Grade by Grade
D. Energy and Society · Thermal and Nuclear Energy

Nuclear Fission and Nuclear Fusion

D3.6 D2.1 A1.10About 70 minutes
Learning goals
  • I can describe nuclear fission and write a balanced fission equation.
  • I can explain how a chain reaction works and how it can be controlled.
  • I can describe nuclear fusion, including the fusion that powers the Sun and deuterium-tritium fusion.
  • I can compare fission and fusion: fuels, conditions, products, energy and challenges.

Words to know

nuclear fission
The splitting of a heavy nucleus (such as uranium-235) into two medium-sized nuclei, releasing neutrons and a large amount of energy.
nuclear fusion
The joining of two light nuclei (such as deuterium and tritium) into a heavier nucleus, releasing a large amount of energy.
chain reaction
A self-sustaining series of fissions in which neutrons from each fission cause more fissions.
critical mass
The smallest amount of fissionable material that can sustain a chain reaction.
binding energy
The energy needed to separate a nucleus into its individual protons and neutrons. More binding energy per nucleon means a more stable nucleus.
plasma
A very hot state of matter in which electrons are stripped from atoms, leaving a gas of charged particles. Fusion happens in plasma.

The same energy source, two ways

About half of Ontario's electricity comes from nuclear fission: splitting uranium nuclei in reactors at Pickering, Darlington and Bruce. The sunlight that grows the maple trees and melts the snow in spring comes from nuclear fusion: joining hydrogen nuclei deep inside the Sun.

One process splits big nuclei apart; the other squeezes small nuclei together. Yet both release energy. How can that be? This lesson explains it, and compares the two.

Why both can release energy

In The Nucleus and Isotopes you learned that the strong nuclear force holds nucleons together. The binding energy of a nucleus is the energy you would need to pull it completely apart into separate protons and neutrons. The larger the binding energy per nucleon, the more tightly bound and stable the nucleus.

Binding energy per nucleon is highest for medium-sized nuclei around iron-56. It is lower for very light nuclei and lower again for very heavy ones.

  • If a heavy nucleus like uranium splits into two medium nuclei, the products are more tightly bound. The difference is released as energy: fission.
  • If two very light nuclei like hydrogen isotopes join to form helium, the product is more tightly bound. Again energy is released: fusion.

In both cases the products have slightly less mass than the starting particles. The missing mass has become energy, as described by Einstein's E = mc², which you work with in the sibling unit Work, Energy and Power.

040801201602002400246810mass number, Abinding energy per nucleon (MeV)H-2Fe-56 (near the peak)U-235He-4fusionfission
Binding energy per nucleon peaks near iron-56. Light nuclei release energy by fusing toward the peak; heavy nuclei release energy by splitting toward it. (Approximate values.)

Nuclear fission

Uranium-235 can be split by a slow-moving neutron. The neutron is absorbed, making uranium-236, which is so unstable that it wobbles and splits, usually within a tiny fraction of a second, into two medium-sized nuclei called fission fragments. It also releases 2 or 3 new neutrons and a large amount of energy (about 200 MeV per fission), mostly as kinetic energy of the fragments. One typical fission is:

¹₀n + ²³⁵₉₂U → ¹⁴¹₅₆Ba + ⁹²₃₆Kr + 3 ¹₀n + energy

Check: mass numbers 1 + 235 = 141 + 92 + 3 = 236 ✓; atomic numbers 0 + 92 = 56 + 36 + 0 = 92 ✓.

The fragments are not always barium and krypton; many different pairs are possible. The fragments are usually radioactive (they have too many neutrons), which is why used reactor fuel is highly radioactive.

nslowneutronU-235U-236(unstable)Ba-141Kr-92nnn3 fastneutronscan splitmore U-235+ energy (about 200 MeV)
Fission of uranium-235. A slow neutron is absorbed, the nucleus splits into two fragments, and three fast neutrons and a large amount of energy are released.

Chain reactions

Each fission releases 2 or 3 neutrons. If, on average, at least one of them causes another fission, the process keeps itself going: a chain reaction.

  • If each fission causes exactly one more fission on average, the reaction runs at a steady rate. This is what a nuclear reactor does.
  • If each fission causes more than one, the number of fissions grows extremely fast. This is uncontrolled.
  • If each causes fewer than one, the reaction dies out.

A chain reaction needs enough fissionable material packed closely together, the critical mass; otherwise too many neutrons escape. Reactors control the reaction with control rods or other devices made of materials that absorb neutrons (such as cadmium or boron), and with a moderator that slows neutrons down so U-235 can capture them. You will see how a CANDU reactor does this in The CANDU Reactor: Inside a Nuclear Power Plant.

n1 fission2 fissions4 fissions8 fissions... and it keepsdoubling unlessneutrons areabsorbed
A chain reaction in which each fission leads to two more. The number of fissions doubles every step: 1, 2, 4, 8... A reactor absorbs the extra neutrons so that each fission causes only one more.
Worked example

Example 1: Balancing a fission equation

Find the missing fragment: ¹₀n + ²³⁵₉₂U → ¹⁴⁰₅₄Xe + X + 2 ¹₀n

  1. Mass numbers: left side 1 + 235 = 236. Right side 140 + A + 2(1). So 236 = 142 + A, giving A = 94.
  2. Atomic numbers: left side 0 + 92 = 92. Right side 54 + Z + 2(0). So Z = 38, which is strontium (Sr).
  3. X = ⁹⁴₃₈Sr.

The missing fragment is strontium-94.

Nuclear fusion

In fusion, two light nuclei join to form a heavier one. Both nuclei are positively charged, so they repel strongly. To get close enough for the strong force to grab them, they must collide at enormous speeds, which means extremely high temperatures (millions of degrees) and high density. At these temperatures matter is a plasma.

In the Sun: gravity squeezes the core to very high density, and the temperature is about 15 million °C. In a series of steps, hydrogen nuclei (protons) fuse to make helium-4. Overall, four hydrogen nuclei become one helium nucleus, and the lost mass becomes the energy that eventually reaches Earth as sunlight.

In fusion research on Earth, the easiest reaction is deuterium-tritium (D-T) fusion:

²₁H + ³₁H → ⁴₂He + ¹₀n + energy (17.6 MeV)

Check: 2 + 3 = 4 + 1 ✓ and 1 + 1 = 2 + 0 ✓.

Scientists in many countries, including the large international ITER project being built in France, are working to hold a plasma hot enough, dense enough and long enough to produce more energy than it takes to run. This has not yet been achieved in a power plant. Hydrogen bombs use uncontrolled fusion; controlled fusion for electricity is still in the research stage.

+ndeuterium²₁H++nntritium³₁Hneeds very hightemperatureand pressure++nnhelium-4⁴₂He+nneutron¹₀n+energy(17.6 MeV)+protonnneutron
Deuterium-tritium fusion. The two nuclei join to form helium-4 and a neutron, releasing 17.6 MeV, which is several times more energy per kilogram of fuel than fission.
FissionFusion
What happensa heavy nucleus splits into two medium nucleitwo light nuclei join into a heavier nucleus
Typical fueluranium-235 (also plutonium-239)deuterium and tritium (in the Sun: ordinary hydrogen)
How it startsabsorbing a slow neutronvery high temperature and pressure (plasma)
Energy per reactionabout 200 MeVabout 17.6 MeV (D-T)
Energy per kilogram of fuelenormous: millions of times more than burning fueleven greater: several times more than fission
Productsradioactive fission fragments, neutronshelium (not radioactive) and neutrons; neutrons can make reactor materials radioactive
Status for electricityused in power plants since the 1950s; about half of Ontario's electricitystill experimental
Main challengeslong-lived radioactive waste; safety; costreaching and containing the conditions; tritium supply; cost
Comparing fission and fusion (expectation D3.6).
Worked example

Example 2: Fission or fusion?

Classify each reaction and explain. (a) ²₁H + ²₁H → ³₂He + ¹₀n (b) ¹₀n + ²³⁹₉₄Pu → ¹³⁴₅₄Xe + ¹⁰³₄₀Zr + 3 ¹₀n

  1. (a) Two light nuclei (deuterium) join to make a heavier one (helium-3): fusion. Check: 2 + 2 = 3 + 1, 1 + 1 = 2 + 0.
  2. (b) A heavy nucleus (plutonium-239) absorbs a neutron and splits into two medium nuclei plus neutrons: fission. Check: 1 + 239 = 134 + 103 + 3 = 240; 94 = 54 + 40.

(a) fusion; (b) fission.

Just for fun

Every second, the Sun turns about 4 million tonnes of its mass into energy by fusion. Don't worry: it is so massive that it has been doing this for about 4.6 billion years and still has billions of years of hydrogen left. Talk about a long-lasting battery.

Hands-on activity

Domino chain reaction

You need: about 30 dominoes (or small blocks, or index cards folded into tents), a table and a phone timer.

  1. Model 1: a single line. Stand 15 dominoes in a straight line, about 2 cm apart. Push the first one and time how long it takes for all to fall. This is like a reaction where each fission causes exactly one more.
  2. Model 2: a branching chain. Arrange dominoes so that each domino knocks down two dominoes in the next row: 1, then 2, then 4, then 8 (15 dominoes in all). Push the first one and time it.
  3. Compare: which model knocked down 15 dominoes faster? Why?
  4. Control rods. Rebuild Model 2 and remove a few dominoes from the middle rows so that, on average, each falling domino knocks down only one more. What happens? What part of a reactor did you just model?
  5. Write two ways in which dominoes are not like real fission (for example, real neutrons move randomly in all directions and some escape; real fission releases energy, while dominoes only release energy that you stored when you stood them up).

What to look for: the branching model falls much faster because the number of falling dominoes doubles each row. Removing dominoes models control rods absorbing neutrons.

Your turn

1

What is the difference between fission and fusion?

2

Why must a neutron be used to start uranium-235 fission, rather than a proton?

3

Find X: ¹₀n + ²³⁵₉₂U → ¹⁴⁴₅₆Ba + ⁸⁹₃₆Kr + X ¹₀n.

4

What is a chain reaction?

5

Why does fusion need extremely high temperatures?

6

Balance: ²₁H + ³₁H → ⁴₂He + X.

7

Which nuclei have the highest binding energy per nucleon?

More practice: warm-up

1

What powers the Sun?

2

Which process is used in Ontario's nuclear power plants?

3

What do control rods do?

4

What is plasma?

5

Name the two hydrogen isotopes used in D-T fusion.

More practice: on your own

1

Find X: ¹₀n + ²³⁵₉₂U → X + ⁹¹₃₆Kr + 3 ¹₀n.

2

Explain why both fission of uranium and fusion of hydrogen release energy, using binding energy per nucleon.

3

What is critical mass, and why does a small lump of uranium-235 not sustain a chain reaction?

4

Give two reasons fusion would be attractive for producing electricity, and one reason it is not yet used.

5

Why are fission fragments usually radioactive?

Challenge

1

Suppose each fission in a sample causes, on average, 2 more fissions, and each step takes 10⁻⁸ s. How many fissions happen in the 50th step? About how long does it take to reach it? Why does this show the need for control?

2

One D-T fusion releases 17.6 MeV and involves 5 nucleons. One U-235 fission releases about 200 MeV and involves 236 nucleons. Compare the energy released per nucleon. What does this suggest about energy per kilogram of fuel?

3

A student says, "Fusion and fission are opposites, so one must absorb energy and the other release it." Explain why the student is wrong.

Check your understanding

Quiz

1.

Nuclear fission is:

2.

Which process produces the Sun's energy?

3.

In ¹₀n + ²³⁵₉₂U → ¹³⁷₅₂Te + X + 2 ¹₀n, what is X?

4.

What keeps a reactor's chain reaction steady?

5.

Why does fusion require extremely high temperatures?

6.

Which statement correctly compares fission and fusion?

For parents and teachers

Big idea: expectation D3.6 asks students to describe and compare nuclear fission and fusion. The unifying idea is binding energy per nucleon: energy is released when nuclei move toward iron-56, either by splitting heavy nuclei or by joining light ones. (The mass-energy calculations with E = mc² belong to the sibling unit Work, Energy and Power.)

How to help: Ask your teen to explain the domino model and what each part represents. Have them balance a fission equation aloud: tops add up, bottoms add up, and do not forget the neutrons.

Common difficulties:

  • Forgetting the extra neutrons when balancing fission equations.
  • Thinking fission and fusion must be opposites in energy.
  • Confusing fission (splitting) with radioactive decay (a nucleus emitting a small particle on its own).
  • Thinking fusion is already used in power plants.

Sensitive topic note: students may ask about nuclear weapons. It is accurate to say that uncontrolled fission and fusion are used in weapons; the course focuses on controlled uses and their impacts.