STARS EVOLUTION


Life of stars like Sun is about 10 billion years. During the evolution, stars are steady because there are two forces: gravity attraction and nuclear fusion pressure. Gravity attraction compress the star and nuclear fusion pressure push the gas out.

This balance is very important!

Star is like thermostat because if gravity grow up, for a decreasing of nuclear temperature, then star contract itself and less volume causes raising temperature and then so nuclear pressure raises up. Balance is established. In the other case, when nuclear fusion pressure raise up there is a raising mass star and then a raising gravity attraction because mass is related with gravity attraction.

This "thermostat" works until star blows hydrogen. After, when hydrogen ends, star becames a change.


Gravity attraction and nuclear fusion pressure work as "thermostat".


Fisic structure

Stars are like an onion. There are several layers rounds them. In the center there is a part called "Core" and it is nucleus of stars. In this zone temperature is about 15.000.000 °C (in a Sun like star) and hydrogen change into elium by the nuclear fusion process. Light spends thounsands of years to came from the nucleus to our eyes because inside layers are dull to light energy.

Stars give out energy on the entire spectrum. Infact stars give out visible light, X ray, infrared ray, gamma ray and radio waves. Arond the stars, moreover, occurs many magnetic storms and Sun is an example because with its magnetic storms breakes down our satellites in orbit around the earth. From the stars' nucleus give out "neutrins" particles that have a very small mass and they have produced in the nuclear fusion process.

When hydrogen runs out then start a new moment for the star.

...How stars die


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