vce physics study design: course planning for units 1 and 2 a powerpoint prepared by dan o’keeffe,...
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VCE Physics Study Design:VCE Physics Study Design:Course Planning for Units 1 and 2Course Planning for Units 1 and 2
A PowerPoint prepared by A PowerPoint prepared by
Dan O’Keeffe, Dan O’Keeffe,
[email protected]@bigpond.com
Course Planning for Units 1 and 2Course Planning for Units 1 and 2
Unit 1, then Unit 2Unit 1, then Unit 2
Sequence of Areas of StudySequence of Areas of Study
For each Area of Study:For each Area of Study:– New conceptsNew concepts– Some Practical ActivitiesSome Practical Activities– Possible Assessment TasksPossible Assessment Tasks
Unit 1: Sequence of Areas of StudyUnit 1: Sequence of Areas of Study
Almost any sequence could be argued for.Almost any sequence could be argued for.
Time: Time: Weeks per AoS is also an issue. Need to Weeks per AoS is also an issue. Need to decide on balance.decide on balance.
Titles of Areas of Study:Titles of Areas of Study: You need to decide on what you will call You need to decide on what you will call
the Areas of Study in your course the Areas of Study in your course documents and teaching: ‘How can documents and teaching: ‘How can thermal effects be explained?’ or thermal effects be explained?’ or ‘Thermodynamics’ or ‘Climate Change’.‘Thermodynamics’ or ‘Climate Change’.
Thermodynamics: New ConceptsThermodynamics: New Concepts
Zeroth law of ThermodynamicsZeroth law of Thermodynamics Internal EnergyInternal Energy First Law of ThermodynamicsFirst Law of Thermodynamics Thermal Radiation: Thermal Radiation:
– Wien and Stefan & BoltzmannWien and Stefan & Boltzmann
Energy FlowEnergy Flow
Zeroth Law of ThermodynamicsZeroth Law of Thermodynamics• A late addition to physics, for completenessA late addition to physics, for completeness• A definition of temperature.A definition of temperature.• ““All heat is of the same kind”All heat is of the same kind”
Internal EnergyInternal Energy
You are heating a substance, what happens to its You are heating a substance, what happens to its atoms and molecules?atoms and molecules?Gas:Gas:
Monatomic: NeMonatomic: Ne
Diatomic: ODiatomic: O22
Multi atom: HMulti atom: H22OO
Liquid:Liquid:Solid:Solid:Atoms and molecules have different types of energy.Atoms and molecules have different types of energy.Only Only translationaltranslational kinetic energy relates to Temp. kinetic energy relates to Temp.
Internal energy Internal energy
First Law of ThermodynamicsFirst Law of Thermodynamics
• Energy is conserved, Energy is conserved, • but done quantitatively and best with a gas examplebut done quantitatively and best with a gas example• Three terms:Three terms:
• Energy can be added Energy can be added toto a a systemsystem, Q, Q• Work can be done Work can be done byby a a systemsystem, W, W• Internal energy can change as a result, Internal energy can change as a result, UU
U = Q – WU = Q – WOnly simple calculations.Only simple calculations.
Energy Transfer by RadiationEnergy Transfer by Radiation
Radiation and Greenhouse EffectRadiation and Greenhouse EffectA significant section with many new physics concepts:A significant section with many new physics concepts:
• SpectrumSpectrumTemperature meansTemperature meansatoms jiggleatoms jiggleelectrons jiggleelectrons jiggle accelerating chargesaccelerating charges electromagnetic radiationelectromagnetic radiation
• Freq, wavelength Freq, wavelength • Energy, powerEnergy, power Increasing frequency
Decreasing wavelength
Increasing energy
Energy Transfer by RadiationEnergy Transfer by Radiation
Radiation and Greenhouse EffectRadiation and Greenhouse Effect• Increased temperature meansIncreased temperature means
atoms jiggle fasteratoms jiggle fasterelectrons jiggle fasterelectrons jiggle fasterhigher frequency radiationhigher frequency radiationhigher energyhigher energy
Thermal RadiationThermal Radiation
Wien’s Law: Wien’s Law: How does the wavelength of maximum intensity vary How does the wavelength of maximum intensity vary with temperature?with temperature?
maxT = constant
Thermal RadiationThermal RadiationStefan-Boltzmann Law: Stefan-Boltzmann Law: How does total energy emitted How does total energy emitted
vary with temperature?vary with temperature?Consider Area under the graph: Consider Area under the graph: PowerPower ∝ ∝ TT44..
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
Light reflected from EarthAverage Value
100 watts per square metre
Light from the SunLight from the SunAverage ValueAverage Value
340 watts 340 watts per square metreper square metre
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
Light from the Sun heats the Earth…Light from the Sun heats the Earth…
Average Value 240 watts per square
metre
Average Value240 watts
per square metre
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
How hot must the Earth be to radiate 240 W/mHow hot must the Earth be to radiate 240 W/m22 ? ?
Average Value 240 watts per square
metre
-18 °C
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
-18 °C
Actual average surface
temperature
33 °CGreenhouse
EffectTemperature for radiation
balance
+15 °C
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
The Earth’s surface is The Earth’s surface is 33 °C 33 °C warmer warmer than it would be if it had no atmospherethan it would be if it had no atmosphere
So So howhow does the atmosphere does the atmosphere
warm the Earth’s surface?warm the Earth’s surface?
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
Nitrogen (NNitrogen (N22),), Oxygen (OOxygen (O22)) & & Argon (Ar) Argon (Ar) • More than 99% of the atmosphere More than 99% of the atmosphere
• These molecules have These molecules have oneone or or twotwo atoms atoms
• They block some They block some ultra-violetultra-violet light, but light, but
• Allow Allow infra-redinfra-red and and visiblevisible radiation through. radiation through.
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
With an atmosphere of With an atmosphere of Nitrogen Nitrogen OxygenOxygen & & Argon, Argon, what would what would
be the surface temperature?be the surface temperature?
-18 °C
Average Value 240 watts per square
metre
Average Value240 watts
per square metre
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
Greenhouse warming is caused by Greenhouse warming is caused by
Water (HWater (H22O)O)
Carbon Dioxide (COCarbon Dioxide (CO22))
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
What is special about What is special about HH22O and COO and CO22??
• Their molecules have Their molecules have threethree atoms, atoms,
• Their Their natural frequenciesnatural frequencies of vibration are in the of vibration are in the infra-red,infra-red,
• They are the earth’s blanket for reflecting certain They are the earth’s blanket for reflecting certain infra-redinfra-red frequencies back down to earth. frequencies back down to earth.
Infra RedUltra Violet Visible
Infrared Radiation absorbed by Water and COInfrared Radiation absorbed by Water and CO22
What determines the Earth’s surface temperature?What determines the Earth’s surface temperature?
Greenhouse Warming
33 °CH2O
CO2
+15oC
–18oC
Global Energy Flows (W/mGlobal Energy Flows (W/m22))
Practical ActivitiesPractical Activities• Introductory activities Introductory activities on phenomena to stimulate on phenomena to stimulate
curiosity and generate students’ questionscuriosity and generate students’ questions• ExperimentsExperiments
Heat capacity: Heat capacity: i) mixing liquids, i) mixing liquids, ii) adding heated block to waterii) adding heated block to wateriii) heat capacity of thermosiii) heat capacity of thermosiv) microwave oven exptiv) microwave oven expt
11stst Law: Law: Calorimeter prac (link to elec)Calorimeter prac (link to elec)Latent Heat:Latent Heat: i) Add ice to hot wateri) Add ice to hot waterMechanical Equivalent of heatMechanical Equivalent of heat
Practical ActivitiesPractical Activities• Experiments ctdExperiments ctd
Absolute Zero from Volume vs TempAbsolute Zero from Volume vs TempRadiation:Radiation: i) Spectra of hot objects, i) Spectra of hot objects,
ii) Stefan-Boltzmann Exptii) Stefan-Boltzmann Expt
• Investigation: Investigation: Keeping it Hot – design, build & testKeeping it Hot – design, build & test
* Discount craft supplies* Discount craft supplies* Reverse Art Truck* Reverse Art Truck
• Spreadsheet: Investigation of a Climate modelSpreadsheet: Investigation of a Climate model
Assessment TasksAssessment Tasks
Written response to a selection of context questions
Exploration of an issue related to thermodynamics
Assessment TasksAssessment Tasks
Issue related to thermodynamics Apply thermodynamic principles to investigate at least one
issue related to the environmental impacts of human activity with reference to the enhanced greenhouse effect.
Consider: * other topics such as solar thermal power,
geo-engineering, blog related discussion ....
* integrating the task into the work program.
* a team approach with a group presentation.
* how much resourcing do you supply.
* how much guidance and structure.
ElectricityElectricity
Extra ContentExtra Content Voltage dividersVoltage dividers Specific reference to thermistors, LDRs, LEDsSpecific reference to thermistors, LDRs, LEDs Energy transfer with reference to transducersEnergy transfer with reference to transducers Specific reference to Residual Current DevicesSpecific reference to Residual Current Devices
So, basically the same, with slightly extra So, basically the same, with slightly extra content, which many currently do.content, which many currently do.
What is Matter?What is Matter?
Big Bang and CosmologyBig Bang and Cosmology
Radioactivity and Nuclear forcesRadioactivity and Nuclear forces Hadrons and Leptons, Baryons Hadrons and Leptons, Baryons
and Mesons, Quarksand Mesons, Quarks Anti-matterAnti-matter
Fission and FusionFission and Fusion Binding energy and E = mcBinding energy and E = mc22
Production of lightProduction of light
Origins of atoms
Particles in the nucleusParticles in the nucleus
Energy from the atomEnergy from the atom
How to group the content?How to group the content?In what order do you want to teach it?In what order do you want to teach it?
What is Matter?What is Matter?
Different approaches are possible.Different approaches are possible.
History of Science view:History of Science view: Radioactivity: decay, half life, nuclear Radioactivity: decay, half life, nuclear
transformations, decay series as well as transformations, decay series as well as and and neutrino.neutrino.
Fission and Fusion: Equations, Binding energy Fission and Fusion: Equations, Binding energy and E = mcand E = mc22..
Discovery of extra particles: anti-particles, Discovery of extra particles: anti-particles, hadrons, then mesons and baryons leading to hadrons, then mesons and baryons leading to quarks.quarks.
What is Matter?What is Matter?
History of Science view ctd:History of Science view ctd: Cosmology: Big Bang theory including Cosmology: Big Bang theory including
inflation, inflation, elementary particle formation, annihilation of anti-matter and matter, commencement of nuclear fusion, cessation of fusion and the formation of atoms.
Production of light: accelerating charges, synchrotron, energy level transition
What is Matter? - ChallengesWhat is Matter? - Challenges
Most of the new stuff!, however …Most of the new stuff!, however …
It is mostly descriptive, so ….It is mostly descriptive, so ….
Treat it to your own comfort level, e.g.Treat it to your own comfort level, e.g. Cover cosmology with a 50 min Brian Cox Cover cosmology with a 50 min Brian Cox
video, orvideo, or Applets from The Particle Adventure, CERN, …Applets from The Particle Adventure, CERN, …
What is Matter? - New ConceptsWhat is Matter? - New ConceptsNuclearNuclear
Anti-matter: Anti-matter: Introduce beta plus decay with beta Introduce beta plus decay with beta minus decay.minus decay.
Neutrino:Neutrino: Introduce to explain energy discrepancy Introduce to explain energy discrepancy in beta decay.in beta decay.
Forces:Forces: Strong and weakStrong and weakMuon, etc:Muon, etc: Alpha spectra is discrete Alpha spectra is discrete internal internal
nuclear structure nuclear structure Yukawa model Yukawa model discovery of muon, then discovery of muon, then meson meson even more particles.even more particles.
Quarks et al:Quarks et al: Explains observed particlesExplains observed particles
Matter
Quarks Leptons
Mesons Baryons
Nuclei
Atoms
Hadrons
Everyday matter Exotic matter
Hadrons: Mesons and BaryonsHadrons: Mesons and Baryons
Mesons:Mesons: made of one quark and one anti-quark,made of one quark and one anti-quark,positive, negative or neutral,positive, negative or neutral,examples: Pion, K-meson, over 100examples: Pion, K-meson, over 100
Baryons:Baryons: made of three quarks,made of three quarks, +2 to -2 in charge,+2 to -2 in charge,examples: neutron, proton, Lambda, examples: neutron, proton, Lambda, Sigma, and …, about 100, …Sigma, and …, about 100, …double charmed bottom, etcdouble charmed bottom, etc
What is Matter? - New ConceptsWhat is Matter? - New ConceptsBinding Energy Curve and E = mcBinding Energy Curve and E = mc22
How quantitativeHow quantitativedo you go?do you go?
Which units?Which units?MeV, JoulesMeV, Joules
Fusion Reaction: Fusion Reaction: 22D + D + 22D = D = 44He He Calculation steps:Calculation steps:1. Mass of 1. Mass of 22D, D, 2. Mass of 2. Mass of 44He, He, 3. Mass diff, 3. Mass diff, 4. Energy release4. Energy release
Production of LightProduction of Light
electromagnetic wave by accelerating charges,, synchrotron radiation at a tangent to a circle, light from transitions between energy levels.
These topics don’t seem to link to the rest of Unit 1.These topics don’t seem to link to the rest of Unit 1.
So, how do you approach these aspects?So, how do you approach these aspects?
CosmologyCosmology
So much descriptive content …So much descriptive content …
How do you approach it?How do you approach it? Brian Cox videoBrian Cox video Images and graphsImages and graphs Story lineStory line
Big Bang Model: Expanding, intensely hot gas of elementary particles. Explains observable universe back to 1 second.
Big Bang model: Explains Hubble constant, background radiation, proportion of H, He and Li.
Does not explain i) uniformity of universe, ii) universe before 1 sec and iii) energy density of the universe,
but inflationary model does.
What is Matter?What is Matter?
Practical ActivitiesPractical Activities
Radioactivity PracsRadioactivity Pracs
Dice pracsDice pracs
What is Matter? - Assessment TasksWhat is Matter? - Assessment Tasks an annotated folio of practical activities data analysis design, building, testing and evaluation of a device an explanation of the operation of a device a proposed solution to a scientific or technological
problem a modelling activity a media response a summary report of selected practical investigations a reflective learning journal/blog related to selected
activities or in response to an issue a test comprising multiple choice and/or short answer
and/or extended response
What is Matter? - Assessment TasksWhat is Matter? - Assessment Tasks
What’s left? a media response
Evaluation of responses in an online discussion
a reflective learning journal/blog related to selected activities or in response to an issue
a test comprising multiple choice and/or short answer and/or extended response
Unit 2Unit 2
Motion Area of Study (with extra content)Motion Area of Study (with extra content)
Options ( 12 on offer)Options ( 12 on offer)
Practical Investigation ( on any of above)Practical Investigation ( on any of above)
Q’ns: Q’ns:
1.1. Do you split Motion or not?Do you split Motion or not?
2.2. Managing several options at same time?Managing several options at same time?
Unit 2 OptionsUnit 2 Options
Why you should run more than one option.Why you should run more than one option. The number of options that students do over the The number of options that students do over the
two years has dropped from 4 to 3 and now to 1.two years has dropped from 4 to 3 and now to 1.
Enrolment data indicates that since the Enrolment data indicates that since the introduction of Detailed Studies, the proportion of introduction of Detailed Studies, the proportion of Year 11 Physics students staying on to do Year 12 Year 11 Physics students staying on to do Year 12 physics has steadily increased, both boys and girls. physics has steadily increased, both boys and girls. Conclusion: Students value them. Conclusion: Students value them.
Students learn about options as well as their own.Students learn about options as well as their own.
MOTIONMOTION
Largely the same, but with extra content:Largely the same, but with extra content: TorqueTorque Rotational equilibriumRotational equilibrium
Differences: Differences: Description of Force: Force Description of Force: Force onon A A byby B B Word ‘Weight’ is not used in the study design.Word ‘Weight’ is not used in the study design.
How do you approach these changes?How do you approach these changes?
Unit 2 OptionsUnit 2 Options
Suggestions for managing more than one option:Suggestions for managing more than one option: Student learning: individual, team based or jigsaw Student learning: individual, team based or jigsaw
method, not teacher directed.method, not teacher directed. Resources are prepared for several options.Resources are prepared for several options. Each teacher decides which ones they are Each teacher decides which ones they are
comfortable offering.comfortable offering. Allow students to choose, with a minimum number Allow students to choose, with a minimum number
of students ( eg 4) required for an option to proceed.of students ( eg 4) required for an option to proceed. Teacher’s role: monitor, guide, support.Teacher’s role: monitor, guide, support. Reporting back to the whole class.Reporting back to the whole class.
Unit 2 Options: AssessmentUnit 2 Options: Assessment
Need to be consistent, but not onerous. Need to be consistent, but not onerous.
Some possibilities are:Some possibilities are: an annotated folio of practical activities
a media response
a summary report of selected practical investigations
a reflective learning journal/blog related to selected activities or in response to an issue
Unit 2 Practical InvestigationUnit 2 Practical Investigation
Now a separate Area of Study.Now a separate Area of Study. The topic a student investigates can come from The topic a student investigates can come from
Motion or any of the 12 Options.Motion or any of the 12 Options. Now more substantial, the Now more substantial, the student ‘designs and
undertakes an investigation involving two independent variables one of which should be a continuous variable. A logbook must be maintained ….’
Topics can include ‘construction and evaluation of a device’.
Unit 2 Practical InvestigationUnit 2 Practical Investigation
Requires class time for planning, design, implementation, data analysis and writing up
Plenty of topics for students to choose from. Preferable to report as:
– A log book with
– A summary in the form of an electronic poster, (e.g. a single powerpoint slide, templates are available).
Year 11 ExamYear 11 Exam
Consider:Consider: assessing the whole year, in preparation for the assessing the whole year, in preparation for the
Year 12 exam,Year 12 exam,
Including generic questions on the practical Including generic questions on the practical investigation.investigation.