Tuesday 16 March 2021

 Resources for Nuclear Debate - link to all the blog posts on this topic

The Big Lie About Nuclear Waste



Problems with Solar in North Africa



How much land does it take to Power the World?



How much Electricity do we need?


Gravitricity



Flywheel - Mechanical Battery



Hydropower



Why Renewables Can't Save the Planet


Supercapacitors



Geothermal Energy Problems


Small Modular Nuclear Reactors


Perscovits Solar Cells


India's Solar Canals



Thursday 4 March 2021

Term 1 Week 5 2021

  Homework:


  • Activity 11A, p.176 Waves & Photons (last week)
  • Activity 11B, p.179 Photoelectric Effect (last week)
  • Activity 11C, p.183 Atomic Line Spectra
  • Activity 11D, p.188-189 Bohr Model of Hydrogen Atom
  • Activity 12A, p.194 E = mc^2

When is now Relativity and Neurology



Nuclear Fission




Nuclear Fission; splitting the atom for beginners



Nuclear Physics: Crash Course Physics #45


Nuclear Chemistry: Crash Course Chemistry #38


Nuclear Chemistry Part 2: Fusion and Fission - Crash Course Chemistry #39


Nuclear Fission

  • The breaking up of a larger nucleus into smaller nuclei
  • The decrease in mass per nucleon, matches the increase in binding energu per nucleon
  • This binding energy per nucleon is a negative energy and represents energy that is lost (radiated away) during the reaction. 
  • Binding energy per nucleon also represents the energy that would need to be added to liberate a nucleon from the nucleus
Nuclear Fission

Fission & Fusion

Nuclear Fusion
  • The joining of smaller nuclei into a larger nucleus
  • The decrease in mass per nucleon, matches the increase in binding energu per nucleon
  • This binding energy per nucleon is a negative energy and represents energy that is lost (radiated away) during the reaction. 
  • Binding energy per nucleon also represents the energy that would need to be added to liberate a nucleon from the nucleus

Nuclear Fusion

Fusion Energy

Binding Energy per Nucleon

Nuclear Reaction E = mc2




Binding Energy per Nucleon

Binding Energy per Nucleon is a negative energy or a debt of energy. This is the amount of energy it would take to liberate a nucleon from the nucleus. This energy was originally radiated off when the nucleus formed.

The energy radiated off, the Binding energy, is lost energy and comes from mass that is lost by the nucleons. Mass per Nucleon shows what is left over once a bound nucleon has radiated away some of its mass.


Mass per Nucleon


Fission:The breaking up of a larger nucleus into smaller daughter nuclei. Anything above Iron will radiate off energy.

Fusion:
The joining of smaller nuclei into a larger nucleus. Anything below Iron will radiate off energy.


Fission & Fusion

Fission

Monday 1 March 2021

Term 1 Week 4 20201

 Homework:


  • Activity 11A, p.176 Waves & Photons (last week)
  • Activity 11B, p.179 Photoelectric Effect (last week)
  • Activity 11C, p.183 Atomic Line Spectra
  • Activity 11D, p.188-189 Bohr Model of Hydrogen Atom

How Quantum Mechanics Saved Physics From Ovens


Photoelectric Effect

Planck's Constant - Sixty Symbols




Atomic Line Spectra

Hydrogen Emission and Absorption Spectra for the visible Balmer Series


Atomic Line Spectra for Hydrogen

Emission & Absorption Lines for Hydrogen


Emission Lines for Hydrogen

Bohr Model of the Hydrogen Atom
Line Spectra & the Bohr Model

Emission and Absorption Line Spectra



Bohr Model of the Hydrogen Atom

Energy Levels


Bohr Model of the Hydrogen Atom