Key Concepts in Chemistry

Chapter 1: Essential Ideas

Section 1.1 Chemistry in Context

  • Strive to recognize chemistry in everyday life.

  • Understand and apply the scientific method.

  • Describe personal experiences using the scientific method.

  • Difference between Theory and Law:

    • Theory: A well-substantiated explanation of an aspect of the natural world based on a body of evidence.

    • Law: A statement based on repeated experimental observations that describe some aspects of the universe.

  • Domains of Chemistry:

    • Macroscopic domain: The realm of ordinary things that are large enough to see with the naked eye.

    • Microscopic domain: The realm of atoms and molecules that can only be seen through special tools.

    • Symbolic domain: The use of symbols (chemical formulas, equations) to represent elements and compounds.

Section 1.2 Phases and Classification of Matter

  • Distinguish between:

    • Solid: Definite shape and volume.

    • Liquid: Definite volume but takes the shape of its container.

    • Gas: No definite volume or shape.

    • Plasma: Ionized gas with free charged particles.

  • Mass vs Weight:

    • Mass: Amount of matter in an object (measured in kilograms).

    • Weight: Gravitational force acting on the mass (measured in newtons).

  • Law of Conservation of Mass: Mass is neither created nor destroyed in a chemical reaction.

    • Calculations: Can be used to predict the amounts of reactants and products in reactions.

  • Distinguish between:

    • Elements: Pure substances that consist of one type of atom.

    • Compounds: Substances formed when two or more elements are chemically bonded.

  • Pure Substance vs Mixture:

    • Pure Substance: Material with a uniform composition (elements and compounds).

    • Mixture: A combination of two or more substances that retain their individual properties.

  • Physical Change vs Chemical Change:

    • Physical Change: Change that does not affect the chemical composition (e.g., melting, freezing).

    • Chemical Change: Change that results in the formation of new chemical substances (e.g., combustion).

  • Physical Properties: Characteristics that can be observed without changing the identity of a substance (e.g., color, boiling point).

  • Homogeneous Mixture vs Heterogeneous Mixture:

    • Homogeneous Mixture: Composition is uniform throughout (e.g., saltwater).

    • Heterogeneous Mixture: Composition is not uniform (e.g., salad).

  • Understanding phase in context of mixtures and states of matter.

Section 1.3 Physical and Chemical Properties

  • Physical Properties: Properties that can be observed or measured without changing the substance's chemical identity (e.g., melting point, boiling point).

  • Chemical Properties: Properties that become evident during a chemical reaction, indicating how a substance interacts with others.

  • Distinguish between:

    • Extensive Physical Properties: Depend on the amount of substance present (e.g., mass, volume).

    • Intensive Physical Properties: Independent of the amount of substance (e.g., density, temperature).

  • Recognize:

    • Physical Changes: Changes that affect one or more physical properties of a substance.

    • Chemical Changes: Changes that result in the formation of new chemical substances.

Section 1.4 Measurements

  • Measurements include:

    • Magnitude: The size or amount of a quantity.

    • Unit: Standardized quantity used to specify measurements (e.g., meter, liter).

    • Uncertainty: Means precision or reliability of a measured value.

  • Significant Digits: The number of meaningful digits in a measurement that contributes to its accuracy.

  • Use of:

    • Significant Figures: Reflects the precision of a measured value.

    • Scientific Notation: Represents very large or very small numbers efficiently.

    • SI Base Units: Seven fundamental units for measurement (e.g., length, mass, time) as listed in Table 1.2 of OpenStax text.

    • SI Prefixes: Represent powers of ten as shown in Table 1.3 of OpenStax text.

    • Derived Units: Units obtained from combining base units (e.g., volume in cubic meters, density in kg/m³).

  • Density Calculations: Relation of mass to volume, expressed as:

    • ext{Density} = rac{ ext{Mass}}{ ext{Volume}}.

Section 1.5 Measurement Uncertainty, Accuracy, and Precision

  • Scientific notation in calculations helps manage the scale of numbers.

  • Report the correct number of significant digits in the results of calculations.

  • Exact Numbers: Counted quantities or defined quantities that have no uncertainty.

  • Rounding: Adjusting numbers to reflect the appropriate amount of significant figures.

  • Precision vs Accuracy:

    • Precision: How consistent repeated measurements are to one another.

    • Accuracy: How close a measurement is to the actual or true value.

Section 1.6 Mathematical Treatment of Results

  • Convert between temperature scales:

    • Celsius (°C), Fahrenheit (°F), and Kelvin (K).

  • Perform calculations using the factor-label method or dimensional analysis:

    • Factor-label approach leverages conversion factors to change units in calculations.

  • Equality: Provides two conversion factors useful for unit conversions.

  • Molar Mass: Acts as a conversion factor linking grams to moles and vice versa.

Chapter 2: Atoms, Molecules, and Ions

Section 2.1 Early Ideas in Atomic Theory

  • Understand the postulates of Dalton’s Atomic Theory:

    • Each element is composed of atoms.

    • Atoms of a given element are identical, while atoms of different elements are different.

    • Compounds are formed when atoms of different elements combine in fixed ratios.

    • A chemical reaction is a rearrangement of atoms.

  • Atomic Theory Components:

    • Atomic symbols: Recognize and understand their meaning.

    • Become familiar with symbols listed in Table 2.1 of OpenStax text.

  • Law of Multiple Proportions: When two elements form more than one compound, the ratios of the masses can be expressed as small whole numbers.

Section 2.2 Evolution of Atomic Theory

  • Important experiments and findings by:

    • J. J. Thompson: Demonstrated that atoms are divisible and discovered the electron's mass to charge ratio (~1897).

    • Robert Milliken: Conducted oil drop experiments to determine the charge of the electron (~1909).

    • Ernest Rutherford: Known for the gold foil experiments leading to the nuclear model of the atom (~1911).

    • Frederick Soddy: Introduced the concept of isotopes (early 1900s).

    • James Chadwick: Provided evidence for the existence of neutrons (~1932).

Section 2.3 Atomic Structure and Symbolism

  • Structure of the atom:

    • Nucleus: Comprised of protons (positive charge) and neutrons (no charge).

    • Electrons: Negatively charged particles surrounding the nucleus.

  • Relative Masses and Charges of atomic particles (see Table 2.2, page 80, OpenStax text).

  • Understanding Atomic Number (Z) and Mass Number (A):

    • Atomic Number (Z): The number of protons in the nucleus.

    • Mass Number (A): Total number of protons and neutrons in an atom.

  • Distinction between:

    • Atoms: Generally neutral entities having balanced charges.

    • Ions: Charged particles formed when atoms gain or lose electrons.

    • Cations: Positively charged ions (loss of electrons).

    • Anions: Negatively charged ions (gain of electrons).

  • Recognition of element symbols in the periodic table and their corresponding elements.

  • Isotopes: Variants of elements that have the same number of protons but different numbers of neutrons.

  • Be proficient in calculating:

    • Average mass of atoms of elements.

    • Percent composition of samples of compounds.

Section 2.4 Chemical Formulas

  • Recognition and understanding of various chemical formulas.

  • Distinguish between formulas for:

    • Ionic Compounds: Compounds formed from ionic bonds (e.g., NaCl).

    • Molecular Compounds: Compounds formed from covalent bonds (e.g., H₂O).

  • Isomers:

    • Structural Isomers: Different connectivity among the same atoms.

    • Geometric Isomers: Different spatial arrangements of atoms in a molecule.

Section 2.5 The Periodic Table

  • Historical figures:

    • Dmitri Mendeleev: Developed an early version of the periodic table (1869).

    • Julius Lothar Meyer: Independently developed a periodic table (1870).

  • Periodic Law: The properties of elements are periodic functions of their atomic numbers.

  • Organization of the Periodic Table:

    • Elements arranged according to increasing atomic number.

    • Elements in the same period (row) share similar properties and energy levels.

    • Elements in the same group (column) have similar chemical behaviors.

  • Metals vs Nonmetals:

    • Metals: Typically found on the left side, possess good conductivity and malleability.

    • Nonmetals: Found on the right, generally poor conductors and brittle.

  • Identification of:

    • Alkali Metals: Group 1, highly reactive.

    • Alkaline Earth Metals: Group 2, reactive metals.

    • Chalcogens: Group 16, diverse group including oxygen and sulfur.

    • Halogens: Group 17, highly reactive nonmetals.

    • Noble Gases: Group 18, inert gases with low reactivity.

    • Transition Metals: Groups 3-12, metals with variable oxidation states.

    • Inner Transition Metals: Lanthanides and Actinides, known for radioactive properties.

  • Recognize trends in Effective Nuclear Charge and Electronegativity across the table.

Section 2.6 Molecular and Ionic Compounds

  • Understanding chemical reactions as a rearrangement of atoms and electrons.

  • General rule: Atoms move towards achieving an octet configuration:

    • Some atoms become ions to form ionic bonds (transfer of electrons).

    • Some share electrons to establish covalent bonds.

  • Ionic Compounds: Form from ionic bonds involving the transfer of electrons.

  • Molecular Compounds: Form from covalent bonds involving shared electrons.

Section 2.7 Chemical Nomenclature (Naming)

  • Distinction between:

    • Organic Compounds: Typically contain carbon and must follow specific naming conventions.

    • Inorganic Compounds: Do not predominantly consist of carbon.

  • Naming rules include:

    • Binary compounds: Use prefixes to denote the number of atoms present.

    • Naming ionic compounds, including those with metals that have variable charges.

    • Naming ionic hydrates, molecular inorganic compounds, binary acids, and oxoacids.

  • Strong Acids and Bases: Familiarity with the six common strong acids (e.g., HCl, H₂SO₄) and strong bases (e.g., NaOH, KOH)

    • Remember that stronger acids correspond to weaker conjugate bases.

Chapter 3: Composition of Substances and Solutions

Section 3.1 Formula Mass and the Mole Concept

  • Determine the formula mass (molar mass) of:

    • Molecules, ionic compounds, polyatomic ions.

  • Mole: The SI unit for chemical quantity.

    • 1 ext{ mol} = 6.02 imes 10^{23} ext{ atoms/molecules/etc.}.

    • Avogadro’s Number: 6.02214179 imes 10^{23}.

  • Understand:

    • The correlation between the number of atoms in moles of different substances.

    • The mass of one mole of various substances differs.

  • Recognize that Molar Mass is the mass (in grams) of one mole, expressed in g/mol, and is numerically equivalent to the atomic mass in atomic mass units (amu).

  • Proficiency in conversions between mass, moles, number of molecules, and number of atoms.

Section 3.2 Determining Empirical and Molecular Formulas

  • Ability to determine:

    • Percent composition from atomic masses.

    • Empirical formulas from grams of elements in samples of compounds (Example 3.9, 3.10, 3.11).

    • Convert empirical formulas to molecular formulas using molecular mass (Example 3.12, 3.13).

Section 3.3 Molarity

  • Concentration: The amount of solute present in a given volume of solution.

    • Solute: The substance that is dissolved.

    • Solvent: The liquid that dissolves the solute.

    • Solution: The homogenous mixture of solute and solvent.

  • Distinction between:

    • Concentrated and Dilute Solutions.

  • Recognize Molarity (M) as:

    • M = rac{ ext{moles of solute}}{ ext{volume of solution in liters}}.

  • Proficiency in calculating:

    • Molar Concentration (Example 3.14).

    • Moles and volumes based on molar concentrations (Example 3.15).

    • Molar concentration from solute mass (Example 3.16).

    • Mass of solute in given volumes (Example 3.17).

    • Volume of solution from given mass of solute (Example 3.18).

Section 3.4 Other Units for Solution Concentrations

  • Become proficient at calculations involving:

    • Mass Percentage: (mass of solute / total mass of solution) × 100% (Examples 3.22, 3.23).

    • Volume Percentage: (volume of solute / total volume of solution) × 100% (Example 3.24).

    • Mass-Volume Percentage: (mass of solute/volume of solution) × 100% (Example 3.25).

    • Parts per Million (ppm) and Parts per Billion (ppb) as measures of concentration (Example 3.25).

Chapter 4: Stoichiometry of Chemical Reactions

Section 4.1 Writing and Balancing Chemical Equations

  • Ability to write balanced chemical equations from reactants.

  • Recognize:

    • Reactants: Substances that undergo change.

    • Products: Substances formed from the reaction.

    • Phase Labels: Indicate the physical state of the reactants and products.

    • Stoichiometric Coefficients: Numbers indicating the ratio of reactants to products.

  • Balancing Equations: Ensure mass and charge are conserved in reactions.

  • Write balanced:

    • Molecular Equations: Full formulas for all reactants and products.

    • Complete Ionic Equations: Show all ions present in solution.

    • Net Ionic Equations: Identify only the species that undergo change.

  • Importance of net ionic equations in predicting outcomes of reactions.

Section 4.2 Classifying Chemical Reactions

  • Distinctions between different reaction types:

    • Redox Reactions: Involves changes in oxidation states.

    • Precipitation Reactions: Formation of solid from a solution.

    • Acid-Base Reactions: Transfer of protons (H⁺ ions).

  • Recognize whether a precipitate is formed from balanced equations.

  • Differentiate between strong and weak acids/bases:

    • Neutralization reactions involve strong acids and bases reacting.

    • Use oxidation state assignments to determine redox occurrence.

    • Identify species oxidized and reduced in redox reactions.

  • Recognize that single displacement and combustion reactions are types of redox reactions.

    • Distinction between decomposition and combination reactions based on redox characteristics.

Section 4.3 Reaction Stoichiometry

  • Utilize stoichiometric coefficients to:

    • Determine moles of reactants needed (Example 4.8).

    • Relate masses of reactants to products (Example 4.10).

    • Relate masses between reactants themselves (Example 4.11).

Section 4.4 Reaction Yields

  • Identify the Limiting Reactant:

    • Determines the maximum amount of product formed in a reaction (Example 4.12).

  • Calculate Percent Yield:

    • ext{Percent Yield} = rac{ ext{Actual Yield}}{ ext{Theoretical Yield}} imes 100 (Example 4.13).

Section 4.5 Quantitative Chemical Analysis

  • Techniques for analytical chemistry:

    • Titration: Method to determine concentration based on neutralization reactions.

    • Gravimetric Analysis: Measure of mass to determine concentration.

    • Combustion Analysis: Used for determining empirical formulas through combustion.

Chapter 5: Thermochemistry

Section 5.1 Energy Basics

  • Define and identify examples of:

    • Kinetic Energy: Energy due to motion.

    • Potential Energy: Stored energy based on position.

    • Thermal Energy: Energy within a system due to temperature.

  • Conversion between Temperature Scales:

    • Celsius (°C), Fahrenheit (°F), Kelvin (K).

  • Units for Energy:

    • Calorie (cal): Amount of energy required to raise the temperature of 1 gram of water 1°C.

    • Joule (J): SI unit of energy (1 cal = 4.184 J).

  • Distinction between:

    • Heat Capacity: Total heat required to change the temperature by a degree.

    • Specific Heat: Heat needed to raise the temperature of 1 gram by 1°C.

    • Molar Heat Capacity: Amount of heat needed for one mole.

  • Calculate:

    • C = rac{q}{ riangle T} and q = c imes m imes riangle T: where q = heat energy, c = specific heat, m = mass, ΔT = change in temperature.

Section 5.2 Calorimetry

  • Describe how Calorimetry measures heat transfer.

  • Distinctions between:

    • Endothermic Processes: Absorb heat.

    • Exothermic Processes: Release heat.

    • System vs Surroundings: The system is the part of the universe we focus on.

  • Apply the relationship:

    • q{ ext{reaction}} = -q{ ext{solution}}

  • Understand the use of bomb calorimeter for constant volume calorimetry.

  • Nutritional calorie (Calorie) is defined as:

    • 1 ext{kcal} = 1,000 ext{cal}.

Section 5.3 Enthalpy

  • State First Law of Thermodynamics:

    • Energy cannot be created or destroyed, only transformed.

  • Concepts and terminology:

    • Internal Energy: Total energy contained within a system.

    • Expansion Work: Work done by a system when it expands against external pressure.

    • State Function: Property determined by state variables (e.g., internal energy, enthalpy).

    • Enthalpy (H) and Change in Enthalpy (ΔH): The heat content of a system at constant pressure.

    • Standard State Conditions: Standard for measuring enthalpy changes at 1 atm and specified temperatures (usually 25°C).

    • Standard Enthalpy of Combustion (ΔH°ₕ): Heat released during combustion of 1 mole of substance.

    • Standard Enthalpy of Formation (ΔH°ₓ): Heat change when one mole of a compound is formed from its elements.

    • Hess’s Law: Total enthalpy change for a reaction is the sum of the enthalpy changes for individual steps.

  • Write thermochemical equations while manipulating them for calculations.

  • Determine heat of reactions from standard enthalpies of formation using Hess's law.

Chapter 6: Electronic Structure and Periodic Trends

Section 6.1 Electromagnetic Energy

  • Convert between wavelength and frequency:

    • Use the equation c =
      u imes ext{λ} where c = speed of light, ν = frequency, and λ = wavelength.

  • Understand relationships between:

    • Energy: Directly proportional to frequency and inversely proportional to wavelength.

  • Familiarize yourself with the electromagnetic spectrum: Range of all wavelengths of electromagnetic radiation.

  • Recognize and analyze Constructive and Destructive Interference: Wave behaviors affecting intensity and amplitude.

  • Identify nodes in standing waves indicating points of no displacement.

  • Distinguish between Continuous Spectrum: All wavelengths vs Line Spectrum: Specific wavelengths emitted by substances.

  • Discuss phenomena such as:

    • Ultraviolet Crisis: Inadequacy of classical physics for electron behavior.

    • Photoelectric Effect: Emission of electrons when light hits a material.

    • Wave-Particle Duality of Light: Light behavior exhibiting both wave-like and particle-like properties.

  • Contributions of early scientists:

    • Balmer: Developed formula for hydrogen spectral lines.

    • Rydberg: Expanded understanding of spectral series.

    • Bohr: Introduced quantized energy levels in star model of the hydrogen atom.

Section 6.2 The Bohr Model

  • Describe Bohr Model of the atom, focusing on discrete energy levels of electrons.

  • Distinction between Ground State (lowest energy configuration) and Excited State (higher energy configurations).

  • Utilize the Rydberg Equation for calculating transition energies of electrons between levels:

    • rac{1}{ ext{λ}} = RH imes igg( rac{1}{n1^2}- rac{1}{n_2^2}igg).

Section 6.3 Development of Quantum Theory

  • Relate wave-particle duality for both light and electrons.

  • Understand and apply Quantum Numbers:

    • Define each of the four quantum numbers:

    • Principal Quantum Number (n): Indicates energy level.

    • Angular Momentum Quantum Number (l): Specifies subshell shape.

    • Magnetic Quantum Number (m): Orientation of orbital.

    • Spin Quantum Number (ms): Direction of electron spin.

  • Define deBroglie Wavelength: Indicates wave nature of particles:

    • ext{λ} = rac{h}{mv}, where h = Planck's constant, m = mass, v = velocity.

  • Understand the Heisenberg Uncertainty Principle: Limits on simultaneously knowing position and momentum of particles.

  • Comprehend Pauli Exclusion Principle: No two electrons in an atom can have the same four quantum numbers.

Section 6.4 Electronic Structure of Atoms

  • Write electron configurations for both atoms and ions based on their energy levels.

  • Draw Orbital Diagrams illustrating electron arrangement in different subshells.

  • Apply principles of:

    • Aufbau Principle: Electrons fill lower-energy orbitals first.

    • Hund’s Rule: Electrons occupy degenerate orbitals singly before pairing.

  • Identify Valence Electrons (electrons in the outermost shell) versus Core Electrons (inner shell electrons).

  • Classify:

    • Main Group Elements: Elements in Groups 1, 2 and 13-18.

    • Transition Elements: Elements in Groups 3-12.

    • Inner Transition Elements: Lanthanides and Actinides.

Section 6.5 Periodic Variations in Element Properties

  • Describe and explain trends within the periodic table:

    • Covalent Radius: Decreases across a period, increases down a group.

    • Effective Nuclear Charge (Z_eff): Increases across a period due to greater nuclear attraction.

    • Ionic Radii: Varies based on charge and environment.

    • Ionization Energy: Energy required to remove an electron.

    • Electron Affinity: Energy change when an electron is added.

    • Metallic Character: Increases down a group, decreases across a period.

  • Recognize Isoelectronic Species: Different elements or ions having the same electron configuration.

Chapter 7: Chemical Bonding and Molecular Geometry

Section 7.1 Ionic Bonding

  • Distinguish between Cations (positively charged ions) and Anions (negatively charged ions), atoms, and molecules.

  • Explain the formation processes of cations and anions:

    • Cations form through loss of electrons (often metals).

    • Anions form through gain of electrons (often nonmetals).

  • Identify properties of ionic compounds:

    • High melting and boiling points, conduct electricity in solution.

  • Compare ions and atoms based on properties such as size and charge.

  • Identify and describe Binary Ionic Compounds: Combustions of two elements.

  • Recognize that attractive forces between ions are isotropic: Equal in all directions.

  • Explain the Inert Pair Effect: Tendency of the two electrons of the outermost s subshell to remain unbonded.

  • Write electron configurations for:

    • Atoms.

    • Anions (gaining electrons).

    • Cations (losing electrons).

Section 7.2 Covalent Bonding

  • Explain the distinctions between covalent and ionic bonds:

    • Covalent bonds form when atoms share electrons (typically nonmetals).

    • Ionic bonds result from the transfer of electrons (typically between metals and nonmetals).

  • Compare properties of molecular compounds with ionic compounds:

    • Molecular compounds typically have lower melting/boiling points.

  • Discuss how covalent bonds form based on electron sharing.

  • Recognize factors affecting bond lengths:

    • Electronegativity, number of shared electron pairs.

  • Understand that:

    • Bond Breaking: Endothermic process (energy absorbed).

    • Bond Making: Exothermic process (energy released).

  • Distinguish between:

    • Polar Covalent Bond: Unequal sharing of electrons.

    • Pure Covalent Bond: Equal sharing of electrons (e.g., in diatomic molecules).

  • Differentiate properties of Effective Nuclear Charge, Electronegativity, and Electron Affinity.

  • Recognize trends in Effective Nuclear Charge, Electronegativity, and Electron Affinity across the periodic table.

  • Identify Polyatomic Ions: Groups of covalently bonded atoms carrying a charge.

Section 7.3 Lewis Symbols and Structures

  • Write Lewis Symbols based on valence shell electron configurations for atoms.

  • Show electron arrangements in ions using Lewis symbols, distinguishing between lone pair and bonding electrons.

  • Explain the Octet Rule: Atoms tend to bond until they have eight electrons in their outermost shell.

  • Distinction between:

    • Single Bonds, Double Bonds, Triple Bonds: Represent different degrees of electron sharing.

  • Draw Lewis Structures by following valence shell arrangements.

  • Recognize exceptions to the octet rule:

    • Electron Deficient Species: Molecules with fewer than eight electrons around an atom.

    • Hypervalent Species: Molecules where central atoms hold more than eight electrons.

Section 7.4 Formal Charge and Resonance

  • Assign Formal Charge to atoms in molecules to determine stability.

  • Use formal charge to evaluate which Lewis structures are more favorable.

  • Explain Resonance: Configuration where two or more valid structures exist for a molecule, not representing real distribution but stability.

  • Distinguish resonance structures from isomers (different connectivity of atoms).

  • Define Resonance Hybrid: The actual molecule represented as a blend of all possible resonance structures.

Chapter 8: Advanced Theories of Covalent Bonding

Section 8.1 Valence Bond Theory

  • Describe the concept of Covalent Bond Formation:

    • Formation through overlap of atomic orbitals, with electrons pairing.

  • Conditions for bond formation include:

    • Proper orientation and sufficient energy during overlap.

  • Discuss the energy changes occurring when forming bonds

    • Closer to stability with bond formation.

  • Distinguish between types of bonds:

    • Sigma Bonds: Formed by head-on overlap of orbitals.

    • Pi Bonds: Formed by side-on overlap, occurring in double/triple bonds.

  • Determine the number of sigma and pi bonds in molecular structures.

Section 8.2 Hybrid Atomic Orbitals

  • Explain limitations of valence bond theory in describes carbon bonding.

  • Define Hybridization: The process in which atomic orbitals mix to form new hybrid orbitals suitable for bonding.

  • Describe hybrid orbital formations for:

    • sp³ Hybridization: One s and three p orbitals (e.g., in methane).

    • sp² Hybridization: One s and two p orbitals.

    • sp Hybridization: One s and one p orbital.

  • Determine the hybridization of a carbon atom based on its bonding structure.

Section 8.3 Multiple Bonds

  • Describe covalent bonds in terms of Orbital Overlap where multiple bonds involve both sigma and pi bonds.

  • Relate Resonance to electron delocalization through pi bonds in structures.

  • Draw atomic orbital energy diagrams displaying formation of sp³, sp², and sp hybrid orbitals.

  • Draw and label Orbital Overlap in molecules such as Ethene, Benzene, and Ethyne.

Section 8.4 Molecular Orbital Theory

  • Characteristics explained by Molecular Orbital Theory include:

    • This theory elucidates the nature of bonding and accounts for paramagnetic and diamagnetic properties of substances.

  • Compare and contrast Valence Bond Theory with Molecular Orbital Theory outlined in Table 8.2 (Page 433).

  • Distinguish between Bonding and Antibonding Orbitals, and sigma and pi interactions.

  • Recognize Molecular Orbital Energy Diagrams for diatomic molecules to determine stability and bond order:

    • Bond Order calculated by:

    • ext{Bond Order} = rac{ ext{(number of bonding electrons - number of antibonding electrons)}}{2}.

Chapter 9: Gases

Section 9.1 Gas Pressure

  • Define Gas Pressure: Force per unit area exerted by gas on walls of its container.

    • Pressure usually measured in pascals (Pa).

  • Introduce the Ideal Gas Law:

    • PV = nRT,

    • where P is pressure, V is volume, n is number of moles, R is the ideal gas constant, and T is temperature in Kelvin.

Section 9.3 Stoichiometry of Gaseous Substances, Mixtures, and Reactions

  • Use the Ideal Gas Law to derive:

    • Gas Density: density can be expressed based on molar mass and conditions of gas.

    • Molar Mass: Can be calculated from gas density and the ideal gas law.

    • Molecular Formula: Determined from experimental mass data using molar relationships.

Section 9.5 Interpret Molecular Speed Diagrams

  • Discuss interpretation of molecular speed diagrams, indicating the distribution of molecular speeds in gas samples (see Figure 9.33 in OpenStax text).

Chapter 10: Liquids and Solids

Intermolecular Forces

  • Describe various types of interactions present in liquids and solids:

    • Dispersion Forces: Weak forces arising from temporary shifts in electron density.

    • Dipole-Dipole Interactions: Occur between polar molecules due to their permanent dipoles.

    • Hydrogen Bonding Interactions: Specifically strong dipole-dipole interactions that occur when hydrogen is bonded to electronegative atoms (e.g., N, O, F).

  • Relate intermolecular forces to physical properties including:

    • Melting Point: The temperature at which a solid becomes a liquid.

    • Boiling Point: The temperature at which a liquid becomes a gas.