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Physics · Class 11

Thermal Properties of Matter

10 free physics experiments and lesson notes for Thermal Properties of Matter, with model limits, worked examples and Tamil explanations.

Bring two blocks into contact

Temperature describes thermal state; heat is energy transferred because temperatures differ. The isolated blocks approach a common temperature determined by their heat capacities. Equal masses do not guarantee a simple average unless their specific heats are also equal.

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Heat a solid, liquid and ideal gas

Heating expands most materials, but coefficients and constraints matter. A solid’s volume coefficient is roughly three times its linear coefficient; a liquid has its own volume coefficient. A constant-pressure ideal gas volume follows absolute temperature.

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Mix hot and cold materials

A calorimeter balances heat lost against heat gained. A larger hot heat capacity pulls the final temperature toward the hot initial value. Specific heat has units J/(kg·K), while total heat capacity is mc.

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Heat ice through state changes

During melting or boiling, heat changes the state while temperature stays constant. Between state changes, heat increases temperature according to the relevant specific heat. The horizontal plateaus represent energy, not a failed heater.

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Shift a blackbody spectrum

Hotter bodies emit much more power and peak at shorter wavelengths. Stefan law controls total power through T⁴; Wien law locates the spectral peak through 1/T. The curve uses Planck spectral radiance.

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Track cooling toward ambient

Newton cooling makes the rate proportional to the current temperature difference. Cooling is fastest initially and slows as the body approaches ambient. If initially colder, the same law predicts warming.

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Compare absorption and emission

A surface that absorbs strongly also emits strongly under matching conditions. In an enclosure of the same temperature, absorbed and emitted power balance for every absorptivity. Unequal temperatures produce a net exchange.

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