What is a binary stellar system?

The binary stellar system is a stellar system with two stars orbiting you. More star systems such as three, etc., are also usually categorized using the same term. Star systems with up to seven -oriented bodies have been classified.

It is assumed that binary star systems are quite common in space and can actually be in most. This is because a cloud of dust that collapses, has stars, often has more than one center of gravity. If they are small clusters, they form planets or brown dwarves, if they are large, forms stars. Binary stars are considered to be mutual accompanying stars.

Binary stellar systems are very important in astronomy because mapping their mutual pathways makes it possible to estimate their mass. Estimating matter is useful for contrast with temperature and obvious luminosity, which helps us determine absolute luminosity and distance. Eclipse binary files where stars in the binary system of our P are regularly burdenedThe respects are particularly useful. The way the eclipse can be used to estimate their size, density, luminance and distance. Eclipsing binary files have been used to measure distance from other galaxies, such as Andromeda Galaxy and Triangulum Galaxy, with an error factor less than 5%.

The nearest stellar system, Alpha Centauri, is a binary star system that consists of two narrowly orbiting stars of the Sun -oriented Red Dwarf -oriented Star. Two central stars have an elliptical orbit around them, reaching 11 AU and separating up to 35 AU and creating a complete cycle every 80 years. Due to the chaotic dynamics of such a system, there is no real "habitable zone" where surface temperatures remain roughly constant. Surface temperature is from year to year.