By the end of the lesson learners should be able to: Identify short, medium and long wavelength waves in the EM spectrum. Describe how these waves are used. Explain why the use of short wavelengths are controlled.

By the end of the lesson learners should be able to: Identify some satellites. Describe what’s meant by a satellite. Explain how satellites are useful.

By the end of the lesson learners will be able to: Identify the uses of alpha, beta and gamma radiation. Describe how they are used in real world applications. Explain why the type of radiation is suited for the role it carries out.

By the end of the lesson learners should be able to: Identify what is meant by a parallax Describe how to convert a distant star, Earth and the Sun into a triangle. Justify which trigonometric formula to use to calculate the distance between a distant star and Earth or the Sun.

By the end of the lesson learners should be able to: Identify the make up of atoms. Describe how cloud chambers are used to detect particles and properties about them. Explain why particle accelerators are useful for explaining the makeup of matter.

By the end of the lesson learners should be able to: Identify what is needed for GPS to work. Describe how a RADAR system detects objects. Explain why a stellar parallax is used to measure the distance of stars instead of RADAR.

All features work when used with google slides. All features should work with PowerPoint, but might need some rearranging. By the end of the lesson learners will be able to: Identify different ideas about the universe from different cultures. Describe the geocentric model of the solar system. Explain the reasoning for the geocentric model.

All features work when used with google slides. All features should work with PowerPoint, but might need some rearranging. By the end of the lesson learners will be able to: Identify the different models of the solar system. Describe what retrograde motion is. Explain why retrograde motion links to a heliocentric model.

All features work when used with google slides. All features should work with PowerPoint, but might need some rearranging. By the end of the lesson learners will be able to: Identify technologies developed since the space programme. Describe some of the risks and benefits of the space programme. Evaluate the space programme.

All features work when used with google slides. All features should work with PowerPoint, but might need some rearranging. By the end of the lesson learners will be able to: Recall how a radio signal is made. Describe how electromagnetic waves are used for communication. Explain the advantages of electromagnetic radiation.

By the end of the lesson learners should be able to: State what’s meant by direct current and alternating current. Describe the contents of a 3 pin plug. Explain why an Earth wire is used in a plug.

By the end of the lesson learners should be able to: State how electrical energy is distributed by the national grid. Describe how the national grid efficiently transfers electrical energy. Explain the use of transformers.

By the end of the lesson learners should be able to: Identify 2 devices used to deal with electrical overload. Describe how fuses and earthing deal with electrical overloads. Explain the movement of electricity and why earthing works.

By the end of the lesson learners should be able to: Identify permanent and induced magnets. Describe what’s meant by a permanent and induced magnet. Explain why magnets are used in industry.

By the end of the lesson learners should be able to: State what is meant by pressure. Describe how gas particles interact with the wall of the container. Explain why each of the following increases pressure: Increasing temperature, Increasing the amount of gas particles, Decreasing volume of the container.

By the end of the lesson learners should be able to: Identify the parts that make up the ear. Describe how the ear manipulates sound. Explain why people can experience hearing loss / damage.

By the end of the lesson learners should be able to: Identify the cause of sound waves. Describe how amplitude, loudness, frequency and pitch are connected. Explain why people can’t talk to another in space.

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.

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.

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.