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Science notes, chapter 8

Radioactivity

Textbook Science Form 3 (KSSM, Dual Language Programme), pages 230–255

What this chapter covers

  • Describe how radioactivity was discovered and who contributed (8.1)
  • Define radioactivity and radioactive decay; give examples of radioactive substances (8.1)
  • State the units of radioactivity and explain half-life, including calculations and graphs (8.1)
  • Explain the formation of positive ions and negative ions (8.2)
  • Differentiate ionising and non-ionising radiation, and compare alpha, beta and gamma radiation (8.3)
  • Give natural and man-made sources of ionising radiation and explain how to keep the dose safe (8.3)
  • Describe the uses of radioactive radiation and the safe handling of radioactive substances and waste (8.4)

8.1Discovery of radioactivity

YearScientistDiscovery
1895Wilhelm Roentgen (German)The X-ray; first Nobel Prize in Physics (1901)
1896Henri Becquerel (French)Radioactivity: a uranium compound blackened a photographic plate even in the dark (Nobel Prize 1903)
1897Marie and Pierre CurieDetected radioactive radiation through its ionising power; extracted polonium and radium from pitchblende (uranium ore)
Radioactivity is the random and spontaneous decay of an unstable nucleus by emitting radioactive radiation: alpha particles (α), beta particles (β) and gamma rays (γ).

The nucleus keeps emitting radiation until it becomes more stable. Examples of radioactive substances: carbon-14, radon-222, thorium-234 and uranium-238.

Alpha decay
U-238 (92 p, 146 n) emits a helium nucleus (2 p, 2 n) and becomes Th-234 (90 p, 144 n).
Beta decay
Th-234 (90 p, 144 n) emits an electron and becomes Pa-234 (91 p, 143 n).
Gamma decay
An unstable Co-60 nucleus (27 p, 33 n) emits a gamma ray and stays Co-60, now more stable.
Marie Curie is the only woman to receive two Nobel Prizes (Physics 1903, Chemistry 1911). She and Pierre had no idea of the risks of prolonged exposure to gamma rays.
Radioactive decay is random: you cannot tell when one particular nucleus will decay. It is spontaneous: heat, pressure or chemicals do not start it.

Units of radioactivity

Radioactivity measures the rate of decay (decays per second).

UnitValue
Becquerel (Bq), the S.I. unit1 Bq = 1 decay per second
Curie (Ci), the first unit1 Ci = 3.7 × 1010 decays per second = 3.7 × 1010 Bq

Half-life

Half-life, T½, is the time taken for the number of undecayed nuclei (or the activity) to fall to half of its original value. Its S.I. unit is the second.
Example: remaining mass (textbook p. 235)
Pa-234 has a half-life of 5.2 hours. Original mass 80 g. Find the mass after 20.8 hours.
Number of half-lives = 20.8 ÷ 5.2 = 4.
80 g → 40 g → 20 g → 10 g → 5 g. Remaining mass = 5 g.
Graph of activity against time falling from 640 Bq to 40 Bq over 120 seconds
Activity of a sample: 640 Bq at 0 s. Half of 640 is 320 Bq, which is reached at 30 s, so the half-life is 30 s. Check: 320 → 160 at 60 s, → 80 at 90 s.
To read a half-life from a graph, take the starting activity, halve it, then read the time on the horizontal axis. Always start from the original value at time 0.
A sample has an activity of 240 Bq. Its half-life is 10 minutes. What is its activity after 30 minutes?
Show answerHide answer
30 ÷ 10 = 3 half-lives. 240 → 120 → 60 → 30. Activity = 30 Bq.

8.2Atom and nucleus

Dalton's Atomic Theory said the atom is the smallest particle and cannot be divided. Science later found smaller particles: protons (positive) and neutrons (neutral) in the nucleus, and electrons (negative) around it. An atom is neutral when protons = electrons.

An ion is a charged particle formed when an atom loses or gains electrons. The number of protons never changes.
IonHow it formsExample
Positive ion (cation)Atom loses electronsNa (11 p, 11 e) loses 1 e → Na+ (11 p, 10 e), charge +1
Negative ion (anion)Atom gains electronsCl (17 p, 17 e) gains 1 e → Cl− (17 p, 18 e), charge −1
Charge = number of protons − number of electrons. Mg with 12 p and 10 e: 12 − 10 = +2, so Mg2+.
A particle has 9 protons and 10 electrons. Is it a positive or negative ion? What is its charge?
Show answerHide answer
Negative ion, because there is one more electron than protons. Charge = 9 − 10 = −1 (fluoride ion, F−).

8.3Ionising and non-ionising radiation

Ionising radiation produces positive and negative ions when it passes through air (or matter). Non-ionising radiation does not.
Non-ionisingIonising
Radio waves, microwaves, infrared, visible light, very low frequency wavesUltraviolet, X-rays, gamma rays (and alpha and beta particles)

Alpha, beta and gamma radiation

Alpha, αBeta, βGamma, γ
NatureHelium nucleusHigh-speed electronElectromagnetic wave
ChargePositiveNegativeNeutral
Ionising powerHighModerateLow
Penetration powerLow (stopped by paper)Moderate (stopped by about 3 mm aluminium)High (needs about 10 cm lead)
Electric fieldBends towards the negative plateBends towards the positive plateNot deflected
Magnetic fieldDeflected one way (upwards in the textbook figure)Deflected the opposite way (downwards)Not deflected (goes straight)
Alpha stopped by paper, beta by aluminium, gamma by lead Alpha bends to the negative plate, beta to the positive plate, gamma goes straight
Penetration and deflection in an electric field.

Textbook Table 8.4, p. 241

The two powers go in opposite orders: the more ionising the radiation, the less it penetrates. Alpha: most ionising, least penetrating. Gamma: least ionising, most penetrating.

Sources of ionising radiation

NaturalMan-made
Cosmic rays (high-energy radiation from outside the Solar System); background radiationNuclear accidents; nuclear tests; radioisotopes used in medicine; background radiation

Background radiation and dose

Background radiation is the ionising radiation in the environment. Absorbed radiation damages body cells, so its effect is measured as a dose. 1 sievert (Sv) means 1 joule of radiation energy absorbed by 1 kg of living tissue. The dose rate is measured with a Geiger counter in microsieverts per hour (μSv/h).

Safe background dose rate: below 0.2 μSv/h (below 1.752 mSv per year).
Source of doseSafety measure
Background radiation (UV)Anti-UV spectacles and umbrellas
Medical X-rayOnly with a doctor's prescription
TelevisionSit at least 2 m away
Contaminated foodDo not eat food from contaminated areas
Cosmic raysLimit the flying hours of pilots and aircrew
Source (textbook Figure 8.11)Estimated dose
TV or computer0.01 mSv/h
Flight (cosmic rays)0.003 mSv/h
Environment (background radiation)0.4 to 1.0 mSv/year
Medical X-ray5.5 mSv per medical test
Example: dose from television (textbook p. 246)
Dose rate from a TV = 0.01 mSv/h. A student watches 2 h a day for 5 days.
Total time = 2 × 5 = 10 h. Dose = 0.01 × 10 = 0.1 mSv.
Cosmic ray dose rises with altitude because the atmosphere absorbs most of it. That is why airline crew, not ground staff, can exceed the safe level.

8.4Uses of radioactive radiation

FieldUse
Archeology and geochronologyCarbon-14 dating: after death, C-14 (half-life 5 700 years, emits beta) is no longer replaced, so its activity shows the age of fossils and artifacts
IndustryBeta radiation checks the thickness of metal sheets; too much beta detected means the sheet is too thin
AgricultureP-32 shows how fast plants absorb phosphate fertiliser; radiation kills beetles and sterilises pests
MedicineGamma rays from Co-60 or Cs-137 kill cancer cells; Na-24 locates blood clots; Tc-99 treats brain tumours; I-131 treats the thyroid
Food preservationGamma rays kill bacteria in food. The Radura logo labels such food
DefenceNuclear weapons: radiation destroys living things and its effect lasts for generations
Example: carbon-14 dating
A fossil has one quarter of the C-14 activity of a living organism. Quarter = 2 half-lives (1 → ½ → ¼).
Age = 2 × 5 700 = 11 400 years.

Safe handling of radioactive substances and waste

  • Store sources and waste in containers with thick lead walls.
  • Shield substances with thick slabs of lead.
  • Handle them with robotic hands, and wear protective clothing.
  • Wear radiation badges to detect the dose absorbed.
  • Dispose of waste safely and properly.
Lead is used because gamma rays penetrate most materials. Its disadvantage is that it is heavy and toxic, so lead clothing is tiring to wear.

Irene Joliot-Curie made the first artificial radioactive element, phosphorus-30, in 1934. Radioactive radiation brings great benefits, so we should be grateful and use it responsibly.

Summary

RememberKey fact
RadioactivityRandom, spontaneous decay of an unstable nucleus emitting α, β or γ
UnitsBq (1 decay/s) and Ci (3.7 × 1010 Bq)
Half-lifeTime for activity or undecayed nuclei to halve
IonLose e → positive; gain e → negative
Ionising powerα > β > γ; penetration γ > β > α
Safe dose rateBelow 0.2 μSv/h