How Does the Sun Shine, why Does the Sun Shine

How and Why Does the Sunshine?

Summary – The Sun shines every day and has been doing that for several billion years. When you wonder why it shines and how it does that, the answers are here. Read on:

The Sun has been powering life on Earth for several billion years now. It's the main – and only source – of power to all ecosystems on Earth and that is what makes life sustain here. Despite being several hundreds of millions of kilometers away from the Sun, Earth receives quite a considerable amount of energy.

While all of this is going on for several billion years, people generally don't care much about it because it's just there, right?

How does the sun shine anyway? Why does it shine? How is it that the Sun produces so much energy continuously and how is it that we receive so much energy from the Sun?

Let's take a look.

The Sun produces energy through what is popularly called nuclear fusion. Hydrogen atoms fuse at a very high temperature and pressure and form helium atoms. And this reaction produces a lot of energy. Because the temperature and pressure are high, these helium atoms undergo further fusion – and the process goes on till atoms of heavier types like carbon are produced.

All of this happens at the core of the Sun where the temperatures are in the range of 15 million Kelvin. By the time you reach the surface of the Sun, the temperature is just about 6000 K. (5700+ degrees Celsius).

The energy produced at the core of the Sun is in the form of heat and light. Light, in the form of photons, are said to take several hundred thousand years to take to reach the sun's surface. Can you imagine that? It is estimated that the energy produced as photons would take about 200,000 years to reach the surface of the sun. It's not because of the size of the sun as such but it's because of all the heat, pressure and radiation within the sun's plasma content.

Once the photos have reached the surface, they travel real fast and reach Earth within 8 minutes.

The Sun's shine – this light and heat – falls on Earth at the rate of 1000 W/m2 and this energy is what sustains life on Earth. The Sun will continue to burn fuel at its core for several million years more and it will also grow in size. In fact, the Sun has been estimated to be just half-way through its lifespan.
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