Course Content
Module 1: Fundamental Concepts of Energy
Welcome to the world of chemical energy! Before we can understand how reactions absorb or release heat, we need to establish a common language. In this foundational module, you will be introduced to the key players: the system (the reaction we care about) and the surroundings (everything else). You will learn the critical difference between heat and temperature and be introduced to Enthalpy (H) , the measure of total heat content in a system. By the end of this module, you will understand that in chemistry, we never measure absolute heat—only changes in heat (ΔH) . This concept is the gateway to everything that follows in the course.
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Exothermic and Endothermic Reactions
Have you ever touched a beaker after a reaction and felt it burn your hand, or noticed it turn icy cold? That is thermochemistry in action! This module dives into the two major classes of energy change. You will learn to identify exothermic reactions (ΔH negative) that release heat, like combustion and neutralization, and endothermic reactions (ΔH positive) that absorb heat, like photosynthesis. More importantly, you will learn to draw and interpret energy profile diagrams—a favorite WAEC and JAMB question. These diagrams visually show the energy "hill" that reactions must climb, introducing the concept of Activation Energy (Ea) .
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Enthalpy Changes of Physical Changes and Chemical Reactions
This is where we get precise. WAEC and JAMB love to test specific definitions. In this module, you will learn the exact language required to score full marks. We will dissect the Standard Enthalpy of Formation (ΔH_f°) —the most important reference point for all energy calculations—and discover why the value for every element in its standard state is zero. You will also master the Enthalpy of Combustion (ΔH_c°) and the constant value associated with the Enthalpy of Neutralization (ΔH_neut) for strong acids and bases. Memorizing these definitions is essential, but understanding them is even more critical.
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Hess’s Law (The Law of Constant Heat Summation)
What if a reaction is too slow, too dangerous, or too difficult to measure in a lab? How do we find its enthalpy change? Enter Hess's Law, one of the most elegant and powerful tools in chemistry. This module teaches you that enthalpy is a "state function"—meaning the path taken from reactants to products doesn't matter; only the start and end points count. You will learn two methods to apply Hess's Law: the algebraic method (manipulating equations) and the energy cycle method (using formation or combustion data). While this is often considered the most challenging topic in thermochemistry, mastering it guarantees you can solve virtually any enthalpy problem thrown at you.
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Bond Enthalpies
Chemical reactions involve breaking old bonds and forming new ones. This module looks at energy from the perspective of these bonds. You will learn about mean bond enthalpy—the average energy required to break a specific type of bond. This allows us to estimate the enthalpy change of a reaction using a simple concept: energy must be supplied to break bonds (endothermic), and energy is released when bonds form (exothermic). The formula ΔH = Σ(Bonds Broken) – Σ(Bonds Formed) will become your new best friend. While this method provides an estimate rather than an exact value, it is a quick and useful tool, especially for gaseous reactions. Module 8: Exam-Focused Revision and Problem Solving
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Thermochemistry I

Heat and Temperature

In everyday language, we often use ‘heat’ and ‘temperature’ interchangeably. In chemistry, they have very specific and different meanings. Understanding this distinction is critical.

Temperature (T) is a measure of the average kinetic energy of the particles (atoms or molecules) in a substance. It tells you how “hot” or “cold” something is.

Units: Degrees Celsius (°C) or Kelvin (K). The Fahrenheit scale is rarely used in scientific contexts.

Analogy: Think of a cup of coffee and a bathtub of warm water. The coffee might have a higher temperature, but the bathtub contains much more total energy.

Heat (q) is the transfer of energy between two objects due to a temperature difference. Heat is energy in transit. An object does not “contain” heat; it contains thermal energy. That thermal energy becomes “heat” only when it is transferred.

Units: Joules (J) or kilojoules (kJ). (1 kJ = 1000 J)

Analogy: In our coffee and bathtub example, if you place an ice cube in the coffee, a lot of heat will transfer quickly because the temperature difference is large. If you place the same ice cube in the warm bath, heat will transfer more slowly. The heat transfer is the process, the temperature is what drives it.

Converting Celsius to Kelvin
When working with gases and many thermodynamic equations, you must use the absolute temperature scale, Kelvin (K). There are no negative temperatures in Kelvin. Converting is easy:

K = °C + 273

Example: Room temperature (25°C) is equal to 25 + 273 = 298 K.

Remember: A change of 1°C is exactly equal to a change of 1 K. So, if a temperature increases by 10°C, it also increases by 10 K.