Education, The science
Proxima Centauri. Red dwarfs. Alpha Centauri System
Proxima Centauri is the star that is closest to the Earth. The name she received from the Latin word proxima, which means "nearest". The distance from it to the Sun is 4.22 light years. However, in spite of the fact that the star is closer to us than the Sun, it can be seen only through a telescope. It is so small that nothing existed about its existence until 1915. The discoverer of the star was Robert Innes, an astronomer from Scotland.
Star System Alpha Centauri
Alpha Centauri V is also not inferior to the "sister" in brightness. Together they are a tight double system. Proxima Centauri is far enough away from them. Between the stars - a distance of thirteen thousand astronomical units (this is farther than from the Sun to the planet Neptune in as many as four hundred times!).
All the stars of the Centaurus system rotate in orbit around their common center of mass. Only Proxima moves very slowly: the period of its circulation takes millions of years. Therefore, this star will remain very close to the Earth for a very long time.
Very small
Red dwarfs
The small star of Proxima refers to the spectral class M with very low luminosity. Another name for celestial bodies of this class is widely known: red dwarfs. Stars with such a small mass are interesting objects. Their internal arrangement is somewhat similar to the structure of giant planets, such as Jupiter. The substance of red dwarfs is in an exotic state. In addition, there are suggestions that planets that are located near such stars can be livable.
In general, red dwarfs are the most frequent stars in our galaxy. More than 80% of all the star bodies of the Milky Way are exactly them. And here is the paradox: they are completely invisible! Do not notice any of them with the naked eye.
Measurement
Until now, the ability to accurately measure the size of such small stars as red dwarfs, because of their weak luminosity, simply was not possible. But today this problem is solved with a special VLT-interferometer (VLT - short for English Very Large Telescope). This device, which operates on the basis of two large 8.2-meter VLT-telescopes located at the Paranal Astronomical Observatory (ESO). These two huge telescopes, separated by 102.4 meters, allow us to measure the celestial bodies with such precision, which simply is beyond the power of other devices. So the astronomers of the Geneva Observatory for the first time received the exact dimensions of such a small star.
The Changing Centauri
Proxima itself is a very dull celestial body. In the ordinary state, its luminosity reaches no more than 11m. Bright it looks only on pictures taken by huge telescopes, such as, for example, "Hubble". However, sometimes the brilliance of a star sharply and significantly increases. Scientists explain this fact by the fact that Proxima Centauri belongs to the class of so-called changeable, or flashing, stars. This is due to strong flares on its surface, which are the results of violent convection processes. They are somewhat similar to those that occur on the surface of the Sun, only much stronger, which leads even to a change in the brightness of the star.
Still quite a child
Many science fiction writers believe that Proxima Centauri is the most suitable star for space exploration and adventure. Some believe that in its Universe there are hidden planets on which other civilizations can be found. Maybe it is, but only the distance from Earth to Proxima Centauri is more than four light years. So, although it is the nearest, but still is far away.
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