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Years 9 and 10 Chemistry

Inside the atom and through reactions. The nuclear atom and its electron shells explain the periodic table; atoms rearrange and are never lost, which is why mass is conserved and equations balance; and reactions happen when particles collide hard enough.

Start1. What's inside an atom?

Inside the atom

Protons, neutrons and electrons; atomic and mass numbers (AC9S9U06, Year 9).

1What's inside an atom?Not started
2Same element, different atoms?Not started
3What comes out of a decaying nucleus?Not started
4How long does radioactivity last?Not started
5From uranium to leadNot started

An unstable nucleus often decays into another unstable one, and a decay chain ends only when a stable nucleus is reached. Each alpha decay lowers the atomic number by 2 and the mass number by 4; each beta decay raises the atomic number by 1 and leaves the mass number alone. Uranium-238 reaches stable lead-206 after eight alpha and six beta decays.

  1. Engage: where does it end?
  2. Explore: follow the chain › Radon to lead
  3. Explore: follow the chain › The long chain
  4. Explain: tracking numbers › Atomic number
  5. Explain: tracking numbers › Mass number
  6. Explain: tracking numbers › Beta step
  7. Explain: tracking numbers › Total fall
  8. Explain: tracking numbers › Alpha count
  9. Explain: tracking numbers › Why it stops
  10. Explain: tracking numbers › In your own words
  11. Evaluate: look back
Start lesson

Equations and conservation of mass

Reactions rearrange atoms; none are made or destroyed; balanced equations show it (AC9S9U07, Year 9).

6What goes in, what comes out?Not started
7Where do the atoms go?Not started
8How do you balance an equation?Not started
9Where does the mass go?Not started

In a chemical reaction atoms are rearranged, not made or destroyed, so the total mass of the reactants equals the total mass of the products. In a closed system the mass reading stays the same. In an open system it can seem to change because a gas escapes (mass falls) or a gas from the air joins in (mass rises); counting the gas shows the mass is still conserved.

  1. Engage: the fizzing flask
  2. Explain: counting everything › Closed system
  3. Explain: counting everything › Magnesium in a flask
  4. Explain: counting everything › Magnesium in air
  5. Explain: counting everything › The log
  6. Explain: counting everything › Balanced equation
  7. Explain: counting everything › In your own words
  8. Evaluate: look back
Start lesson

Atoms and the periodic table

Electron shells, and why elements in a group behave alike (AC9S10U06, Year 10).

10How are the electrons arranged?Not started
11Why do elements in a group behave alike?Not started

Elements in the same group have the same number of outer-shell electrons, so they react in similar ways. Group 1 metals lose their one outer electron easily; group 17 non-metals gain one easily; group 18 has full shells and hardly reacts.

  1. Engage: three fizzing metals
  2. Explore: group 1
  3. Explain: outer electrons decide › Sort by group
  4. Explain: outer electrons decide › Noble gases
  5. Explain: outer electrons decide › Predict X
  6. Explain: outer electrons decide › Sodium and chlorine
  7. Explain: outer electrons decide › In your own words
  8. Evaluate: look back
Start lesson
12Why does the periodic table repeat?Not started
13Use the table to predictNot started

The periodic table is not a list to look up but a tool for prediction. An element's group gives its number of outer electrons, and so how reactive it is and what it bonds with; its period gives its number of shells. From the position alone you can predict whether an element is a metal, how it reacts and what its atom looks like.

  1. Engage: a stranger in group 1
  2. Explore: read the table › Group 2, period 3
  3. Explore: read the table › Group 17, period 2
  4. Explore: read the table › Group 18, period 3
  5. Explain: predicting › Outer electrons
  6. Explain: predicting › Shells
  7. Explain: predicting › Down a group
  8. Explain: predicting › Bonding
  9. Explain: predicting › Noble gases
  10. Explain: predicting › In your own words
  11. Evaluate: look back
Start lesson

Reaction rates

Particles must collide with enough energy to react: collision theory (AC9S10U07, Year 10).

14What kind of reaction is it?Not started
15Why does heat speed up reactions?Not started

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For teachers: Teacher guide (notes, answers, solutions, slides and worksheets)