Wednesday, 9 June 2021

Term 2 Week 6 2021

  Homework:

  • Act 15A, p. 173-176, Particles and Half-Life
  • Act 16A, p. 181, Nuclear Reactions
  • Act 5A, p,53, Pulses and Waves
  • Worksheet on Superposition and Reflection

Basic Properties of Waves
waves transfer energy through a medium without transferring the medium itself

  • Cycle - a basic repeating unit in a wave
  • Amplitude A (m) - the distance from the middle point to the top of a crest, or bottom of a trough
  • Wavelength 𝜆 (m) - the distance/length of one cycle
  • Period T (s = s per cycle) - the time it takes for one cycle to pass a point
  • Frequency f (Hz = cycles per second) - the number of cycles that pass in one second

T = 1/f & f = 1/T


  • Wave Speed v (ms-1) the speed of a wave
v = 𝜆/T & v = f𝜆


Wave Properties

Frequency & Period

Wave Phase

Pendulum Waves

Longitudinal Waves
particle displacement in the medium is parallel to the direction of wave propagation e.g. sound waves, primary earthquake waves

Transverse Waves
particle displacement in the medium is perpendicular to the direction of wave propagation e.g. light and other electromagnetic waves, secondary earthquake waves



  • Superposition of Waves: two waves traveling through each other will not change each other motion in any way, but they will add to one another when they overlap
    • Constructive Interference - Reinforcement - In Phase
    • Destructive Interference - Cancellation - Out of Phase



Reflection on A String
Hard Boundary
Wave reflects on opposite side (opposite phase)
Same Amplitude, A
Same Wavelength, 𝛌
Same Wave Speed, v

Reflection on A String
Soft Boundary
Wave reflects on same side (same phase)
Same Amplitude, A
Same Wavelength, 𝛌
Same Wave Speed, v

Refraction on A String
Fast to Slow Boundary
Relation of waves to Incident Wave
Reflected Wave - same speed - same wavelength 𝛌 - opposite phase
Refracted Wave - slower speed - smaller wavelength 𝛌 - same phase

Refraction on A String
Slow to Fast Boundary
Relation of waves to Incident Wave
Reflected Wave - same speed - same wavelength 𝛌 - same phase
Refracted Wave - faster speed - larger wavelength 𝛌 - same phase

Term 2 Week 4 2021

  Homework:

  • Act 15A, p. 173-176, Particles and Half-Life
  • Act 16A, p. 181, Nuclear Reactions

Nuclear Reactions:
  • Conservation of Atomic Number
  • Conservation of Nucleon Number
  • Conservation of Mass-Energy E = Δmc2

E = Δmc2




Nuclear Fusion in the Sun

Binding Energy comes from the change in mass from individual nucleons to being combined into a nucleus. This is energy lost by the nucleons joined together in a nucleus and must be returned in order to separate the nucleons
E = Δmc2

Element formation in Stars Nuclear Fusion



Binding Energy Per Nucleon

Mass Per Nucleon


Nuclear Reactions

Fission Fusion and Radioactive Decay

Fission & Fusion

Natural Nuclear Fission Reactor

Wednesday, 19 May 2021

Term 2 Week 3 2021

 Homework:

  • Act 11A, p.130, Momentum and Impulse
  • Act 11B, p. 133-134, Collisions
  • Act 10A, p. 117-118, F = ma
  • Act 10B, p. 123-124, Force, Motion, Equilibrium, Torque
  • Act 15A, p. 173-176, Particles and Half-Life


Models of the Atom


History of the Atom

Models of the Atom Timeline



Discovery of the Electron: Cathode Ray Tube Experiment


Discovery of the Nucleus: Rutherford's Gold Foil Experiment


Charge of an Electron: Millikan's Oil Drop Experiment


Atomic Structure: Discovery of the Neutron


Parts of the Atom


Isotopes
Isotopes are versions of an atom or an element that have the same number of protons, but different numbers of neutrons



What are Isotopes?




Radioactive Decay
Alpha, Beta & Gamma Radiation



  • Alpha particles are emitted by a larger nucleus that has too many Protons
  • Beta particles are emitted by a nucleus that has too many Neutrons
  • Gamma photons are emitted by a nucleus that has too much Energy (is in an exited state)





Alpha Decay

Beta Decay


Radiation

Types of Radiation

Is radiation dangerous?

The Most Radioactive Places on Earth

Millisieverts and Radiation - Sixty Symbols

Half Life Calculations


Term 2 Week 1 2021

 Homework:

  • Act 11A, p.130, Momentum and Impulse
  • Act 11B, p. 133-134, Collisions
  • Act 10A, p. 117-118, F = ma
  • Act 10B, p. 123-124, Force, Motion, Equilibrium, Torque

Forces


Mass on a Slope

Drawing a Free Body Diagram


Net Force - PhET Application - link here

What is a Force?


What Forces are Acting on You?

Best Film on Newton's Third Law Ever

What is Gravity

The Difference Between Mass & Weight


Misconception About Falling Objects

    Torque
    𝝉 = F L⦜
    𝝉: Torque (Nm)
    F: applied Force (N)
    L⦜: Length of lever at right angles to the applied force (m)

    • Torque (Moments) in Level 2 Physics will involve Static Systems
    • Therefore the Torques are balanced and the Forces are balanced - Newton's Laws of Motion apply to turning forces as well as linear forces
    • PhET - Torque Balancing Act simulation

    Bridge support forces moments


    Torque (Moments anout a point)
    Static (unmoving) systems will be used for this section. Therefore all forces, linear and turning, are balanced






    Torque

Sunday, 2 May 2021

Term 1 Week 11 2021

 Homework:

  • Act 11A, p.130, Momentum and Impulse
  • Act 11B, p. 133-134, Collisions

Momentum

Conservation of Momentum
In the absence of external forces the total momentum of a system is always conserved

Impulse
The change in Momentum for a single object
ΔP = Pf - Pi
&
ΔP = FΔt
&
ΔP = mΔv
  • The unis are eithor Ns or kgms-1 , this is the same unit and the one that is used depends on the context
  • Impulse on one object is always equal and opposite to the impulse on the other onject - Newton's Third Law



Physics of Car Crashes (Impulse)

Impulse


Impulse


Impulse examples///Homemade Science with Bruce Yeany



Momentum

Impulse