• Shuffle
    Toggle On
    Toggle Off
  • Alphabetize
    Toggle On
    Toggle Off
  • Front First
    Toggle On
    Toggle Off
  • Both Sides
    Toggle On
    Toggle Off
  • Read
    Toggle On
    Toggle Off
Reading...
Front

Card Range To Study

through

image

Play button

image

Play button

image

Progress

1/143

Click to flip

Use LEFT and RIGHT arrow keys to navigate between flashcards;

Use UP and DOWN arrow keys to flip the card;

H to show hint;

A reads text to speech;

143 Cards in this Set

  • Front
  • Back
  • 3rd side (hint)

Mass Number

Total number of protons and neutrons in the nucleus of an atom.

Atomic Number

Number of protons in the nucleus of an atom.

Ions

Ions have different number of protons and electrons.

Isotopes

Isotopes of an element are atoms with the same number of protons but a different number of neutrons.

Bohr's model

Electrons exist in shells, each shell has a fixed energy. When an electron moves between shells electromagnetic radiation is emitted or absorbed.

Relative Atomic Mass

The average weighted mass of an atom of an element compared to 1/12th of an atom of carbon-12.

Relative Isotopic Mass

The average weighted mass of an isotope of an element compared to 1/12th of an atom of carbon-12.

Relative molecular mass

The average weighted mass of a molecule compared to 1/12th of an atom of carbon-12.

Relative Formula Mass

The average mass of a formula unit, compared to 1/12th of an atom of carbon-12.

Mole (definition)

Amount of substance or 6.02x10^23 particles (the Avogadro constant)

Moles of a substance (calculation)

Mass of a substance / Molar mass

Moles (from the number of atoms or molecules)

Number of particles / number of particles in a mole (6.02x10^23)

Molar mass

The mass of one mole of something.

Moles of a gas

Volume in dm3 (cm3) / 24 (000)

Ideal gas equation

pV = nRT

Moles of a solution

(Concentration x Volume) / 1000

Empirical def.

The smallest whole number ratio of atoms of each element in a compound.

Molecular Formula

The actual number of atoms of each element in a molecule

How do you find the molecular formula from the empirical formula?

1.) Find the empirical mass


2.) Divide molecular mass by the empirical mass


3.) Multiply empirical formula by that number

Reaction Stoichiometry

The ratios of reactants to products

Nitrates molecular ion

Carbonates molecular ion

Sulfates molecular ion

Hydroxide molecular ion

Ammonium molecular ion

Hydrochloric acid

Sulfuric acid

Nitric acid

Sodium Hydroxide

Potassium Hydroxide

Ammonia

Strong acids

Very little reverse reaction, nearly all the acid dissociates (ionise)

Acid + Base

Salt + Water

Metal + Acid

Salt + Hydrogen

Metal Oxide + Acid

Salt + Water

Metal Hydroxide + Acid

Salt + Water

Metal Carbonate + Acid

Salt + Water + Carbon Dioxide

Hydrated salts

A solid salt containing water of crystallisation

Anhydrous salts

A salt that doesn't contain water of crystallisation

How do you find the formulas of hydrated salts?

1.). Mass of anhydrous salt - mass of hydrated salt = mass of water


2.) Mass of water/18 = Moles of water


3.) Mass of anhydrous/Mr of anhydrous = Moles of anhydrous


4.) Divide both mole numbers by moles of anhydrous

Methyl Orange

Yellow to red when adding acid to alkali

Phenophalein

Pink to colourless when adding acid to alkali

How do you prepare a standard solution?

1.) Weigh out solid


2.) Transfer to a beaker, washing with distilled water


3.) Add water until completely dissolved.


4.) Transfer to volumetric flask, washing rod and beaker with distilled water


5.) Fill volumetric flask until bottom of meniscus reaches graduation line (use a pipette to add the last few drops)

Percentage Yield =

(Actual yield/theoretical yield) x 100

% Atom Economy =

Mr of desired product/Mr of total products

Addition reaction

The reactants combine to form a single product.


A + B -> AB

Substitution Reaction

Atoms from one reactant are swapped with atoms from another reactant.


AB + CD -> AD + CB

Advantages of high atoms economy in industry

Less waste - costs less


Oxidation Rules

1.) Unconfined element = 0


2.) Ions have the same oxidation number as their charge


3.) Oxygen is always 2- unless told to work it out


4.) Hydrogen is always 1+ unless in a metal hydride where it is 1-

Oxidising agents

Accept electrons and gets reduced

Reducing agents

Donates electrons and get oxidised

Redox reaction

Reduction and oxidation happen simultaneously

Shape of an s-orbital

Spherical

Shape of a p-orbital

Dumbbell

Maximum electrons in an s-subshell

2

Maximum electrons in a p sub shell

6

Maximum electrons in a d sub shell

10

Maximum electrons in an f sub shell

14

Maximum electrons the 1st shell

2

Maximum electrons the 2nd shell

8

Maximum electrons the 3rd shell

18

Maximum electrons the 4th shell

32

Ionic Bonding

The electrostatic attraction between oppositely charge ions. Ionic crystals form a giant ionic lattice.

Properties of ionic compounds

Conduct electricity when molten or aqueous because the ions are free to move.


Doesn't conduct when solid because ions are fixed in place.


High melting and boiling point due to strong electrostatic forces that require a lot of energy to break.


Ionic compounds are soluble

Covalent Bonding

Shared pair of electrons

Dative Covalent Bonding

One atom provides both of the shared electrons

Electron Repulsion

Lone pairs of electrons repel more than bonding pairs of electrons

Tetrahedral

Bonding pairs 4


Lone pairs 0


Bond angle 109.5°


Example CH4

Linear

Bonding pairs 2Lone pairs 0Bond angle 18Example BeCl 2

Non-linear

Bonding pairs 2Lone pairs 2Bond angle 104.5°Example H2O

Trigonal Planar

Bonding pairs 3Lone pairs 0Bond angle 120°Example BeF3

Trigonal Pyramidal

Bonding pairs 3Lone pairs 1Bond angle 107°Example NH3

Trigonal Bipyramidal

Bonding pairs 5Lone pairs 0Bond angle 120° and 90°Example PCl 5

Octahedral

Bonding pairs 6Lone pairs 0Bond angle 90°Example SF6

Electronegativity

The ability of an atom to attract the bonding electrons in a covalent bond

Non - Polar bonds

Atoms have equal electronegativity

Polar Bond

Atoms have different electronegativity

Polar molecule

Asymmetrical

Non polar molecule

Symmetrical

Permanent dipole-dipole interaction

The slightly - and slightly + charges on a polar molecule cause weak electrostatic attraction between molecules

Induced Dipole-Dipole Interactions

An uneven distribution of electrons in the electron charge cloud causes a temporary dipole which induces another temporary dipole in a neighbouring molecule - domino effect

Hydrogen Bonding

Only occurs when hydrogen is bonded to oxygen, nitrogen or fluorine. A weak bond from between the H on one molecule and the lone pair on another molecule

Properties of simple covalent compounds

Low melting and boiling point due to weak intermolecular forces, do not conduct electricity and are insoluble.


Molecule containing H-bonding have a significantly high boiling point

First Ionisation Energy

The energy needed to remove 1 mole of electrons from 1 mole of gaseous atoms

Factors affecting ionisation energy

1.) Nuclear charge - the more protons, the more positive the charge, the stronger the attraction.


2.) Atomic Radius - An electron close to the nuclear is more attracted than one further away.


3.) Shielding - more electrons between the out electron and the nucleus, the less attraction

Trends in ionisation energy down a group

Generally fall due to extra shell, so the atomic radius increases and reduces attraction

Trends in ionisation energy across a period

Ionisation energy generally increases because there are more protons, so a higher nuclear charge and a smaller atomic radius.

Drop in ionisation energy between Group 2 and 3

caused by outer electron in group 3 being in a p orbital rather than an s orbital.

Drop in ionisation energy between Group 5 and 6

Due to electron repulsion

Successive Ionisation Energy

The energy need to remove 1 mole of electrons from 1 mole of gaseous ions

Trends in Successive Ionisation Energy

Successive ionisation energy increases due to electrons being remove from an increasingly positive ion - less repulsion between remaining electrons.


There is a big jump when a new shell is broken into.

Graphite

Carbon atoms arranged in sheets bonded to 3 other carbons and a delocalised electron. Sheets held together by induced dipole-dipole forces.


Properties: can conduct electricity, a good lubricant, low density, high melting point, insoluble.

Diamond

Carbon atoms bonded to 4 other carbons, tetrahedral shape.


Properties: very high melting point, extremely hard, good thermal conduct, insoluble.


Silicon

Forms a crystal lattice structure like diamond with similar properties.

Graphene

One layer of graphite, a two-dimensional shape, good electrical conductor, extremely strong,incredibly light.


Used in high speed electronics and aircraft technology.

Metallic Bonding

The electrostatic attraction between positive metal cations and delocalised electrons.

Properties of metals

High melting point due to strong electrostatic attraction. Malleable. Good electrical conductor. Insoluble.

Group 2

Reactivity decreases down the group because there is less shielding and a small atomic radius so it is hard to lose the outer electrons. Used to neutralize acidic soil and excess stomach acid.

Colour and state of Fluorine

Pale yellow gas

Colour and state of Chlorine

Green gas

Colour and state of Bromine

Red-brown liquid

Colour and state of iodine

Grey solid

Group 7 Reactivity

Reactivity decreases down the group because there is more electron shielding and a bigger atomic radius so there is less nuclear attraction.


Melting and boiling point increase down the group.


Volatility decreases down the group.

Group 7 displacement

Fluorine displaces Chlorine.


Chlorine displaces Bromine.


Bromine displaces Iodine.

Chlorine water

Colourless

Bromine water

Orange

Iodine water

Brown

Bromine water and potassium iodide

Solution goes orange to brown

Chlorine water and potassium bromide

Solution goes from colourless to orange

Addition of hexane to halogens

Violet/pink - iodine


Orange/red - bromine


Pale yellow/green - chlorine

Test for Halides

Add silver nitrate and a few drops of dilute nitric acid.


Chlorine - white precipitate, dissolves in dilute ammonia


Bromine - cream precipitate, dissolves in concentrated ammonia


Iodine - yellow precipitate, doesn't dissolve in concentration or dilute ammonia.

Disproportionation reactions

A single element is simultaneously reduced and oxidised

Bleach

Chlorine gas reacts with aqueous sodium hydroxide to form chloric acid (bleach) and water

Enthalpy Change

The heat energy transferred in a reaction at constant pressure

Standard conditions

100kPa and 298°K (25℃)

Standard Enthalpy change of reaction

The enthalpy change when a reaction occurs in the molar quantities under standard conditions

Standard enthalpy change of formation

The enthalpy change when one mole of a compound is formed from its elements in their standard states, under standard conditions

Standard enthalpy change of combustion

The enthalpy change when one mole of a substance is completely burned in oxygen under standard conditions

Standard enthalpy change of neutralisation

The enthalpy change when solutions of an acid and an alkali react to form one mole of water under standard conditions

Exothermic reactions

Give out energy to their surroundings - products have less energy than reactants. Will have a negative enthalpy change of reaction.

Endothermic reactions

Take in energy from surroundings - products have more energy than reactants. Enthalpy change is positive.

Activation energy

The minimum amount of energy needed to begin breaking reactant bonds and start a chemical reaction.

Bond dissociation energy

The amount of energy you needed per mole to break the attraction in a bond

Bond breaking

Exothermic

Bond making

Endothermic

Enthalpy change of reaction =

Total energy absorbed - total energy released

Equation for enthalpy change

q = mc🔺T

Calculating standard enthalpy change of combustion

1.) q = mc🔺T


2.) n = mass / mr


3.) 🔺c H = q / n

Calculating standard enthalpy change of reaction

1.) q = mc🔺T


2.) n = mass / Mr


3.) 🔺r H = q / n ( x number of moles reacting in a balanced equation)

Hess's Law

The total enthalpy change of a reaction is always the same, no matter which route is taken.

Collision theory

A reaction won't take place unless two particles collide with the minimum amount of Kinect energy needed.

Enthalpy Profile Diagram

Boltzmann distributions

The effect of temperature on rate of reaction

Increased temperature mean molecules have more kinetic energy so more molecule will have at least the activation energy.

The effect of concentration on rate of reaction

Increased concentration means more molecules in a given volume so a higher chance of collisions

Catalyst

Increase the rate of reaction by lowering the activation energy

Heterogeneous catalyst

In a different phase from the reactants.


Example - Haber Process uses a solid iron catalyst


Homogeneous catalyst

In the same physical state as the reactants

Catalytic converters

Reduce the pollution released into the atmosphere by speeding up the reaction 2CO + 2NO --> 2CO2 + N2

Rate of reaction =

Amount of reactants used or products formed / time

Dynamic Equilibrium

Where the forward and backward reaction occur at the same rate

Le Chatelier Principal

If there is a change in concentration, pressure or temperature the equilibrium will move to help counteract the change.

Equilibrium: change in concentration

Increase the concentration of reactants, equilibrium shift right to make more product.