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Comprehensive study notes for high school chemistry, covering key concepts such as the properties and structure of matter, quantitative chemistry, reactive chemistry, and drivers of reactions. It includes definitions, explanations, examples, and practical applications, making it a valuable resource for students preparing for exams or deepening their understanding of the subject.
Typology: Cheat Sheet
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Green: Subheading/title (heading 3) Bold: definition/sub subheading/significant word Blue: syllabus points (title) Normal: content
Molecule: An element or compound containing non-metal atoms covalently bonded
Ion: Charged atom, pos - cation , neg - anion
Covalent bond: ‘Sharing’ of electron(s) between two non-metal atoms Ionic bond: ‘Sharing’ of electron(s) between a metal and a non-metal
Validity: variables; reliability; accuracy; if the experiment tested the aim; good method Accuracy: correct use of equipment; correct calibration of equipment Reliability: repetition; consistent results
Independent variable: What you are changing; x Dependent variable: What you are measuring; dependent on x; f(x) or y Aim: What you aim to achieve/figure out in the experiment Hypothesis: What you predict; ‘If _____ then ____ Method: Numbered steps on how to conduct the experiment Conclusion: What did you infer from the results Discussion: The significance of your findings; what could you have changed Graph: line/curve of best fit; numbered; title on the side; title; independent on the x axis; points plotted with crosses
Law of conservation of mass: Matter cannot be created nor destroyed only changed; mass of the reactants must balance the mass of the products.
Alloy: Mixture predominantly metal with other substances, e.g. bronze or rose gold
Polyatomic Ions
Polyatomic ion (radical) IUPAC Name Charge
SO 3 2-^ sulfite ion -
SO 4 2-^ sulfate ion -
NO 3 2-^ nitrite ion -
CO 3 2-^ carbonate ion -
PO 4 3-^ phosphate ion -
NH 4 +^ ammonium ion +
● explore homogeneous mixtures and heterogeneous mixtures through practical investigations:
Separation Techniques
Decantation: Separation of mixtures based on density, for heterogeneous and immiscible mixtures composed in layers. Physically pouring the less dense layer off the top of the mixture.
Separating funnel: Separating mixtures based on density, for heterogeneous, immiscible mixtures. Immiscible mixture goes in the separating funnel and the denser substance is separated out.
Centrifuge: Separating mixtures based on density. The use of centrifugal force forces the denser substance to the end of the tube being able to be decanted off after.
Magnetic separation: Based on the physical property of magnetism, using a magnet to separate the magnetic substance from the one that is not.
Evaporation/Crystallisation: Separation based on evaporation point in a mixture, could be immiscible or miscible mixtures. Evaporation allows for the solute to evaporate in a natural environment from the solute and is slower. Crystallisation is the direct application of heat to drive off the solvent.
Filter Funnel: Separation based on particle size of a mixture, could be suspension. Insoluble particles in a substance are trapped by the filter paper leaving the liquid in the beaker.
Distillation: Separation based on boiling points. Two miscible substances with different boiling points are heated up and the substance with the lower boiling point evaporates and is collected. If there are multiple substances or with very close boiling points, use fractional distillation.
Paper Chromatography: Separation based on solubility. Tests if a reaction has occurred if the two substances create a new dot in a new position, if still two dots then reaction did not occur. Also tests purity of a substance.
Sieve: Separation due to particle size.
Properties ● classify the elements based on their properties and position in the periodic table through their:
Metal properties:
Naming Substances ● investigate the nomenclature of inorganic substances using International Union of Pure and Applied Chemistry (IUPAC) naming conventions
If a compound contains a cation : the cation will be first, then the anion with the suffix ‘ide’ Cations : keep their name Anions : end in ide If a compound contains oxygen : the compound will end in ate or ite Two oxygen atoms : end in ‘ate’ Three oxygen atoms : end in ‘ite’
For Ionic compounds:
Valency
Valence shell: The outermost shell of the atom, containing valence electrons that usually dictate the reactivity of the atom
Valency: The ability of an atom to combine with other elements or combinations of elements (polyatomics)
Number of valence electrons: Increases left to right across the periodic table
History ● examining spectral evidence for the Bohr model and introducing the Schrödinger model Bohr: Created the Bohr model of the atom in 1913 with distinct electron shells. One of the limitations of Bohr’s model was that electrons with the same energy were in the same shell
Schrödhinger: Created the most recent atomic model in 1926 where the electrons exist in energy waves and their locations are based on averages where they most likely will be, also SPDF. Also called electron cloud model
Structure of the Atom ● investigate the basic structure of stable and unstable isotopes by examining:
Structure: Protons and neutrons tightly packed together in the nucleus, protons have a positive charge and usually repel each other but nuclear force compacts them. Electrons are on the outside of the nucleus in orbitals, held together by electrostatic forces of attraction, the positive protons attract the negative electrons.
● model the atom’s discrete energy levels, including electronic configuration and spdf notation Orbitals: S, P, D and F orbitals, can be used in SPDF notation to describe which shells fill up and how many electrons an atom has
Isotopes
Isotope: Atoms of an element that have a differing number of neutrons in the nucleus. Have the same atomic number but different mass numbers. Have identical or very similar properties to their other isotopes. Relative abundance (atomic mass) is the average of all isotopes mass in nature
● calculate the relative atomic mass from isotopic composition Calculating the relative atomic mass: Adding the number of protons to the number of neutrons for the specific isotope of the element you're considering. For example, a carbon-12 atom has 6 protons and 6 neutrons, and so has a relative atomic mass of 12.
Calculating relative abundance: sum of (percentage abundance x isotope mass number) / 100 (or sum of all isotopes)
Radioisotopes
Radioisotope: When a nuclei has an unstable number of neutrons they will emit radiation ● investigate the properties of unstable isotopes using natural and human-made radioisotopes as examples, including but not limited to:
Why are some isotopes radioactive: They may be too large, (the mass attractions overcome the electrostatic forces making it unstable). Or if their ratio from protons to neutrons is too high
Flame Tests ● investigate energy levels in atoms and ions through:
Heating of an atom: When an atom is heated electrons jump up an energy level, then jump back down as that is unstable but due to the law of conservation of mass they emit a photon of light specific to the atom when jumping back down.
To identify atom: because each atom emits a specific colour
Light emission spectra: When the light the atoms create passes through a prism, it produced a number of coloured lines, related to the electronic structure within atoms
Shielding Effect
The attractive force of the nucleus on the outermost electrons is lessened by the shielding of the force from other closer orbiting electrons
Trends ● demonstrate, explain and predict the relationships in the observable trends in the physical and chemical properties of elements in periods and groups in the periodic table, including but not limited to:
Electronegativity: The ability of an atom to attract electrons Ionisation energy: The energy required to remove electrons from the outermost shell of an atom
Atomic radius: increases top to bottom (each period adds an orbital) and decreases left to right (because as the atomic number increases so does the attractive nucleus force pulling the atom together)
Melting point: Metals and metalloids generally have higher melting points (as metals have high intermolecular forces making it harder for heat to separate them into a liquid)
Electronegativity: Increases across a period as the atoms have a higher charge and a smaller radius increasing their force of attraction
Ionisation energy: Increases as it is harder to remove an electron across a period, making the energy required far higher as well
Group 1: Highly reactive with water as they only have 1 electron in the valence shell so when they move that electron all the energy goes into that electron creating a highly reactive reaction. More reactive as you move down
Group 2: react with water but less vigorously than group 1
Group 8: Noble gases, are unreactive as full valence shell, also have a high ionisation energy
Covalent Bonding
Types of Bonding ● explore the similarities and differences between the nature of intermolecular and intramolecular bonds and the strength of the forces associated with each, in order to explain the:
Dispersion force : Temporary dipoles, exist in all molecules but are so weak that they are irrelevant when there are other forces active Dipole - dipole : Formed when molecules have atoms with different electronegativity, stronger than dispersion, for example HCl, more elections would sit around the Cl atom rather than the H, making it more electronegative. Therefore the Cl pole is more negative, and the H is more positively charged
Hydrogen bonding : A special case of dipole-dipole, only looks at molecules that have the most electronegative atoms in them, N, O or F, e.g. H2O, ammonia or HFNH
Shape of Molecules
Turn out different because electrons repel each other
Formula BeCl 2 BCl 3 CH 4 NH 3 H 2 O
Name of molecule
Beryllium Chloride
Boron trichloride
Methane Ammon ia Water
Bonding Pairs
Valence Electrons
Lone Pairs 0 0 0 1 2
Angles between bonding pairs
Name of shape
Linear Trigonal Planar
Tetrahedral Triagonal Pyramid
Bent
Image
Intermolecular forces
Allotropy ● Made up of the same element with different 3D structure. The arrangement of the atoms ○ Covalent bonding, hence covalent network lattices
Writing chemical equations (types of chemical reactions assumed knowledge) Balancing chemical equations Conservation of mass Mole concept and related calculations Concentration and Molarity Gas Laws
Chemical Reactions & Stoichiometry ● conduct practical investigations to observe and measure the quantitative relationships of chemical reactions, including but not limited to:
Stoichiometry : quantities and ratios of chemical species in a chemical reaction, enabling us to predict the yield of products, whether a reactant is limiting or in excess
Yield: amount produced
Limiting reagent:
Aqueous (aq): dissolved in water
Writing Chemical Reactions:
How to conduct stoichiometry:
Excess reactant: When there is too much reactant in a chemical reaction
Mass-Volume Stoichiometry:
Mole Concept ● conduct a practical investigation to demonstrate and calculate the molar mass (mass of one mole) of:
Avogadro’s Number (Avogadro’s Constant):
Relative Atomic Mass: All atomic weights are relative to mass of carbon-
Molecular mass: The mass of a molecule that is the sum of all the masses of all the atoms contained in the molecule
Mole set mass:
n (moles, mol) =
number of molecules/atoms
Avogadro’s number
Calculations Using Moles C 6 H 12 O 6 = molecular formula CH 2 O = empirical formula → the lowest ratio To find mass of unknown:
Chemical concentrations are expressed in terms of molarity (symbol C ) which expresses the number of atoms, ions or molecules in a certain volume rather than simply the mass per volume.
UNIT DESCRIPTION EXAMPLE OF USE
gL-^
Mass of solute, in g, per litre of solution A bottle of bleach gives the concentration of sodium, hypochlorite as 56gL-
mgL-^
Mass of solute, in mg, per litre of solution Sydney’s water supply has calcium ion concentration typically around 5-10mgL-
molL-^
Moles per litre of solution Hydrochloric acid used in analysis in a laboratory is labelled as 1. mol L-
%(w/w) Percentage by mass; describes the mass of solutes, in g, per 100g of solution
A bottle of hydrogen peroxide is labelled 10%(w/w)
%(w/v) Percentage mass by volume; describes the mass of solute in g, per 100mL solution
Saline drips are a solution of 0.9%(w/v) sodium chloride
%(v/v) Percentage by volume; describes the volume of solute in mL, per 100mL solution
Alcohol content of wine might be 13.5% v/v
ppm Parts per million, e.g. mass, in g, per million equivalent to mg kg-1, or mgL-
The legal limit of mercury, for safe human consumption is 0.5ppm for most species of Australian fish
Ppb Parts per billion, e.g. mass in g, per billion equivalent to μgkg-1, or μgL-
The world Health organisations guideline value for a safe level of arsenic in drinking water is 10ppb
Dilution
Pressure
Boyle’s Law
- (Temperature is constant)
Charles’s Law
- (Pressure is constant)
Gay Lussac’s Law
- (Volume is constant)
Combined Gas Law!
- P 1 V 1 /T 1 = P 2 V 2 /T 2