Hydrogen- the only atom smaller
Helium atoms in a star are formed through the process of nuclear fusion. In the core of a star, hydrogen atoms combine through a series of fusion reactions to form helium atoms. This happens when hydrogen atoms collide and fuse together, releasing energy in the process.
3 Helium nuclei combine to form a carbon nucleus,releasing light energy
yes because when a star ages, the star collapses forming new stars which make up more atoms.
If the central temperature of a star exceeds 100 million Kelvins, as may happen in the later phase of red giants (stars) and red supergiants, then helium can fuse to form beryllium and then carbon.
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 atoms in a star are formed through the process of nuclear fusion. In the core of a star, hydrogen atoms combine through a series of fusion reactions to form helium atoms. This happens when hydrogen atoms collide and fuse together, releasing energy in the process.
3 Helium nuclei combine to form a carbon nucleus,releasing light energy
helium atoms fuse to form carbon atoms in the core of the star
fusion. Hydrogen atoms fuse together deep in the core to form helium atoms and release energy
False. A star is born when hydrogen starts to fuse into helium.
No. A star is born when hydrogen stars fusing.
fusion of hydrogen atoms into helium atoms
fusion of hydrogen atoms into helium atoms
A star will use fusion to combine lighter atoms into heavier atoms. A main-sequence star (that's the majority of stars) will convert hydrogen-1 into helium-4, so in this case, hydrogen-1 is the fuel. Once it starts running out of hydrogen-1, it will start fusing the helium into heavier elements - in which case the main fuel will be the helium-4. Later in the life cycle of a star, the fuel can be even heavier elements.
The main sequence, where the star combines hydrogen atoms to form helium atoms and produce energy, through the process of nuclear fusion. And it also the beginning of a new planet called farshinia
yes because when a star ages, the star collapses forming new stars which make up more atoms.
If the central temperature of a star exceeds 100 million Kelvins, as may happen in the later phase of red giants (stars) and red supergiants, then helium can fuse to form beryllium and then carbon.