A comprehension lesson that teaches students how to measure force using practical equipment as well as calculate resultant forces.
Progress checks are available following each success criteria
Tasks are differentiated to suit the needs of each learner.
Learning objective: Develop an understanding of how forces interact within a pair or multiples in perpendicular directions.
By the end of the lesson learners should be able to:
Success criteria:
State how forces are represented.
Describe how to calculate the resultant force.
Calculate forces in horizontal and vertical directions.
Powerpoint contains 30 slides.
A comprehension lesson that teaches students how to measure speed by using the formula triangle with some reference to practical applications.
Support sheets are also included to guide students should it be needed.
Tasks are differentiated to suit the needs of each learner.
By the end of the lesson students should be able to:
Success criteria:
I can calculate speed using the equation triangle.
I can analyse how to measure speed effectively using specific equipment
I can justify why objects appear to be travelling faster or slower with reference to relative motion.
Learning objective: To apply the idea of speed to real life instances.
Powerpoint contains 18 slides and a lesson plan is also attached.
Defnyddais google slides are gyfer addysgu’r wers hon. Ddylai bod o’n gweithio yn yr un modd drwy Microsoft PowerPoint ond efallai fydd angen ailosod rhai agweddau.
Erbyn diwedd y wers ddylech fod yn gallu:
Adnabod beth sydd yn achosi’r Haf a’r Gaeaf
Disgrifio sut mae’r Haul yn ymbelydru golau.
Egluro’r cysylltiad rhwng gogwyddo’r Ddaear â’r Tymhorau.
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 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.
Originally created for the BTEC Applied Science level 3 qualification Unit 5 - Physics.
By the end of the lesson learners should be able to:
Recall the ideal gas equation.
Describe how scientists calculated absolute zero.
Evaluate different thermometers.
The resource contains past paper questions and mark scheme answers.
Slides were originally created using google slides, opening in microsoft powerpoint might cause slight misalignment - open in google slides to avoid this.
Originally created for the BTEC Applied Science level 3 qualification Unit 5 - Physics.
By the end of the lesson learners should be able to:
Recall the equations involving work done by movement and work done by pressure expansion.
Describe how the area of cylinder heads affect the movement of fluids in hydraulics.
Use multiple equations to calculate the work, force and distance moved by hydraulic cylinders.
The resource contains past paper questions and mark scheme answers.
Slides were originally created using google slides, opening in microsoft powerpoint might cause slight misalignment - open in google slides to avoid this.
By the end of the lesson learners should be able to:
Identify pivots.
Describe how a moment is made.
Explain why doors have their handle on the furthest point from the pivot.
A revision session containing a mind map (with guidance and without).
A Powerpoint containing a quiz session (10 questions) - excellent for a starter / plenary.
Answers to each section of the mind map within the Powerpoint.
By the end of the lesson learners will be able to:
State what is meant by nuclear fission.
Describe how nuclear fission can cause a chain reaction.
Explain why nuclear fission must be controlled.
A revision session containing a mind map (with guidance and without).
A Powerpoint containing a quiz session (10 questions) - excellent for a starter / plenary.
Answers to each section of the mind map within the Powerpoint.
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.
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 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 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.