Answer:
Below some thoughs about sun's life cycle
Step-by-step explanation:
The sun is a massive, luminous ball of gas at the center of our solar system. It is a star, and like all stars, it is in the process of burning through the hydrogen fuel that powers it. This process, known as nuclear fusion, releases a tremendous amount of energy in the form of light and heat, which is what makes the sun shine so brightly.
The sun has been shining for billions of years, and it still has a long way to go before it reaches the end of its life cycle. Currently, the sun is in the main sequence phase of its life, during which it is fusing hydrogen into helium at its core. This phase is expected to last for another 5 billion years or so.
Over time, the sun will begin to run out of hydrogen fuel and will start to expand, eventually becoming a red giant. This will cause it to grow so large that it will swallow up the inner planets, including Earth. Eventually, the sun will shed its outer layers, leaving behind a hot, dense core known as a white dwarf.
The sun will continue to cool and fade over the next few billion years, eventually becoming a cold, dark cinder known as a black dwarf. It is not yet known if the sun will end its life in this way, or if it will undergo a more dramatic fate, such as a supernova explosion.
No matter what happens, the sun will continue to play a crucial role in the life of our solar system for billions of years to come. It provides the light and heat necessary for life on Earth, and will continue to do so until the end of its life cycle.