CBSE Weightage:

Class 11 — Thermal Properties of Matter

Class 11 — Thermal Properties of Matter — chapter strategy, formulas, PYQs, and traps

5 min read

Chapter Overview & Weightage

Thermal Properties of Matter is a 4-5 mark chapter in Class 11 boards, but its concepts feed directly into Thermodynamics (next chapter) and Kinetic Theory (also Class 11). Master this and the next two chapters become much smoother.

YearMarks AskedQuestion Type
20245Numerical on heat conduction + theory
20234Calorimetry + thermal expansion
20225Stefan’s law + radiation
20213Specific heat numerical
20204Newton’s law of cooling

CBSE has been alternating between conduction problems and calorimetry numericals year after year. Expect at least one of these in the 2026 paper.

Key Concepts You Must Know

  • Temperature scales — Celsius, Fahrenheit, Kelvin conversions
  • Thermal expansion — linear (α\alpha), areal (β=2α\beta = 2\alpha), volume (γ=3α\gamma = 3\alpha)
  • Specific heatcc (for solids/liquids), CpC_p and CvC_v (for gases)
  • Latent heatLfL_f (fusion), LvL_v (vaporization)
  • Calorimetry — principle of mixtures
  • Heat transfer — conduction (Fourier), convection, radiation (Stefan’s law)
  • Newton’s law of cooling — exponential approach to ambient temperature
  • Black body radiation — Wien’s displacement, Stefan-Boltzmann

Important Formulas

L=L0(1+αΔT),V=V0(1+γΔT)L = L_0(1 + \alpha \Delta T), \quad V = V_0(1 + \gamma \Delta T)

Use when finding new dimensions after heating/cooling. For a metal rod heated from 20°C20°\text{C} to 120°C120°\text{C}, plug ΔT=100\Delta T = 100.

Q=mcΔTQ = mc \Delta T

Use when calculating heat to raise temperature of a substance without state change.

Q=mLQ = mL

Use during phase changes — temperature stays constant while QQ goes into breaking molecular bonds.

Qt=kAdTdx\frac{Q}{t} = -kA\frac{dT}{dx}

For steady-state through a slab: Qt=kA(T1T2)L\dfrac{Q}{t} = \dfrac{kA(T_1 - T_2)}{L}.

P=σϵAT4P = \sigma \epsilon A T^4

For net radiation between body at TT and surroundings at T0T_0: Pnet=σϵA(T4T04)P_{net} = \sigma \epsilon A (T^4 - T_0^4).

dTdt=k(TT0)\frac{dT}{dt} = -k(T - T_0)

Solution: TT0=(TiT0)ektT - T_0 = (T_i - T_0) e^{-kt}.

Solved Previous Year Questions

PYQ 1 (CBSE 2024)

A copper rod and an iron rod of equal length and cross-section are joined end-to-end. The free end of copper is at 100°C100°\text{C} and free end of iron at 0°C0°\text{C}. Find the temperature of the junction. (kCu=400k_{Cu} = 400, kFe=80k_{Fe} = 80 W/m K.)

Heat flow through both rods is equal in steady state: kCuA(100T)L=kFeA(T0)L\dfrac{k_{Cu} A (100 - T)}{L} = \dfrac{k_{Fe} A (T - 0)}{L}.

400(100T)=80T    40000400T=80T    T=40000/480=83.3°C400(100 - T) = 80T \implies 40000 - 400T = 80T \implies T = 40000/480 = 83.3°\text{C}.

Answer: T83.3°CT \approx \mathbf{83.3°\text{C}}.

PYQ 2 (CBSE 2023)

50 g50 \text{ g} of ice at 0°C0°\text{C} is added to 200 g200 \text{ g} water at 30°C30°\text{C}. Find final temperature. (Lf=80 cal/gL_f = 80 \text{ cal/g}, c=1 cal/g°Cc = 1 \text{ cal/g}°\text{C}.)

Heat released by water cooling to 0°C0°\text{C}: 200×1×30=6000 cal200 \times 1 \times 30 = 6000 \text{ cal}.

Heat to melt ice: 50×80=4000 cal50 \times 80 = 4000 \text{ cal}.

Excess heat after melting all ice: 60004000=2000 cal6000 - 4000 = 2000 \text{ cal}.

This warms the now-250 g250 \text{ g} water: T=2000/(250×1)=8°CT = 2000/(250 \times 1) = 8°\text{C}.

Answer: Final temperature =8°C= \mathbf{8°\text{C}}.

PYQ 3 (CBSE 2022)

A black body at T=300 KT = 300 \text{ K} radiates power P1P_1. If the temperature is doubled, find the new power P2P_2. (σ=5.67×108\sigma = 5.67 \times 10^{-8}, area 1 m21 \text{ m}^2.)

By Stefan’s law, PT4P \propto T^4. So P2/P1=(600/300)4=16P_2/P_1 = (600/300)^4 = 16.

P1=σT4=5.67×108×(300)4=459.3 WP_1 = \sigma T^4 = 5.67 \times 10^{-8} \times (300)^4 = 459.3 \text{ W}. So P2=7349 WP_2 = 7349 \text{ W}.

Answer: P2=16P1=7349 WP_2 = 16 P_1 = \mathbf{7349 \text{ W}}.

Difficulty Distribution

  • Easy (1-2 marks): Definitions, unit conversions, simple plug-ins.
  • Medium (3 marks): Calorimetry mixtures, conduction in single rods, expansion problems.
  • Hard (5 marks): Composite walls (series/parallel conduction), cooling curves, radiation in cavities, blackbody questions.

About 60% of marks come from medium and 30% from easy. Prep accordingly.

Expert Strategy

Topper’s approach: Memorize the four big formulas (heat equation, latent heat, Fourier, Stefan) cold. CBSE problems are mostly direct applications — recognize which formula applies, plug in. Don’t get distracted by Wien’s displacement or convection unless explicitly asked.

For conduction in series, treat each material like a resistor: total thermal resistance = sum of individual resistances. Rthermal=L/(kA)R_{thermal} = L/(kA). This trick handles 90% of composite-wall problems in 3 lines.

Common Traps

Trap 1: Forgetting that LfL_f is needed for 0°C0°\text{C} ice → 0°C0°\text{C} water transition. Many students just use mcΔTmc\Delta T — wrong.

Trap 2: Using α\alpha for volume expansion. Volume expansion uses γ=3α\gamma = 3\alpha, not α\alpha.

Trap 3: In Stefan’s law, students often forget the fourth power and write T2T^2 or linear. T4T^4 — engrave it.

Trap 4: Newton’s law of cooling assumes small temperature differences. For very hot bodies cooling to room temperature, use Stefan’s law.

Trap 5: Mixing units of specific heat (cal/g vs J/kg). 1 cal/g°C=4184 J/kg K1 \text{ cal/g}°\text{C} = 4184 \text{ J/kg K}. Always check.