Language of Chemistry
Chemistry is the study of matter, its chemical and physical properties, and the chemical and physical changes it undergoes.
Matter is anything that has mass and occupies space.
Atoms are the building blocks of matter.
An element is made of the same kind of atoms.
A compound is made of two or more different elements.
Energy is the ability to do work or accomplish some change.
Composition of Matter
Pure substances have distinct properties and a composition that doesn't vary from sample to sample, e.g., salt.
An element is a substance that cannot be decomposed into simpler substances, e.g., oxygen gas.
A compound is a substance composed of two or more different elements, meaning it contains two or more kinds of atoms, e.g., water.
Mixtures are a combination of two or more substances in which each substance retains its own identity and can be separated from each other.
Homogeneous mixtures are uniform throughout, e.g., vanilla ice-cream.
Heterogeneous mixtures do not have the same composition, properties, and appearance throughout, e.g., muesli.
Classification of Matter
A decision flow chart can be used to classify matter.
States of Matter
Gas: Molecules are far apart and move at high speed.
Liquid: Molecules are packed more closely but still move rapidly, allowing them to slide over each other.
Solid: Molecules are held together, usually in a definite arrangement.
Plasma
Properties of Matter
A property is any characteristic that allows us to recognize a type of matter and distinguish it from other types.
Properties of matter relate to its composition (the kind of atoms it contains) and its structure (the arrangement of those atoms).
Examples:
Hydrogen
Oxygen
Carbon
Physical Properties
Physical properties can be observed without changing a substance into another substance.
Examples: boiling point, density, mass, volume.
Chemical Properties
Chemical properties can only be observed when a substance is changed into another substance.
Examples: flammability, corrosiveness, reactivity with acid.
Intensive Properties
Intensive properties are independent of the amount of the substance present.
Examples: density, boiling point, color.
Extensive Properties
Extensive properties are dependent on the amount of the substance present.
Examples: mass, volume, energy.
Changes of Matter
Physical Changes
Physical changes are changes in matter that do not change the composition of a substance.
Examples: changes of state, temperature, volume.
Chemical Changes
Chemical changes are changes that result in new substances.
Examples: combustion, oxidation, decomposition.
Quiz
Classify the following as either a chemical or physical property:
Color - Physical
Flammability - Chemical
Hardness - Physical
Odor - Physical
Taste - Physical
Classify the following as either a chemical or physical change:
Boiling water becomes steam - Physical
Butter turns rancid - Chemical
Burning of wood - Chemical
Mountain snow melting in spring - Physical
Decay of leaves in winter - Chemical
Elements
Elements are pure substances that cannot be split by chemical methods into anything smaller.
92 elements occur naturally.
25 are essential for life.
Most common elements in living organisms:
65.0% Oxygen (O)
18.5% Carbon (C)
9.5% Hydrogen (H)
3.3% Nitrogen (N)
1.5% Calcium (Ca)
1.0% Phosphorus (P)
Elements are usually found chemically combined with other elements in compounds.
Each element has its own:
Name and chemical symbol
The symbols are mostly abbreviations of their English names, with a few exceptions (e.g., Na, K, Fe, Ag, Au, Hg).
Characteristic physical properties, e.g., density, electrical conductivity, melting point, and boiling point.
Characteristic chemical properties, e.g., reactions with water, oxygen, acids, and other chemicals.
The Periodic Table
In 1867, Russian scientist Dmitri Mendeleev proposed arranging the elements in order of increasing mass.
He noticed that chemical properties repeated in a regular way.
Periods: The rows in the periodic table.
Groups: The columns in the periodic table.
Diagram of the Periodic Table
[Image of the periodic table with groups and periods labeled]
Chemistry Sub-disciplines
Traditionally, chemistry has been divided into 3 or 4 sub-disciplines, but there is much overlap between them.
Inorganic Chemistry: The chemistry of metals and their salts.
Organic Chemistry: The chemistry of molecules with a carbon backbone.
Physical Chemistry: Measures the interaction of matter and energy.
Analytical Chemistry: Qualitative and quantitative observations and spectroscopy.
Structure of an Atom
Atoms are made of a central nucleus surrounded by orbiting electrons.
The nucleus is made up of a combination of protons and neutrons.
Protons are positively charged (+1).
Neutrons are uncharged.
Overall, the nucleus is positively charged.
The positive charge of the protons is balanced by the negative charge of the electrons.
Electrons are negatively charged (-1).
Number of protons = number of electrons.
Overall, the atom is neutral.
Diagram of an Atom
[Image of an atom with protons and neutrons in the nucleus and electrons orbiting the nucleus]
Relative Masses
The protons and neutrons account for essentially all the mass of an atom.
Electrons are much smaller than neutrons and protons.
Particle | Relative Mass | Relative Charge |
Proton | 1 | +1 |
Neutron | 1 | 0 |
Electron | ~0 | -1 |
Atomic Number (Z)
The atomic number defines the identity of the element.
It ascends numerically from 1 to 118.
Different for each element.
Equals the number of protons.
Since number of electrons = number of protons, it also:
Determines the number of electrons.
Determines the arrangement of electrons.
Determines how it reacts.
Determines the chemical properties.
Example:
Li 7 3
In this example, the atomic number (Z) of Lithium (Li) is 3.
Atomic Mass (Ar)
Protons and neutrons have a relative mass = 1.
Electrons have a relative mass ~ 0.
Therefore: Number of protons + Number of neutrons = Atomic mass.
Example:
Li 7 3
In this example, the atomic mass (Ar) of Lithium (Li) is 7.
Isotopes
Atomic masses are not usually whole numbers, e.g., Ar of Carbon = 12.011.
All carbon atoms have 6 protons.
Most carbon atoms have 6 neutrons: ¹²C.
A small proportion have 7, 13, or 14 neutrons: ¹¹C, ¹³C, and ¹⁴C.
These are isotopes.
The mass number is the average.
¹⁴C is a radioisotope and the basis of carbon-14 dating.
Isotopes of hydrogen have special names:
Hydrogen ¹H (0 neutrons)
Deuterium ²H (1 neutron)
Tritium ³H (2 neutrons) - unstable and radioactive.
Example:
C 12 6
In this example, the atomic mass of the most common isotope of Carbon is 12.
Chemical Properties of an Atom are Determined by its Number of Electrons
The number of electrons determines how an atom will react with other atoms.
Example:
Oxygen
Atomic Number (Z) = 8
Therefore, the number of electrons = 8
O 16 8
Number of protons + Number of neutrons = Atomic mass
Electron Shells
Electrons orbit the nucleus in shells at different distances.
The inner (1st) shell contains a maximum of 2 electrons.
Hydrogen (Z = 1) has 1 electron - 1
Helium (Z = 2) has 2 electrons - 2
Its shell is full.
So it is inert (unreactive/stable).
H
He
The second shell fills one electron at a time from Lithium (Li) to Neon (Ne).
Neon's outer shell is full, so it is inert.
The second shell contains a maximum of 8 electrons.
Li 2,1 Be 2,2 B 2,3 C 2,4 N 2,5 O 2,6 F 2,7 Ne 2,8
The third shell is stable with 8 electrons.
The third shell fills one electron at a time from Sodium (Na) to Argon (Ar).
Argon's outer shell is full, so it is inert.
Na 2,8,1 Mg 2,8,2 Al 2,8,3 Si 2,8,4 P 2,8,5 S 2,8,6 Cl 2,8,7 Ar 2,8,8
Electrons and Shells
The energy of electrons in each shell increases the further away from the nucleus they are.
Electrons always occupy the lowest energy electron shell available first.
Maximum number of electrons for each electron shell = 2n², where n = shell number.
Shell 1 = 2 x 1² = 2
Shell 2 = 2 x 2² = 8
Shell 3 = 2 x 3² = 18
Shell 4 = 2 x 4² = 32
Electron Orbitals
Electrons in a shell are further subdivided into orbitals named s, p, d, f.
Orbitals are the space in which an electron is likely to be found.
Each orbital can contain up to 2 electrons but no more.
Different orbitals have different energy levels.
Electrons fill the lowest energy level orbitals first.
Shapes of Orbitals
An orbital is a volume in which an electron is likely to exist.
Each orbital can contain up to 2 electrons.
One s orbital:
[Image of a spherical s orbital]
Three p orbitals:
[Image of three dumbbell-shaped p orbitals along the x, y, and z axes]
Five d orbitals:
[Image of five d orbitals with complex shapes]
Seven f orbitals:
[Image of seven f orbitals with even more complex shapes]
Shells and Orbitals
Shell Number | Number of Orbitals |
1 | 1s |
2 | 2s 2p |
3 | 3s 3p 3d |
4 | 4s 4p 4d 4f |
5 | 5s 5p 5d 5f |
6 | 6s 6p 6d |
7 | 7s |
Each orbital can contain a maximum of 2 electrons.
Shells & Orbitals - Some Rules
Aufbau principle:
Electrons fill orbitals in order from lowest energy to highest.
Pauli exclusion principle:
No more than 2 electrons in one orbital.
Hund's rule:
Orbitals of equal energy (degenerate orbitals) are partially filled before any orbital is completely filled.
Orbitals of equal energy are said to be degenerate.
Filling Orbitals According to the Aufbau Principle
1s
2s 2p
3s 3p 3d
4s 4p 4d 4f
5s 5p 5d 5f
6s 6p 6d
7s
4s fills before 3d
5s fills before 4d and 4f
Examples and Notation
Hydrogen H Z = 1 1s¹
Helium He Z = 2 1s²
Oxygen O Z = 8 1s² 2s² 2p⁴
Shell number | orbital | Number of electrons | Paired electrons | Electron |
1 | s | 2 | 2 | ↑↓ |
2 | s | 2 | 2 | ↑↓ |
2 | p | 4 | 2 | ↑↓ ↑ ↑ |
Example of Hund's Rule
Filling p orbitals:
Fill un paired before paired
Electronic Configuration of First 11 Elements
Element | Z | Shell Configuration | Full Configuration | Shorthand Configuration |
H | 1 | 1 | 1s¹ | 1s¹ |
He | 2 | 2 | 1s² | 1s² |
Li | 3 | 2,1 | 1s² 2s¹ | [He] 2s¹ |
Be | 4 | 2,2 | 1s² 2s² | [He] 2s² |
B | 5 | 2,3 | 1s² 2s² 2p¹ | [He] 2s² 2p¹ |
C | 6 | 2,4 | 1s² 2s² 2p² | [He] 2s² 2p² |
N | 7 | 2,5 | 1s² 2s² 2p³ | [He] 2s² 2p³ |
O | 8 | 2,6 | 1s² 2s² 2p⁴ | [He] 2s² 2p⁴ |
F | 9 | 2,7 | 1s² 2s² 2p⁵ | [He] 2s² 2p⁵ |
Ne | 10 | 2,8 | 1s² 2s² 2p⁶ | [He] 2s² 2p⁶ |
Na | 11 | 2,8,1 | 1s² 2s² 2p⁶ 3s¹ | [Ne] 3s¹ |
Shells, Orbitals, and the Periodic Table
[Image of the periodic table with the s, p, d, and f blocks labeled]
Valence Shell
The valence shell is the outermost electron shell of an atom.
Atoms react to complete their valence shell electrons.
A full valence shell = stability
For the elements we are currently considering, this involves achieving 8 electrons in a shell.
Exception: H: 2 electrons capacity of 1st shell
Octet rule: Atoms will readily gain, lose, or share electrons to have 8 electrons in their outer shell.
Valency: The number of electrons an atom needs to gain, lose, or share to complete its valence shell.
Arrangement of Electrons
Stable atoms have complete valence shells.
1st (inner) orbital (1s²): 2 electrons
2nd orbital (2s², 2p⁶): 8 electrons
3rd orbital: may contain up to 18, but 8 are stable
Inert (Noble) gases have complete valence (outer) shells.
They are stable and unreactive.
All atoms react to achieve this stability.
Stability is achieved by forming bonds:
Ionic & Covalent bonds
International System Units of Measurement
Base International System (SI) Units
kilogramme, rather than gram, is used in definitions of derived units.
Key conversion: units °C = units K.
0°C = 273.15 K.
Base Quantity | Name | Symbol |
Length | meter | m |
Mass | kilogram* | kg |
Time | second | s |
Current | ampere | A |
Temperature | kelvin | K |
Amount of substance | mole | mol |
Luminous intensity | candela | cd |
Derived Units of International System (SI)
Derived Quantity | Name | Symbol | Common Units | SI Base Units |
Angle | radian | rad | ||
Frequency | Hertz | Hz | s⁻¹ | |
Force, weight | Newton | N | kg·m·s⁻² | |
Pressure | Pascal | Pa | N·m⁻² | kg·m⁻¹·s⁻² |
Energy, work | Joule | J | N·m | kg·m²·s⁻² |
Power | Watt | W | J·s⁻¹ | kg·m²·s⁻³ |
Electric charge | coulomb | C | A·s | |
Electrical potential | volt | V | W·A⁻¹ | kg·m²·s⁻³·A⁻¹ |
Magnetic flux | Weber | Wb | V·s | kg·m²·s⁻²·A⁻¹ |
Magnetic density | Tesla | T | Wb·m⁻² | kg·s⁻²·A⁻¹ |
Radioactivity | Becquerel | Bq | s⁻¹ |
International System (SI) Prefixes
Prefix | Symbol | Factor | Decimal |
Tera | T | 10¹² | 1,000,000,000,000 |
Giga | G | 10⁹ | 1,000,000,000 |
Mega | M | 10⁶ | 1,000,000 |
Kilo | k | 10³ | 1,000 |
hecto | h | 10² | 100 |
deca | da | 10 | 10 |
10⁰ | 1 | 1 | |
deci | d | 10⁻¹ | 0.1 |
centi | c | 10⁻² | 0.01 |
Milli | m | 10⁻³ | 0.001 |
Micro | µ | 10⁻⁶ | 0.000 001 |
Nano | n | 10⁻⁹ | 0.000 000 001 |
Pico | p | 10⁻¹² | 0.000 000 000 001 |
Femto | f | 10⁻¹⁵ | 0.000 000 000 000 001 |
Litre (L)
Often abbreviated as L in US literature and text.
Metric measurement of volume of liquids.
1 Litre (L) = 10⁻³ m³
= 1 dm³
= 10³ cm³
Commonly used in the laboratory.
1 mL = 1 cm³
Density of Water
Water is at its maximum density at 4°C.
Below 4°C, water expands.
Which is why solid water is less dense than its liquid form.
And ice floats.
At 4°C, water density = 1 g/mL.
A useful approximation in most laboratory situations.
Moles and Molarity
The problem with measuring mass in grams:
Atoms of different elements have different masses.
1 atom of hydrogen has less mass than 1 atom of carbon.
1 g of hydrogen contains more atoms of hydrogen than 1 g of carbon contains atoms of carbon.
Moles (mol)
Recall Carbon:
6 protons and 6 neutrons
Mass of ¹²C = 12 atomic mass units (amu).
12 g of ¹²C contains 6.022 x 10²³ atoms.
6.022 x 10²³ is Avogadro's number (or constant).
mass of 1 mole ¹²C = 12 g exactly.
The mass of an element is:
the mass of 1 atom in amu
the mass of 1 mole atoms in grams
A mole is just a number:
Like a dozen
6.022 x 10²³ of any item is a mole.
A mole of atoms consists of 6.022 x 10²³ atoms.
A mole of molecules consists of 6.022 x 10²³ molecules.
The mass of every element may be expressed in terms of its amu, and defines the mass of a mole of that element in grams.
"Mole" is usually abbreviated to "mol".
Key equation:
Number of Moles (mol) = mass (g) / Mr (g)
Molarity (M)
The concentration of a solution is given by the amount of solute dissolved in a volume of solvent.
Molarity = Number of moles of solute per liter of solvent.
Key equations:
Molarity (M) = Number of moles / volume (L)
Molarity (M) = mass (g) / (Mr (g) x volume (L)) or mass (g) x 1000 / (Mr (g) x volume (mL))
Chemical Formulae
Empirical formula
Represents the chemical composition of a compound at a minimum.
Shows which elements are present in the compound and the relative amount of each.
Molecular formula
Indicates the numbers of each type of atom in a molecule.
They are the same as empirical formulas for molecules that only have one atom of a particular type, but otherwise, may have larger numbers.
Example: Glucose
Empirical formula: CH₂O (ratio: 1:2:1)
Molecular formula: C₆H₁₂O₆ (number of atoms 6:12:6)
Empirical and Molecular Formulae
[Image of a table with empirical and molecular formulas for various compounds]
Elemental Analysis
Elemental analysis is a process where a sample of some material is analyzed for its elemental and sometimes isotopic composition.
E.g., soil, waste, or drinking water, bodily fluids, minerals, chemical compounds.
Qualitative elemental analysis: Determines what elements are present.
Quantitative elemental analysis: Determines how much of each element is present.
Elemental analysis falls within analytical chemistry.
Uses:
To determine whether a sample is the desired compound.
To confirm its purity.
Quiz 1. Empirical and Molecular Formula
After elemental analysis, a compound was found to contain 55.81% C, 7.02% H, and 37.17% O. Determine its empirical formula.
The corresponding number of moles are:
C = 55.81 / 12.01115 = 4.646 mol
H = 7.02 / 1.00797 = 6.96 mol
O = 37.17 / 15.9994 = 2.323 mol
Divide by the smallest number:
C = 4.646 / 2.323 = 2
H = 6.96 / 2.323 = 3
O = 2.323 / 2.323 = 1
Empirical formula: C₂H₃O
Quiz 2. Empirical and Molecular Formula
Determine the percentage of Ca, C, and O in 1.785 g of a sample of calcite, containing 0.715 g Ca, 0.214 g C, and 0.856 g O.
The corresponding percentages are:
Ca = (0.715 / 1.785) x 100 = 40%
C = (0.214 / 1.785) x 100 = 12%
O = (0.856 / 1.785) x 100 = 48%
Q3. Empirical and Molecular Formula
Determine the percentage of C, H, and S in the following molecular compound C₂H₆S.
From the molecular formula, 1 molecule of C₂H₆S contains:
2 atoms of C
6 atoms of H
1 atom of S
1 mole C₂H₆S = (12.0115 × 2) + (1.007 × 6) + 32.064 = 62.134 g
Therefore:
2 moles C = (24.0223 / 62.134) × 100 = 38.662%
6 moles H = (6.0478 / 62.134) × 100 = 9.7335%
1 mole S = (32.064 / 62.134) × 100 = 51.604%
Chemical Equations
The Chemical Equation and the Information It Conveys
Chemical equation: Shorthand notation of a chemical reaction.
Describes:
All the substances that react.
All the products that form.
Physical states.
Experimental conditions.
Reactants (starting materials): The substances that undergo change in the reaction.
Products: Substances produced by the reaction.
The Experimental Basis of a Chemical Equation
A chemical equation represents a chemical change:
One or more substances are changed into new substances.
Different chemical and physical properties.
Evidence of a Reaction Occurring
Release of a gas:
E.g., CO₂ is released when acid is placed in a solution containing CO₃²⁻ ions.
Formation of a solid (precipitate):
E.g., A solution containing Ag⁺ ions mixed with a solution containing Cl⁻ ions.
Heat is produced or absorbed:
E.g., Acid and base are mixed together.
Color changes
Types of Chemical Reactions
Combination
Decomposition
Single-replacement
Double-replacement
Combination Reactions
The joining of two or more elements or compounds, producing a product of different composition.
A + B → AB
Examples of Combination Reactions:
Combination of a metal and a nonmetal to form a salt:
Na(s) + Cl₂(g) → 2NaCl(s)
Combination of hydrogen and chlorine molecules to produce hydrogen chloride:
H₂(g) + Cl₂(g) → 2HCl(g)
Formation of water from hydrogen and oxygen molecules:
2H₂(g) + O₂(g) → 2H₂O(l)
Reaction of magnesium oxide and carbon dioxide to produce magnesium carbonate:
MgO(s) + CO₂(g) → MgCO₃(s)
Decomposition Reactions
Produce two or more products from a single reactant.
Reverse of a combination reaction.
AB → A + B
Examples of Decomposition Reactions:
Heating calcium carbonate to produce calcium oxide and carbon dioxide:
CaCO₃(s) → CaO(s) + CO₂(g)
Removal of water from a hydrated material:
CuSO₄·5H₂O(s) → CuSO₄(s) + 5H₂O(g)
Single-Replacement Reactions
Single-replacement: One atom replaces another in the compound, producing a new compound.
A + BC → B + AC
Example:
Replacement of silver by copper in silver nitrate:
Cu(s) + 2AgNO₃(aq) → 2Ag(s) + Cu(NO₃)₂(aq)
Double-Replacement Reactions
Two compounds undergo a "change of partners".
Two compounds react by exchanging atoms to produce two new compounds.
AB + CD → AD + CB
Example:
Formation of solid lead chloride from lead nitrate and sodium chloride:
Pb(NO₃)₂(aq) + 2NaCl(aq) → PbCl₂(s) + 2NaNO₃(aq)