Since hydrogen atoms in the sun are fused into helium atoms, the amount of helium is increasing and the amount of hydrogen is decreasing.
The amount of hydrogen will decrease and the amount of helium will increase.
Hydrogen and helium, the most common elements in the Universe.Hydrogen and helium, the most common elements in the Universe.Hydrogen and helium, the most common elements in the Universe.Hydrogen and helium, the most common elements in the Universe.
Starts with pure hydrogen, fused to helium in increasing proportion as the sun ages.
mostly hydrogen and helium
Hydrogen and helium. Mostly hydrogen.
The sun is fusing hydrogen atoms together, turning them into helium.
The nuclear fusion in a star's core converts hydrogen into helium. Therefore the amount of hydrogen in a star is constantly decreasing.
The amount of hydrogen will decrease and the amount of helium will increase.
The amount of hydrogen will decrease and the amount of helium will increase.
The amount of hydrogen will decrease and the amount of helium will increase.
Hydrogen and Helium, with the former decreasing and the latter increasing. Rigel is fusing H into He at a prodigious rate and in a million years or so will start to collapse as its fuel runs out.
Hydrogen and helium, the most common elements in the Universe.Hydrogen and helium, the most common elements in the Universe.Hydrogen and helium, the most common elements in the Universe.Hydrogen and helium, the most common elements in the Universe.
Because Hydrogen is the fuel of Stars, hydrogen consumed and Helium is formed.
Starts with pure hydrogen, fused to helium in increasing proportion as the sun ages.
The fusion of two hydrogen atoms yielding a helium atom expels a large amount energy.
Hydrogen and a small amount of Helium.
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.