Why Does Iron Mark the Limit for Energy-Producing Fusion in Stars?

In summary, the buildup of heavier elements in the nuclear fusion processes in stars is limited to elements below iron due to the fact that fusion of iron would consume energy instead of producing it. This is because the ratio of atomic mass to number of nucleons is at its minimum for iron, making both fusion and fission processes for iron require energy input rather than releasing energy. This may seem contradictory, but the key is understanding the differences between fusion and fission and their effects on different elements.
  • #1
ay2k
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The buildup of heavier elements in the nuclear fusion processes in stars is limited to elements below iron, since the fusion of iron would subtract energy rather than provide it



The fusion of two nuclei lighter than iron generally releases energy while the fusion of nuclei heavier than iron absorbs energy; vice-versa for the reverse process, nuclear fission.

These two statements semm contradictory. Which one is actually correct? If both are actually correct, can someone please explain that what is the point that I am missing?
 
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  • #2
They are not contradictory. The basic idea is that ratio of atomic mass to number of nucleons is at the minimum for iron.

The point is that fusion of elements lighter than iron releases energy, while fission of elements heavier than iron releases energy. For iron both processes require energy input.
 
  • #3


Both statements are actually correct and they are not contradictory. This is because the energy released or absorbed during fusion or fission reactions is determined by the concept of binding energy.

Binding energy is the amount of energy required to hold the nucleus of an atom together. It is the result of the strong nuclear force, which is the strongest force in nature and holds protons and neutrons together in the nucleus. The stronger the binding energy, the more stable the nucleus is.

In nuclear fusion, lighter elements combine to form heavier elements, releasing energy in the process. This is because the resulting nucleus has a higher binding energy than the individual nuclei that fused together. This is why fusion reactions up to iron release energy.

However, when heavier elements are fused, the resulting nucleus has a lower binding energy than the individual nuclei that fused together. This means that energy is actually required to hold the nucleus together, resulting in a net energy loss. This is why fusion reactions beyond iron absorb energy.

On the other hand, in nuclear fission, a heavy nucleus splits into smaller nuclei, releasing energy. This is because the resulting nuclei have a higher binding energy than the original nucleus. However, when lighter elements undergo fission, the resulting nuclei have a lower binding energy and energy is required to hold them together, resulting in a net energy loss.

Therefore, it is not a matter of one statement being correct and the other being incorrect, but rather understanding that the concept of binding energy plays a crucial role in determining the energy released or absorbed during nuclear fusion and fission reactions.
 

1. What is binding energy?

Binding energy is the amount of energy required to keep the nucleus of an atom together. It is essentially the "glue" that holds the protons and neutrons together in the nucleus.

2. How is binding energy measured?

Binding energy is measured in units of energy, typically either electron volts (eV) or kilojoules per mole (kJ/mol). It can be calculated by subtracting the mass of the separated nucleons (protons and neutrons) from the mass of the nucleus, and converting the mass difference into energy using Einstein's famous equation, E=mc^2.

3. What is nuclear fusion?

Nuclear fusion is the process of combining two or more atomic nuclei to form a heavier nucleus. This process releases a tremendous amount of energy, and is the same process that powers the sun and other stars.

4. How does binding energy play a role in nuclear fusion?

In nuclear fusion, the nuclei of atoms are brought close enough together that the strong nuclear force overcomes the repulsive electromagnetic force between the positively-charged protons. This results in the nuclei fusing together to form a heavier nucleus, releasing a large amount of energy in the process. This energy is the result of the conversion of some of the mass of the nuclei into energy, as described by Einstein's equation.

5. What are the potential applications of binding energy and fusion?

One potential application of fusion is as a source of clean and nearly limitless energy. If fusion reactions can be harnessed and controlled on Earth, it could provide a virtually unlimited source of energy without producing harmful radioactive waste. However, there are still significant technical challenges to overcome before fusion can be a viable energy source.

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