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2.9.3Forces, Space and Radioactivity

Fusion

5 min read 5 parts Lesson 40 of 41 Unit quiz

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Section 1 of 5What Is Fusion?

2.9.3 Fusion

Nuclear fusion is the joining of two light nuclei to form a heavier nucleus, releasing energy.

Reactants
  • Light nuclei such as hydrogen isotopes, deuterium and tritium, are the fuels for fusion.
Product
  • Two light nuclei combine to form a larger nucleus, such as helium, and a neutron may be released.
Energy released
  • The new nucleus has slightly less mass than the starting nuclei, and the difference is released as energy.
Source of starlight
  • Fusion in the cores of stars, such as the Sun, produces the energy they radiate.

Section 2 of 5Conditions for Fusion

Conditions for Fusion
Electrostatic repulsion
  • Nuclei are positively charged, so they repel each other strongly when they are close together.
High temperature
  • Millions of degrees are needed so that nuclei move fast enough to overcome the repulsion and collide.
High pressure
  • Extreme pressure keeps the nuclei close together so collisions happen often enough to sustain the reaction.
Plasma
  • At these temperatures atoms lose their electrons, forming a hot gas of charged particles called plasma.

Section 3 of 5Fusion Power on Earth

1
Scientists heat a small amount of deuterium and tritium to over a hundred million degrees in a doughnut-shaped reactor.
2
Strong magnetic fields hold the hot plasma away from the walls, because no material could contain it directly.
3
The nuclei fuse, and the neutrons released carry energy that could be used to produce steam.
4
So far, experimental reactors use more energy to run than they produce for any sustained period.
5
If fusion can be made to work, it would provide a large energy supply with little long-lived radioactive waste.

Section 4 of 5Fusion Compared with Fission

Fusion Compared with Fission
Fuel
  • Fusion uses hydrogen isotopes, which are abundant in sea water, while fission uses rarer uranium or plutonium.
Waste
  • Fusion produces far less long-lived radioactive waste than fission.
Safety
  • Fusion cannot run away as a chain reaction, since the conditions are hard to maintain.
Development
  • Fission power stations are in use today, but fusion remains experimental.
FeatureFissionFusion
ProcessLarge nucleus splitsSmall nuclei join
ConditionsNeutron neededExtreme heat and pressure
Current usePower stationsExperimental

Section 5 of 5Exam Checklist & Tips

2.9.3 – Key Points for the Exam

  • Nuclear fusion The joining of two light nuclei to form a heavier nucleus.
  • Plasma A very hot gas in which the atoms have lost electrons.
  • Deuterium An isotope of hydrogen with one proton and one neutron.
  • Tritium An isotope of hydrogen with one proton and two neutrons.

Common Mistakes

  • Mixing up fission and fusion; fission splits large nuclei and fusion joins small nuclei.
  • Forgetting that nuclei repel each other, which is why fusion needs such high temperatures.
  • Saying that fusion happens in a nuclear power station today; it is not yet a commercial energy source.
  • Thinking the energy comes from the nuclei burning; it comes from a small loss of mass.
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