Year 10 Physics Learning Cycle 3 Overview How objects behave can always be predicted Learning Cycle Overview: Line of enquiry 1: Hypothesis 1 Hypothesis 2 How do objects fall? Falling objects travel with a constant velocity An objects terminal velocity is dependent on its weight Line of enquiry 2: Hypothesis 3 Hypothesis 4 How do objects stretch? Forces can only change the velocity of objects A springs stretch is dependent on the force applied Line of enquiry 3: Hypothesis 5 Hypothesis 6 Hypothesis 7 Hypothesis 8 How can forces and energy be linked? Work done is a measure of energy Gravitational potential energy is easily destroyed Momentum makes objects easier to stop Momentum is conserved Week 1 Week 1 Week 1/2 Year 10 Physics | Learning Cycle 2 | Medium Term Plan | Science 2015/16 How objects behave can always be predicted Line of enquiry two: How are waves different to each other? Intentions for learning from AQA GCSE specification: In this line of enquiry pupils should understand that: Waves transfer energy. Waves may be either transverse or longitudinal. All types of electromagnetic waves travel at the same speed through a vacuum (space). Electromagnetic waves form a continuous spectrum. The order of electromagnetic radiation Longitudinal waves show areas of compression and rarefaction Waves can be reflected, refracted and diffracted. The terms frequency, wavelength and amplitude. All waves obey the wave equation Radio waves, microwaves, infrared and visible light can be used for communication. The normal is a construction line perpendicular to the reflecting surface at the point of incidence. The angle of incidence is equal to the angle of reflection. The image produced in a plane mirror is virtual. Sound waves are longitudinal waves and cause vibrations in a medium, which are detected as sound. The pitch of a sound is determined by its frequency and loudness by its amplitude. Echoes are reflections of sounds. Lesson 3: All waves can be bounced back Lesson 1: All waves are the same Lesson 2: Electromagnetic waves all travel at the same speed Key words: longitudinal, transverse, wavelength, frequency Key words: vacuum Learning Intentions: Students should develop an understanding that: There are two types of wave which both carry energy All waves can be measured using ideas of frequency and wavelength to calculate wave speed Learning Intentions: Students should develop an understanding that: Electromagnetic waves are transverse waves Electromagnetic waves increase in energy and frequency as you go along the spectrum Success Criteria: Recall the two types of wave Describe the differences between the two types of wave Measure wavelength, and frequency for different waves Calculate the speed of a wave using the wave equation Success Criteria: Recall the names of the electromagnetic spectrum in order Describe what each part of the electromagnetic spectrum could be used for Describe how electromagnetic waves are different to each other Describe how electromagnetic waves are similar to each other Lesson 4: Virtual reality exists in mirrors Lesson 5: Sound can’t be reflected Key words: reflection, refraction, diffraction Key words: normal, incidence, reflection, virtual Key words: longitudinal, amplitude, frequency, pitch, volume Learning Intentions: Students should develop an understanding that: All waves can reflect, refract and diffract Learning Intentions: Students should develop an understanding that: Reflection follows specific laws to do with angles Reflected images in mirrors are virtual Learning Intentions: Students should develop an understanding that: Sounds are controlled by a combination of frequency and amplitude Echoes are just reflections of sound Success Criteria: Recall what the three terms mean Describe when diffraction is maximised Investigate how waves refract Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Peer assessed exam questions Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Peer assessed calculations & diagrams Success Criteria: Measure the angles of incidence and reflection accurately Describe how the angle of reflection and incidence are related mathematically Explain what is meant by virtual image Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Peer assessed practical skills Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Teacher assessed exam questions Success Criteria: Describe how sound waves travel differently to light waves Recall the meaning of amplitude Explain how sound waves can be changed in pitch Explain how sound waves can be changed in volume Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Teacher assessed exam question Year 10 Physics | Learning Cycle 2 | Medium Term Plan | Science 2015/16 How objects behave can always be predicted Line of enquiry two: How do waves change at speed? Intentions for learning from AQA GCSE specification: In this line of enquiry pupils: If a wave source is moving relative to an observer there will be a change in the observed wavelength and frequency. This is known as the Doppler effect. There is an observed increase in the wavelength of light from most distant galaxies. The further away the galaxies are, the faster they are moving, and the bigger the observed increase in wavelength. This effect is called red-shift. How the observed red-shift provides evidence that the universe is expanding and supports the ‘Big Bang’ theory (that the universe began from a very small initial point). Cosmic microwave background radiation (CMBR) is a form of electromagnetic radiation filling the universe. It comes from radiation that was present shortly after the beginning of the universe. The ‘Big Bang’ theory is currently the only theory that can explain the existence of CMBR. Lesson 8: There is lots of evidence for the ‘Big Bang’ theory Key words: big bang, CMBR, Learning Intentions: Students should develop an understanding that: There are two bits of evidence for the big bang Success Criteria: Recall what the big bang theory is Explain how redshift provides evidence for the big bang theory Explain how CMBR provides evidence for the big bang theory Evaluate why scientists believe the big bang theory to be true Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Teacher assessed exam questions Lesson 6: Cars change pitch based on direction Lesson 7: Galaxies moving towards the Milkyway appear blue Key words: Doppler effect Key words: redshift Learning Intentions: Students should develop an understanding that: Wavelength changes when wave sources are moving Learning Intentions: Students should develop an understanding that: Redshift causes galaxies to appear red Success Criteria: Recall how wavelengths are stretched out when objects move away from you Recall how wavelengths are compressed when objects move towards you Describe how these changes in wavelength affect both sound and light Success Criteria: Explain why all galaxies appear red Evaluate why some galaxies may appear more red than others Explain why galaxies furthest away are the most red Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Peer assessment of Doppler effect explanations Feedback Focus: Knowledge input | Check | Development | REACH | Improvement Details: Teacher assessed exam questions
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