PLANET EARTH.
Among the celestial bodies existing in infinite space, there is the planet on which we live - Earth. The earth was not always the way we know it now. Like the rest of the planets, it appeared about 5 billion years ago from a rotating cloud of hot gases. At this time, solid particles began to form in it. There were more and more of them, and gradually the cloud thickened, which turned into a hot, dense ball.
The surface of this ball gradually cooled, and finally a hard crust formed. That's what they call it - the earth's crust. Beneath it the Earth still retains heat.
In the youth of our planet, the earth’s crust was thin and fragile, its hot interiors and magma often burst out through volcanic openings. During the eruptions of these numerous volcanoes, hot magma poured onto the surface of the Earth, and with it gases, including water vapor, escaped. Gradually, they formed the air shell of the planet - the atmosphere. As the globe cooled, the steam turned into water, giving rise to the World Ocean, which covered most of the Earth's surface, where life arose about 1.5 billion years ago.
The earth has the shape of a ball. But it's hard to notice. Therefore, in ancient times there were different ideas about the Earth and its shape. The ancient Greeks, Phoenicians and Indians believed that the Earth was flat, like a pancake, and surrounded by mountains on all sides. And above the Earth, on four huge pillars, lies a crystal bowl - the sky. The Indians of North America were sure that the world worked like this: the Earth is a whale swimming among endless waters; the man and woman are the personification of Humanity, and the sky is a soaring mighty eagle. And in Asia and Ancient India it was believed that the Earth was a flat or slightly elongated disk, like a drop on a table, that rested on the backs of four giant elephants (according to the number of cardinal directions). The elephants, in turn, stand on the back of a huge turtle. When elephants get tired and shift from foot to foot, earthquakes occur. In the center of the earth rises Mount Meru - the center of the universe, around which the sun, planets and stars revolve. In Ancient China, they believed that the Earth was a cake with cut off edges. In the Middle Ages, scientists thought that the Earth was covered with a cap on which the stars were mounted.
The first to understand that our Planet has the shape of a ball were the sages and philosophers in Ancient Greece. Already two and a half thousand years ago they knew that the most perfect figure in nature is a ball. This means, they reasoned, that the Earth must be spherical. They managed to find a simple proof: when a ship goes out to sea, we, standing on the shore, first see it in its entirety, then the deck disappears, then the sail slowly sinks. But the ship did not sink to the seabed, it was simply hidden from our view by the convex surface of the Earth. It was not only Europeans who came to the idea that the earth was spherical. The Aztec Indians in North America depicted the planets in the form of balls with which the gods played.
For the first time people began to talk about the Earth as a ball in the third century BC. In the Middle Ages, the church forbade talking about the Earth as a ball, declaring it heresy. So how did people know that the Earth is a sphere? A long time ago people noticed that the higher you rise, the farther you can see. Climbing a tree allows you to see something that you cannot see standing on Earth. And once you climb the mountain, you can see very far away. All this comes from the fact that the Earth is not flat, like a table, but round, like a ball. And a person, compared to the Earth, is too small to see it all at once. So he sees only to the horizon, where heaven and earth meet. You rise higher and the horizon moves away. In addition, the horizon in open areas (in the sea, in the steppe) is always seen as a circle.
Important evidence that the Earth is spherical was the sea voyage of Ferdinand Magellan, a native of Portugal. It took his expedition about three years (1519 - 1522) to travel around the globe: going to the west and returning to the same port from the east. After this voyage there was no longer any doubt about the sphericity of the Earth.
Another proof of the sphericity of the Earth was lunar eclipses. During lunar eclipses, the Earth's shadow on the Moon is round.
And finally, on April 12, 1961, Yu. A. Gagarin, the first cosmonaut of the Earth, was able to see our planet from the outside, from space, which also provided evidence of the sphericity of the Earth. The picture shows that the Earth has the shape of a ball. The darker areas in the image are water, the lighter areas are land, and the lightest areas are clouds. Scientists have been able to calculate the size of the Earth. It turned out. To go around the globe, you need to travel 40,000 km.
Earth is the third planet from the Sun and the largest of the terrestrial planets. However, it is only the fifth largest planet in terms of size and mass in the Solar System, but surprisingly, it is the densest of all the planets in the system (5.513 kg/m3). It is also noteworthy that Earth is the only planet in the solar system that people themselves have not named after a mythological creature - its name comes from the old English word "ertha", which means soil.
It is believed that the Earth was formed somewhere around 4.5 billion years ago, and is currently the only known planet where the existence of life is possible in principle, and the conditions are such that life is literally teeming on the planet.
Throughout human history, people have sought to understand their home planet. However, the learning curve turned out to be very, very difficult, with many mistakes made along the way. For example, even before the existence of the ancient Romans, the world was understood as flat, not spherical. A second clear example is the belief that the Sun revolves around the Earth. It was only in the sixteenth century, thanks to the work of Copernicus, that people learned that the Earth was actually just a planet orbiting the Sun.
Perhaps the most important discovery about our planet over the past two centuries is that the Earth is both a common and unique place in the solar system. On the one hand, many of its characteristics are rather ordinary. Take, for example, the size of the planet, its internal and geological processes: its internal structure is almost identical to the three other terrestrial planets in the solar system. On Earth, almost the same geological processes occur that form the surface, which are characteristic of similar planets and many planetary satellites. However, with all this, the Earth simply has a huge number of absolutely unique characteristics that strikingly distinguish it from almost all currently known terrestrial planets.
One of the necessary conditions for the existence of life on Earth is without a doubt its atmosphere. It consists of approximately 78% nitrogen (N2), 21% oxygen (O2) and 1% argon. It also contains very small amounts of carbon dioxide (CO2) and other gases. It is noteworthy that nitrogen and oxygen are necessary for the creation of deoxyribonucleic acid (DNA) and the production of biological energy, without which life cannot exist. In addition, oxygen present in the ozone layer of the atmosphere protects the planet's surface and absorbs harmful solar radiation.
What's interesting is that a significant amount of the oxygen present in the atmosphere is created on Earth. It is formed as a byproduct of photosynthesis, when plants convert carbon dioxide from the atmosphere into oxygen. Essentially, this means that without plants, the amount of carbon dioxide in the atmosphere would be much higher and oxygen levels much lower. On the one hand, if carbon dioxide levels rise, it is likely that the Earth will suffer from a greenhouse effect like this. On the other hand, if the percentage of carbon dioxide became even slightly lower, then the reduction in the greenhouse effect would lead to a sharp cooling. Thus, current carbon dioxide levels contribute to an ideal comfortable temperature range of -88°C to 58°C.
When observing the Earth from space, the first thing that catches your eye is oceans of liquid water. In terms of surface area, oceans cover approximately 70% of the Earth, which is one of the most unique properties of our planet.
Like the Earth's atmosphere, the presence of liquid water is a necessary criterion for supporting life. Scientists believe that life on Earth first appeared 3.8 billion years ago in the ocean, and the ability to move on land appeared in living creatures much later.
Planetologists explain the presence of oceans on Earth for two reasons. The first of these is the Earth itself. There is an assumption that during the formation of the Earth, the planet's atmosphere was able to capture large volumes of water vapor. Over time, the planet's geological mechanisms, primarily its volcanic activity, released this water vapor into the atmosphere, after which in the atmosphere, this vapor condensed and fell to the surface of the planet in the form of liquid water. Another version suggests that the source of water was comets that fell to the surface of the Earth in the past, ice which predominated in their composition and formed the reservoirs that exist on Earth.
Ground surface
Despite the fact that most of the Earth's surface is located under its oceans, the "dry" surface has many distinctive features. When comparing the Earth to other solid bodies in the solar system, its surface is strikingly different because it does not have craters. According to planetary scientists, this does not mean that the Earth has escaped numerous impacts from small cosmic bodies, but rather indicates that evidence of such impacts has been erased. There may be many geological processes responsible for this, but scientists identify the two most important - weathering and erosion. It is believed that in many ways it was the dual impact of these factors that influenced the erasure of traces of craters from the face of the Earth.
So weathering breaks surface structures into smaller pieces, not to mention chemical and physical methods of atmospheric exposure. An example of chemical weathering is acid rain. An example of physical weathering is the abrasion of river beds caused by rocks contained in flowing water. The second mechanism, erosion, is essentially the effect on the relief of the movement of particles of water, ice, wind or earth. Thus, under the influence of weathering and erosion, the impact craters on our planet were “erased”, due to which some relief features were formed.
Scientists also identify two geological mechanisms that, in their opinion, helped shape the Earth's surface. The first such mechanism is volcanic activity - the process of release of magma (molten rock) from the interior of the Earth through breaks in its crust. Perhaps it was due to volcanic activity that the earth's crust was changed and islands were formed (the Hawaiian Islands are a good example). The second mechanism determines mountain building or the formation of mountains as a result of compression of tectonic plates.
Structure of planet earth
Like other terrestrial planets, the Earth consists of three components: the core, mantle and crust. Science now believes that the core of our planet consists of two separate layers: an inner core of solid nickel and iron and an outer core of molten nickel and iron. At the same time, the mantle is a very dense and almost completely solid silicate rock - its thickness is approximately 2850 km. The bark also consists of silicate rocks and varies in thickness. While continental crust ranges from 30 to 40 kilometers in thickness, oceanic crust is much thinner, only 6 to 11 kilometers.
Another distinctive feature of Earth relative to other terrestrial planets is that its crust is divided into cold, rigid plates that rest on a hotter mantle below. In addition, these plates are in constant motion. Along their boundaries, as a rule, two processes occur simultaneously, known as subduction and spreading. During subduction, two plates come into contact producing earthquakes and one plate rides on the other. The second process is separation, where two plates move away from each other.
Earth's orbit and rotation
It takes the Earth approximately 365 days to complete its orbit around the Sun. The length of our year is related largely to the average orbital distance of the Earth, which is 1.50 x 10 to the power of 8 km. At this orbital distance, it takes on average about eight minutes and twenty seconds for sunlight to reach the Earth's surface.
At an orbital eccentricity of .0167, the Earth's orbit is one of the most circular in the entire solar system. This means that the difference between Earth's perihelion and aphelion is relatively small. As a result of this small difference, the intensity of sunlight on Earth remains essentially the same year-round. However, the position of the Earth in its orbit determines one season or another.
The Earth's axial tilt is approximately 23.45°. In this case, the Earth takes twenty-four hours to complete one rotation around its axis. This is the fastest rotation among the terrestrial planets, but slightly slower than all the gas planets.
In the past, the Earth was considered the center of the Universe. For 2000 years, ancient astronomers believed that the Earth was static and that other celestial bodies traveled in circular orbits around it. They came to this conclusion by observing the obvious movement of the Sun and planets when observed from Earth. In 1543, Copernicus published his heliocentric model of the solar system, which places the Sun at the center of our solar system.
Earth is the only planet in the system that was not named after mythological gods or goddesses (the other seven planets in the solar system were named after Roman gods or goddesses). This refers to the five planets visible to the naked eye: Mercury, Venus, Mars, Jupiter and Saturn. The same approach with the names of the ancient Roman gods was used after the discovery of Uranus and Neptune. The word “Earth” itself comes from the old English word “ertha” meaning soil.
Earth is the densest planet in the solar system. The density of the Earth differs in each layer of the planet (the core, for example, is denser than the crust). The average density of the planet is about 5.52 grams per cubic centimeter.
The gravitational interaction between the Earth causes tides on Earth. It is believed that the Moon is blocked by the Earth's tidal forces, so its rotation period coincides with the Earth's and it always faces our planet with the same side.
It is so nice to know that planet Earth has proven to be the most suitable for various forms of life. The temperature conditions here are ideal, there is enough air, oxygen and safe light. It's hard to believe that once upon a time none of this existed. Or almost nothing but a molten cosmic mass of indeterminate shape, floating in zero gravity. But first things first.
Explosion on a universal scale
Early theories of the origin of the universe
Scientists have put forward various hypotheses to explain the birth of the Earth. In the 18th century, the French claimed that the cause was a cosmic catastrophe resulting from the collision of the Sun with a comet. The British claimed that an asteroid flying past the star cut off part of it, from which a whole series of celestial bodies subsequently appeared.
German minds have moved further. They considered a cold dust cloud of incredible size to be the prototype for the formation of planets in the solar system. Later they decided that the dust was hot. One thing is clear: the formation of the Earth is inextricably linked with the formation of all the planets and stars that make up the solar system.
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At what speed does the Earth move around its axis and the Sun?
Today, astronomers and physicists are unanimous in the opinion that the Universe was formed after Big Bang. Billions of years ago, a giant fireball exploded into pieces in outer space. This caused a gigantic ejection of matter, the particles of which had colossal energy. It was the power of the latter that prevented the elements from creating atoms, forcing them to repel each other. This was also facilitated by high temperatures (about a billion degrees). But after a million years, space cooled to approximately 4000º. From this moment, the attraction and formation of atoms of light gaseous substances (hydrogen and helium) began.
Over time, they grouped into clusters called nebulae. These were the prototypes of future celestial bodies. Gradually, the particles inside spun faster and faster, increasing in temperature and energy, causing the nebula to shrink. Having reached a critical point, at a certain moment a thermonuclear reaction began, promoting the formation of a nucleus. Thus the bright Sun was born.
The emergence of the Earth - from gas to solid
The young star had powerful gravitational forces. Their influence caused the formation of other planets at different distances from accumulations of cosmic dust and gases, including the Earth. If you compare the composition of different celestial bodies of the solar system, it will become noticeable that they are not the same.
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Earth collisions with meteorites
Mercury is mainly composed of a metal that is most resistant to sunlight. Venus and Earth have a rocky surface. But Saturn and Jupiter remain gas giants due to their greatest distance. By the way, they protect other planets from meteorites, pushing them away from their orbits.
Formation of the Earth
The formation of the Earth began according to the same principle that underlay the appearance of the Sun itself. This happened approximately 4.6 billion years ago. Heavy metals (iron, nickel) as a result of gravity and compression penetrated into the center of the young planet, forming the core. The high temperature created all the conditions for a series of nuclear reactions. A separation of the mantle and core occurred.
The heat generated melted and ejected light silicon to the surface. It became the prototype of the first crust. As the planet cooled, volatile gases burst out from the depths. This was accompanied by volcanic eruptions. Molten lava later formed rocks.
Gas mixtures were held at a distance around the Earth by gravity. They formed an atmosphere, initially without oxygen. Encounters with icy comets and meteorites led to the appearance of oceans from condensation of vapors and melted ice. Continents separated and reconnected, floating in a hot mantle. This was repeated many times over almost 4 billion years.