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Physics Distribution of Topics
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MIDTERM
WEEK DAYS TOPICS COMPETENCIES1 5 Input of Pre-requisite
informationDay 1: Day 2:Day 3:
2 5 Aristotelian vs. Galilean Views of Motion
Horizontal motion Vertical motion Projectile motion
Galileo’s Uniform Accelerated Motion
Compare and contrast the Aristotelian conceptions of vertical motion, horizontal motion, and projectile motion.explain how Galileo inferred that objects in vacuum fall with uniform acceleration, and that force is not necessary to sustain horizontal motion
3 2 Graphs x vs. t v vs. t a vs. t
Day 1-2: explain how the position vs. time, and velocity vs. time graphs of constant velocity motion are different from those of constant acceleration
2 1st Law of Motion vs. Galileo’s assertion that force is not necessary to sustain horizontal motion
Day 3-4: Explain the subtle distinction between Newton’s 1st law of Motion (or Law of Inertia) and Galileo’s assertion that force is not necessary to sustain horizontal motion
4 5 Newton’s Law of Gravitation(explaining the rate of free fall of objects with different masses)
Use algebra, Newton’s 2nd Law of Motion, and Newton’s Law of Universal Gravitation to show that, in the absence of air resistance, objects close to the surface of the Earth fall with identical accelerations independent of their massesapply Kepler’s 3rd law of planetary motion to objects in the solar system
FINALS
9-10 Maxwell’s EquationUnification of Electricity and Magnetism
Explain the contribution of Franklin, Coulomb, Oersted, Ampere, Biot-Savart, Faraday, and Maxwell to our understanding of electricity and magnetism (computations)
11 Dispersion, Scattering, Interference, and DiffractionNewton’s and Descartes’ Theory of Light (Dispersion of Light through Prisms)
Differentiate scattering, interference, and diffraction Explain how Newton and Descartes described the emergence of light in various colors through prisms (concepts and computations)
12-13 Special Theory of Relativity
Relativity of Simultaneity
Time Dilation Length contraction Mass-energy
equivalenceCosmic Speed Limits
Explain how special relativity resolved the conflict between Newtonian mechanics and Maxwell’s electromagnetic theoryExplain the consequences of the postulates of Special Theory of Relativity (e.g. relativity of simultaneity, time dilation, length contraction, mass-energy equivalence, and cosmic speed limit)
14 General Theory of RelativityDoppler EffectsCosmic Ladder
Expansion of the UniverseDoppler Shifts
Explain the consequences of the postulates of General Relativity (e.g. correct predictions of shifts in the orbit of Mercury, gravitational bending of light, and black holes) (concepts)
Explain how the speeds and distances of far-off objects are estimated (e.g. Doppler Effect and Cosmic Distance Ladder)
Explain how we know that we live in an expanding universe, which used to be hot and is approximately 14 billion years old. (g11 1st sem)
Explain how Doppler Effects and transits can be used to detect extra solar planets
15 Wavelength-Speed-Frequency relationPhotoelectric EffectPhoton Energy (E=hf) Applications
Red Light (Emergency Rooms)
UV light (sunburn)
How we see colorsElectron Diffraction
Apply the wavelength-speed-frequency relation Explain how the photon concept and the fact that
the energy of a photon is directly proportional to its frequency can be used to explain why red light is used in photographic dark rooms, why we get easily sunburned in ultraviolet light but not in visible light, ad how we see colors
Cite experimental evidence showing that electrons can behave like waves
16 FINALS