Energy: The capacity to do work; it exists in various forms and can be converted from one form to another.
Radiant Energy: This energy originates from the sun and is the primary energy source for Earth, essential for processes such as photosynthesis in plants.
Thermal Energy: Linked to the random motion of atoms and molecules, it plays a crucial role in determining the temperature of a substance.
Chemical Energy: Stored within the bonds of chemical substances; this energy is released or absorbed during chemical reactions, making it a key factor in thermochemistry.
Nuclear Energy: Found in the collection of neutrons and protons in an atom, nuclear energy is released during nuclear reactions such as fission or fusion.
Potential Energy: This type of energy is available based on an object's position within a gravitational field or its configuration within a system.
Heat: Defined as the transfer of thermal energy between two bodies at different temperatures, heat flow is critical for understanding thermal processes in both chemical reactions and physical changes.
Temperature: A measure of the average thermal energy of the particles in a substance, temperature is a key determinant of the direction of heat transfer.
Thermochemistry: The branch of chemistry that deals with the study of heat changes that occur during chemical reactions and phase changes.
System: Refers to the specific area of study within the universe, allowing us to focus on particular interactions and energy changes.
Types of Systems:
Open System: Allows for the exchange of both mass and energy with its surroundings.
Closed System: Energy can be exchanged, but mass remains constant within the system.
Isolated System: Neither mass nor energy can be exchanged with the surroundings, idealized to simplify calculations.
Surroundings: Consists of everything outside the defined system that can interact with it in terms of heat and work.
Exothermic Process: A reaction that releases heat to the surroundings, effectively transferring thermal energy from the system. Example Reaction: 2H₂ (g) + O₂ (g) → 2H₂O (l) + energy. This process results in an increase in temperature of the surroundings.
Endothermic Process: A reaction that absorbs heat from the surroundings into the system. Example Reaction: H₂O (g) → H₂O (l) + energy. This process typically results in a decrease in the temperature of the surroundings.
First Law of Thermodynamics: States that energy can change forms but is conserved; it cannot be created or destroyed. Mathematically represented as DE_system + DE_surroundings = 0, indicating the total energy change in a system is equal and opposite to the energy change in its surroundings.
Change in Internal Energy (DE): DE is calculated from the contributions of heat exchange (q) and work (w) done on or by the system. Formula: DE = q + w.
Work (w): Calculated from pressure (P) and volume change (DV). Common formulas include w = -PDV, showing work done on/by the system depending on whether the volume increases or decreases.
Example Calculation of Work Done:
(a) Expansion against vacuum:
DV = 3.8 L, P = 0 atm → w = 0 joules
(b) Expansion against constant pressure:
DV = 3.8 L, P = 3.7 atm
w = -14.1 L·atm; converting to joules:
w = -14.1 L·atm x 101.3 J/L·atm = -1430 J
Enthalpy (H): A measure of heat flow at constant pressure, with significant implications in the study of thermochemistry, as it helps quantify the energy changes during a chemical reaction.
Relation: The change in enthalpy (ΔH) can be calculated from the equation ΔH = ΔE + PΔV, where P represents pressure, and ΔV represents the change in volume.
Endothermic Reaction Example: H₂O(s) → H₂O(l), ΔH = +6.01 kJ/mol, indicating the energy needed to convert ice to water.
Exothermic Reaction Example: CH₄(g) + 2O₂(g) → CO₂(g) + 2H₂O(l), ΔH = -890.4 kJ/mol, showcasing energy released during combustion.
Stoichiometric coefficients represent moles of reactants and products and must be considered when calculating enthalpy changes.
Reversing a reaction changes the sign of ΔH, reflecting the opposite nature of energy changes when the reaction is run in reverse.
Multiplying the entire equation by a factor (n) results in ΔH changing by the same factor, facilitating scalability in calculations.
Specific Heat (s): Defines the amount of heat required to raise the temperature of 1 g of a substance by 1°C, crucial for understanding thermal properties of materials.
Heat Capacity (C): The total heat needed to raise the temperature of a given quantity (m) of material by 1°C, calculated as C = m x s.
Heat absorbed or released can be calculated using formulas: q = m x s x Δt (for the change in temperature) or q = C x Δt.
For temperature changes, Δt is defined as tfinal - tinitial, helping to ascertain changes in thermal energy of the system.
Constant-Volume Calorimetry: A method that assumes no heat is exchanged with the surroundings, allowing for precise measurements of reaction heat.
Constant-Pressure Calorimetry: Verifies that the heat absorbed by the solution equals the heat change occurring in the reaction, crucial for practical applications of thermodynamics in reactions.
Detailed calculations of heat change through specific example scenarios in calorimetry are essential for demonstrating principles of thermodynamics, heat capacities, and enthalpy changes effectively.
Molar heat of combustion calculations are performed based on specific examples to illustrate practical applications of thermochemistry.
States that the total enthalpy change for a reaction is the sum of enthalpy changes for individual steps, allowing for calculations to be simplified regardless of the reaction pathway taken.
Tables depicting standard enthalpies of formation for various compounds and elements at specified temperatures allow for reference in calculating ΔH for reactions.
Enthalpy changes are measured under standard conditions, often at 1 atm pressure and 25°C, providing context for comparing different substances and reactions.