yes because when a star ages, the star collapses forming new stars which make up more atoms.
Hydrogen atoms are used to produce helium atoms with larger masses in nuclear fusion. During the fusion process, hydrogen isotopes (such as deuterium and tritium) combine to form helium, releasing vast amounts of energy in the process. Oxygen atoms are not typically involved in nuclear fusion reactions to produce helium.
Normal "main sequence" stars fuse hydrogen into helium during most of the star's life. The core of a star gets so hot that the hydrogen atoms begin to fuse together. As hydrogen only has 1 proton when if fuses with another hydrogen atom it has 2 protons so has become helium.
helium as it contains 2 protons, while hydrogen only contains 1. Additionally, the orbit of the 2 electrons in a neutral helium atom would also be larger than the orbit of the single electron in hydrogen.
The reactants are Hydrogen atoms and products are Helium atoms. Because Helium atoms are larger than Hydrogen atom, large amount of energy is released from the net binding energy that resulted during the fusion process.
An equal mass of helium would contain fewer atoms compared to hydrogen, as each helium atom is four times heavier than a hydrogen atom. This is because the atomic mass of a helium atom is roughly four times that of a hydrogen atom.
Hydrogen atoms are used to produce helium atoms with larger masses in nuclear fusion. During the fusion process, hydrogen isotopes (such as deuterium and tritium) combine to form helium, releasing vast amounts of energy in the process. Oxygen atoms are not typically involved in nuclear fusion reactions to produce helium.
Hydrogen atoms fuse to become helium atoms during the process of nuclear fusion in stars. This process releases a large amount of energy and is the source of the sun's energy.
When two hydrogen atoms fuse to become one helium atom.
In nuclear fusion, atoms of hydrogen isotopes such as deuterium and tritium are used to produce helium atoms with larger masses. The fusion reaction involves the combination of these hydrogen isotopes to form helium, releasing a significant amount of energy in the process.
When two hydrogen atoms fuse to become one helium atom.
The two main categories are (1) fusion: joining small atoms into larger atoms, such as hydrogen-1 into helium-4, and (2) fission, the splitting of certain large atoms, such as U-235.The two main categories are (1) fusion: joining small atoms into larger atoms, such as hydrogen-1 into helium-4, and (2) fission, the splitting of certain large atoms, such as U-235.The two main categories are (1) fusion: joining small atoms into larger atoms, such as hydrogen-1 into helium-4, and (2) fission, the splitting of certain large atoms, such as U-235.The two main categories are (1) fusion: joining small atoms into larger atoms, such as hydrogen-1 into helium-4, and (2) fission, the splitting of certain large atoms, such as U-235.
Hydrogen atoms fuse into helium.
10g of helium has fewer atoms. This is because the atomic mass of helium is much higher than that of hydrogen, so the same mass of helium contains fewer atoms than the same mass of hydrogen.
Normal "main sequence" stars fuse hydrogen into helium during most of the star's life. The core of a star gets so hot that the hydrogen atoms begin to fuse together. As hydrogen only has 1 proton when if fuses with another hydrogen atom it has 2 protons so has become helium.
Hydrogen and helium make about 98% of the atoms in the solar system !
helium atoms
The sun fuses hydrogen atoms to produce helium atoms in its core through a process called nuclear fusion. This process generates a tremendous amount of energy in the form of light and heat, which sustains life on Earth.