic hydrogen creates a strong magnetic field around Jupiter.
Saturn
The sixth planet from the Sun has an amazing ring system. Due to its rapid rotation around its axis, Saturn seems to be flattened at the poles. Wind speeds at the equator reach 1800 km/h. The width of Saturn's rings is 400,000 km, but they are only a few tens of meters thick. The inner parts of the rings rotate around Saturn faster than the outer ones. The rings are primarily made up of billions of small particles, each orbiting Saturn as its own microscopic satellite. These "micro-satellites" are likely made of water ice or rocks covered in ice. Their size ranges from a few centimeters to tens of meters. There are also larger objects in the rings - stone blocks and fragments up to hundreds of meters in diameter. The gaps between the rings arise under the influence of the gravitational forces of seventeen moons (Hyperion, Mimas, Tethys, Titan, Enceladus, etc.), which cause the rings to split. The composition of the atmosphere includes: CH 4, H 2, He, NH 3.
Uranus
Seventh from 
Sun planet. It was discovered in 1781 by the English astronomer William Herschel, and named after Greek about the sky god Uranus. The orientation of Uranus in space differs from the other planets of the solar system - its axis of rotation lies, as it were, “on its side” relative to the plane of revolution of this planet around the Sun. The axis of rotation is inclined at an angle of 98 o. As a result, the planet faces the Sun alternately with the north pole, the south, the equator, and the middle latitudes. Uranus has more than 27 satellites (Miranda, Ariel, Umbriel, Titania, Oberon, Cordelia, Ophelia, Bianca, Cressida, Desdemona, Juliet, Portia, Rosalind, Belinda, Peck, etc.) and a system of rings. At the center of Uranus is a core made of rock and iron. The composition of the atmosphere includes: H 2, He, CH 4 (14%).
Neptune
E Its orbit intersects with Pluto's orbit in some places. The equatorial diameter is the same as that of Uranus, although ra Neptune is located 1627 million km further from Uranus (Uranus is located 2869 million km from the Sun). Based on these data, we can conclude that this planet could not be noticed in the 17th century. One of the striking achievements of science, one of the evidence of the unlimited cognition of nature was the discovery of the planet Neptune through calculations - “at the tip of a pen.” Uranus, the planet next to Saturn, which for many centuries was considered the most distant planet, was discovered by W. Herschel at the end of the 18th century. Uranus is hardly visible to the naked eye. By the 40s of the XIX century. accurate observations have shown that Uranus deviates barely noticeably from the path it should follow, taking into account the disturbances from all the known planets. Thus, the theory of the movement of celestial bodies, so strict and accurate, was put to the test. Le Verrier (in France) and Adams (in England) suggested that if disturbances from the known planets do not explain the deviation in the movement of Uranus, it means that the attraction of an as yet unknown body acts on it. They almost simultaneously calculated where behind Uranus there should be an unknown body producing these deviations with its gravity. They calculated the orbit of the unknown planet, its mass and indicated the place in the sky where the unknown planet should have been located at that time. This planet was found through a telescope at the place they indicated in 1846. It was named Neptune. Neptune is not visible to the naked eye. On this planet, winds blow at speeds of up to 2400 km/h, directed against the rotation of the planet. These are the strongest winds in the solar system.
Atmospheric composition: H 2, He, CH 4. Has 6 satellites (one of them is Triton).
Neptune is the god of the seas in Roman mythology.
Until recently, astronomers believed that the concept of a planet applied exclusively to the solar system. Everything that is beyond its boundaries are unexplored cosmic bodies, most often stars of very large scale. But, as it turned out later, the planets, like peas, are scattered throughout the Universe. They vary in their geological and chemical composition, and may or may not have an atmosphere, all depending on their interaction with the nearest star. The arrangement of planets in our solar system is unique. It is this factor that is fundamental for the conditions that have formed on each individual space object.
Our space home and its features
In the center of the solar system there is a star of the same name, which is classified as a yellow dwarf. Its magnetic field is enough to hold nine planets of varying sizes around their axis. Among them there are dwarf rocky cosmic bodies, immense gas giants that reach almost the parameters of the star itself, and “middle” class objects, which include the Earth. The arrangement of the planets of the solar system does not occur in ascending or descending order. We can say that relative to the parameters of each individual astronomical body, their location is chaotic, that is, the large alternates with the small.
SS structure
To consider the location of the planets in our system, it is necessary to take the Sun as a reference point. This star is located in the center of the SS, and it is its magnetic fields that correct the orbits and movements of all surrounding cosmic bodies. There are nine planets orbiting the Sun, as well as a ring of asteroids that lies between Mars and Jupiter, and the Kuiper Belt, which lies beyond Pluto. In these gaps, individual dwarf planets are also distinguished, which are sometimes attributed to the main units of the system. Other astronomers believe that all these objects are nothing more than large asteroids, on which life cannot arise under any circumstances. They also assign Pluto itself to this category, leaving only 8 planetary units in our system.
The order of the planets
So, we will list all the planets, starting with the one closest to the Sun. In first place are Mercury, Venus, then Earth and Mars. After the Red Planet there passes a ring of asteroids, behind which begins a parade of giants consisting of gases. These are Jupiter, Saturn, Uranus and Neptune. The list is completed by dwarf and icy Pluto, with its equally cold and black satellite Charon. As we said above, there are several more dwarf space units in the system. The location of dwarf planets in this category coincides with the Kuiper belts and asteroids. Ceres is located in an asteroid ring. Makemake, Haumea and Eris are in the Kuiper Belt.
Terrestrial planets
This category includes cosmic bodies that, in their composition and parameters, have much in common with our home planet. Their depths are also filled with metals and stone, and either a full atmosphere or a haze that resembles it is formed around the surface. The location of the terrestrial planets is easy to remember, because these are the first four objects that are located directly next to the Sun - Mercury, Venus, Earth and Mars. Characteristic features are small size, as well as a long period of rotation around its axis. Also, of all the terrestrial planets, only the Earth itself and Mars have satellites.
Giants consisting of gases and hot metals
The location of the planets of the solar system, which are called gas giants, is the most distant from the main star. They are located behind the asteroid ring and stretch almost to the Kuiper belt. There are four giants in total - Jupiter, Saturn, Uranus and Neptune. Each of these planets consists of hydrogen and helium, and in the core region there are metals that are hot to a liquid state. All four giants are characterized by an incredibly strong gravitational field. Due to this, they attract numerous satellites, which form almost entire asteroid systems around them. SS gas balls rotate very quickly, which is why whirlwinds and hurricanes often occur on them. But, despite all these similarities, it is worth remembering that each of the giants is unique in its composition, size, and gravitational force.
Dwarf planets
Since we have already looked in detail at the location of the planets from the Sun, we know that Pluto is the furthest away and its orbit is the most gigantic in the SS. It is he who is the most important representative of dwarfs, and only he from this group is the most studied. Dwarfs are those cosmic bodies that are too small for planets, but too large for asteroids. Their structure may be comparable to Mars or Earth, or it may simply be rocky, like any asteroid. Above we have listed the most prominent representatives of this group - these are Ceres, Eris, Makemake, Haumea. In fact, dwarfs are found not only in the two SS asteroid belts. They are often called the satellites of gas giants, which are attracted to them due to the enormous
The solar system is our cosmic region, and the planets in it are our homes. Agree, each house should have its own number.
In this article you will learn about the correct location of the planets, as well as why they are called this way and not otherwise.
Let's start with the Sun.
Literally, the star of today's article is the Sun. They named him that, according to some sources, in honor of the Roman god Sol, he was the god of the heavenly body. The root “sol” is present in almost all languages of the world and in one way or another gives an association with the modern concept of the Sun.
From this luminary begins the correct order of objects, each of which is unique in its own way.
Mercury
The very first object of our attention is Mercury, named after the divine messenger Mercury, distinguished by his phenomenal speed. And Mercury itself is by no means slow - due to its location, it rotates around the Sun faster than all the planets in our system, being, moreover, the smallest “house” revolving around our luminary.
Interesting Facts:
- Mercury revolves around the Sun in an ellipsoidal orbit, not a round one like other planets, and this orbit is constantly shifting.
- Mercury has an iron core, making up 40% of its total mass and 83% of its volume.
- Mercury can be seen in the sky with the naked eye.
Venus
“House” number two in our system. Venus was named after the goddess- a wonderful patroness of love. In size, Venus is only slightly inferior to our Earth. Its atmosphere consists almost entirely of carbon dioxide. There is oxygen in its atmosphere, but in very small quantities.
Interesting Facts:
Earth
The only space object on which life has been discovered is the third planet in our system. For living organisms to live comfortably on Earth, there is everything: suitable temperature, oxygen and water. The name of our planet comes from the Proto-Slavic root “-zem”, meaning “low”. Probably, it was called that way in ancient times because it was considered flat, in other words “low”.
Interesting Facts:
- Earth's satellite The Moon is the largest satellite among the satellites of the terrestrial planets - the dwarf planets.
- It is the densest planet among the terrestrial group.
- Earth and Venus are sometimes called sisters because they both have atmospheres.
Mars
The fourth planet from the Sun. Mars is named after the ancient Roman god of war for its blood-red color, which is not bloody at all, but, in fact, iron. It is the high iron content that gives the surface of Mars its red color. Mars is smaller than Earth, but has two satellites: Phobos and Deimos.
Interesting Facts:
Asteroid belt
The asteroid belt is located between Mars and Jupiter. It acts as a boundary between the terrestrial planets and the giant planets. Some scientists believe that the asteroid belt is nothing more than a planet that has shattered into fragments. But so far the whole world is more inclined to the theory that the asteroid belt is a consequence of the Big Bang that gave birth to the galaxy.
Jupiter
Jupiter is the fifth “house”, counting from the Sun. It is two and a half times heavier than all the planets in the galaxy combined. Jupiter is named after the ancient Roman king of the gods, most likely due to its impressive size.
Interesting Facts:
Saturn
Saturn is named after the Roman god of agriculture. The symbol of Saturn is the sickle. The sixth planet is widely known for its rings. Saturn has the lowest density of all the natural satellites orbiting the Sun. Its density is even lower than that of water.
Interesting Facts:
- Saturn has 62 satellites. The most famous of them: Titan, Enceladus, Iapetus, Dione, Tethys, Rhea and Mimas.
- Saturn's moon Titan has the most significant atmosphere of all the system's moons, and Rhea has rings, like Saturn itself.
- The composition of the chemical elements of the Sun and Saturn is most similar than that of the Sun and other objects in the solar system.
Uranus
The seventh “house” in the solar system. Sometimes Uranus is called the “lazy planet”, because during rotation it lies on its side - the tilt of its axis is 98 degrees. Also, Uranus, the lightest planet in our system, and its moons are named after the characters of William Shakespeare and Alexander Pope. Uranus itself is named after the Greek god of the sky.
Interesting Facts:
- Uranus has 27 moons, the most famous of which are Titania, Ariel, Umbriel and Miranda.
- The temperature on Uranus is -224 degrees Celsius.
- One year on Uranus is equal to 84 years on Earth.
Neptune
The eighth and last planet of the solar system is located quite close to its neighbor Uranus. Neptune got its name in honor of the god of the seas and oceans. Apparently, it was given to this space object after researchers saw Neptune's deep blue color.
Interesting Facts:
About Pluto
Pluto has officially ceased to be considered a planet since August 2006. It was considered too small and declared an asteroid. The name of the former planet of the galaxy is not at all the name of some god. The discoverer of this now asteroid named this space object after his daughter’s favorite cartoon character, Pluto the dog.
In this article, we briefly looked at the positions of the planets. We hope you found this article useful and informative.
This is a system of planets, in the center of which there is a bright star, a source of energy, heat and light - the Sun.
According to one theory, the Sun was formed along with the Solar System about 4.5 billion years ago as a result of the explosion of one or more supernovae. Initially, the Solar System was a cloud of gas and dust particles, which, in motion and under the influence of their mass, formed a disk in which a new star, the Sun, and our entire Solar System arose.
At the center of the solar system is the Sun, around which nine large planets revolve in orbit. Since the Sun is displaced from the center of planetary orbits, during the cycle of revolution around the Sun the planets either approach or move away in their orbits.
There are two groups of planets:
Terrestrial planets: And . These planets are small in size with a rocky surface and are closest to the Sun.
Giant planets: And . These are large planets, consisting mainly of gas and characterized by the presence of rings consisting of icy dust and many rocky chunks.
And here does not fall into any group because, despite its location in the solar system, it is located too far from the Sun and has a very small diameter, only 2320 km, which is half the diameter of Mercury.
Planets of the Solar System
Let's begin a fascinating acquaintance with the planets of the Solar System in order of their location from the Sun, and also consider their main satellites and some other space objects (comets, asteroids, meteorites) in the gigantic expanses of our planetary system.
Rings and moons of Jupiter: Europa, Io, Ganymede, Callisto and others...
The planet Jupiter is surrounded by a whole family of 16 satellites, and each of them has its own unique features...
Rings and moons of Saturn: Titan, Enceladus and others...
Not only the planet Saturn has characteristic rings, but also other giant planets. Around Saturn, the rings are especially clearly visible, because they consist of billions of small particles that revolve around the planet, in addition to several rings, Saturn has 18 satellites, one of which is Titan, its diameter is 5000 km, which makes it the largest satellite in the solar system...
Rings and moons of Uranus: Titania, Oberon and others...
The planet Uranus has 17 satellites and, like other giant planets, there are thin rings surrounding the planet that have practically no ability to reflect light, so they were discovered not so long ago in 1977, completely by accident...
Rings and moons of Neptune: 
Triton, Nereid and others...
Initially, before the exploration of Neptune by the Voyager 2 spacecraft, two satellites of the planet were known - Triton and Nerida. An interesting fact is that the Triton satellite has a reverse direction of orbital motion; strange volcanoes were also discovered on the satellite that erupted nitrogen gas like geysers, spreading a dark-colored mass (from liquid to vapor) many kilometers into the atmosphere. During its mission, Voyager 2 discovered six more moons of the planet Neptune...