from energy spectrum of the of the sun
it normally done in laboratory even for finding the elements present.
The sun is mostly made of gas (around 75% hydrogen and 24% helium), with a small rocky core at its center. The intense heat and pressure at the core create nuclear reactions that power the sun's energy.
About 74% of the Sun's mass is hydrogen. This element is essential for nuclear fusion reactions that power the Sun, converting hydrogen into helium and releasing energy in the process.
It is because of the nuclear fusion reactions which power the Sun. They produce energy by converting hydrogen into helium. In fact it's more complicated than the question suggests, but that's the basic idea.
Stars are primarily made of Hydrogen gas (or Hydrogen plasma).The primary reaction in stars to produce energy is called Fusion where two Hydrogen molecules combine to produce one Helium molecule.Thus, a second common element in stars would be Helium (also usually found in plasma form).
The sun is primarily composed of hydrogen and helium, which together make up more than 90 percent of its mass. Hydrogen accounts for about 74 percent, while helium makes up approximately 24 percent. These two gases are crucial for the nuclear fusion processes that power the sun.
Hydrogen has more lifting power than helium because it is lighter. This means that a given volume of hydrogen can lift more weight than the same volume of helium.
Nuclear fusion on the sun changes hydrogen into helium. This process releases energy in the form of light and heat. It is the source of the sun's power and the reason for its brightness and warmth.
When two hydrogen atoms react, they can combine to form helium through nuclear fusion. This process releases a tremendous amount of energy and is the basis for the power source of the sun and other stars.
On earth, for power production, the most likely fuel source will be hydrogen isotopes, not helium 3
Hydrogen and helium are the most abundant elements in the universe. And stars use them for power. To put it simply, hydrogen is fused into helium, and helium into carbon. All the heavier elements are made from there up through iron. The trans-iron elements are made is a supernova. It could be argued that hydrogen and helium are the basic building blocks of other elements.
When hydrogen is converted to helium through nuclear fusion, a large amount of energy is released. This process is the main source of energy in stars like our Sun. It involves the fusion of hydrogen nuclei (protons) to form helium nuclei, releasing photons and neutrinos in the process.
A main sequence star gets its energy by fusing hydrogen-1 into helium-4.
When hydrogen atoms fuse together in the sun's core, they create helium. This process releases energy in the form of light and heat, which provides the sun's power.
Our sun gets energy from fusing hydrogen atoms with neutrons to form helium atoms.
The sun is mostly made of gas (around 75% hydrogen and 24% helium), with a small rocky core at its center. The intense heat and pressure at the core create nuclear reactions that power the sun's energy.
About 74% of the Sun's mass is hydrogen. This element is essential for nuclear fusion reactions that power the Sun, converting hydrogen into helium and releasing energy in the process.
The Sun is about 70% hydrogen, 28% helium, and 2% "other". When the Sun gets to about 50% hydrogen, the amount of helium present will seriously interfere with the hydrogen fusion, and the Sun will begin to collapse under its own gravity. The Sun's core is currently around 15 million degrees Kelvin. As the Sun collapses, the increasing pressure will heat the Sun, and when it gets to about 45 million degrees, the Sun will begin fusing helium and with the new power source will expand into a red giant. We expect this to happen in about 4 billion years, perhaps a little more.