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 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 should be able to: Solve to identify resultant forces. Describe how a resultant force affects the object. Create free body diagrams / vector diagrams.

Lessons created to match the activate 3 scheme of work. All features work when used with google slides. All features should all work with powerpoint but might need some rearranging. By the end of the lesson learners will be able to: Recall the trend in electrical demand over the years. Describe how electricity is produced. Compare different means of producing electricity.

Lessons created to match the activate 3 scheme of work. All features work when used with google slides. All features should all work with powerpoint but might need some rearranging. By the end of the lesson learners will be able to: State what is meant by reaction time. Describe how technology is used in sport. Explain why technology saves lives during crashes.

Lessons created to match the activate 3 scheme of work. All features work when used with google slides. All features should all work with powerpoint but might need some rearranging. By the end of the lesson learners will be able to: Recall some techniques for seeing inside the body. Describe how optical fibres work. Describe some techniques for seeing inside the human body.

Lessons created to match the activate 3 scheme of work. All features work when used with google slides. All features should all work with powerpoint but might need some rearranging. A practical activity is also included including a set of results. By the end of the lesson learners will be able to: Recall the devices used in a hospital. Describe how a thermistor is affected by temperature. Explain why thermistors are needed.

Lessons created to match the activate 3 scheme of work. All features work when used with google slides. All features should all work with powerpoint but might need some rearranging. A practical activity is also included including a set of results. By the end of the lesson learners will be able to: State the equation for efficiency. Describe how an LDR detects light. Explain why LED lights are now used instead of older bulbs.

Lessons created to match the activate 3 scheme of work. All features work when used with google slides. All features should all work with powerpoint but might need some rearranging. By the end of the lesson learners will be able to: Identify analogue and digital. Describe the uses of digital and analogue signals. Explain why waves are useful.

A revision mat for activate 3 - Detection in Physics.

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 carrier waves. Describe how waves can be modulated by amplitude or frequency. Explain why radio receivers are often able to detect a signal over a large area.

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 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.

By the end of the lesson learners should be able to: State what is meant by the habitable zone. Describe how we can communicate with aliens on other planets. Explain why the light we receive on Earth from a star / exoplanet can tell us about its elemental makeup.

By the end of the lesson learners will be able to: Identify reflecting and refracting telescopes Describe how both telescopes work. Explain how the size of exoplanets can be determined using a telescope.

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 I will be able to: Identify the structure of beta and alpha radiation. Describe how to calculate nuclear equations. Justify which element is produced from a nuclear equation.