This lesson has been designed to help students to explain the relationship between current and resistance in thermistors and LDRs. This can be a topic which students do not engage with or understand well, so this lesson has tried to add engagement with useful tips to deepen their knowledge. A number of quick competitions are used to introduce key terms such as semiconductor and then the key points explained. Students are given an exemplary answer for the thermistor so they can see how their work should be set out when trying to explain the graph produced by a LDR. Progress checks have been written into the lesson at regular intervals so that students can assess their understanding and any misconceptions can be addressed. This lesson has been designed for GCSE students.

This lesson has been designed to explore the range of energy sources which are used on Earth and specifically looks at why an increase in the use of renewable sources is critical for the future. The student’s scientific understanding is challenged at each step of the lesson but there is also a mathematical element running throughout. The lesson begins by challenging the students to predict which energy sources contributed the greatest % when presented with a pie chart. Students cover this topic in other subjects like Geography, so the lesson aims to build on this and consolidate the essential understanding. A range of renewable sources are discussed and key terms such as carbon-neutral taken on further. This lesson has been designed for GCSE students but parts could be used with younger students who are looking at

An engaging lesson which uses a range of tasks to ensure that students understand the meaning of the term, background radiation, and are able to name a number of sources of this type of radiation. The start of the lesson focuses on the definition of background radiation and the idea that is all around us is revisited again a number of times during the lesson. Through a range of activities and discussion points, students will meet the different sources as well as the % that they each contribute. It seemed appropriate to challenge some mathematical and scientific skills at this point so students will represent the data in a pie chart form. Related topics are discussed such as Chernobyl. Progress checks are written into the lesson at regular intervals so the students can constantly assess their understanding. This lesson is designed for GCSE students.

A fully-resourced lesson that explores how resistance, current and potential difference differ between series and parallel circuits. This knowledge needs to be sound in order for students to be able to carry out circuit calculations. The lesson includes a practical and task-based lesson presentation (24 slides) and an accompanying worksheet. The lesson begins by challenging the students to recognise the key difference between the two circuits, in that in a parallel circuits, the electrons can follow more than one route. Moving forwards, each physical factor is investigated in each type of circuits and students carry out tasks or calculations to back up any theory given. Helpful analogies and hints are provided to guide the students through this topic which is sometimes poorly understood. Students will be challenged to use the V = IR equation on a number of occasions so that they are comfortable to find out any of these three factors. Progress checks have been written into the lesson at regular intervals so that students are constantly assessing their understanding and any misconceptions can be addressed. This has been written for GCSE students, but could be potentially used with higher ability KS3 students.

A concise, fast-paced lesson that looks at the orbits of both natural and artifical satellites. The lesson has been written to build on the student’s knowledge of space from KS3 and add key details such as the gravitational pull between the different celestial objects. Students will learn how the speed of the orbiting object and the gravitational pull ensure that the object remains in orbit and consider what would happen should the speed change. Students are briefly introduced to a number of orbits of artificial satellites as well as the uses. This lesson has been designed for GCSE students

A fast paced lesson which focuses on the equation for work done and using this in calculations. The lesson includes a student-led lesson presentation and a question worksheet which together explore the different problems that students can encounter when attempting these questions and therefore acts to eliminate any errors. There is a big mathematical element to the lesson which includes the need to rearrange formula, understand standard form and to convert between units as this is a common task in the latest exams. Students will learn that some questions involve the use of two equations as they are needed to move from a mass to a force (weight) before applying the work done equation. The last part of the lesson looks at how work done is involved in the calculation for power. This lesson has been designed for GCSE students.

A fast-paced lesson that looks at weight and how this differs on different planets depending upon the gravitational field strength. At the start of the lesson, the students are shown the equation to calculate gravity force and weight and are challenged to spot a difference (if there is one)! Time is then taken to explain how weight is the term used when a mass comes into the gravitational field of the Earth (or other planets). A quick understanding check, with the gravitational field strength Olympics, is used to see whether students can calculate this field and their mathematical skills are tested with a number of conversions needed to do so. Moving forwards, students are shown a number of masses and weights on the Earth and the Moon so they can see how mass does not change but weight will be different. The final task challenges them to apply their new-found knowledge to calculate their mass on the Earth, the Moon and Jupiter. This lesson has been designed for GCSE students but it is suitable for KS3 students who are exploring the Universe topic.

An informative lesson which guides students through the commonly misunderstood topic of drawing free body diagrams and using them to calculate resultant forces. The lesson begins by ensuring that students understand that force is a vector quantity and therefore arrows in diagrams can be used to show the magnitude and direction. Drawing free body diagrams is poorly understood and therefore time is taken to go through the three key steps in drawing these diagrams. Each of these steps is demonstrated in a number of examples, so students are able to visualise how to construct the diagrams before they are given the opportunity to apply their new-found knowledge. The rest of the lesson focuses on calculating resultant forces when the forces act in the same plane and also when they are at angles to each other. Again, worked examples are shown before students are challenged to apply. Progress checks are written into the lesson at regular intervals so that students can constantly assess their understanding and any misconceptions can be addressed. This lesson has been designed for GCSE students

This lesson has been written for GCSE students and aims to ensure that they can explain in detail why light changes direction due to refraction. The key to the explanation is the use of the correct terms in context so the start of the lesson challenges the students to come up with the key words of light, bend, normal, density and speed when given a range of clues. The next part of the lesson works with the students to bring these key terms together to form a definition of refraction. Moving forwards, the relationship between density of a medium and the speed of light through that medium is discussed so that there is a clear understanding of why light bends one way or the other. The next task uses the definition to apply to a practical situation to draw a diagram of light moving from air to glass. The final part of the lesson involves a range of practicals so this topic can be explored further.

A fully-resourced lesson which includes a concise lesson presentation (16 slides) and accompanying worksheet that guides students through the use of the gravitational potential energy equation to calculate energy, mass and height. The lesson begins by challenging students to work out the factors involved in calculating gravitational potential energy having been given a scenario with some balls on shelves. The students will discover that mass and height affect the energy size and that a third factor, gravity constant, is involved. The rest of the lesson focuses on using the equation to calculate energy, mass and height. In terms of the latter, students have to carry out an engaging task to work out the height that three flags have to be hoisted to during a medal ceremony. This lesson has been written for GCSE students.

A fully-resourced lesson which focuses on using the kinetic energy equation to calculate energy, mass and speed. The lesson includes a lesson presentation (23 slides) which guides students through the range of calculations and accompanying worksheets which are differentiated. The lesson begins with the students being drip fed the equation so they are clear on the different factors involved. They are challenged to predict whether increasing the mass or increasing the speed will have a greater effect on the kinetic energy before testing their mathematical skills to get results to support their prediction. Moving forwards, students are shown how to rearrange the equation to make the mass the subject of the formula so they can use their skills when asked to calculate the speed. The final task of the lesson brings all of the learning together to tackle a set of questions of increasing difficulty. These questions have been differentiated so that students who need extra assistance can still access the learning. This lesson has been written for GCSE students

An engaging lesson presentation (28 slides) and accompanying worksheet, which together look at how to calculate efficiency and explores how efficiency can be increased by reducing the ways that energy is transferred to less useful stores. The lesson begins by looking at the key term, dissipated, and ensuring that students understand that energy being dissipated to a thermal energy store is one of the main reasons why efficiency will be low. Moving forwards, students are introduced to the equation to calculate efficiency and shown how to leave the answer as a decimal or percentage. Mathematical skills are challenged when calculating the efficiency as a number of units have to be converted. The rest of the lesson looks at a range of methods that can be used to reduce losses. Students will work with the teacher to understand how lubrication works and then a homework task gets them to explore how insulation in homes reduces heat losses. This lesson has been designed for GCSE students.

A fully-resourced lesson which looks at the calculation of a turning force and uses this to apply the principle of moments. The lesson includes an engaging and informative lesson presentation (24 slides) and a series of worksheets, some of which contain questions which have been differentiated. The lesson begins by getting the students to read through the scene from Friends which involves the famous “PIVOT”. This word has been removed from the scene and so students have to work out what it is and how it could relate to a Physics lesson. The rest of the lesson focuses on the range of calculation questions that students can face, which get progressively more difficult. At each stage of the lesson, students are guided through examples and given hints on points to be conscious of so that any silly mistakes can be eradicated. The principle of moments question worksheet has been differentiated two ways so that those students who need extra assistance are still able to access the learning. A homework question is also included in the lesson. This lesson has been written for GCSE students but should higher ability KS3 students want to really test themselves, it could be used with them.

A quick, concise lesson presentation (15 slides) which together with a question worksheet focuses on ensuring that students can define an isotope and pick these substances out from a selection of substances. The lesson begins by looking at the number of sub-atomic particles in an aluminium atom so that students can recall what is shown by the atomic and mass numbers. This will enable students to calculate the number of protons, neutrons and electrons in three given isotopes and as a result, complete a definition of these substances. The remainder of this short lesson involves 4 application questions where students either have to recognise isotopes from a table or from a diagram and also are asked to write out the formula of an isotope. Ideally this lesson will be taught in conjunction with a lesson on atomic structure.

A concise lesson presentation (22 slides) and question worksheet, which together focus on the challenge of applying the equations of motion to calculation questions. Students are given this equation on the data sheet in the exam - therefore, this lesson shows them how they will be expected to rearrange in it four ways. For this reason, the start of the lesson revisits the skills involved in rearranging the formula, beginning with simple tasks and building up to those that involve indices as are found in this equation. Once students have practised these skills, they are challenged to answer 4 questions, although 1 is done together with the class to visualise how to set out the working. This lesson has been designed for GCSE students

An informative and student-led lesson presentation (32 slides), accompanied by a reaction diagram and task worksheet, which together look at the key details of nuclear fission reactions. The lesson begins by introducing the students to the name of this reaction and to that of a neutron before they are challenged to recall the properties of this sub-atomic particle as this knowledge plays an important role in their understanding. Moving forwards, students will learn that two isotopes of uranium are involved and will discover and work out how one isotope is changed into the other. Diagrams accompany the theory throughout so that students can visualise how the reaction progresses. They are shown how to work out the two daughter nuclei that are produced in the reaction and how an equation can be written to represent nuclear fission. Progress checks have been written into the lesson at regular intervals so that students can constantly assess their understanding and any misconceptions can be immediately addressed. This lesson has been designed for GCSE students (14 - 16 year olds in the UK)

An engaging, practical-based lesson presentation (34 slides), accompanied by a practical worksheet and differentiated questions worksheet, which together guide students through the different calculation questions which involve the half-life. The lesson begins by introducing the students to the definition of a half-life and then showing them an example with I-131 so they can visualise how the half-life doesn’t change (and that radioactivity is measured in Bq). Moving forwards, the students will follow the given instructions to create the results to plot a decay curve and will be shown how to use this curve to determine the half-life of an isotope. The remainder of the lesson focuses on the different calculation questions that can be found on exam papers and uses a step by step guide to help them to handle the increasing difficulty. Students will be challenged to apply their new found knowledge to a set of 5 questions and this worksheet has been differentiated two ways so that those who need extra assistance, can still access the learning. Progress checks have been written into the lesson at regular intervals so that students can constantly assess their understanding. This lesson has been designed for GCSE students (14 - 16 years old in the UK)

An engaging, practical-based lesson presentation (22 slides), accompanied by a practical worksheet and application questions which together explore how the extension of a spring is related to force according to Hooke’s Law. The lesson begins by introducing the name of the law and looking at the equation which connects the force, extension and spring constant. As spring constant is likely to be a new term to students, time is taken to look at the definition of this key term. Students are given hints throughout the lesson about potential issues to look out for, including the unit of spring constant being N/m when the majority of springs are small enough that their extension will be measured in cm or mm. Moving forwards, students will follow the provided experimental method to carry out the investigation and produce a set of results which can be used to plot the line. The two distinct sections of the line are discussed and the actual words of Hooke’s Law are given and again discussed and considered. The final part of the lesson involves the students being challenged to apply their knowledge of the law to a range of application questions and assessing against the displayed mark scheme. This lesson has been written for GCSE students but can be used with KS3 students who are studying the extension of a spring

An informative lesson presentation (37 slides) and associated question worksheet which looks at the key properties of alpha, beta and gamma radiation. Students are given key pieces of information during the lesson and are then challenged to use their knowledge of related topics such as atomic structure and waves to complete the information table about the types of radiation. By the end of the lesson, students will be able to compare the types of radiation on form, charge, relative mass, penetrating power and equation symbols. Progress checks have been written into the lesson at regular intervals so that students can constantly assess their understanding. This lesson has been written for GCSE students (14 - 16 year olds in the UK).

A fully-resourced lesson which looks at speed and velocity as scalar and vector quantities and then guides students through a range of questions which challenge them to calculate both of these forms of motion. The lesson includes an engaging lesson presentation (44 slides) and differentiated worksheets containing questions. The lesson begins by introducing the terms magnitude and direction so that students can learn how scalar and vector quantities differ. Students will learn that speed is a scalar quantity and velocity is a vector quantity and then be questioned through a crossroads scenario to understand how speed can stay the same but as soon as an object changes direction, the velocity changes. Moving forwards, the students are given the equation to calculate speed and a few simple questions are worked through before they have to do a series of their own questions to find the average speeds for walking, running and cycling. A pair of more difficult speed questions are then attempted which challenge the students to convert from metres per seconds to miles per hour and to calculate the speed of a bicycle by calculating the distance travelled by the sensor on the wheel. This task is differentiated so that students who need some assistance will still be able to access the work. A quiz competition is then used to introduce students to the range of equations which contain velocity and then having been given them, they have to rearrange the formula to make velocity the subject and apply to some further questions. The final task of the lesson brings all the work together in one final competition where students have to use their new-found knowledge of speed and velocity to get TEAM POINTS. Progress checks have been written into the lesson at regular intervals to allow the students to check their understanding and any misconceptions to be addressed immediately. This lesson has been written for GCSE students and links between the other topics on the curriculum but could be used with KS3 students who are finding the topic of speed too simple and are needing a challenge