Cells (tissues, organs, and systems, cell division and reproduction)
Metabolism (Digestion and Gas exchange)
Interaction between organisms (food chains and food webs)
Everything in the universe, including all matter on Earth, is formed from unique combinations of tiny, neutral particles called atoms
Atoms of the same kind come together to form elements
To this date, there are 118 elements that have been discovered
The elements' names have been placed in a chart called the periodic table
The placement of each element in this "warehouse" is based on the characteristics of that particular atom
Atom
The smallest component of an element that has the properties of that element
Atom
Consists of electrons, protons, and neutrons
Electron
A negatively charged subatomic particle with no known substructure
Proton
The positively charged particle found in the center of the atom
Neutron
A particle in the nucleus that has a mass similar to the proton but no charge
Isotopes
Atoms of the same element that differ in the number of neutrons
Bohr model
Concentric circles around a central nucleus, electrons travel in set energy levels
Quantum model
Regions within the atom where there is a high probability of finding the electrons (electron orbitals), electrons move within the electron cloud at high speeds
The accepted modern atomic theory states that an atom consists of a positively charged, centrally located nucleus containing protons and neutrons, and negatively charged electrons are found in the area around the nucleus in the electron cloud
Valence electrons
Electrons found in the outermost energy level of an atom, determine the atom's reactivity
Dmitri Mendeleev organized the elements into a periodic table based on their physical and chemical properties
Henry Moseley proposed organizing the elements by atomic number, which resolved anomalies in Mendeleev's table
Periodic law
The physical and chemical properties of the elements are periodic functions of their atomic numbers
Classifications of elements
Metals
Nonmetals
Metalloids
Metals
Dense, shiny solids, high melting points, malleable and ductile, good conductors of heat and electricity
Nonmetals
Dull surface, poor conductors of heat and electricity, low melting points, brittle
Metalloids
May be shiny or dull, can conduct heat and electricity but not as well as metals
Main groups
Group 1: Alkali metals
Group 2: Alkaline earth metals
Group 17: Halogens
Group 18: Noble gases
Alkali metals
Silver-colored, soft metals, highly reactive, have one valence electron
Alkaline earth metals
Silver-colored, soft metals, slightly less reactive than alkali metals, have two valence electrons
Halogens
Highly reactive nonmetals, rarely found in elemental form, have seven valence electrons
Noble gases
Nonreactive gases, odorless and colorless, have a full octet of valence electrons
Transition metals
Variable number of valence electrons, ductile and malleable, good conductors of heat and electricity, high density and melting/boiling points, compounds are usually colored
Inner transition metals (lanthanides and actinides)
Rare earth elements, expensive to obtain, used in various modern industries and applications, most actinides are radioactive
Periodic trends can be explained by the attraction of valence electrons to the nucleus, repulsion between electrons, and energy levels within the atom
Atomic radius
Measurement from the nucleus of one atom to the outermost shell of electrons
All the actinides are radioactive, and most do not occur naturally on Earth. Instead, they can only be created in laboratories under very specific conditions, and most have incredibly short half-lives.
Periodic Trends
Predict Properties with Trends
Characteristics can be used to determine trends
Trends can be explained by attraction to nucleus, repulsion of electrons, and energy levels
Atomic radius
Measurement from nucleus of one atom to nucleus of same type of atom it is touching, then divided in half
Moving from left to right on periodic table
Atomic radii decrease
Moving down a group
Atomic radii increase
Ion
Atom with a charge, determined by number of electrons gained or lost