Monday, 25 May 2026

Week 6 Term 2 2026 Nuclear Reactions

 Homework

Models of the Atom & Radioactivity

  • Act 15A, p.173-176 Models of the Atom and Radioactivity
  • Ex 5A, p. 151-155 Models of the Atom
  • Ex 5B, p.160-171 Radioactivity

Nuclaer Reactions
  • Act 16A, p. 181, Nuclear Reactions
  • Ex 5C, p.175-182 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

Sunday, 10 May 2026

Week 4 Term 2 2026 Models of the Atom

 Homework

  • Act 15A, p.173-176 Models of the Atom and Radioactivity
  • Ex 5A, p. 151-155 Models of the Atom
  • Ex 5B, p.160-171 Radioactivity


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


Tuesday, 28 April 2026

Week 2 Term 2 Torque

  Homework

Vectors
  • Act 9A Vectors p.108-109
  • Ex 4A Vectors p.90-94

Kinematics

  • Act 8B Graphs of motion p.101
  • Act 8C Kinematics p.102
  • Ex 4E Kinematics p.115-117

Projectile Motion
  • Act 12B Projectile Motion p.140-141
  • Ex 4F Projectile Motion p.119-124

Forces
  • Act 10A Forces p.117-118
  • Act 10B Forces p.123-124
  • Ex 4B Forces p.97-104
Circular Motion
  • Act 13A p.148-149 Circular Motion
  • Ex 4H p.132-134 Circular Motion

Energy
  • Act 14B, p. 158-160 Combined Mechanics
  • Ex 4J, p. 143-147 Energy, Work, Power

Springs
  • Act 14A p.155 Energy & Springs
  • Ex 4I p.137-141 Springs

Momentum & Impulse
  • Act 11A, p.130 Momentum and Impulse
  • Act 11B, p. 133-134 Collisions
  • Ex 4D, p.108-112 Momentum P = mv
  • Ex 4C, p.105-107 Impulse ΔP = FΔt

Torque
  • Act 10B, p.123-124, Torque
  • Ex 4G p.125-130 Torque

    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

Torque and Equilibrium


Sunday, 19 April 2026

Term 2 Week 1 Momentum & Impulse

 Homework

Vectors
  • Act 9A Vectors p.108-109
  • Ex 4A Vectors p.90-94

Kinematics

  • Act 8B Graphs of motion p.101
  • Act 8C Kinematics p.102
  • Ex 4E Kinematics p.115-117

Projectile Motion
  • Act 12B Projectile Motion p.140-141
  • Ex 4F Projectile Motion p.119-124

Forces
  • Act 10A Forces p.117-118
  • Act 10B Forces p.123-124
  • Ex 4B Forces p.97-104
Circular Motion
  • Act 13A p.148-149 Circular Motion
  • Ex 4H p.132-134 Circular Motion

Energy
  • Act 14B, p. 158-160 Combined Mechanics
  • Ex 4J, p. 143-147 Energy, Work, Power

Springs
  • Act 14A p.155 Energy & Springs
  • Ex 4I p.137-141 Springs

Momentum & Impulse
  • Act 11A, p.130 Momentum and Impulse
  • Act 11B, p. 133-134 Collisions
  • Ex 4D, p.108-112 Momentum P = mv
  • Ex 4C, p.105-107 Impulse ΔP = FΔt
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)


Momentum and Impulse Explained





Impulse


Impulse


Impulse examples///Homemade Science with Bruce Yeany



Momentum

Impulse


Monday, 30 March 2026

Term 1 Week 9 Springs

 Homework

Vectors
  • Act 9A Vectors p.108-109
  • Ex 4A Vectors p.90-94

Kinematics

  • Act 8B Graphs of motion p.101
  • Act 8C Kinematics p.102
  • Ex 4E Kinematics p.115-117

Projectile Motion
  • Act 12B Projectile Motion p.140-141
  • Ex 4F Projectile Motion p.119-124

Forces
  • Act 10A Forces p.117-118
  • Act 10B Forces p.123-124
  • Ex 4B Forces p.97-104
Circular Motion
  • Act 13A p.148-149 Circular Motion
  • Ex 4H p.132-134 Circular Motion

Energy
  • Act 14B, p. 158-160 Combined Mechanics
  • Ex 4J, p. 143-147 Energy, Work, Power

Springs
  • Act 14A p.155 Energy & Springs
  • Ex 4I p.137-141 Springs


Hooke's Law

Hooke's Law Introduction - Force of a Spring



Hooke's Law F = -kx



Elastic Potential Energy


Intro to Springs and Hooke's Law


Potential Energy Stored in a Spring

How Hard Can You Hit A Golf Ball?