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PHYSICS, M7 2025 HSC 19 MC

A system consists of a sealed glass jar containing some oxygen and a small strip of magnesium.

The magnesium reacts with the oxygen to produce magnesium oxide as a product. Energy is released from the system in this reaction.

The mass of the system will

  1. increase because oxygen is added to the magnesium.
  2. decrease because energy is removed from the system.
  3. increase because energy is added to the system by the reaction.
  4. decrease because magnesium and oxygen are lost in the reaction.
Show Answers Only

\(B\)

Show Worked Solution

Option \(B\) is correct.

  • The system is sealed, so no matter enters or leaves – the magnesium and oxygen simply rearrange into magnesium oxide inside the jar.
  • Energy is released from the system and according to Einstein’s mass-energy equivalence \((E = mc^2)\), this lost energy corresponds to a decrease in mass.

Other options:

  • \(A\) is incorrect. No oxygen is added – it was already in the sealed jar.
  • \(C\) is incorrect. Energy is released (removed), not added to the system.
  • \(D\) is incorrect. No magnesium or oxygen is lost – they’re converted to magnesium oxide within the sealed system.

\(\Rightarrow B\)

Filed Under: Light and Special Relativity Tagged With: Band 5, smc-3699-80-E = mc^2

PHYSICS, M8 EQ-Bank 22

Einstein's equation `E = mc^(2)`  is one of the most important equations in the history of physics.

Justify this statement.   (7 marks)

--- 14 WORK AREA LINES (style=lined) ---

Show Answers Only

Position Statement

  • Einstein’s equation `E=mc^2` is among physics’ most important equations because it reveals mass-energy equivalence and explains fundamental processes from atomic to cosmic scales.

Nuclear Applications

  • The equation explains energy from nuclear fission and fusion processes. It shows how tiny amounts of matter convert to enormous energy in nuclear reactions.
  • The mass defect in atoms directly relates to binding energy through `E=mc^2` and this principle drives nuclear reactors that power cities and nuclear weapons.
  • These applications are responsible for revolutionising both energy production and global politics.

Cosmic and Particle Physics

  • Stars produce energy by converting mass to energy through fusion reactions. The Sun converts 4 million tonnes of mass to energy every second using this principle
  • Particle accelerators create new particles by converting kinetic energy into mass. This allows scientists to study fundamental matter structure and discover new particles.
  • Furthermore, mass dilation near light speed also follows from this mass-energy relationship.

Reinforcement

  • While other equations like Newton’s gravity law are important, they lack the broad applicability of `E=mc^2`.
  • No other single equation explains phenomena from subatomic particles to stellar processes.
  • The equation unified our understanding of matter and energy as different forms of the same thing.
  • This justifies calling `E=mc^2` one of history’s most important physics equations.
Show Worked Solution

Position Statement

  • Einstein’s equation `E=mc^2` is among physics’ most important equations because it reveals mass-energy equivalence and explains fundamental processes from atomic to cosmic scales.

Nuclear Applications

  • The equation explains energy from nuclear fission and fusion processes. It shows how tiny amounts of matter convert to enormous energy in nuclear reactions.
  • The mass defect in atoms directly relates to binding energy through `E=mc^2` and this principle drives nuclear reactors that power cities and nuclear weapons.
  • These applications are responsible for revolutionising both energy production and global politics.

Cosmic and Particle Physics

  • Stars produce energy by converting mass to energy through fusion reactions. The Sun converts 4 million tonnes of mass to energy every second using this principle
  • Particle accelerators create new particles by converting kinetic energy into mass. This allows scientists to study fundamental matter structure and discover new particles.
  • Furthermore, mass dilation near light speed also follows from this mass-energy relationship.

Reinforcement

  • While other equations like Newton’s gravity law are important, they lack the broad applicability of `E=mc^2`.
  • No other single equation explains phenomena from subatomic particles to stellar processes.
  • The equation unified our understanding of matter and energy as different forms of the same thing.
  • This justifies calling `E=mc^2` one of history’s most important physics equations.

Filed Under: Light and Special Relativity, Origins of Elements, Properties of the Nucleus Tagged With: Band 3, Band 4, Band 5, smc-3699-80-E = mc^2, smc-3700-60-Mass-Energy Equivalence, smc-3703-20-Conservation of Mass-Energy

PHYSICS, M7 2021 HSC 16 MC

The Sun has an energy output of `3.85 × 10^{28}\ `W.

By how much does the Sun's mass decrease each minute?

  1. `4.28 × 10^{11}` kg
  2. `2.57 × 10^{13}` kg
  3. `1.28 × 10^{20}` kg
  4. `7.70 × 10^{21}` kg
Show Answers Only

`B`

Show Worked Solution

Energy released = `3.85 xx 10^(28) xx 60 = 2.31 xx 10^(30)\` J/min

`E` `=mc^2`  
`m` `=(E)/(c^(2))=(2.31 xx10^(30))/((3xx10^(8))^(2))=2.57 xx10^(13)\ \text{kg}`  

 
`=>B`


♦ Mean mark 45%.

Filed Under: Light and Special Relativity Tagged With: Band 5, smc-3699-80-E = mc^2

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