BackGeneral Chemistry: Thermochemistry, Atomic Structure, and Periodic Trends Study Guide
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Thermochemistry
Internal Energy and Work
The internal energy (ΔE) of a system is a fundamental concept in thermodynamics, representing the total energy contained within the system. Changes in internal energy occur when heat is absorbed or released and when work is done by or on the system.
Formula: where q is heat and w is work.
Example: If a system absorbs 220 J of heat and does 100 J of work on the surroundings, .
Endothermic and Exothermic Processes
Endothermic processes absorb heat from the surroundings, while exothermic processes release heat.
Endothermic Example: Melting of a solid (e.g., ice melting to water).
Exothermic Process: ΔH is negative for exothermic reactions, indicating heat is released.
Standard Enthalpy of Formation (ΔHfo)
The standard enthalpy of formation of an element in its most stable form is zero.
Elements with ΔHfo = 0: O2(g), N2(g), F2(g), S8(s), Br2(l), Ca(s)
Calculating Heat Consumed in a Reaction
To determine the heat consumed or released, use stoichiometry and the enthalpy change for the reaction.
Example: For the decomposition of CH3OH(l), if ΔHrxn = +128.1 kJ and 50.0 g of CH3OH(l) decomposes, calculate the moles and multiply by ΔHrxn per mole.
Calculation: ;
Specific Heat and Calorimetry
Specific heat capacity is the amount of heat required to raise the temperature of one gram of a substance by one degree Celsius.
Formula:
Example: To heat 50.0 g of lead from 25°C to 45°C,
Hess's Law
Hess's Law states that the total enthalpy change for a reaction is the sum of the enthalpy changes for individual steps.
Example: Given reactions:
2S(s) + 3O2(g) → 2SO3(g), ΔH = -790 kJ
S(s) + O2(g) → SO2(g), ΔH = -297 kJ
Find: ΔH for 2SO2(g) + O2(g) → 2SO3(g):
Enthalpy of Reaction from Standard Enthalpies of Formation
The enthalpy change for a reaction can be calculated using standard enthalpies of formation:
Formula:
Example Table:
Substance | ΔHfo (kJ/mol) |
|---|---|
CO (g) | -110.5 |
O2 (g) | 0 |
CO2 (g) | -393.5 |
CaCO3 (s) | -1207.0 |
Calculation for 2CO(g) + O2(g) → 2CO2(g):
Atomic Structure and Electron Configuration
Electron Configuration
Electron configuration describes the arrangement of electrons in an atom's orbitals.
Full and Condensed Configuration for Se: 1s22s22p63s23p64s23d104p4
For Ti2+: 1s22s22p63s23p63d2
Quantum Numbers and Orbitals
Quantum numbers describe the properties of atomic orbitals and the electrons in them.
Number of s and p orbitals in n=2 shell: One s orbital, three p orbitals; total electrons = 8
Electron Subshells
Order of filling: 1s, 2s, 2p, 3s, 3p, 4s, 3d, 4p, 4d, 4f
Light and Electromagnetic Radiation
Frequency, Wavelength, and Energy
Light exhibits both wave and particle properties. The relationship between frequency (ν), wavelength (λ), and the speed of light (c) is:
Formula:
Example: For ν = 1.20 × 1013 s-1,
Photon Energy
Formula:
Example: For λ = 8.0 m,
Spectra
Atoms and molecules emit or absorb light at specific wavelengths, producing spectra.
Line Spectrum: Contains only specific wavelengths; characteristic of elements.
Periodic Trends
Trends in the Periodic Table
Periodic trends describe how properties of elements change across periods and down groups.
Atomic Radius: Increases down a group, decreases across a period.
Ionization Energy: Increases across a period, decreases down a group.
Isoelectronic Series
Isoelectronic species have the same number of electrons but different nuclear charges.
Example: B5+, S2-, As3-, Te2-
Ionization of Aluminum
Ionization energy is the energy required to remove an electron from an atom or ion.
Second Ionization of Aluminum:
Summary Table: Key Thermochemistry Data
Substance | ΔHfo (kJ/mol) |
|---|---|
CO (g) | -110.5 |
O2 (g) | 0 |
CO2 (g) | -393.5 |
CaCO3 (s) | -1207.0 |
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