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Honors Chemistry Unit 13 Review: Nuclear Chemistry

Nuclear chemistry is about what happens inside the nucleus, where unstable atoms decay and nuclei can split or fuse, releasing far more energy per gram of material than chemical reactions do. After this unit, you should be able to balance nuclear equations, compare types of radiation, explain fission and fusion, and solve half-life problems.

Read the big ideas first, then work through each topic's notes and try the checkpoint question before moving on.

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What is Honors Chemistry unit 13?

Most chemical reactions involve changes in electron arrangement while the nuclei stay the same. This unit focuses on the nucleus, where protons and neutrons can rearrange and one element can change into another.

Honors Chemistry Unit 13 covers nuclear chemistry. You learn the main types of radioactive decay (alpha, beta, gamma, plus positron emission and electron capture) and how to write and balance nuclear equations by conserving mass number and atomic number. You also learn how ionizing radiation affects living tissue and how it's used in medicine and industry, and how fission and fusion release energy through E=mc2E = mc^2. The unit ends with half-life, the time it takes for half of a radioactive sample to decay, which you'll use in calculations and in radiometric dating like carbon-14.

Unstable nuclei decay in predictable ways.

Each decay mode changes the nucleus by a set amount. Alpha emission lowers the mass number by 4 and the atomic number by 2, beta-minus emission raises the atomic number by 1, and gamma emission changes neither. Once the decay mode is given, you can use these rules to identify the daughter nuclide.

Radiation can be harmful and useful at the same time.

Ionizing radiation can remove electrons from atoms and damage DNA, which makes high doses harmful. Controlled doses can treat cancer or sterilize supplies. In medical imaging, detectors locate radiation emitted by a tracer to show where it travels in the body.

Nuclear reactions turn a small amount of mass into a huge amount of energy.

In fission and fusion, the products have slightly less total mass than the reactants. That mass difference becomes energy through E=mc2E = mc^2. Per gram of fuel, a nuclear reaction releases millions of times more energy than burning coal or gasoline.

The nucleus follows its own rules, and you can predict them.

In nuclear equations, total mass number and electric charge balance. Many spontaneous nuclear changes release energy because the products have less total rest mass, and a large sample decays at a rate set by the isotope's half-life.

Under ordinary conditions, temperature and pressure have almost no effect on decay rates. Chemical environment can slightly affect decay modes that involve atomic electrons, such as electron capture. If you can balance a nuclear equation and count half-lives, you can handle most problems in this unit.

Honors Chemistry unit 13 topics

Unit 13 review notes

13.1

Types of Radioactivity and Nuclear Reactions

Radioactivity happens when an unstable nucleus breaks down on its own and gives off particles or energy. A nucleus is usually unstable because its neutron-to-proton ratio is off or because it is too large. No element with an atomic number greater than 82 has a stable isotope. Bismuth-209 is radioactive, but its half-life is extremely long.

The three decay types you'll use most change the nucleus in set ways. Alpha decay ejects 24He^{4}_{2}\text{He}, so the mass number drops by 4 and the atomic number drops by 2. Beta decay turns a neutron into a proton and ejects an electron, −10e^{0}_{-1}\text{e}, so the atomic number rises by 1 and the mass number stays the same. Gamma emission releases a high-energy photon, 00γ^{0}_{0}\gamma, which changes neither number. Positron emission (+10e^{0}_{+1}\text{e}) and electron capture both lower the atomic number by 1.

Unlike a chemical reaction, a nuclear reaction can turn one element into another. This is called transmutation. To balance a nuclear equation, the top numbers (mass) must add up the same on both sides, and so must the bottom numbers (charge).

Worked example. Uranium-238 undergoes alpha decay. What forms? The mass number is 238−4=234238 - 4 = 234. The atomic number is 92−2=9092 - 2 = 90, which is thorium. So 92238U→90234Th+24He^{238}_{92}\text{U} \rightarrow ^{234}_{90}\text{Th} + ^{4}_{2}\text{He}. To check, confirm that 238=234+4238 = 234 + 4 and 92=90+292 = 90 + 2.

  • Mass number (A): Mass number is the total number of protons and neutrons in a nucleus, and it is written as the top number in nuclear notation.
  • Atomic number (Z): Atomic number is the number of protons in a nucleus, and it is written as the bottom number and decides which element the atom is.
  • Transmutation: Transmutation is the change of one element into another through a nuclear reaction.
  • Positron: A positron is a particle that has the mass of an electron but a +1 charge, and it is written +10e^{0}_{+1}\text{e}.

Check yourself. Carbon-14 undergoes beta decay. What is the product? (Answer: Nitrogen-14. The mass number stays 14 and the atomic number goes from 6 to 7, so 614C→714N+−10e^{14}_{6}\text{C} \rightarrow ^{14}_{7}\text{N} + ^{0}_{-1}\text{e}.)

RadiationSymbolChange in mass numberChange in atomic numberTypical shielding
Alpha$^{4}_{2}\text{He}$Decreases by 4Decreases by 2Paper, clothing, or the outer layer of skin
Beta$^{0}_{-1}\text{e}$No changeIncreases by 1Plastic or thin metal
Positron$^{0}_{+1}\text{e}$No changeDecreases by 1Plastic or another low-Z material stops the positrons, then lead or concrete reduces the 511 keV gamma photons from annihilation
Gamma$^{0}_{0}\gamma$No changeNo changeThick lead or concrete reduces exposure
13.2

Effects of Radioactivity

Alpha, beta, and gamma radiation are all ionizing. That means they carry enough energy to knock electrons off the atoms they hit. In living tissue, ionization can break chemical bonds, including bonds in DNA. Cells can usually repair damage from small doses. Large doses can cause radiation sickness, and long-term exposure raises cancer risk.

How dangerous a source is depends partly on where it is. Outside the body, the outer layer of skin stops alpha particles, while penetrating gamma rays can expose deeper tissue. An alpha emitter inside the body, such as inhaled radon gas, can cause severe localized damage because alpha particles deposit energy over a very short distance. The total risk still depends on the isotope's activity, energy, location, and the dose received. Absorbed dose is measured in grays (Gy), while equivalent and effective dose are measured in sieverts (Sv) to account for biological effects. A typical person in the U.S. gets about 3 mSv per year from natural background sources.

The same damage that makes radiation risky also makes it useful. Radiotherapy targets tumors because fast-dividing cancer cells are more vulnerable to DNA damage. Technetium-99m (half-life about 6 hours) is a common imaging tracer. Iodine-131 treats thyroid disease because the thyroid absorbs iodine. Gamma rays from cobalt-60 can sterilize sealed medical supplies and reduce pathogens or insects in food. This irradiation does not make the food radioactive.

  • Ionizing radiation: Ionizing radiation has enough energy to remove electrons from atoms and break chemical bonds.
  • Radioactive tracer: A radioactive tracer is a small amount of a radioisotope whose radiation can be detected to follow where it goes in the body or a system.
  • Sievert (Sv): The sievert is the unit for equivalent and effective dose, which account for how much biological damage a given type of radiation causes.

Check yourself. Why is external exposure to a contained alpha source usually less dangerous than taking an alpha emitter into the body? (Answer: The outer layer of skin stops alpha particles. Inside the body, alpha particles can deposit a large amount of energy in nearby living tissue. You should still never handle a radioactive source without proper controls.)

13.3

Nuclear Fission and Fusion Processes

Fission and fusion can release energy because the products have less total rest mass than the reactants. That decrease in rest mass becomes released energy through E=mc2E = mc^2, and since c2c^2 is enormous, a tiny mass change means a huge amount of energy. A nucleus also has a mass defect, which is the difference between its actual mass and the total mass of its separate protons and neutrons.

Fission splits a heavy nucleus. A slow neutron hits uranium-235, which splits into two mid-sized fragments plus 2 or 3 neutrons. Those neutrons split more nuclei in a chain reaction. Control rods of boron or cadmium absorb extra neutrons to keep it steady, and the heat makes steam that spins a turbine.

Fusion joins light nuclei. In deuterium-tritium fusion, deuterium and tritium form helium-4 and a neutron. Because both nuclei are positive and repel, practical D-T systems use plasma temperatures around 100 million K and must confine the plasma long enough for enough reactions to occur. Deuterium is abundant, but tritium is scarce and would need to be bred from lithium. No fusion power plant currently supplies electricity to the grid.

Worked example. Find xx in 92235U+01n→56141Ba+3692Kr+x 01n^{235}_{92}\text{U} + ^{1}_{0}\text{n} \rightarrow ^{141}_{56}\text{Ba} + ^{92}_{36}\text{Kr} + x\,^{1}_{0}\text{n}. The left side has mass 235+1=236235 + 1 = 236. The fragments add to 141+92=233141 + 92 = 233, so x=3x = 3 neutrons. The atomic numbers check out too, since 92=56+3692 = 56 + 36.

  • Chain reaction: A chain reaction is a self-sustaining series of fissions in which neutrons from one split cause more splits.
  • Critical mass: Critical mass is the minimum amount of fissile material needed to sustain a chain reaction under a specific set of conditions, such as the material's density, shape, and surroundings.
  • Mass defect: Mass defect is the difference between the mass of a bound nucleus and the total mass of its separate protons and neutrons, and it reflects the energy holding the nucleus together.

Check yourself. What do control rods do in a fission reactor? (Answer: They absorb neutrons, so fewer neutrons are available to cause more fissions. Pushing them in slows the reaction, and pulling them out speeds it up.)

FeatureFissionFusion
What happensA heavy nucleus splits into smaller onesLight nuclei join into a heavier one
Typical fuelUranium-235, plutonium-239Deuterium and tritium (hydrogen isotopes)
Conditions neededA neutron can trigger a single fission. A sustained chain reaction needs suitable neutron energies and a critical configuration of fuelVery high temperature plus enough particle density and confinement time
Where it happens nowNuclear power plantsStars, including the sun, and experimental reactors
WasteFission products and transuranic elements; some remain hazardous for thousands of years or longerHelium, tritium-handling waste, and neutron-activated reactor materials; less long-lived high-level waste is expected than from fission
13.4

Half-life and Radioactive Decay

A half-life is the time it takes for half of the radioactive nuclei in a sample to decay. Each isotope has its own half-life. Iodine-131 is about 8 days, carbon-14 is about 5,730 years, and uranium-238 is about 4.5 billion years. Ordinary changes in temperature, pressure, and chemical bonding have almost no effect on half-life, though electron capture can shift very slightly with chemical environment.

Decay is exponential, not linear. After one half-life, 1/2 of the sample remains, after two 1/4 remains, and after three 1/8 remains. The general formula is N=N0(12)nN = N_0 \left(\tfrac{1}{2}\right)^{n}, where n=t/t1/2n = t / t_{1/2} is the number of half-lives. Half-life describes large groups of atoms, so you can't predict when any single atom will decay.

Radiocarbon dating relies on this. While an organism is alive, it exchanges carbon with its environment and keeps a carbon-14 ratio close to that of its surroundings. After death, its carbon-14 decays. Measuring what remains can estimate the age of once-living material up to about 50,000 years old.

Worked example. A sample contains 80.0 mg of iodine-131 (t1/2=8.0t_{1/2} = 8.0 days). How much remains after 24 days? The number of half-lives is n=24/8.0=3n = 24 / 8.0 = 3. The mass left is 80.0×(1/2)3=80.0/8=10.080.0 \times (1/2)^3 = 80.0 / 8 = 10.0 mg, so 70.0 mg has decayed.

Some honors classes also use N=N0e−λtN = N_0 e^{-\lambda t} with λ=0.693/t1/2\lambda = 0.693 / t_{1/2}, which also works when the time isn't a whole number of half-lives.

  • Half-life ($t_{1/2}$): Half-life is the time it takes for half of the radioactive nuclei in a sample to decay.
  • Decay constant ($\lambda$): The decay constant gives the probability per unit time that a radioactive nucleus will decay, and it equals 0.693/t1/20.693 / t_{1/2}.
  • Radiometric dating: Radiometric dating estimates a material's age from a radioactive isotope's known half-life and measured isotope ratios, often the ratio of a parent isotope to its daughter product.

Check yourself. A piece of wood has 25% of the carbon-14 found in living trees. About how old is it? (Answer: 25% is (1/2)2(1/2)^2, so two half-lives have passed. That's 2×5,730≈11,4602 \times 5{,}730 \approx 11{,}460 years.)

Key terms

TermDefinition
IsotopeIsotopes are atoms of the same element that have the same number of protons but different numbers of neutrons.
Radioactive decayRadioactive decay is the spontaneous breakdown of an unstable nucleus, which releases particles or energy.
Alpha particleAn alpha particle is a helium-4 nucleus, $^{4}_{2}\text{He}$, with two protons and two neutrons.
Beta particleA beta particle is a high-speed electron, $^{0}_{-1}\text{e}$, that a nucleus emits when one of its neutrons turns into a proton.
Gamma rayA gamma ray is a high-energy photon released from a nucleus, and it changes neither the mass number nor the atomic number.
Nuclear fissionNuclear fission is the splitting of a heavy nucleus into smaller nuclei, which releases energy and neutrons.
Nuclear fusionNuclear fusion is the joining of light nuclei into a heavier nucleus, which releases energy.
Half-lifeA half-life is the time it takes for half of the radioactive nuclei in a sample to decay.
Mass defectMass defect is the difference between the mass of a bound nucleus and the total mass of its separate protons and neutrons, and it corresponds to energy through $E = mc^2$.

Mistakes to avoid in Nuclear Chemistry

Treating half-life as if decay were linear

If half is gone after one half-life, it's tempting to think the rest is gone after two. Each half-life removes half of what is left, not half of the original. After two half-lives 25% remains, and after three 12.5% remains. Count the half-lives and multiply by 1/2 once for each one.

Balancing only the mass numbers

Many errors come from checking the top numbers and forgetting the bottom ones. Both the mass numbers and the atomic numbers must add up the same on each side. Once you find the missing atomic number, use the periodic table to name the element.

Assuming the most penetrating radiation is always the most harmful

Gamma rays penetrate farther, but penetration and biological effect are different. Alpha particles are blocked by the outer layer of skin, yet an internal alpha emitter can cause severe localized damage because alpha particles deposit energy over a short distance. For the same absorbed dose, alpha radiation generally has a greater biological effect than beta or gamma radiation.

Mixing up fission and fusion

Both release energy from a change in mass, so the names blur together. Fission means splitting a heavy nucleus like uranium-235, and it already powers reactors today. Fusion means joining light nuclei like hydrogen isotopes, which happens in the sun but not yet in power plants.

Study unit 13 other ways

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