A complete lesson covering section 5.2.1 and 5.2.2 of the OCR Physics specification- circular motion It covers circular motion, centripetal force and acceleration and all associated equations. The lesson closes with a practical investigating and analysing circular motion Lots of students activities included All activities in PPT as I aim to reduce photos=copying

A complete lesson covering section 5.3.3 a-e of the OCR Physics specification- free and forced oscillations and damping of SHM. This covers the difference between free and forced oscillations and the effect of resonance. It then looks at damping especially as a means of reducing the effects of resonance for example in earthquakes. Includes a starter, full notes and lots of student independent tasks. I always try to reduce photocopying so all activities are found in the PPT. All answers provided

A complete lesson covering section 5.4.1 a- e of the OCR Physics specification- gravitational fields It includes a starter, full notes, various independent activities and a differentiated summary at the end The lesson covers gravitational fields, the law of gravitation and calculating gravitational field strength All answers included I aim to reduce photocopying so all resources are within the PPT (31 slides in total)

A complete lesson covering points 5.5.1 b-f of the OCR Physics specification- the life cycle of stars. It starts with the formation of stars from dust and gas then works though the various stages of the life cycle for all sizes of stars. It includes the Chandrasekhar limit as a determiner of which cycle a star will go through. It includes links to several videos on you-tube and a card sort work sheet. The lesson includes lots of independent tasks including a variety of calculation questions All answers included I aim tor educe photocopying so the majority of activities are in the PPT- 38 slides in total

A complete lesson covering sections 5.5.1e and 5.5.3 a-k of the OCR Physics specification- stellar radiation and luminosity and stellar spectrum. It starts by looking at the way that objects produce electromagnetic radiation and the link to temperature. It then looks at Wien’s displacement law and Stefan’s law including calculations and comparisons of luminosity and temperature. It then move son to look at spectra and how electrons produce photons of light after being excited. It then closes by looking at the difference between emission and absorption spectrum and how they can be sued to analyse stars. Includes lots of independent activities All answer included I aim to reduce photocopying so all resources are in the PPT- 49 slides in total

A complete lesson covering sections 5.5.3 d-o of the OCR Physics specification- the big bang theory, the cosmological principle, the Doppler effect and red shift. The lesson starts by covering the Doppler effect in sound and how this also applies to red shift in light. It the covers how this and CMBR act as evidence for the origins of the universe in the big bang. It covers the Hubble constant, how its value is not exact and how it can be sued to estimate the age of the universe. The lesson closes by looking at the events immediately following the big bang and how the universe is believed to have changed. The lesson includes lots of calculations and multiple student activities All answers are provided I aim tor educe photocopying so all resources are within the PPT- a total of 50 slides

A complete revision lesson covering section 6.5.1-3 of the AQA trilogy course- forces. It covers forces and their interactions, work done and energy transfer and elasticity. The lesson includes a variety of student led activities, retrieval practice and exam questions All answers provided