What kind of solar system do we have? How I easily learned the names of the planets

Universe (space)- this is the entire world around us, limitless in time and space and infinitely varied in the forms that eternally moving matter takes. The boundlessness of the Universe can be partially imagined on a clear night with billions of different sizes of luminous flickering points in the sky, representing distant worlds. Rays of light at a speed of 300,000 km/s from the most distant parts of the Universe reach the Earth in about 10 billion years.

According to scientists, the Universe was formed as a result of the “Big Bang” 17 billion years ago.

It consists of clusters of stars, planets, cosmic dust and other cosmic bodies. These bodies form systems: planets with satellites (for example, the solar system), galaxies, metagalaxies (clusters of galaxies).

Galaxy(late Greek galaktikos- milky, milky, from Greek gala- milk) is a vast star system that consists of many stars, star clusters and associations, gas and dust nebulae, as well as individual atoms and particles scattered in interstellar space.

There are many galaxies of different sizes and shapes in the Universe.

All stars visible from Earth are part of the Milky Way galaxy. It got its name due to the fact that most stars can be seen on a clear night in the form of the Milky Way - a whitish, blurry stripe.

In total, the Milky Way Galaxy contains about 100 billion stars.

Our galaxy is in constant rotation. The speed of its movement in the Universe is 1.5 million km/h. If you look at our galaxy from its north pole, the rotation occurs clockwise. The Sun and the stars closest to it complete a revolution around the center of the galaxy every 200 million years. This period is considered to be galactic year.

Similar in size and shape to the Milky Way galaxy is the Andromeda Galaxy, or Andromeda Nebula, which is located at a distance of approximately 2 million light years from our galaxy. Light year— the distance traveled by light in a year, approximately equal to 10 13 km (the speed of light is 300,000 km/s).

To visualize the study of the movement and location of stars, planets and other celestial bodies, the concept of the celestial sphere is used.

Rice. 1. Main lines of the celestial sphere

Celestial sphere is an imaginary sphere of arbitrarily large radius, in the center of which the observer is located. The stars, Sun, Moon, and planets are projected onto the celestial sphere.

The most important lines on the celestial sphere are: the plumb line, zenith, nadir, celestial equator, ecliptic, celestial meridian, etc. (Fig. 1).

Plumb line- a straight line passing through the center of the celestial sphere and coinciding with the direction of the plumb line at the observation point. For an observer on the Earth's surface, a plumb line passes through the center of the Earth and the observation point.

A plumb line intersects the surface of the celestial sphere at two points - zenith, above the observer's head, and nadire - diametrically opposite point.

The great circle of the celestial sphere, the plane of which is perpendicular to the plumb line, is called mathematical horizon. It divides the surface of the celestial sphere into two halves: visible to the observer, with the vertex at the zenith, and invisible, with the vertex at the nadir.

The diameter around which the celestial sphere rotates is axis mundi. It intersects with the surface of the celestial sphere at two points - north pole of the world And south pole of the world. The north pole is the one from which the celestial sphere rotates clockwise when looking at the sphere from the outside.

The great circle of the celestial sphere, the plane of which is perpendicular to the axis of the world, is called celestial equator. It divides the surface of the celestial sphere into two hemispheres: northern, with its summit at the north celestial pole, and southern, with its peak at the south celestial pole.

The great circle of the celestial sphere, the plane of which passes through the plumb line and the axis of the world, is the celestial meridian. It divides the surface of the celestial sphere into two hemispheres - eastern And western.

The line of intersection of the plane of the celestial meridian and the plane of the mathematical horizon - noon line.

Ecliptic(from Greek ekieipsis- eclipse) is a large circle of the celestial sphere along which the visible annual movement of the Sun, or more precisely, its center, occurs.

The plane of the ecliptic is inclined to the plane of the celestial equator at an angle of 23°26"21".

To make it easier to remember the location of stars in the sky, people in ancient times came up with the idea of ​​combining the brightest of them into constellations.

Currently, 88 constellations are known, which bear the names of mythical characters (Hercules, Pegasus, etc.), zodiac signs (Taurus, Pisces, Cancer, etc.), objects (Libra, Lyra, etc.) (Fig. 2).

Rice. 2. Summer-autumn constellations

Origin of galaxies. The solar system and its individual planets still remain an unsolved mystery of nature. There are several hypotheses. It is currently believed that our galaxy was formed from a gas cloud consisting of hydrogen. At the initial stage of galaxy evolution, the first stars formed from the interstellar gas-dust medium, and 4.6 billion years ago, the Solar System.

Composition of the solar system

The set of celestial bodies moving around the Sun as a central body forms Solar system. It is located almost on the outskirts of the Milky Way galaxy. The solar system is involved in rotation around the center of the galaxy. The speed of its movement is about 220 km/s. This movement occurs in the direction of the constellation Cygnus.

The composition of the Solar System can be represented in the form of a simplified diagram shown in Fig. 3.

Over 99.9% of the mass of matter in the Solar System comes from the Sun and only 0.1% from all its other elements.

Rice. 3. Composition of the Solar System

Sun

Sun- this is a star, a giant hot ball. Its diameter is 109 times the diameter of the Earth, its mass is 330,000 times the mass of the Earth, but its average density is low - only 1.4 times the density of water. The Sun is located at a distance of about 26,000 light years from the center of our galaxy and revolves around it, making one revolution in about 225-250 million years. The orbital speed of the Sun is 217 km/s—so it travels one light year every 1,400 Earth years.

Rice. 4. Chemical composition of the Sun

The pressure on the Sun is 200 billion times higher than at the surface of the Earth. The density of solar matter and pressure quickly increase in depth; the increase in pressure is explained by the weight of all overlying layers. The temperature on the surface of the Sun is 6000 K, and inside it is 13,500,000 K. The characteristic lifetime of a star like the Sun is 10 billion years.

Table 1. General information about the Sun

The chemical composition of the Sun is about the same as that of most other stars: about 75% is hydrogen, 25% is helium and less than 1% is all other chemical elements (carbon, oxygen, nitrogen, etc.) (Fig. 4 ).

The central part of the Sun with a radius of approximately 150,000 km is called the solar core. This is a zone of nuclear reactions. The density of the substance here is approximately 150 times higher than the density of water. The temperature exceeds 10 million K (on the Kelvin scale, in terms of degrees Celsius 1 °C = K - 273.1) (Fig. 5).

Above the core, at distances of about 0.2-0.7 solar radii from its center, is radiant energy transfer zone. Energy transfer here is carried out by absorption and emission of photons by individual layers of particles (see Fig. 5).

Rice. 5. Structure of the Sun

Photon(from Greek phos- light), an elementary particle capable of existing only by moving at the speed of light.

Closer to the surface of the Sun, vortex mixing of the plasma occurs, and energy is transferred to the surface

mainly by the movements of the substance itself. This method of energy transfer is called convection, and the layer of the Sun where it occurs is convective zone. The thickness of this layer is approximately 200,000 km.

Above the convective zone is the solar atmosphere, which constantly fluctuates. Both vertical and horizontal waves with lengths of several thousand kilometers propagate here. Oscillations occur with a period of about five minutes.

The inner layer of the Sun's atmosphere is called photosphere. It consists of light bubbles. This granules. Their sizes are small - 1000-2000 km, and the distance between them is 300-600 km. About a million granules can be observed on the Sun at the same time, each of which exists for several minutes. The granules are surrounded by dark spaces. If the substance rises in the granules, then around them it falls. The granules create a general background against which large-scale formations such as faculae, sunspots, prominences, etc. can be observed.

Sunspots- dark areas on the Sun, the temperature of which is lower than the surrounding space.

Solar torches called bright fields surrounding sunspots.

Prominences(from lat. protubero- swell) - dense condensations of relatively cold (compared to the surrounding temperature) substance that rise and are held above the surface of the Sun by a magnetic field. The occurrence of the Sun's magnetic field can be caused by the fact that different layers of the Sun rotate at different speeds: the internal parts rotate faster; The core rotates especially quickly.

Prominences, sunspots and faculae are not the only examples of solar activity. It also includes magnetic storms and explosions, which are called flashes.

Above the photosphere is located chromosphere- the outer shell of the Sun. The origin of the name of this part of the solar atmosphere is associated with its reddish color. The thickness of the chromosphere is 10-15 thousand km, and the density of matter is hundreds of thousands of times less than in the photosphere. The temperature in the chromosphere is growing rapidly, reaching tens of thousands of degrees in its upper layers. At the edge of the chromosphere there are observed spicules, representing elongated columns of compacted luminous gas. The temperature of these jets is higher than the temperature of the photosphere. The spicules first rise from the lower chromosphere to 5000-10,000 km, and then fall back, where they fade. All this happens at a speed of about 20,000 m/s. Spi kula lives 5-10 minutes. The number of spicules existing on the Sun at the same time is about a million (Fig. 6).

Rice. 6. The structure of the outer layers of the Sun

Surrounds the chromosphere solar corona- outer layer of the Sun's atmosphere.

The total amount of energy emitted by the Sun is 3.86. 1026 W, and only one two-billionth of this energy is received by the Earth.

Solar radiation includes corpuscular And electromagnetic radiation.Corpuscular fundamental radiation- this is a plasma flow that consists of protons and neutrons, or in other words - sunny wind, which reaches near-Earth space and flows around the entire magnetosphere of the Earth. Electromagnetic radiation- This is the radiant energy of the Sun. It reaches the earth's surface in the form of direct and diffuse radiation and provides the thermal regime on our planet.

In the middle of the 19th century. Swiss astronomer Rudolf Wolf(1816-1893) (Fig. 7) calculated a quantitative indicator of solar activity, known throughout the world as the Wolf number. Having processed the observations of sunspots accumulated by the middle of the last century, Wolf was able to establish the average I-year cycle of solar activity. In fact, the time intervals between years of maximum or minimum Wolf numbers range from 7 to 17 years. Simultaneously with the 11-year cycle, a secular, or more precisely 80-90-year, cycle of solar activity occurs. Uncoordinatedly superimposed on each other, they make noticeable changes in the processes taking place in the geographical shell of the Earth.

The close connection of many terrestrial phenomena with solar activity was pointed out back in 1936 by A.L. Chizhevsky (1897-1964) (Fig. 8), who wrote that the overwhelming majority of physical and chemical processes on Earth are the result of the influence of cosmic forces. He was also one of the founders of such science as heliobiology(from Greek helios- sun), studying the influence of the Sun on the living matter of the geographical envelope of the Earth.

Depending on solar activity, such physical phenomena occur on Earth as: magnetic storms, the frequency of auroras, the amount of ultraviolet radiation, the intensity of thunderstorm activity, air temperature, atmospheric pressure, precipitation, the level of lakes, rivers, groundwater, salinity and activity of the seas and etc.

The life of plants and animals is associated with the periodic activity of the Sun (there is a correlation between solar cyclicity and the duration of the growing season in plants, the reproduction and migration of birds, rodents, etc.), as well as humans (diseases).

Currently, the relationships between solar and terrestrial processes continue to be studied using artificial Earth satellites.

Terrestrial planets

In addition to the Sun, planets are distinguished as part of the Solar System (Fig. 9).

Based on size, geographic characteristics and chemical composition, planets are divided into two groups: terrestrial planets And giant planets. The terrestrial planets include, and. They will be discussed in this subsection.

Rice. 9. Planets of the Solar System

Earth- the third planet from the Sun. A separate subsection will be devoted to it.

Let's summarize. The density of the planet’s substance, and taking into account its size, its mass, depends on the location of the planet in the solar system. How
The closer a planet is to the Sun, the higher its average density of matter. For example, for Mercury it is 5.42 g/cm\ Venus - 5.25, Earth - 5.25, Mars - 3.97 g/cm3.

The general characteristics of the terrestrial planets (Mercury, Venus, Earth, Mars) are primarily: 1) relatively small sizes; 2) high temperatures on the surface and 3) high density of planetary matter. These planets rotate relatively slowly on their axis and have few or no satellites. In the structure of the terrestrial planets, there are four main shells: 1) a dense core; 2) the mantle covering it; 3) bark; 4) light gas-water shell (excluding Mercury). Traces of tectonic activity were found on the surface of these planets.

Giant planets

Now let's get acquainted with the giant planets, which are also part of our solar system. This , .

Giant planets have the following general characteristics: 1) large size and mass; 2) rotate quickly around an axis; 3) have rings and many satellites; 4) the atmosphere consists mainly of hydrogen and helium; 5) in the center they have a hot core of metals and silicates.

They are also distinguished by: 1) low surface temperatures; 2) low density of planetary matter.

The solar system is a system of planets that includes its center, the Sun, as well as other objects in space. They revolve around the Sun. Until recently, “planet” was the name given to 9 objects in space that revolve around the Sun. Scientists have now established that beyond the boundaries of the solar system there are planets that orbit stars.

In 2006, the Union of Astronomers proclaimed that the planets of the solar system are spherical space objects revolving around the Sun. On the scale of the solar system, the Earth appears extremely small. In addition to the Earth, eight planets revolve around the Sun in their individual orbits. All of them are larger than the Earth in size. Rotate in the plane of the ecliptic.

Planets in the Solar System: types

Location of the terrestrial group in relation to the Sun

The first planet is Mercury, followed by Venus; Next comes our Earth and, finally, Mars.
Terrestrial planets do not have many satellites or moons. Of these four planets, only Earth and Mars have satellites.

Planets that belong to the terrestrial group are highly dense and consist of metal or stone. Basically, they are small and rotate around their axis. Their rotation speed is also low.

Gas giants

These are the four space objects that are at the greatest distance from the Sun: Jupiter is at No. 5, followed by Saturn, then Uranus and Neptune.

Jupiter and Saturn are impressively sized planets made of hydrogen and helium compounds. The density of gas planets is low. They rotate at high speeds, have satellites and are surrounded by rings of asteroids.
The “ice giants,” which include Uranus and Neptune, are smaller; their atmospheres contain methane and carbon monoxide.

Gas giants have a strong gravitational field, so they can attract many cosmic objects, unlike the terrestrial group.

According to scientists, asteroid rings are the remains of moons changed by the gravitational field of the planets.

Dwarf planet

Dwarfs are space objects whose size does not reach the size of a planet, but exceeds the dimensions of an asteroid. There are a great many such objects in the Solar System. They are concentrated in the Kuiper belt region. The satellites of the gas giants are dwarf planets that have left their orbit.

Planets of the Solar System: the process of emergence

According to the cosmic nebula hypothesis, stars are born in clouds of dust and gas, in nebulae.
Due to the force of attraction, substances come together. Under the influence of the concentrated force of gravity, the center of the nebula contracts and stars form. Dust and gases transform into rings. The rings rotate under the influence of gravity, and planetasimals are formed in the whirlpools, which increase in size and attract cosmetic objects to themselves.

Under the influence of gravity, planetesimals are compressed and acquire spherical shapes. The spheres can unite and gradually turn into protoplanets.



There are eight planets within the solar system. They revolve around the Sun. Their location is as follows:
The closest “neighbor” of the Sun is Mercury, followed by Venus, followed by the Earth, then Mars and Jupiter, further from the Sun are Saturn, Uranus and the last one, Neptune.

Our Solar System consists of the Sun, the planets orbiting it, and smaller celestial bodies. All of these are mysterious and surprising because they are still not fully understood. Below will be indicated the sizes of the planets of the solar system in ascending order, and a brief description of the planets themselves.

There is a well-known list of planets, in which they are listed in order of their distance from the Sun:

Pluto used to be in last place, but in 2006 it lost its status as a planet, as larger celestial bodies were found further away from it. The listed planets are divided into rocky (inner) and giant planets.

Brief information about rocky planets

The inner (rocky) planets include those bodies that are located inside the asteroid belt separating Mars and Jupiter. They got their name “stone” because they consist of various hard rocks, minerals and metals. They are united by a small number or absence of satellites and rings (like Saturn). On the surface of rocky planets there are volcanoes, depressions and craters formed as a result of the fall of other cosmic bodies.

But if you compare their sizes and arrange them in ascending order, the list will look like this:

Brief information about the giant planets

The giant planets are located beyond the asteroid belt and are therefore also called outer planets. They consist of very light gases - hydrogen and helium. These include:

But if you make a list by the size of the planets in the solar system in ascending order, the order changes:

A little information about the planets

In modern scientific understanding, a planet means a celestial body that revolves around the Sun and has sufficient mass for its own gravity. Thus, there are 8 planets in our system, and, importantly, these bodies are not similar to each other: each has its own unique differences, both in appearance and in the components of the planet themselves.

- This is the planet closest to the Sun and the smallest among the others. It weighs 20 times less than the Earth! But, despite this, it has a fairly high density, which allows us to conclude that there are a lot of metals in its depths. Due to its strong proximity to the Sun, Mercury is subject to sudden temperature changes: at night it is very cold, during the day the temperature rises sharply.

- This is the next planet closest to the Sun, in many ways similar to Earth. It has a more powerful atmosphere than Earth, and is considered a very hot planet (its temperature is above 500 C).

- This is a unique planet due to its hydrosphere, and the presence of life on it led to the appearance of oxygen in its atmosphere. Most of the surface is covered with water, and the rest is occupied by continents. A unique feature is the tectonic plates, which move, albeit very slowly, resulting in changes in the landscape. The Earth has one satellite - the Moon.

– also known as the “Red Planet”. It gets its fiery red color from a large amount of iron oxides. Mars has a very thin atmosphere and much lower atmospheric pressure compared to Earth. Mars has two satellites - Deimos and Phobos.

is a real giant among the planets of the solar system. Its weight is 2.5 times the weight of all the planets combined. The surface of the planet consists of helium and hydrogen and is in many ways similar to the sun. Therefore, it is not surprising that there is no life on this planet - there is no water and a solid surface. But Jupiter has a large number of satellites: 67 are currently known.

– This planet is famous for the presence of rings consisting of ice and dust revolving around the planet. With its atmosphere it resembles that of Jupiter, and in size it is slightly smaller than this giant planet. In terms of the number of satellites, Saturn is also slightly behind - it has 62 known. The largest satellite, Titan, is larger than Mercury.

- the lightest planet among the outer ones. Its atmosphere is the coldest in the entire system (minus 224 degrees), it has a magnetosphere and 27 satellites. Uranium consists of hydrogen and helium, and the presence of ammonia ice and methane has also been noted. Because Uranus has a high axial tilt, it appears as if the planet is rolling rather than rotating.

- despite its smaller size than , it is heavier and exceeds the mass of the Earth. This is the only planet that was found through mathematical calculations, and not through astronomical observations. The strongest winds in the solar system were recorded on this planet. Neptune has 14 moons, one of which, Triton, is the only one that rotates in the opposite direction.

It is very difficult to imagine the entire scale of the solar system within the limits of the studied planets. It seems to people that the Earth is a huge planet, and, in comparison with other celestial bodies, it is so. But if you place giant planets next to it, then the Earth already takes on tiny dimensions. Of course, next to the Sun, all celestial bodies appear small, so representing all the planets in their full scale is a difficult task.

The most famous classification of planets is their distance from the Sun. But a listing that takes into account the sizes of the planets of the Solar System in ascending order would also be correct. The list will be presented as follows:

As you can see, the order has not changed much: the inner planets are on the first lines, and Mercury occupies the first place, and the outer planets occupy the remaining positions. In fact, it doesn’t matter at all in what order the planets are located, this will not make them any less mysterious and beautiful.

Previously, a planet was any cosmic body that orbits a star, emits light that is reflected by that star, and is larger than an asteroid. Even in Ancient Greece, they talked about 7 planets as luminous bodies that move across the sky against the backdrop of stars. These are Mercury, Sun, Venus, Mars, Moon, Jupiter, Saturn. Please note that the Sun is indicated here, which is a star, and the Moon is a satellite of our Earth. The earth is not included in this list because the Greeks considered it the center of everything.

In the 15th century, Copernicus discovered that the center of the system was the Sun, not the Earth. He laid out his statements in his work “On the Revolution of the Celestial Spheres.” The Moon and Sun were removed from the list, and planet Earth was included. When telescopes were invented, three more planets were discovered. Uranus in 1781, Neptune in 1846, Pluto in 1930, which, by the way, is no longer considered a planet.

At the moment, researchers are giving a new meaning to the word “planet”, namely: it is a celestial body that satisfies 4 conditions:

• The body must rotate around the star.
• Have a spherical or approximately spherical shape, that is, the body must have sufficient gravity.
• It doesn't have to be a star.
• The celestial body should not have other large bodies near its orbit.

A star is a body that emits light and has a powerful source of energy.

Planets in the Solar System

The solar system includes the planets and other objects that orbit the sun. 4.5 billion years ago, condensations of clouds of stellar matter began to form in the Galaxy. The gases heated up and radiated heat. As a result of an increase in temperature and density, nuclear reactions began, hydrogen turned into helium. This is how the most powerful source of energy arose - the Sun. This process took tens of millions of years. Planets with satellites were created. The formation of the solar system ended completely about 4 billion years ago.

Today, the solar system includes 8 planets, which are divided into two groups. The first is the terrestrial group, the second is the gas giants. The terrestrial planets - Venus, Mercury, Mars and Earth - are composed of silicates and metals. The gas giants - Saturn, Jupiter, Neptune and Uranus - are composed of hydrogen and helium. The planets have different sizes, both in comparison between the two groups and among themselves. Accordingly, the giants are much larger and more massive than the terrestrial planets.

Mercury is closest to the Sun, followed by Neptune. Before characterizing the planets of the Solar System, we need to talk about its main object - the Sun. This is the star through which all living and nonliving things in the system began to exist. The sun is a spherical, plasma, hot ball. A large number of space objects revolve around it - satellites, planets, meteorites, asteroids and cosmic dust. This star appeared about 5 billion years ago. Its mass is 300 thousand times greater than the mass of our planet. The core temperature is 13 million degrees Kelvin, and at the surface - 5 thousand degrees Kelvin (4727 degrees Celsius). In the Milky Way galaxy, the Sun is one of the largest and brightest stars. The distance from the Sun to the center of the Galaxy is 26,000 light years. The Sun makes a complete revolution around the galactic center every 230-250 million years.

Mercury

It is closest to the Sun and is the smallest planet in the solar system. The planet has no satellites. There are many craters on the surface of Mercury, which were formed by many meteorites that fell on the planet more than 3 billion years ago. Their diameter is varied - from a couple of meters to 1000 kilometers. The planet's atmosphere is composed mainly of helium and is blown by wind from the Sun. Temperatures can reach +440 degrees Celsius. The planet completes a revolution around the Sun in 88 Earth days. A day on the planet is equal to 176 Earth hours.

Venus

Venus is the second planet from the Sun. Its dimensions are close to the size of the Earth. The planet has no satellites. The atmosphere consists of carbon dioxide with admixtures of nitrogen and oxygen. The air pressure is 90 atmospheres, which is 35 times more than on Earth. Venus is called the hottest planet because its dense atmosphere, carbon dioxide, proximity to the Sun and the greenhouse effect create very high temperatures on the planet's surface. It can reach 460 degrees Celsius. Venus can be seen from the surface of the Earth. This is the brightest cosmic object after the Moon and the Sun.

Earth

The only planet suitable for life. Maybe it exists on other planets, but no one can say this with certainty yet. It is the largest in its group in terms of mass, density and size. Its age is more than 4 billion years. Life began here more than 3 billion years ago. Earth's satellite is the Moon. The atmosphere on the planet is radically different from others. Most of it consists of nitrogen. This also includes carbon dioxide, oxygen, water vapor and argon. The ozone layer and magnetic field make the level of solar and cosmic radiation less. Due to the content of carbon dioxide in the Earth's atmosphere, a greenhouse effect is formed on the planet. Without it, the temperature on the Earth's surface would be 40 degrees lower. Islands and continents occupy 29% of the planet's surface, and the rest is the World Ocean.

Mars

It is also called the “red planet” due to the presence of large amounts of iron oxide in the soil. Mars is the seventh largest planet in the solar system. Two satellites fly near the planet - Deimos and Phobos. Due to the too thin atmosphere and the far distance from the Sun, the average annual temperature of the planet is minus 60 degrees. At some points during the day, temperature changes can reach 40 degrees. The presence of volcanoes and craters, deserts and valleys, and polar ice caps distinguishes Mars from other planets in the solar system. Also here is the highest mountain - the extinct Olympus volcano, which reached a height of 27 kilometers. Valles Marineris is the largest canyon among the planets. Its length is 4500 km and its depth is 11 m.

Jupiter

It is the largest planet in the solar system. Jupiter is 318 times heavier than Earth and 2.5 times more massive compared to other planets. The main components of the planet are helium and hydrogen. Jupiter emits a lot of heat - 4*1017 W. To become a star like the Sun, it must reach 70 times its current mass. The planet has the largest number of satellites - 63. Europa, Callisto, Ganymede and Io are the largest of them. Ganymede is also the largest moon in the entire solar system and is even larger than Mercury. Jupiter's atmosphere hosts many vortices that have a brownish-red colored band of clouds, or a giant storm, known as the Great Red Spot since the 17th century.

Saturn

Like Jupiter, it is a large planet that follows Jupiter in size. The ring system, which consists of particles of ice of various sizes, rocks and dust, distinguishes this planet from others. It has one fewer satellites than Jupiter. The largest are Enceladus and Titan. In composition, Saturn resembles Jupiter, but in density it is inferior to the simplest water. The atmosphere looks quite homogeneous and calm, which can be explained by a dense layer of fog. Saturn has enormous wind speeds, it can reach 1800 km per hour.

Uranus

This planet was discovered first using a telescope. Uranus is the only planet in the solar system that lies on its side and orbits the sun. Uranus has 27 moons, which are named after characters in Shakespeare's plays. The largest among them are Titania, Oberon and Umbriel. Uranus contains a large number of high-temperature modifications of ice. It is also the coldest planet. The temperature here is minus 224 degrees Celsius.

Neptune

It is the farthest planet from the Sun, although until 2006 this title belonged to Pluto. This planet was discovered without the help of a telescope, but by mathematical calculations. The existence of Neptune was suggested to scientists by Uranus, on which strange changes were discovered while moving in its own orbit. The planet has 13 satellites. The largest among them is Triton. Its peculiarity is that it moves opposite to the planet. The strongest winds in the solar system blow in the same direction, the speed of which reaches 2200 km per hour. Neptune and Uranus have similar compositions, but it is also similar in composition to Jupiter and Saturn. The planet has an internal heat source, from which it receives 2.5 times more energy than from the Sun. There is methane in the outer layers of the atmosphere, which gives the planet a blue tint.

That's how mysterious the world of Space is. Many satellites and planets have their own characteristics. Scientists are making changes to this world, for example, they excluded Pluto from the list of planets.

Study the planets on the portal website - it’s very interesting.

Rotation of planets

All planets, in addition to their orbit, also rotate around their own axis. The period during which they make a full revolution is defined as an epoch. Most of the planets in the Solar System rotate in the same direction on the axis as the Sun, but Uranus and Venus rotate in the opposite direction. Scientists observe a big difference in the length of the day on the planets - Venus takes 243 Earth days to complete one revolution around its axis, while the gas giant planets need only a couple of hours. The rotation period of exoplanets is unknown, but their close proximity to the stars means that eternal day reigns on one side, and eternal night on the other.

Why are all the planets so different? Due to the high temperature closer to the star, the ice and gas evaporated very quickly. The giant planets failed to form, but an accumulation of metal particles occurred. Thus, Mercury was formed, which contains the largest amount of metals. The further we are from the center, the lower the temperature. Celestial bodies appeared, where a significant percentage was made up of rocks. The four planets that are located closer to the center of the solar system are called the inner ones. With the discovery of new systems, more and more questions arise. New research will help answer them.

Scientists claim that our system is unique. All planets are built in strict order. The largest one is closer to the Sun, respectively, the smallest one is further away. Our system has a more complex structure, because the planets are not arranged according to their mass. The sun makes up more than 99 percent of all objects in the system.