The Life of a Star

One evening, when Jimmy and his father camped together, he asked his father how to make a star. His father says there are high quality stars, high quality stars, low quality stars. The star's life cycle follows three general patterns each associated with a series of initial masses. They will give birth, evolve and die, as human stars have a lifecycle. Little Jimmy said how this is possible. First of all, stars must be born. Many astronomers believe that stars will be formed when large compression waves passing through gas clouds create a dense gas knot with clouds.

The life cycle of a star depends on its quality. The higher the quality, the shorter the life cycle. The quality of stars depends on the mass of the material available in the nebula, the huge gas it produces and the dust cloud. Eventually hydrogen in the nebula will be drawn together by gravity and start to rotate. As the gas rotates faster, the gas is heated to become the original star. The final temperature reaches 15,000,000 degrees and nuclear fusion occurs in the center of the cloud. Clouds start to shine, shrink a little, and stabilize. It is a major binary star at present and is shining for millions to billions of years at this stage. This is the stage where our sun is now.

Scientists say that stars will be resurrected when gas clouds collapse to form the original stars. As the primitive star continues to crash, it enters the "main line" stage. This is where the stars illuminate most of the night. Main line stars have a long life under human standards but these stars will go through several cycles before they finish their lives. Hydrogen bombs and main line stars have one thing in common. They are to generate enormous amounts of energy by fusing hydrogen atoms. The sun like Sirius is the main star. The higher the quality of the main line star, the more it looks blue. For example, Sirius is bigger than the sun, but it is more blue than the sun. These types of stars have limited supply of hydrogen to supply fuel to the fusion process. When hydrogen runs out, the color of the main line star changes to red, making it a brighter superstar.

Welcome to the newborn 's life. The main sequence star is a series of stars based on size and surface temperature, from bright and blue shining stars in the upper left corner of the H - R chart to cold, dark and red stars in the lower right corner of the chart. The new star's life begins with the main flow. These mature stars experienced significant changes after consuming all the hydrogen in their cores. When hydrogen is consumed, stars expand away from the main line and form a red gigantic star. At this new stage, heavy elements such as oxygen and carbon begin to form by fusion of enamel. The expansion - collapse - expansion process of this star forms a light element present in the universe (until Fe)