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A Science teacher since 2016 creating and sharing resources he uses with his own classes.

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A Science teacher since 2016 creating and sharing resources he uses with his own classes.
Ionisation Energy
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Ionisation Energy

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By the end of the lesson learners should be able to: •Identify the S, P and D blocks. •Describe what is meant by an ionisation energy. •Explain why the ionisation energy changes through groups and periods.
Trends in the Periodic Table
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Trends in the Periodic Table

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By the end of the lesson learners should be able to: Identify the trends in atomic radius across a period. Identify the trend in atomic radius down a group. Describe the trend in melting points across a period. Explain why this trend occurs by mentioning the types of bonding. Suitable for KS5 students (Yrs 17-18)
Refraction
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Refraction

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By the end of the lesson learners should be able to: State what is meant by refraction. Describe how light refracts through mediums. Explain why refraction is useful.
Wave speed
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Wave speed

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By the end of the lesson learners should be able to: Identify a wavelength. Describe how to calculate wave speed. Explain why wave speed can change.
Metals and Non-Metals
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Metals and Non-Metals

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By the end of the lesson learners should be able to: Identify metals and non-metals. Describe 2 properties of metals and non-metals. Explain why non-metals can harm the environment
Acceleration
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Acceleration

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By the end of the lesson learners should be able to: State the equation for acceleration Describe how to measure the acceleration of an object. Explain why a change in acceleration indicates a change in direction
Velocity Time and  Speed Time Graphs
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Velocity Time and Speed Time Graphs

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By the end of the lesson learners will be able to: Identify acceleration, constant velocity and deceleration on a velocity-time graph. Describe how to calculate distance travelled using a velocity-time graph. Compare the movement of two objects on a velocity-time graph.
Newton's First Law
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Newton's First Law

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By the end of the lesson learners will be able to: State Newton’s First law. Calculate Resultant Forces. Explain why changing in speed requires a force.
Vectors and Scalars
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Vectors and Scalars

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By the end of the lesson learners should be able to: Identify scalars and vectors. Compare scalars and vectors. Convert scalars into vectors.
Wave Phases
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Wave Phases

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By the end of the lesson learners should be able to: Identify different types of waves. Describe how to measure properties of waves. Compare constructive and destructive interference.
Distance Time Graphs
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Distance Time Graphs

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By the end of the lesson learners should be able to: State the formula for speed. Describe what’s shown in a distance-time graph Explain why the gradient is the same as the speed on a distance-time graph.
Energy Stores and Transfers
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Energy Stores and Transfers

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By the end of the lesson learners will be able to: Identify the 8 energy stores. Describe how energy can be transferred. Justify the type of energy transfer within a system.
Mass and Weight
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Mass and Weight

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By the end of the lesson learners will be able to: State what’s meant by mass. Describe how to calculate weight. Compare mass and weight.
Momentum
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Momentum

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By the end of the lesson learners will be able to: Identify the effect of force. Describe how to calculate force. Explain why mass and acceleration affects force.
Background Radiation
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Background Radiation

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By the end of the lesson learners will be able to: Identify what’s meant by a radioactive atom. Describe how a GM tube measures radiation. Explain why radioactive sources become less dangerous as time passes.
Alpha Beta and Gamma Radiation
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Alpha Beta and Gamma Radiation

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By the end of the lesson learners will be able to: Identify the 3 types of radiations. Describe properties of each type of radiation. Explain why the atomic and mass numbers change after some radioactive emissions.
Kinetic and Gravitational Energy
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Kinetic and Gravitational Energy

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By the end of the lesson learners will be able to: State what is meant by kinetic and gravitational energy. Describe how to calculate kinetic and gravitational energy. Explain why pendulums within a closed system will remain swinging at a fixed height.