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

THERMOCHEMISTRY

Chemical energy is a form of potential energy stored in chemical bonds. Molecules store energy in the arrangement and strength of bonds; breaking bonds requires energy, forming bonds releases energy. Energy changes during a chemical reaction determine whether heat is absorbed or released.

Thermochemistry is the aspect of chemistry that deals with the energy changes that accompany physical and chemical processes.

Thermodynamics is the science of interconversion of energy.

Terminologies Used In Thermodynamics

System: A system refers to a sample specified in the universe for study or consideration. There are different types of systems:

(i) Closed system: This is a system that does not allow for the exchange of matter between the system and its surroundings, such that matter is restricted within the system. However, such a system exchanges energy with the surroundings.

(ii) Open system: This is a system that exchanges both matter and energy with its surroundings. In other words, such a system allows energy and matter to flow across its boundary.

(iii) Isolated system: This is a system that neither allows energy nor matter to transverse its boundary.

Boundary: The boundary of a system is the region that encloses the system, and separates it from its surroundings.

Surroundings: The surroundings of a system is the part of the universe beyond the boundary of a system. The surroundings interact with the system when such is desired.

Universe: A universe consists of a system and its surroundings.

Thermodynamic process: A thermodynamic process occurs when a system undergoes a change of state. The different types of processes encountered in chemical thermodynamics are:

Isothermal process: This is a process that occurs at constant temperature.

Isobaric process: This is a process that occurs at constant pressure.

Isochoric process: This is a process that occurs at constant volume.

Property: A property refers to the characteristic or feature of a system which is
observable at any instant of time. The different types of properties encountered
in thermodynamics are:
(i) Extensive property: This is a property that depenΔS on the mass of a
system. Examples include internal energy, weight, volume, and heat capacity.
(ii) Intensive property: This is a property that is independent of the mass of a
system. For example, the density and specific heat capacity of a substance are
constant, regardless of the mass under consideration.
(iii) Microscopic property: This is a property that is associated with the
individual molecules of a system, e.g., velocity of a molecule, volume of a
molecule, energy of a molecule, etc.
(iv) Macroscopic property: This is a property that is associated with the whole
system, and it can be thought of as being the sum of the contributions of all the
molecules that constitute the system. Examples include density, pressure,
viscosity, volume, etc.
(v) State property: This is a property that is independent of the history of the system. In other worΔS, it is a property that does not depend on how a substance was prepared. Examples include internal energy, temperature, density, volume, etc.

State: The state of a system is a collection of macroscopic properties which partially or fully describe its characteristics at any specific time. When there is a change in any of such properties, then the system is said to undergo a change of
state.