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Tamil Nadu Board of Secondary EducationSSLC (English Medium) Class 6

Temperature and Heat

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Topics

Estimated time: 22 minutes
  • Introduction
  • Definition: Heat
  • Definition: Temperature
  • Formula: Average Kinetic Energy and Temperature
  • Formula: Heat Exchange
  • Characteristics
  • How Heat Affects Matter
  • Significance
  • Real-Life Examples
  • Summary
Maharashtra State Board: Class 11

Introduction

Temperature and heat are fundamental concepts in thermodynamics and physical science. When two bodies at different temperatures come in contact, energy is transferred between them as heat until they reach the same temperature — a state called thermal equilibrium. This topic helps us understand how energy moves between systems and how matter behaves when heated across its solid, liquid, and gas states.

Maharashtra State Board: Class 11

Definition: Heat

"Heat is energy in transit. When two bodies at different temperatures are brought in contact, they exchange heat."

Maharashtra State Board: Class 11

Definition: Temperature

"Temperature is a physical quantity that defines the thermodynamic state of a system."

Maharashtra State Board: Class 11

Formula: Average Kinetic Energy and Temperature

\[E_k=\frac{3}{2}k_BT\]

Where:

  • Ek = Average kinetic energy of the molecules (in joules)
  • kB = Boltzmann constant = 1.380649 × 10−23 J/K
  • T = Absolute temperature (in kelvin)
Maharashtra State Board: Class 11

Formula: Heat Exchange

Q = mcΔT

Where:

  • Q = Heat absorbed or released (in joules)
  • m = Mass of the substance (in kg)
  • c = Specific heat capacity (J/kg·K)
  • ΔT = Change in temperature (Tfinal−Tinitial)
Maharashtra State Board: Class 11

Characteristics

Property Heat Temperature
Nature A form of energy (energy in transit) A measure of the degree of hotness or coldness
SI Unit Joule (J) Kelvin (K) or Celsius (°C)
CGS Unit Erg
Other Unit Calorie (cal)
Symbol Q T
Depends on Temperature difference between systems Average kinetic energy of particles
Dimension [M1L2T−2] [M0L0T0K1]
Flow direction Always from hot body to cold body Does not flow

States of Matter — Key Characteristics

Property Solid Liquid Gas
Shape Definite Not definite (takes container shape) Not definite
Volume Definite Definite Not definite
Particle motion Vibrate about fixed positions Move within constraints Move freely
Interatomic spacing ~10−10 m ~Twice that of solids ~10−9 m (at NTP)
Intermolecular forces Strong Weaker than solids Negligible (ideal gas)
Maharashtra State Board: Class 12

How Heat Affects Matter

When a body is at a different temperature from its surroundings, heat transfer takes place until both reach the same temperature (thermal equilibrium). The source explains this process through the behaviour of particles in each state of matter:

In Solids:

  • Particles vibrate about fixed equilibrium positions and possess kinetic energy.
  • When heated, particles vibrate with higher energy → temperature increases.
  • The energy supplied becomes internal energy (increased kinetic energy of atoms/molecules).
  • Near the melting point, heat weakens bonds between particles instead of raising the temperature.

In Liquids:

  • Bonds are weaker; particles can move but remain close together.
  • Mean distance between particles is roughly the same as in solids.
  • Liquids have definite volume but no definite shape.
  • On further heating, kinetic energy increases → temperature rises.

In Gases:

  • At the boiling point, particles overcome intermolecular forces and move freely.
  • For an ideal gas, there are no forces between molecules (kinetic theory of gases).
  • Gases have neither definite volume nor shape.

Maharashtra State Board: Class 11

Significance

  • Heat transfer governs everyday phenomena — from warming of cold water to cooling of hot tea.
  • The concept of thermal equilibrium is the basis of the Zeroth Law of Thermodynamics.
  • Understanding temperature in terms of average kinetic energy connects microscopic particle behaviour to macroscopic properties like temperature.
  • Knowledge of unit conversions (Joule, Calorie, Erg) is essential for solving numerical problems in thermodynamics.
  • Dimensional analysis of heat and temperature helps verify equations and solve advanced physics problems.
Maharashtra State Board: Class 12

Real-Life Examples

  • Ice-cold water warming up on a table: The water absorbs heat from the warmer surroundings until it reaches room temperature (thermal equilibrium).
  • Hot tea cooling down: The hot tea loses heat to the cooler air around it until both reach the same temperature.
  • A metal spoon in hot coffee: The spoon heats up because heat transfers from the hot coffee to the cooler spoon through molecular collisions.
  • A warm car on a cold day: Heat from inside the car gradually transfers to the cold outside air until equilibrium is reached.
  • Clinical thermometer: Works on the principle that the mercury inside reaches thermal equilibrium with the body, giving an accurate temperature reading.
Maharashtra State Board: Class 11

Summary

  • Heat is energy in transit — it transfers between bodies due to a temperature difference.
  • Temperature is a physical quantity that defines the thermodynamic state and measures the average kinetic energy of particles.
  • When two bodies at different temperatures come in contact, heat flows from the hotter to the cooler body until thermal equilibrium is reached.
  • In solids, heating increases particle vibration (kinetic energy); near the melting point, heat weakens bonds without raising the temperature.
  • Liquids have weaker bonds than solids but stronger than gases; they have definite volume but no definite shape.
  • In gases (ideal), there are no intermolecular forces; particles move freely with no definite shape or volume.
  • Interatomic spacing: solids ~10−10 m, gases at NTP ~10−9 m.
  • SI unit of heat: Joule (J); CGS unit: Erg; 1 J = 107 erg.
  • 1 calorie = 4.184 J.
  • Dimensional formula: Heat = [M1L2T−2]; Temperature = [M0L0T0K1].
  • Average kinetic energy formula: Ek = \[\frac {3}{2}\]kBT, linking microscopic particle energy to macroscopic temperature.
 

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