Plasma brightest celestial object is a large chunk remain with the gravity of stars near the Sun, which is the world's largest primary energy source in the world. We can see the other stars on the night sky. If there is sun avoidance. History The most prominent stars on the celestial sphere are grouped together into a constellation. And the brightest stars are named specifically. Astronomers have made many more stellar roster. To serve as a standard for naming a star throughout the life of the star. It will shine a light on the reaction thermoelectric nuclear fusion at the core of the star. The release of energy from the interior of stars. Then radiate out into space. Nearly all chemical elements heavier than helium, occur naturally and have all originated from the star. This may be due to synthesize the nucleus of the star during the star is still alive. Or the synthesis of nuclei, supernova explosions of stars after the end of its lifespan. Astronomers can determine the size of the mass, age, chemical composition. And many other properties of a star by observing the light spectrum and movement in space. The total mass of the stars in order to determine the evolution and fate at the end of a star. All other properties of a star such as diameter, rotation, movement and temperature are determined by its evolutionary history. A sequence diagram between the temperature on the brightness of the star lots. The known Diagram of NBC's Harry Cook - Russell (HR diagram) helps to identify the age and model of stellar evolution for stars formed from molecular clouds that collapse with hydrogen as the main component. The helium And other elements heavier than a certain amount. Once the stellar core is dense enough. Some hydrogen is converted into helium through nuclear fusion continues [1] of the rest of the star will take energy away from the core through the process radiant and convective heat transfer compound. The star's internal pressure prevents it from collapsing further its own gravity. When a star runs out of hydrogen fuel at its core. The star has a mass at least 0.4 times that of the Sun [2] inflate into a red giant. In some cases, These stars to fuse heavier elements at the core or in shells around the core of a red giant star then evolves into a degenerate form. Some of the material is recycled into the material between the stars. These substances give rise to a new generation of stars, which is the ratio of heavy elements than [three] binary stars and multiple star systems composed of two stars or more, which bound together by gravity. And most often revolving around each other in stable orbits. When the stars in binary systems, the two planets orbit too close. Gravitational interactions between the stars could have an enormous impact on their evolution [4] Stellar can be gathered in a large structure anchored by gravity, such as star clusters or galaxies.
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