When hydrogen atoms fuse together inside the sun, they form helium atoms through a process called nuclear fusion. This fusion process releases a tremendous amount of energy in the form of light and heat, which is what powers the sun and sustains life on Earth.
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.
Hydrogen atoms have one proton in their nuclei. When two hydrogen atoms fuse together they make one helium atom that contains two protons in its nucleus. This is called nuclear fusion, which powers the stars in the universe.
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 hydrogen nuclei fuse together, they can form helium. This fusion process is the energy source for stars, including our sun, where hydrogen nuclei combine to form helium through a series of nuclear reactions.
Nuclear fusion is the process that fuses hydrogen atoms together to form helium. This process occurs in the core of stars, including our sun, where high temperatures and pressures allow hydrogen nuclei to overcome their electrostatic repulsion and combine to form helium nuclei.
Hydrogen is in the sun, when the hydrogen atoms fuse (join together) they make helium in stars. this gives out lots of heat and light.
If the hydrogen atoms get close enough together, and hot enough, they will eventually fuse into helium. This is what happens inside stars.
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.
The gas formed when hydrogen atoms fuse is helium. Stars do this.
Hydrogen atoms fuse into helium.
fusion. Hydrogen atoms fuse together deep in the core to form helium atoms and release energy
In nuclear fusion, four hydrogen atoms fuse together to form one helium atom. This process releases a large amount of energy in the form of heat and light.
The enormous heat and pressure at the center of a star causes atoms to fuse together, releasing enormous amounts of energy. Most stars fuse hydrogen, but larger stars that have exhausted the hydrogen in their cores may fuse heavy elements.
Hydrogen atoms have one proton in their nuclei. When two hydrogen atoms fuse together they make one helium atom that contains two protons in its nucleus. This is called nuclear fusion, which powers the stars in the universe.
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.
Atoms can fuse together to form molecules or compounds.
The 'ionic' nuclei of Hydrogen atoms (protons).