Creating a Program to Trace Binary Stars

Overview The beginning of this project is a way to determine whether two stars become binary numbers and track their predicted trajectories. The program itself grows more to draw the trajectory of the star which may be irregular but may be a binary orbit. The result starts with complete orbit of Capella C and Capella D. From there I have tested the switching speed to create different forecast maps. These charts show exactly the same information as the original message, but the only change is the starting direction.

I. The first type appears in "Double star system". "Bost star" is two stars running around the same point. One of them is a carbon-oxygen "white dwarf" (a star near the end of the year that uses most fuel and then collapses to a certain size). Fellow stars steal substances, so it accumulates too much material and causes an explosion called supernova II. When the star is exhausted, it happens at the end of the star's lifetime When this happens, a part of its mass will flow into the core, resulting in the core becoming very heavy and unable to withstand its own gravity (Due to the high quality of the core). Collapse and lead to a huge explosion "supernova"

The evolution of the main back row of binary stars may be quite different from the evolution of a single star of the same mass. If a binary star is close enough, when one star spreads to a red giant it may overflow that Roche leaf, it is the area around the star where matter is bound by gravity. On a star, the substance moves to another star. . When Roche's leaves are infringed, various phenomena including contact binary system, common envelope binary system, catastrophic variable system, and type Ia supernova can occur.

Approximately 5% of all known neutron stars are binary members. The formation and evolution of binary neutron stars can be a complex process. Neutron stars are observed with binary stars with regular main sequence stars, red giants, white dwarfs, or other neutron stars. According to modern binary evolution theory, it is expected that neutron star will also exist in a binary system with black hole's companion star. The combination of binary data including two neutron stars or neutron stars and black holes is expected to be the main cause of detectable gravitational wave emissions.