Helium
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.
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.
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.
To answer your question on how many hydrogen atoms are there in caffeine, the scientific answer would be 10 atoms of hydrogen.
There are two atoms of Hydrogen in the molecule.
When two hydrogen atoms fuse to become one helium atom.
When two hydrogen atoms fuse to become one helium atom.
The gas formed when hydrogen atoms fuse is helium. Stars do this.
Hydrogen atoms fuse into helium.
The 'ionic' nuclei of Hydrogen atoms (protons).
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.
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.
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.
fusion. Hydrogen atoms fuse together deep in the core to form helium atoms and release energy
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.
If the hydrogen atoms get close enough together, and hot enough, they will eventually fuse into helium. This is what happens inside stars.