🧪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.
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 Properties and Trends
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