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"Solar system. Planets and their satellites". Part 1

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The system may be a set of planets and tiny bodies current round the central star — our Sun. we'll bring up the Sun and our satellite the Moon severally, furthermore as a separate section on tiny bodies of the system. these days we'll bring up planets. All the planets are often divided into 2 conditional teams — inner planets and outer planets — by location from the Sun, to the orbit of the world or once.
Let's stipulate right away some basic ideas regarding bodies of system and their orbits. to live distances within the system, AN Astronomical Unit is employed. it's adequate to the common distance from the world to the Sun, which is 149 597 870 metric linear unit. It takes concerning eight.3 minutes to travel this distance to the sunshine flying at today's quickest renowned speed of three00,000 kilometers per second. Thus, we tend to see our Sun because it was eight.3 minutes past.

The nighest purpose of the orbit to the Sun of the bodies of the system is named point of periapsis, and also the most distant is swindle. The distances of those points from the Sun area unit constant because the point of periapsis distance Q and also the swindle distance Q. each of those orbital parts of the heavenly body (q and Q) area unit measured in astronomical units (abbreviated as a.u.). The rotation amount around the Sun P is measured in Earth years (1 Earth year is concerning 365.25 days). additionally to those parts of the orbit, their area unit many others that totally describe the sort of orbit of our body into consideration, however, this is often a subject for a separate spoken language.
So, let's begin with the inner planets — i.e. those planets, whose orbits lie nearer to the Sun than the world one. They embrace (in the order of distance from the Sun) Mercury and Venus.

Both inner planets have the amount of the simplest visibility from the world after they reach the instant of elongation — the best distance from the Sun within the sky. There area unit western and Japanese elongations of planets. once the western elongation happens, the inner planet is west of the Sun and, consequently, is visible within the sky before sunrise within the morning. once the world within the Japanese elongation it's visible to the east of the Sun and is discovered within the evening sky straightaway once sunset. If the inner planet is between the world and also the Sun, this position is named rock bottom affiliation, however, if the Sun is relative to the world, it's aforesaid that it's within the high affiliation. throughout the connections the world isn't visible, our bright daytime shining interferes with its observations. Thus, we tend to see that the inner planets within the sky don't seem to be off from the Sun, and area unit visible either within the evening at sunset or within the morning at sunrise. each planet have a phase transition within the telescope (like the Moon). I.e. you'll be able to see not solely the full circumference of a disk however conjointly a slim reap hook or “half” of a disk.
Now let's look into each planets in additional detail.

Mercury, whose orbit around the Sun is eighty-eight days (0.24 g.), is that the nighest to the Sun of the planets (an average of concerning zero.39 U.S. or fifty-eight million kilometers), and in size — 4879 metric linear unit, the littlest of them. within the pictures taken from the orbiter, he demonstrates a landscape terribly like the satellite — the surface is totally lined with craters. The temperature distinction on the world is incredibly high — throughout the day the temperature on the surface reaches +400 degrees, and in the dead of night the surface is cooled to -180 degrees Anders Celsius.
The Mercury telescope is visible as a tiny low disk with a diameter of four.5 seconds to thirteen seconds of arc looking on the gap from the world. Details thereon area unit mistily guessed even in fairly giant telescopes. Mercury's luster varies from -2.4 to 5.5 links on the average.

The brightest planet in our sky is actually Venus. In its most brilliance, it reaches -4.7 stellar worth. The diameter of its disk, discovered within the telescope, ranges from sixty-six seconds of arc within the nearest position to the world to nine.7 seconds within the most remote.
The period of Venus' orbit around the Sun is adequate to 225 days (0.62 g.), and its distance from the Sun is adequate to 108 million metric linear unit (0.72 a.u.). The diameter of Venus is barely 650 metric linear unit smaller than the Earth's and equals to 12100 metric linear unit. Venus incorporates a terribly solid atmosphere and from the world, we tend to see solely a cloudy layer and mistily — changes in it. below the thick layer of clouds the “greenhouse effect” is made and also the temperature on the world reaches high values. Our Venus machines have recorded temperatures of +475 degrees Anders Celsius and pressures of concerning ninety atmospheres on the surface. Venus clouds consist not of vapor, as on Earth, however of eightieth of acid and CO2. a lot of terrible conditions area unit tough to imagine. therefore the conditions on the surface of the world area unit getting ready to crucial, that makes it tough enough to review the “morning star” of the orbiter.

This concludes the first part of this article, in the second part we will discuss the outer planets.