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Chapter 9: Chemical Bonding I – Lewis Theory (General Chemistry Study Notes)

Study Guide - Smart Notes

Tailored notes based on your materials, expanded with key definitions, examples, and context.

Lewis Theory: An Overview

Fundamental Concepts

  • Valence electrons play a fundamental role in chemical bonding.

  • Electron transfer leads to ionic bonds.

  • Electron sharing leads to covalent bonds.

  • Electrons are transferred or shared to give each atom a noble gas configuration (the octet rule).

  • The octet rule generally applies to main group elements.

Lewis Symbols

Representation of Atoms

  • A chemical symbol represents the nucleus and the core electrons.

  • Dots around the symbol represent valence electrons.

  • Example: Carbon (C) has the electron configuration 1s22s22p2, so its Lewis symbol is C with four dots.

  • Group numbers help determine the number of valence electrons (e.g., Group 14 elements have 4 valence electrons).

Lewis Structures for Ionic Compounds

Constructing Ionic Lewis Structures

  • Determine how many electrons each atom must gain or lose to achieve a noble gas configuration.

  • Use multiples of one or both ions to balance the number of electrons.

  • Ionic compounds are rarely molecular; their formulas represent charge and mass-balanced ions.

  • In Lewis notation, ions are separated using square brackets, e.g., [Ba2+][O2−].

  • Example: Magnesium chloride: Mg2+ and two Cl− ions.

Covalent Bonding

Electron Sharing

  • In true covalent bonding, electrons are shared between atoms.

  • No atom attracts the electrons from another; the sharing is equal (unless the bond is polar).

  • Bond pairs are shared electrons; lone pairs are non-bonding electrons.

  • Example: H2 molecule: two H atoms share electrons to form a single bond.

Coordinate Covalent Bonds

Special Covalent Bonds

  • A coordinate covalent bond forms when both electrons in a bond are donated by one atom (the Lewis base) to another atom (the Lewis acid).

  • Example: Ammonia (NH3) donates a lone pair to H+ to form ammonium (NH4+).

  • All N–H bonds in NH4+ are equivalent.

  • Chloride ion (Cl−) forms by transfer of a bonding pair to chlorine, resulting in an octet and a charge of −1.

Multiple Covalent Bonds

Double and Triple Bonds

  • Multiple bonds result from more than one bonding electron pair being shared.

  • Each double bond contains 4 electrons (2 per bond).

  • Each triple bond contains 6 electrons (3 per bond).

  • Example: CO2 has two double bonds; N2 has a triple bond.

Polar Covalent Bonds

Unequal Sharing of Electrons

  • Polar covalent bonds share electrons unequally due to differences in electronegativity.

  • Results in partial positive (δ+) and partial negative (δ−) charges.

  • Example: H–Cl bond: H is δ+, Cl is δ−.

Electronegativity

Trends and Applications

  • Electronegativity (EN) is the ability of an atom in a molecule to attract shared electrons.

  • EN increases across a period and up a group in the periodic table.

  • Difference in EN between atoms determines bond polarity and ionic/covalent character.

  • Large ΔEN (≥2.0) indicates ionic bond; smaller ΔEN indicates covalent bond.

Slater's Rules

Calculating Effective Nuclear Charge (Zeff)

  • Slater's Rules estimate the shielding effect and Zeff for valence electrons.

  • Formula:

  • S = sum of shielding contributions from other electrons.

  • Higher Zeff leads to higher electronegativity.

Electron Type

Shielding Contribution

Same group (ns/np)

0.35

n-1 shell

0.85

n-2 or lower

1.00

Percent Ionic Character

Bond Character Continuum

  • Bonds range from purely covalent to purely ionic.

  • Percent ionic character increases with electronegativity difference.

  • Example: KF is mostly ionic; HCl is more covalent.

Writing Lewis Structures

General Guidelines

  • All valence electrons must be shown.

  • Electrons are usually paired.

  • Each atom typically requires an octet (except H, which needs only 2 electrons).

  • Multiple bonds may be needed, especially for C, N, O, S, and P.

Skeletal Structure

Identifying Atom Positions

  • Identify central and terminal atoms.

  • Hydrogen atoms are always terminal and can only accommodate two electrons.

  • Central atoms are generally those with the lowest electronegativity (except H and O).

  • Carbon atoms are always central in organic compounds.

  • Inorganic structures are usually compact and symmetrical; organic structures may not be.

Strategy for Writing Lewis Structures

Stepwise Approach

  1. Count the total number of valence electrons.

  2. Draw a skeletal structure.

  3. Place two electrons in each bond.

  4. Identify terminal atoms and complete their octets.

  5. Subtract electrons used from the total; place remaining electrons on the central atom.

  6. If atoms lack octets, form multiple bonds as needed.

Formal Charge

Calculating and Using Formal Charge

  • Formal charge (FC) helps determine the most plausible Lewis structure.

  • Formula:

  • Structures with the lowest formal charges are preferred.

  • Negative formal charges are usually placed on the most electronegative atoms.

Resonance Structures

Delocalization of Electrons

  • Some molecules cannot be represented by a single Lewis structure; instead, multiple resonance structures are drawn.

  • The real structure is a hybrid of all resonance forms.

  • Example: Ozone (O3) has two resonance structures; bond order is 1.5.

  • Bond order formula:

Exceptions to the Octet Rule

Types of Exceptions

  • Odd-electron species: Molecules with an odd number of electrons (radicals).

  • Incomplete octets: Some elements (e.g., B, Be) are electron-deficient and do not achieve an octet.

  • Expanded octets: Elements in Period 3 and below can have more than eight electrons (e.g., SF6, PCl5).

Bond Order and Bond Length

Relationship Between Bonding and Structure

  • Bond order: Number of shared electron pairs between two atoms.

  • Single bond: order = 1; double bond: order = 2; triple bond: order = 3.

  • Higher bond order = shorter and stronger bond.

  • Bond length: Distance between nuclei of bonded atoms.

Bond

Bond Length (pm)

C–C

154

C=C

134

C≡C

120

N–N

145

N=N

125

N≡N

110

O–O

148

O=O

121

Bond Energies

Energy Required to Break Bonds

  • Bond energy: Energy required to break one mole of a bond in gaseous molecules.

  • Shorter bonds are stronger and require more energy to break.

  • Bond energies can be used to estimate enthalpy changes in reactions.

  • Formula:

Bond

Bond Energy (kJ/mol)

H–H

436

C–H

413

C–C

348

C=C

614

C≡C

839

N–N

163

N=N

418

N≡N

941

O–O

146

O=O

498

Practice Problems and Examples

Sample Calculations and Applications

  • Calculate the number of valence electrons for a molecule (e.g., acetone, C3H6O: 24 electrons).

  • Draw Lewis structures for molecules and ions (e.g., HCN, glycine).

  • Assign formal charges and select the most plausible Lewis structure.

  • Draw resonance structures and calculate average bond order (e.g., NO3−: bond order = 1.33).

  • Estimate enthalpy changes using bond energies.

Summary Table: Key Lewis Structure Rules

Rule

Description

Octet Rule

Atoms (except H) tend to have 8 electrons in their valence shell

Formal Charge

Lowest formal charge preferred; negative charge on most electronegative atom

Resonance

Delocalization of electrons; real structure is a hybrid

Exceptions

Odd electrons, incomplete octets, expanded octets

Additional info:

  • These notes are based on lecture slides and annotated class notes for a General Chemistry course (CHEM 1050), focusing on Lewis Theory and chemical bonding.

  • Tables and values are inferred from standard textbook data (Tro, "Chemistry: A Molecular Approach").

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