Currently in progress
enthalpy
represented by H
the total energy of a system, some of which is stored as potential energy in chemical bonds; aka “heat content”
standard enthalpy change of reaction
represented by ∆H°
heat transferred in a reaction under standard conditions (101.3 kPa, 298 K)
exothermic reaction
a chemical reaction in which heat energy is released to the surroundings
endothermic reaction
a chemical reaction in which energy is absorbed from the surroundings
calorimetry
a technique used to measure the enthalpy associated with a particular change
heat capacity
The amount of energy that a given mass of substance (either 1 g or 1 kg) can absorb that produces a 1ºC increase in temperature
Hess’s Law
states that the enthalpy change for a reaction is the same, regardless of the reaction route. This means that the enthalpy changes of multiple reaction steps can be added in order to determine the enthalpy change for the overall reaction
average bond of enthalpy
represented by D
the amount of energy that must be supplied to break 1 mole of chemical bonds in an isolated molecule in the gaseous state
It’s also the amount of energy released when this bond forms
They are a measure of the strength of the covalent bond
They are also called bond dissociation energies
standard state
the standard thermodynamic conditions chosen for substances when listing or comparing thermodynamic data
1 atm pressure (760.0 mmHg or 101.3 kPa) and 25ºC (298 K)
standard enthalpy change of formation
represented by ΔH_f°
the enthalpy change for the formation of one mole of a substance in its standard state from its elements in their reference form and in their standard states
standard enthalpy of combustion
represented by ∆H_cΘ
the enthalpy change when 1 mole of the compound undergoes complete combustion in excess oxygen under standard conditions
It’s always exothermic
Enthalpies of formation of many oxides are equivalent to the enthalpies of combustion of the element
lattice enthalpy
the energy required to convert one mole of a substance from the solid state as a compound to the gaseous state as ions
enthalpy change of atomization
the enthalpy change to convert an element in its standard state to one mole of gaseous atoms
electron affinity
the enthalpy change for one mole of gaseous atoms to gain electrons and form a mole of anions
For most atoms this is exothermic
Gaining a 2nd electron is endothermic because of the repulsion between the electron and the negative ion
ionization energy
the enthalpy change for one mole of gaseous atoms to lose electrons and form a mole of cations
enthalpy of formation
the enthalpy change for the formation of one mole of a substance in its standard state from its elements in their reference form and in their standard states
Construct a Born-Haber cycle and use it to calculate an enthalpy change.
enthalpy of formation = enthalpy of atomization(s) + ionization energies + electron affinities + lattice enthalpy
solvation (dissolution)
any stabilizing interaction of a solute and the solvent or a similar interaction of solvent with groups of insoluble material
entropy (S)
the amount of randomness or disorder of a system
The natural tendency of the universe is towards greater disorder
A positive entropy change indicates a system is more disordered
A negative entropy change indicates a system is less disordered (more ordered)
standard molar entropy ( S°) a.k.a. absolute entropies
the entropy change of one mole of the pure substance at 1 atm pressure being heated from 0 K to 298 K (in J/K mol)
∆S° = ΣS° (products) - ΣS° (reactants)
First Law of Thermodynamics
in any process, spontaneous or non-spontaneous, the total energy content of a system and its surroundings is constant
Second Law of Thermodynamics
in any spontaneous process, the total entropy of a system and its surroundings always increases