الشمس كرة من غازات ملتهبة وقودها الذرة .. في سبيل موسوعة علمية .. الدكتور أحمد ذكي

The sun is a ball of fiery gases fueled by corn

It's a ball of inflamed gases, the most intense
The temperature at its surface is thousands of degrees, and this temperature increases the deeper we go into the interior of the sun, until when we reach the core we find that it has reached about 14 million degrees Celsius, and we find that the pressure of the gases there has increased until it reaches 220 thousand million atmospheric pressures.

There is no fuel in the world that gives this heat other than nuclear fuel. This heat results from the transformation of the hydrogen gas contained in the sun into helium gas, by an atomic reaction, not in which the atom is split as happens in the element uranium, but by the reaction in which the nucleus of the atom fuses with the nucleus of the atom, the hydrogen atom with the hydrogen atom, to produce helium gas, and with it large amounts of... the heat .

They estimate that the sun (burns) in about a second
564 million tons of hydrogen produces helium, and thus it releases as much energy as a few thousand millions of hydrogen bombs produce when they are detonated.

Scientists calculated that they found that if an amount of the sun's hydrogen is transformed, it is equivalent to one percent of its weight
to

(A picture of spots on the sun, in its niter disk, and they are standing in relation to the flammable gases around them. The reason for this is that they are less flammable, so they appear as if they are standing. This picture was taken from a balloon that scientists raised in the Earth’s atmosphere to the layer of air known as the stratosphere to be clearer, because The decrease in the earth's air between it and the sun.)

Helium, this will be enough to provide it with the energy that will make it continue to illuminate for another thousand million years.
It is God’s blessing that the sun “burns” its fuel only to the extent that compensates for the energy it loses through radiation. Scientists have no evidence that the sun is getting hotter or colder over the years.

The sun is the closest star to us:

The sun is the closest star to us, but it is one of the yellowest stars and one of the least luminous stars. Rather, He fills us with immensity and fills us with light, due to His proximity to us.

The star closest to us in distance from the sun is 300,000 times as far away from us as the sun is from us. The average distance of the sun from us is 93,000,000 miles.

- The sun’s luminous disk, Photosphere:

It is the bright disc that the eye sees, as deep as it can see. From it comes enormous sunlight, and the temperature of this surface reaches about 6000 degrees Celsius, and it drops slightly towards the edges of the disk.
The disk appears with a telescope as if it is composed of a granular surface, which are bright grains that cover about a third of the surface. The diameter of the grain is about 700 miles. It results from the eruption of very hot gases emerging from the depths of the sun. After a few minutes, the effervescent pill cools down and descends to the temperature of the surrounding surface areas.

Brighter areas appear on this surface, branching and ramifying. Some have called them solar faculae.

(One of the galaxies in the sky. It is the galaxy known by its symbol Messier 51)