Module 1: Structure of Matter (Atoms and Molecules)

Basic Definitions of Science and Matter

  • Observation: The act of obtaining qualitative information through the senses.

  • Qualitative Information: Non-numerical data describing qualities, such as color, texture, or smell (e.g., "the cauliflower is purple," "the metal handle was cold").

  • Quantitative Information: Numerical data obtained through measurement (e.g., "I am sixteen years old," "the salt water boils at 106!"C106\,\text{!"C}").

  • Data: A collection of observations and measurements recorded during an investigation.

  • Hypothesis: A tentative, testable explanation for an observation (e.g., "Concrete can be dissolved in boiling water").

  • Experiment: A controlled procedure carried out to test a hypothesis.

  • Theory: A well-substantiated explanation of some aspect of the natural world based on a body of facts that have been repeatedly confirmed (e.g., "Gases are composed of tiny billiard-like particles in constant motion which are colliding and transferring energy").

  • Scientific Law: A statement based on repeated experimental observations that describes some aspects of the universe; it always applies under the same conditions (e.g., "In any chemical reaction, matter is not created or destroyed").

Review of Matter and Classification

  • Atom: The smallest unit of an element that retains the properties of that element.

  • Molecule: Two or more atoms chemically bonded together.

  • Pure Substance: A form of matter that has a constant composition and properties that are consistent throughout; it can be an element or a compound.

  • Element: A pure substance that cannot be broken down into simpler substances by chemical means; made up of only one type of atom.

  • Compounds: Pure substances composed of two or more different elements chemically combined in fixed proportions. The properties of a compound are generally very different from the elements that compose it.

  • Ion: An atom or molecule with a net electric charge due to the loss or gain of one or more electrons.

  • Cation: A positively charged ion (++).

  • Anion: A negatively charged ion (-−).

  • Mixtures: Physical combinations of two or more substances where each substance retains its own chemical identity.

  • Heterogeneous Mixture: A mixture where the components are not uniformly distributed (e.g., cookie batter, fruit salad).

  • Homogeneous Mixture: A mixture where the components are uniformly distributed; also called a Solution (e.g., vitamin C dissolved in water, milk, paint).

  • Physical Property: A characteristic of a substance that can be observed or measured without changing the identity of the substance (e.g., melting point, density).

  • Physical Changes: Changes that affect the form of a chemical substance but not its chemical composition (e.g., snow melting, building a sandcastle).

  • Chemical Changes: Processes where one or more substances are altered into one or more new and different substances (e.g., logs burning, digestion, rust, fireworks exploding).

A Brief History of Atomic Theory and Bohr Model

  • Subatomic Particles:

    • Proton: Located in the nucleus; charge of +1+1; mass of approximately 1amu1\,\text{amu}.

    • Neutron: Located in the nucleus; neutral charge (00); mass of approximately 1amu1\,\text{amu}.

    • Electron: Located in shells orbiting the nucleus; charge of 1-1; mass is approximately 11836\frac{1}{1836} of a proton (usually ignored in atomic mass calculations).

  • Atomic Number: The number of protons in the nucleus; defines the element.

  • Atomic Mass: The sum of the number of protons and neutrons in an atom.

  • Atomic Weight: The weighted average mass of all naturally occurring isotopes of an element.

  • Isotopes: Atoms of the same element (same atomic number) with different numbers of neutrons (different atomic mass).

  • Isotope Calculation Example: Chlorine is 76% Chlorine-35 and 24% Chlorine-37.

    • Atomic Weight=(35×0.76)+(37×0.24)=35.48amu\text{Atomic Weight} = (35 \times 0.76) + (37 \times 0.24) = 35.48\,\text{amu}.

  • The Rutherford Model Problem: According to classical physics, an electron orbiting a nucleus would constantly accelerate, radiate energy, and eventually spiral into the nucleus.

  • Bohr Model:

    • Electrons exist in specific electron shells (energy levels) at fixed distances from the nucleus.

    • Valence Electrons: Electrons in the outermost shell.

    • Period number on the periodic table indicates the number of electronic shells.

    • Group number (for main group elements) indicates the number of valence electrons.

Introduction to Quantum Theory

  • Quantum: The minimum amount of any physical entity involved in an interaction.

  • Photon: A particle representing a quantum of light or other electromagnetic radiation.

  • Wave-Particle Duality: Light and matter (protons, electrons) exhibit both wave-like and particle-like properties.

  • Electronic Transition: When an electron moves between energy levels.

    • Moving to a higher shell: Absorbs a photon (energy).

    • Moving to a lower shell: Emits a photon (energy).

  • De Broglie Equation: λ=hmv\lambda = \frac{h}{mv}

    • λ\lambda is wavelength, hh is Planck's constant, mm is mass, and vv is velocity.

    • Objects with smaller mass and lower velocity act more like waves (longer wavelength).

  • Quantum Mechanical Structure:

    • Electron Shell: Designated by principal quantum number nn.

    • Sub-shell: Found within shells (s, p, d, f).

    • Orbital: A region of space within a sub-shell where there is a high probability of finding an electron. One orbital can hold a maximum of 2 electrons.

    • Shapes: s-orbitals are spherical; p-orbitals are dumbbell-shaped.

Electron Configurations and Ionization

  • Electron Configuration Rules:

    • Electrons fill the lowest energy orbitals first (Aufbau principle).

    • Core Notation: A shorthand using the noble gas from the previous period (e.g., Sn core is [Kr]).

  • Exceptions: Certain elements (like Cr or Cu) fill d-subshells differently to achieve stability.

  • Ions:

    • Isoelectronic: Species that have the same electron configuration (e.g., Mg2+Mg^{2+} and NeNe).

    • Transition metal cations often lose s-electrons before d-electrons.

Periodic Trends

  • Atomic Radii:

    • Increases down a Group (more shells).

    • Decreases across a Period (higher effective nuclear charge pulls electrons closer).

  • Ionic Radii:

    • Cations are smaller than their parent atoms (loss of electron/shell).

    • Anions are larger than their parent atoms (electron-electron repulsion).

  • Ionization Energy (IE): The energy required to remove an electron from an atom.

    • Large atoms have low IE (electrons are further from nucleus and easier to remove).

    • IE increases across a period and decreases down a group.

    • Metals generally have lower IE than non-metals.

  • Electrostatic Forces: The forces of attraction/repulsion between charged particles.

Electronegativity and Chemical Bonding

  • Electronegativity: The tendency of an atom to attract shared electrons in a chemical bond. Fluorine (FF) is the most electronegative element.

  • Combining Capacity (Valence): The number of bonds an atom can form.

  • Types of Bonds:

    • Nonpolar Covalent: Electrons are shared equally (minimal difference in electronegativity).

    • Polar Covalent: Electrons are shared unequally; they move closer to the more electronegative atom.

    • Ionic Bond: Electrons are transferred from one atom to another (large difference in electronegativity).

Lewis Structures and VSEPR Theory

  • Lewis Structure: A diagram showing the bonding between atoms and the lone pairs of electrons.

  • Octet Rule: Atoms tend to form bonds to achieve eight valence electrons.

    • Exceptions: Hydrogen (22), Boron (66), and Expanded Octets (elements in period 3 or below using d-orbitals).

  • VSEPR Theory (Valence Shell Electron Pair Repulsion): Electron pairs repel each other, dictating the 3D shape of molecules.

  • Coordination Number (CN): The sum of bonded atoms and lone pairs on a central atom.

  • Geometries:

    • CN=2CN = 2: Linear (180180^{\circ}).

    • CN=3CN = 3: Trigonal Planar (120120^{\circ}).

    • CN=4CN = 4: Tetrahedral (109.5109.5^{\circ}).

    • CN=5CN = 5: Trigonal Bipyramidal (90/12090^{\circ}/120^{\circ}).

    • CN=6CN = 6: Octahedral (9090^{\circ}).

  • Molecular Shapes: Refers only to the position of atoms (not lone pairs), e.g., Bent, Trigonal Pyramidal, See-saw, T-shape, Square Planar.

Polarity and Intermolecular Forces (IMF)

  • Bond Dipole: Indicated by an arrow (\rightarrow) pointing toward the more electronegative atom. The length represents the magnitude of the charge difference.

  • Molecular Polarity: Determined by the vector sum of bond dipoles. Symmetrical molecules may have polar bonds but be non-polar overall.

  • Intermolecular Forces vs. Intramolecular Forces:

    • Intramolecular: Forces within a molecule (chemical bonds).

    • Intermolecular: Forces between molecules.

  • Types of IMF (from weakest to strongest):

    • London Dispersion Forces: Present in all molecules; caused by temporary dipoles.

    • Dipole-Dipole Interactions: In polar molecules.

    • Hydrogen Bonding: A strong dipole-dipole force occurring when H is bonded to N, O, or F.

  • Physical Properties: Stronger IMF leads to higher boiling points. "Like dissolves like" (polar substances dissolve in polar solvents).