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Thermal Properties of Matter — Class 11 MCQs with Answers

Class 11 CBSE Physics · Chapter 10

66 practice questions · 22 Easy · 22 Medium · 22 Hard · Updated

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Practise the most important Class 11 CBSE Physics questions from Chapter 10, "Thermal Properties of Matter". You get 6 timed quizzes made from 66 NCERT-based MCQs, with answers and explanations. The questions are split into 22 Easy, 22 Medium and 22 Hard. Warm up on the basics, then move on to the exam-level questions that top scorers in CBSE & Maharashtra HSC Board exams, JEE Main, MHT-CET, JEE Advanced and NEET UG get right.

To score well in "Thermal Properties of Matter", focus on numericals, derivations and applying concepts. Each MCQ here is timed and uses exam-style marking (+4 correct, −1 wrong, 0 skipped). This helps you stay accurate when time is short, just as real papers need. Every question has a short explanation, so a wrong answer becomes a quick lesson. It is the fastest way to fix gaps before a test.

Use this chapter for focused revision. Start with the Easy set to check your basics on Thermal Properties of Matter, then move to Medium and Hard to practise applying them. Your accuracy, streaks and XP save automatically. This chapter also adds to your overall Class 11 Physics mastery score. Try the 6 sample questions below: tap an option to see the answer and a worked explanation. Sign in free to start practising.

Thermal Properties of Matter — important questions & MCQs with answers (Class 11 Physics)

6 solved questions from this chapter's difficulty levels, each with its answer and explanation. Tap an option to check yourself.

0 of 6 answered

  1. Q1 of 6Easy

    0°C in Kelvin:

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    Answer: 273.15 K

    Explanation: Kelvin scale: K = °C + 273.15, so 0°C = 273.15 K exactly. 0 K is absolute zero (−273.15°C), the tempting wrong pick since it swaps the roles of 0°C and 0 K.

  2. Q2 of 6Easy

    Heat transfer through vacuum is by:

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    Answer: Radiation

    Explanation: Conduction needs a solid medium and convection needs a fluid to carry matter, but radiation is electromagnetic waves needing no medium — the only mode that crosses vacuum, like sunlight reaching Earth.

  3. Q3 of 6Medium

    30°C = ? K

    Show answer

    Answer: 303.15

    Explanation: K = °C + 273.15, so 30°C = 30 + 273.15 = 303.15 K. Subtracting 30 from 273.15 instead of adding gives the wrong 243.15 K.

  4. Q4 of 6Medium

    Rod of length 1 m, α = 1.2 × 10⁻⁵ /°C. Expansion when heated 100°C:

    Show answer

    Answer: 1.2 mm

    Explanation: Linear expansion: ΔL = αL₀ΔT = 1.2×10⁻⁵ × 1 × 100 = 1.2×10⁻³ m = 1.2 mm. Misplacing the decimal gives the tempting 1.2 cm or 0.12 mm — a factor-of-10 slip is the trap here.

  5. Q5 of 6Hard

    Heat to melt 1 kg ice at 0°C, heat the water to 100°C and vaporize it (L_f = 80 cal/g, c_water = 1 cal/g°C, L_v = 540 cal/g):

    Show answer

    Answer: 720,000 cal

    Explanation: Total heat sums three stages for 1 kg: melting (80×1000 cal), warming water 0→100°C (100×1000 cal, since c_water=1 cal/g°C), and vaporizing (540×1000 cal), giving 720,000 cal total.

  6. Q6 of 6Hard

    Mixing 100 g ice at 0°C with 200 g water at 50°C. Final state (L_f = 80 cal/g, c_w = 1):

    Show answer

    Answer: All water at ≈6.7°C

    Explanation: The 200 g of water cooling 50°C releases 200×1×50 = 10000 cal, while melting all 100 g of ice needs only 100×80 = 8000 cal. So every gram melts and the surplus 2000 cal warms the 300 g of water by 2000/300 ≈ 6.7°C. Ignoring the latent heat entirely gives the tempting 33°C.

Thermal Properties of Matter notes: key concepts (Class 11 Physics)

Heat as energy in transit and its effects: temperature scales, linear, areal and volumetric expansion, specific and latent heat, the calorimetry principle for mixtures, and the three modes of heat transfer with the laws that govern conduction, Stefan-Boltzmann radiation and Newton's cooling.

Heat and temperature
Temperature measures the average kinetic energy of molecules and decides the direction of heat flow; heat is the energy actually in transit because of a temperature difference.
Temperature scales
Celsius, Fahrenheit and the absolute Kelvin scale. A change of one kelvin equals a change of one degree Celsius, so the two agree on differences but not on values.
Absolute zero
0 K, the temperature at which molecular motion is minimum. It is the natural zero of the Kelvin scale and cannot be reached in practice.
Linear expansion
A solid rod lengthens in proportion to its original length and the temperature rise, the constant being the coefficient of linear expansion α.
A solid rod of length L at temperature T (top). After its temperature rises by ΔT (bottom) the same rod, held at its left end, has lengthened to L + ΔL; the extra length ΔL is shown exaggerated. The increase is proportional to the original length and to the temperature rise, ΔL = αLΔT, where α is the coefficient of linear expansion.
Areal and volume expansion
For an isotropic solid the areal coefficient is about 2α and the volumetric coefficient about 3α, since expansion happens along every dimension at once.
Anomalous expansion of water
Between 0 °C and 4 °C water CONTRACTS on heating, reaching maximum density at 4 °C. This is why lakes freeze from the top and aquatic life survives beneath.
A sketch of the volume of a fixed mass of water against its temperature from 0 °C to 10 °C. From 0 °C the volume falls as the water is heated, reaching a minimum at 4 °C, and then rises again above 4 °C. Minimum volume at 4 °C means maximum density there. The change is exaggerated for clarity.
Specific heat capacity
The heat needed to raise unit mass through one degree. Water's unusually high value of 4186 J kg⁻¹ K⁻¹ makes it an excellent coolant.
Thermal capacity
The heat needed to raise the temperature of a whole body by one degree, equal to mass times specific heat. It is a property of the object, not the material.
Latent heat
The heat absorbed or released during a change of state at CONSTANT temperature, going entirely into breaking or forming molecular bonds.
The heating curve of water, not to scale: temperature against heat supplied at a steady rate, starting with ice below 0 °C. The temperature of the ice rises until 0 °C, then stays constant while the ice melts (latent heat of fusion). The water then warms steadily to 100 °C, where the temperature again stays constant while it boils (latent heat of vaporisation, a longer flat stretch). Only after all the water has become steam does the temperature rise again.
Latent heat of fusion and vaporisation
For water, 334 J g⁻¹ to melt ice and 2260 J g⁻¹ to boil water. The vaporisation value is far larger, which is why steam burns are so severe.
Calorimetry principle
In an isolated system the heat lost by hot bodies equals the heat gained by cold ones. Every mixture problem is this single equation.
Conduction
Heat transfer by molecular vibration and free electrons without bulk movement of matter — the dominant mode in solids, especially metals.
Thermal conductivity
The material constant in the conduction law. Metals have high values, while air, wool and cork are poor conductors and therefore good insulators.
A uniform bar of length L and cross-sectional area A connects a hot reservoir at temperature T₁ to a cold reservoir at a lower temperature T₂. In the steady state heat flows along the bar from the hot end to the cold end at a rate H, the heat current, given by H = KA(T₁ − T₂)/L, where K is the thermal conductivity of the material.
Convection
Heat transfer by the actual movement of a heated fluid, which becomes less dense and rises. It explains sea breezes, land breezes and boiling.
Radiation
Heat transfer by electromagnetic waves, needing NO medium at all — the only mode by which the Sun's energy reaches the Earth across empty space.
Newton's law of cooling
For a small temperature excess, the rate of cooling is proportional to the difference between the body's temperature and its surroundings.
A cooling curve: the temperature T of a hot body against time t. The temperature falls quickly at first, while the body is much hotter than its surroundings, and more and more slowly as it approaches the surroundings' temperature T₀ (dashed line), because the rate of cooling is proportional to the temperature difference T − T₀.
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Thermal Properties of Matter — FAQs

What are the key concepts in Class 11 Physics Thermal Properties of Matter?+

Heat as energy in transit and its effects: temperature scales, linear, areal and volumetric expansion, specific and latent heat, the calorimetry principle for mixtures, and the three modes of heat transfer with the laws that govern conduction, Stefan-Boltzmann radiation and Newton's cooling. Key ideas include Heat and temperature, Temperature scales, Absolute zero, Linear expansion, Areal and volume expansion, Anomalous expansion of water.

What does Class 11 Physics Chapter 10 (Thermal Properties of Matter) cover on XamBaaz?+

It has 66 NCERT-based MCQs on "Thermal Properties of Matter": 22 Easy, 22 Medium and 22 Hard. Together they make 6 timed quizzes, and you never get the same set twice. Every question has an instant explanation. They help you prepare for CBSE & Maharashtra HSC Board exams, JEE Main, MHT-CET, JEE Advanced and NEET UG.

Are these "Thermal Properties of Matter" questions free to practise?+

Yes. Sign in with Google to practise "Thermal Properties of Matter" free. Full unlimited access is ₹1,999/year. One year from the day you pay. You stay in Class 11 till 31 March; on 1 April your account moves up to Class 12 and the rest of your year carries over. No chapter is charged separately.

How should I revise "Thermal Properties of Matter" for the exam?+

Start with the Easy quiz to check your basics, then try Medium and Hard to practise applying them. There are 6 timed quizzes on this chapter, so you can come back for a fresh set instead of one you have seen. Read each explanation, retry the questions you miss, and track your accuracy until it stays high.

Are these "Thermal Properties of Matter" MCQs available with answers?+

Yes. 6 sample questions are on this page with answers: tap an option, or "Show answer", to see the correct option and a step-by-step explanation. Sign in free with Google to start practising, with instant scoring.

Is there negative marking in the "Thermal Properties of Matter" quizzes?+

Yes. The timed quizzes use exam-style marking: +4 for a right answer, −1 for a wrong one and 0 for a skip, the same negative marking as JEE Main, JEE Advanced and NEET UG. MHT-CET and CBSE board papers have no negative marking. Our mocks for those are scored their way.

What are the important questions from Thermal Properties of Matter (Class 11 Physics)?+

The questions that matter most test Heat and temperature, Temperature scales, Absolute zero, Linear expansion, Areal and volume expansion, Anomalous expansion of water. This page shows 6 solved important MCQs with answers and explanations. Sign in to practise all 66 questions on the chapter as timed quizzes.

Is there an online quiz for Thermal Properties of Matter?+

Yes — Class 11 Physics Thermal Properties of Matter has timed online quizzes at Easy, Medium and Hard levels, with instant scoring and a worked explanation on every question. The first quiz on the chapter is free.

Are there question answers and extra questions for Thermal Properties of Matter (Class 11 Physics)?+

Yes. This page has 6 solved questions on Thermal Properties of Matter, each with the correct answer and a short explanation. Sign in to practise all 66 questions on the chapter as timed quizzes.

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