By the end of the lesson learners should be able to: Recall the equation for resistance Describe what is meant by resistance Calculate the resistance of a component of a circuit

By the end of the lesson learners will be able to: State some sources of infrared radiation Describe uses of radiation Explain how energy is transferred through radiation

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.

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.

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. 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.

By the end of the lesson learners will be able to: Identify the 3 transfers of heat. Describe each process of heat transfer. Explain why double glazed windows reduce the amount of heat loss in a home.

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.

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. 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.

By the end of the lesson learners will be able to: Identify the forces working during a crash. Describe how the reduce the crashing force. Explain why crumple zones and slower driving cause less damage during a crash.

By the end of the lesson learners should be able to: Identify what causes day and night time. Describe how the Earth moves: Through rotating: Around the Sun: Explain the link between the rotation of the Earth and the effect on days.

By the end of the lesson learners should be able to: Identify action and reaction forces. Describe Newton’s third law. Explain why people might experience pain when placing a force on an object.

By the end of the lesson learners will be able to: Identify low, mid and high energy waves. Describe how to protect yourself from exposure to energy waves. Explain why there is strict government guidelines for the use of gamma and X-rays

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 changes after the Big Bang. Describe the timescale of the universe. Explain why the universe is expanding.

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 power. Describe how power can be calculated. Explain why changing the time that energy is transferred in affects power.

By the end of the lesson learners should be able to: State some examples of elastic and inelastic objects. Describe the effect of two pulling forces on an elastic object. Explain the incident that can cause an elastic object to become inelastic.