In simple terms
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Thermal equilibrium
Cambridge 9702 Paper 4 — Thermal equilibrium (14.1). Senpai Corner diagram-backed pilot with premium structure and live visuals.
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Thermal Equilibrium: A state where there is no net flow of thermal energy between objects in thermal contact. They are at the same temperature.
- 2
Temperature vs. Heat: Temperature is a measure of the average kinetic energy of particles in a substance. Heat (or thermal energy) is the energy transferred from a hotter region to a colder region.
- 3
Zeroth Law: If A is in equilibrium with C, and B is in equilibrium with C, then A is in equilibrium with B. This is the basis for using thermometers.
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Internal Energy: The sum of the random kinetic and potential energies of the particles in a system.
What this topic covers
The official Cambridge syllabus points this lesson works through.
- 14.1.1
Understand that (thermal) energy is transferred from a region of higher temperature to a region of lower temperature
- 14.1.2
Understand that regions of equal temperature are in thermal equilibrium
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Key formulas
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Full topic notes
Formal explanation with the rigour you need for the exam.
Understanding Thermal Equilibrium
Thermal equilibrium occurs when two or more objects in thermal contact reach the same temperature. At this point, there's no longer a net flow of thermal energy from one object to another. Energy might still be exchanged at a microscopic level, but on average, the rate of energy flowing in one direction equals the rate flowing in the opposite direction. This stable state means all parts of the system are at a uniform temperature.
The Zeroth Law of Thermodynamics
This law might sound trivial, but it forms the foundation for temperature measurement. It states: If object A and object B are both in thermal equilibrium with a third object C, then objects A and B are also in thermal equilibrium with each other. Think of object C as a thermometer – if two objects give the same reading on a thermometer, they must be at the same temperature.
Thermal Equilibrium: A state where there is no net flow of thermal energy between objects in thermal contact. They are at the same temperature.
Temperature vs. Heat: Temperature is a measure of the average kinetic energy of particles in a substance. Heat (or thermal energy) is the energy transferred from a hotter region to a colder region.
Zeroth Law: If A is in equilibrium with C, and B is in equilibrium with C, then A is in equilibrium with B. This is the basis for using thermometers.
Internal Energy: The sum of the random kinetic and potential energies of the particles in a system.
Temperature: The Measure of Hotness
Temperature is a fundamental physical quantity that gives us a quantitative measure of how 'hot' or 'cold' something is. At a microscopic level, it's directly related to the average random kinetic energy of the particles (atoms or molecules) within a substance. The faster these particles vibrate or move, the higher the temperature.
The Kelvin Scale and Absolute Zero
While Celsius (°C) is common, the Kelvin (K) scale is the SI unit for absolute temperature and is used in almost all physics formulas. It's an absolute scale, meaning 0 K represents the lowest possible temperature, known as absolute zero. At absolute zero (-273.15 °C), particles possess the minimum possible kinetic energy. A change of 1 Kelvin is exactly equivalent to a change of 1 degree Celsius.
To convert Celsius to Kelvin: K = C + 273.15
Internal Energy: The Total Energy Within
The internal energy of a system is the total sum of the random kinetic and potential energies of all its particles. The kinetic energy component is due to the random motion of particles (translation, rotation, vibration) and is directly linked to temperature. The potential energy component arises from the intermolecular forces between particles. When a substance changes state, its potential energy changes significantly, even if its temperature (and thus average kinetic energy) remains constant.
Specific Heat Capacity (c)
When you add thermal energy to a substance, its temperature usually rises. Specific heat capacity (c) quantifies how much energy is needed to change the temperature of a unit mass of a substance by 1 Kelvin (or 1 °C) without a change of state. Substances with high specific heat capacity (like water) require a lot of energy to heat up, making them excellent coolants.
Energy transferred during temperature change: . Units for c: J kg⁻¹ K⁻¹
Q = energy transferred (J)
m = mass of the substance (kg)
c = specific heat capacity (J kg⁻¹ K⁻¹)
ΔT = change in temperature (K or °C)
Specific Latent Heat (L)
Sometimes, adding energy to a substance doesn't increase its temperature, but instead changes its state (e.g., melting ice into water or boiling water into steam). This energy is called latent heat. Specific latent heat (L) is the energy required to change the state of 1 kg of a substance without changing its temperature. The energy supplied goes into altering the potential energy of the particles by breaking or forming intermolecular bonds.
There are two main types:
Energy transferred during state change: Q = mL \ Units for L: J kg⁻¹
Evaporation is a fascinating example of a cooling process related to latent heat. When a liquid evaporates, higher-energy particles escape from the liquid surface. This reduces the average kinetic energy of the remaining particles in the liquid, leading to a decrease in the liquid's overall temperature.
Specific latent heat of fusion (L_f): For changes between solid and liquid (melting/freezing).
Specific latent heat of vaporisation (L_v): For changes between liquid and gas (boiling/condensation).
L_v is typically much larger than L_f because more energy is needed to completely separate particles into a gas.
Experimental Determination of 'c' and 'L'
The specific heat capacity and specific latent heat of substances can be determined experimentally, most commonly using an electrical method. For specific heat capacity, a known mass (m) of the substance is heated by an electrical heater of known power (P) for a measured time (t). The initial and final temperatures are recorded to find the change (ΔT). The energy supplied is E = Pt. By equating E = mcΔT, 'c' can be calculated. For specific latent heat, a similar setup is used, but the substance is held at its melting or boiling point. The energy (E = Pt) required to change the state of a measured mass (m) is recorded, and L is found using E = mL.
Sources of Error and Mitigation
The primary source of error in these experiments is heat loss to the surroundings. This makes the calculated values of 'c' and 'L' higher than the true values, as not all the supplied electrical energy goes into heating the substance. To mitigate this:
- Use insulation (lagging) around the container.
- Place a lid on the container to reduce heat loss by convection and evaporation.
- Polish the outer surfaces to reduce heat loss by radiation.
- A more advanced technique is to start the experiment with the substance at a temperature below room temperature and end it at an equal temperature above room temperature, allowing heat lost in the second half to be roughly balanced by heat gained in the first half.
Worked examples
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Calculate the total energy required to heat 0.50 kg of water from 20 °C to 100 °C and then completely boil it. \ (Given: Specific heat capacity of water = 4200 J kg⁻¹ K⁻¹, Specific latent heat of vaporisation of water = 2.26 × 10⁶ J kg⁻¹).
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- Energy to heat the water (Q₁): \ We use Q = mcΔT. \ Mass (m) = 0.50 kg \ Specific heat capacity (c) = 4200 J kg⁻¹ K⁻¹ \ Temperature change (ΔT) = 100 °C - 20 °C = 80 K (Note: A change of 80 °C is the same as 80 K). \ Q₁ = 0.50 kg × 4200 J kg⁻¹ K⁻¹ × 80 K = 168,000 J \ \ 2. Energy to boil the water (Q₂): \ We use Q = mL. \ Mass (m) = 0.50 kg \ Specific latent heat of vaporisation (Lᵥ) = 2.26 × 10⁶ J kg⁻¹ \ Q₂ = 0.50 kg × 2.26 × 10⁶ J kg⁻¹ = 1,130,000 J \ \ 3. Total energy (Q_total): \ Q_total = Q₁ + Q₂ \ Q_total = 168,000 J + 1,130,000 J = 1,298,000 J \ Therefore, the total energy required is approximately 1.30 × 10⁶ J (to 3 significant figures).
A 0.20 kg block of copper at 95.0 °C is placed into 0.50 kg of water in a well-insulated container. The initial temperature of the water is 25.0 °C. Calculate the final temperature of the copper and water once thermal equilibrium is reached. (Specific heat capacity of copper = 385 J kg⁻¹ K⁻¹, Specific heat capacity of water = 4200 J kg⁻¹ K⁻¹).
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- Principle: Assuming the container is perfectly insulated, the heat energy lost by the hot copper block will be equal to the heat energy gained by the colder water. This is the principle of conservation of energy. \ \ \ 2. Formula: Let the final equilibrium temperature be . \ \ \ 3. Substitution: \ \ Note: We can use °C here because we are dealing with temperature differences, and a change of 1°C is equal to a change of 1K. \ \ 4. Calculation: \ \ \ \ \ \ \ \ 5. Final Answer: The final equilibrium temperature is 27.5 °C (to 3 significant figures).
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Glossary
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What defines thermal equilibrium between two objects?
No net transfer of thermal energy between them, resulting in a uniform temperature.
Key takeaways
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- ✓
Thermal Equilibrium: A state where there is no net flow of thermal energy between objects in thermal contact. They are at the same temperature.
- ✓
Temperature vs. Heat: Temperature is a measure of the average kinetic energy of particles in a substance. Heat (or thermal energy) is the energy transferred from a hotter region to a colder region.
- ✓
Zeroth Law: If A is in equilibrium with C, and B is in equilibrium with C, then A is in equilibrium with B. This is the basis for using thermometers.
- ✓
Internal Energy: The sum of the random kinetic and potential energies of the particles in a system.
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