Assembly diagram of the solar bracket of Sun Rain

What is the structure of the Sun made of?

The Sun is not only made of the glowing gas that we see with a telescope. It has, exactly like the Earth, different layers at different temperatures. Every layer has its own features which makes them interesting. Below is a figure of the structure of the Sun with all the different layers and components named.

What are the different layers of the Sun?

The names of these layers, in order of their presence from the core of the sun are as follows: Inner Layers 1) Core 2) Radiative Zone 3) Convection Zone Outer Layers 1) Photosphere 2) Chromosphere 3) Transition Region 4) Corona It forms the regions on or around the central core that acts as the energy-generating center of the sun.

What are the parts of the inner layer of the Sun?

The parts of the inner layer are: 1. Core Temperature: 15,000,000 Kelvin Density: 150,000 g/cm 3 (150 times as dense as water) It is the innermost layer of the sun, which is extremely dense where nuclear fusion generates energy in terms of photons by converting hydrogen into helium.

What are the different parts of the Sun?

Parts of the Sun: This illustration shows the different parts of the Sun, from the hot core where the energy is generated through regions where energy is transported outward, first by radiation, then by convection, and then out through the solar atmosphere. The parts of the atmosphere are also labeled the photosphere, chromosphere, and corona.

What is the chemical composition of the Sun?

The Sun is primarily composed of hydrogen and helium. The chemical composition changes in the layers as it moves further from the core. The layers are shown above in the structure of the sun diagram. The core is approximately 64% helium, surrounded by shell-fusing hydrogen which accounts for 35% of the core's mass.

What are solar prominences?

Solar prominences are immense clouds of relatively cooler, dense plasma suspended above the Sun’s surface by the Sun’s magnetic field. They appear as bright, loop-like structures when viewed against the dark backdrop of space, but as dark filaments against the bright solar disk. Where They Occur: