Sun will continue to expand up to half its mass is lost into space. However, this temperature is still able to push the release of the exterior of the Sun is composed of hydrogen and helium from the core. Carbon in the core of the Sun can not be burnt by the sun-sized star will not be able to produce heat that can burn carbon. At this stage, the sun began to enter the dying phase. The process is ongoing encouragement repeatedly until the outside of the Sun seems to be in layers. As a result, the core becomes unstable and in a short time into a super hot to encourage further solar blankets quickly. However, very high temperatures is not easily released into the solar blanket.

At that temperature, will burn helium into carbon and oxygen. During development, the core of the Sun continued to shrink until its temperature reaches 100 million K.

However, when that happens, most of the Earth is about to evaporate first. In the development of both a red giant star which is larger, the Earth will be swallowed by the Sun. This condition makes the sun more and expand until its radius reaches 1,000 times the original radius of the Sun.

The burning of hydrogen into helium in the solar blanket will make a blanket temperature increased. Although the temperature dropped to 3500 K, the temperature was still significant enough to trigger a drastic temperature rise on Venus and Earth. Swallowing planets around Deployment sun will swallow Mercury, a distance of 58 million kilometers. Development that affects the Sun's surface temperature drop as indicated by the color of the star changes from whitish yellow to red. In this phase, the judge continued, the Sun evolve into a red giant star. Burning hydrogen in the core blanket will make the outer layer of the Sun expands until its radius reaches 10-100 times its original radius. As a result, hydrogen in the blanket core (outer layer), the Sun will burn. However, this depreciation will increase the temperature of the Sun's core. The absence of energy that sustains the core makes the core of the Sun is shrinking. However, the core of the Sun has not had a temperature sufficient to burn helium in need at 100 million K. In 5 billion years into the future, hydrogen in the core of the Sun is expected to burn into helium. Core temperature is much different from the Sun's surface temperature is only around 5500 K-6000 K. The temperature has now reached 15 million K. Sun's core Sun's core size is only 10 percent of the overall solar ball. 'We started burning hydrogen will be a sign of the birth of the Sun,' said professor of stellar evolution Astronomy Study Program Institut Teknologi Bandung, Judge L sit. When the infant sun's core temperature reaches 10 million K, the burning of hydrogen into helium was in progress. The new radius of about half a radius of the Sun today. At that time, the temperature of the Sun is 150,000 K and emitting red light from the gravitational energy globule, not a nuclear reaction at its core. This radiation makes the material compression process to slow down until the process of gravitational collapse may be resisted. Compression is followed by an increase in core temperature that allows the globule globule emit radiation. When certain parts of the giant cloud of disturbed balance, that part will experience compression and eventually collapse and form a globule (dense clouds). In comparison, the distance between the Earth and the Sun is only 8 minutes of light. The cloud stretched as far as 480 trillion kilometers (50 light years). The sun formed from giant clouds of gas and contains a very tenuous atomic particles with a temperature of 3 degrees Kelvin (K) or minus 270 degrees Celsius. An estimated 5 billion years from now, the Sun will evolve into a red giant star radius can reach 1,000 times the radius of the Sun today. Since its birth 4.6 billion years ago, until now 37 percent hydrogen which is the main fuel the Sun has burned into helium.

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