🧪AP Chemistry Unit 1 – Atomic Structure and Properties

Atomic structure and properties form the foundation of chemistry. This unit explores the fundamental building blocks of matter, from subatomic particles to electron configurations. Understanding these concepts is crucial for grasping chemical behavior and reactivity. The periodic table organizes elements based on their atomic structure, revealing trends in properties across periods and groups. This knowledge enables predictions about element behavior, bonding, and interactions, essential for understanding chemical reactions and material properties.

Fundamental Concepts

  • Matter consists of atoms, the smallest unit of an element that retains its properties
  • Atoms are composed of subatomic particles: protons, neutrons, and electrons
  • Protons have a positive charge, neutrons have no charge, and electrons have a negative charge
    • The number of protons in an atom determines its atomic number and element identity
    • Atoms are electrically neutral when the number of protons equals the number of electrons
  • Elements are pure substances composed of only one type of atom (gold, oxygen)
  • Compounds are substances made up of two or more elements chemically combined in a specific ratio (water, salt)
  • Mixtures contain two or more substances that are not chemically combined and can be separated by physical means (air, salt water)
  • Chemical reactions involve the rearrangement of atoms to form new substances with different properties

Atomic Theory and Models

  • Dalton's atomic theory proposed that atoms are indivisible and indestructible particles
    • This theory laid the foundation for modern atomic understanding but had limitations
  • Thomson's plum pudding model suggested that electrons are embedded in a positively charged "pudding"
    • Experiments with cathode rays led to the discovery of electrons
  • Rutherford's gold foil experiment provided evidence for the nuclear model of the atom
    • Most of an atom's mass and positive charge is concentrated in a small, dense nucleus
    • Electrons orbit the nucleus in a relatively large space
  • Bohr's model introduced the concept of energy levels for electrons
    • Electrons can only occupy specific energy levels and can move between them by absorbing or emitting energy
  • The quantum mechanical model describes electrons as having wave-like properties and existing in orbitals
    • This model incorporates the Heisenberg uncertainty principle and Schrödinger's wave equation

Subatomic Particles

  • Protons are positively charged particles located in the nucleus of an atom
    • The number of protons determines an element's atomic number and identity
    • Protons have a mass of approximately 1 atomic mass unit (amu)
  • Neutrons are electrically neutral particles found in the nucleus alongside protons
    • Neutrons contribute to the mass of an atom but do not affect its atomic number
    • Like protons, neutrons have a mass of about 1 amu
  • Electrons are negatively charged particles that orbit the nucleus in energy levels or orbitals
    • Electrons are much lighter than protons and neutrons, with a mass of approximately 1/1836 amu
    • The number of electrons in an atom determines its chemical properties and reactivity
  • Quarks are even smaller particles that make up protons and neutrons
    • Protons consist of two up quarks and one down quark
    • Neutrons consist of one up quark and two down quarks
  • Leptons are another type of subatomic particle that includes electrons and neutrinos
    • Neutrinos have very little mass and rarely interact with other particles

Electron Configuration

  • Electron configuration describes the arrangement of electrons in an atom's orbitals
  • Electrons occupy orbitals in order of increasing energy, following the Aufbau principle
    • The Aufbau principle states that electrons fill orbitals starting with the lowest energy level
  • Orbitals are designated by their principal quantum number (n), angular momentum quantum number (l), and magnetic quantum number (m)
    • The principal quantum number represents the energy level or shell (1, 2, 3, etc.)
    • The angular momentum quantum number represents the subshell (s, p, d, f)
    • The magnetic quantum number represents the orientation of the orbital in space
  • The Pauli exclusion principle states that no two electrons in an atom can have the same set of four quantum numbers
    • This means that each orbital can hold a maximum of two electrons with opposite spins
  • Hund's rule states that electrons in the same subshell will occupy separate orbitals with parallel spins before pairing up
  • Electron configurations can be written using the noble gas notation, which abbreviates the configuration using the previous noble gas (Ne, Ar, Kr)

Periodic Table Organization

  • The periodic table arranges elements in order of increasing atomic number
  • Elements are organized into periods (rows) and groups (columns) based on their electron configurations and properties
    • Periods represent the number of electron shells in an atom
    • Groups contain elements with similar electron configurations and chemical properties
  • The periodic table is divided into four blocks based on the type of subshell being filled: s-block, p-block, d-block, and f-block
    • The s-block includes alkali metals and alkaline earth metals
    • The p-block includes nonmetals, halogens, and noble gases
    • The d-block contains transition metals
    • The f-block includes lanthanides and actinides
  • Metals are located on the left side of the periodic table and tend to be shiny, malleable, and good conductors of heat and electricity
  • Nonmetals are located on the right side of the periodic table and are generally poor conductors of heat and electricity
  • Metalloids, located along the stair-step line, have properties intermediate between metals and nonmetals (silicon, germanium)
  • Atomic radius is the distance from the nucleus to the outermost electron shell
    • Atomic radius generally decreases from left to right across a period due to increasing effective nuclear charge
    • Atomic radius increases down a group because of additional electron shells
  • Ionization energy is the energy required to remove an electron from a neutral atom in the gaseous state
    • Ionization energy generally increases from left to right across a period due to increasing effective nuclear charge
    • Ionization energy decreases down a group because of increased atomic radius and shielding effect
  • Electron affinity is the energy change that occurs when an electron is added to a neutral atom in the gaseous state
    • Electron affinity generally becomes more negative from left to right across a period
    • Electron affinity becomes less negative down a group due to increased atomic radius and shielding effect
  • Electronegativity is the ability of an atom to attract electrons in a chemical bond
    • Electronegativity increases from left to right across a period and decreases down a group
    • Electronegativity values are used to predict the type of bonding between elements (ionic, covalent, or polar covalent)

Isotopes and Nuclear Chemistry

  • Isotopes are atoms of the same element with different numbers of neutrons
    • Isotopes have the same atomic number but different mass numbers
    • The mass number is the sum of the number of protons and neutrons in an atom
  • Isotopes can be stable or unstable (radioactive)
    • Stable isotopes do not undergo radioactive decay and have a constant number of protons and neutrons over time
    • Unstable isotopes, or radioisotopes, undergo radioactive decay to achieve a more stable configuration
  • Radioactive decay is the process by which an unstable nucleus emits particles or energy to form a more stable nucleus
    • Alpha decay involves the emission of an alpha particle (two protons and two neutrons)
    • Beta decay involves the emission of a beta particle (an electron) and the conversion of a neutron to a proton
    • Gamma decay involves the emission of high-energy photons (gamma rays) to release excess energy
  • Half-life is the time required for half of a given quantity of a radioactive isotope to decay
    • The half-life is constant for a specific isotope and can range from fractions of a second to billions of years
  • Nuclear reactions, such as fission and fusion, involve changes in the nucleus of an atom
    • Nuclear fission is the splitting of a heavy nucleus into lighter nuclei, releasing energy (used in nuclear power plants)
    • Nuclear fusion is the combining of light nuclei to form a heavier nucleus, releasing large amounts of energy (occurs in the Sun)

Real-World Applications

  • Atomic structure and properties play a crucial role in various fields, including materials science, energy production, and medicine
  • Understanding electron configurations helps predict chemical bonding and reactivity, which is essential for designing new materials (semiconductors, catalysts)
  • Radioisotopes are used in nuclear medicine for diagnostic imaging and cancer treatment
    • Technetium-99m is commonly used in bone scans and heart imaging
    • Iodine-131 is used to treat thyroid cancer and hyperthyroidism
  • Carbon dating, which relies on the radioactive decay of carbon-14, is used to determine the age of organic materials (fossils, artifacts)
  • Atomic spectroscopy techniques, such as atomic absorption and emission spectroscopy, are used for elemental analysis in environmental monitoring and quality control
  • Quantum dots, which are nanoscale semiconductor crystals with size-dependent electronic properties, are used in LED displays and solar cells
  • Nuclear power plants harness the energy released from nuclear fission reactions to generate electricity
  • Research in nuclear fusion aims to develop a clean and virtually limitless energy source for the future


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© 2024 Fiveable Inc. All rights reserved.
AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.