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Chemistry-124-Weekly-Summaries-1

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Week 1
Lecture 1 - Introduction to chemistry
MACROSCOPIC VS SUBMICROSCOPIC
2KI (aq) + Pb(NO3)2 (aq)  2KNO3 (aq) + PbI2 (s)
-
Pb2+ (aq) and I- (aq) combine to form ppt (yellow)
Ppt is insoluble in water
PbI2 is ionic – forms a 3D structure
CLASSIFYING MATTER
-
-
Physical State:
 Gas
 Solid
 Liquid
Composition:
 Element
 Compound
 Mixture
PHYSICAL STATES OF MATTER
-
Gas, liquid and solid
Can also exist in supercritical state between gas and liquid
Mobility of atoms decreases from Gas>Liquid>Ice
Density usually decreases from Solid>Liquid>Gas (Ice has Lower density than water because
of arrangement)
COMPOSITION OF MATTER
-
Substance = matter of uniform composition throughout sample
Substance divided into two categories:
 Element – Atoms or molecules consisting of one kind of atom
 Compounds – molecules consisting of two pr more different kinds of atoms
MIXTURES
-
Two or more substances together
Exhibit properties of the substances that comprise it
Either:
Heterogeneous – variation in composition throughout sample
Homogeneous (also called solution) – constant composition throughout sample
CLASSIFICATION OF MATTER – BASED ON COMPOSITION
DIFFERENT PROPERTIES OF MATTER
PROPERTY
Physical
Chemical
Intensive
Extensive
DESCRIPTION
Observed w/out changing a
substance into another
substance
When a substance is changed
into another substance
Independent of amount of
substance that is present –
important when identifying a
substance
Depend on amount of
substance present
EXAMPLE(S)
Colour, odour, density, melting
point, boiling point and
hardness
Flammability
Density, boiling point or colour
Mass, volume or energy
SEPARATION OF MIXTURES – METHODS
-
Filtration:


Separation of solid and liquid
Solid filtered out of liquid
-
Distillation:
 Separates liquid from liquid
 Uses different boiling point of substances
 Boils solution to vaporize substance 1
 Substance 1 then condenses and collects in receiving flask
 After substance 1 is boiled then only substance 2 remains in flask
-
Chromatography:
 Mixture dissolved in the solvent
 Solvent is added throughout the process
 Components separate
 Each component is collected as it reaches bottom of the chromatography column
Lecture 2 – Introduction to Chemistry
SI BASE UNITS USED:
-
Length = Meter (m)
Mass = Kilogram (Kg)
Temperature = Kelvin (K)
Time = Second (s)
Amount of Substance = Mole (mol)
Electric Current = Ampere (A)
Luminous Intensity = Candela (cd)
METRIC SYSTEM PREFIXES:
PREFIX
GigaMegaKiloDeciCentiMilliMicroNanoPicoFemto-
ABBREVIATION
G
M
k
d
c
m
µ
n
p
f
TEMPERATURE
-
Celsius scale – based on properties of water
 0ᵒC = freezing point of water
 100ᵒC = boiling point of water
MEANING
109 – billion
106 – million
103 – thousand
10-1 – one tenth
10-2 – one hundredth
10-3 – one thousandth
10-6 – one millionth
10-9 – one billionth
10-12
10-15
-
-
Kelvin scale – based on properties of gases
 No negative temperatures
 Lowest possible temperature = absolute zero (0 K)
ᵒC + 273 = K
TOOLS TO MEASURE VOLUMES OF LIQUID
-
-
Deliver variable volumes:
 Graduated cylinder
 Syringe
 Burette
Deliver specific volume
 Pipette
Hold a specific volume:
 Volumetric flask
Volume (m3) is not an SI unit because it is derived from length
LENGTH, VOLUME AND MASS
-
Litre (L) = cube 1dm long on each side (dm 3)
Millilitre (mL) = cube 1cm long on each side (cm 3)
Microlitre (µL) = cube 1mm long on each side (mm3)
1L = 1000cm3
1kg = 1000g
1g = 1000mg
DENSITY
-
Density = mass per unit volume (g/cm3)
Densities of select substances @25ᵒC
SUBSTANCE
Air
Balsa wood
Ethanol
Water
Ethylene glycol
Table sugar
Table salt
Iron
Mercury
Gold
Osmium
DENSITY (G/CM3)
0.001
0.16
0.79
1.00
1.09
1.59
2.16
7.87
13.53
19.32
22.59
UNCERTAINTY IN MEASUREMENTS
-
Different measuring devices = different uses and degrees of accuracy
All
-
measured numbers have some degree of inaccuracy
Last digit measured is considered reliable but not exact (e.g. 28.88mL)
PRECISION AND ACCURACY
EXPERIMENTAL ERROR
Error∈measurement =Experimentally determined value−accepted value
Percentage error=
Error∈ Measurement
X 100 %
Accepted Value
DETERMINATE VS INDETERMINATE ERRORS
Sume of the Squares of the Deviations for each Measuremnet
√ ¿ the Avereage
Standard Deviation=
¿
One Less thanthe Number of Measurements
SIGNIFICANT FIGURES – THE ROLE OF ZEROS
SIGNIFICANT FIGURES – IN CALCULATIONS
-
Rule 1 – when adding or subtracting, the number of decimal places in answer is equal to the
number of decimal places in number with fewest digits after decimal point
Rule 2 – in multiplication or division, the number of sig.fig in answer is determined by
quantity with fewest sig.fig
Rule 3 – number rounded off, last digit to be retained is increased by one only if following
digit 5 or greater
Lecture 3 – Introduction to Chemistry
ATOMIC STRUCTURE
Particle
Charge
Proton
1+
Neutron
Neutral
Electron
1- Unified atomic mass unit (u): 1.66054 x 10 -24 g
- Electron charge = -1.6022 x 10-19C
ATOMIC MASS
-
Carbon – standard
Mass (amu)
1.0073
1.0087
5.486 x 10-4
-
12
C mass = exactly 12u
1u = 1.66054 x 10-24 g
Hydrogen was standard with mass of 1
Different isotopes of carbon are taken into account – leads to average atomic mass of 12.01u
MASS NUMBERS
-
Mass number = protons + neutrons
Atomic number = protons or electrons
23
11Na – 11e, 11p and 12n (12n = 23-11)
ISOTOPES
-
Atoms of same
element with different
masses, due to them
having different numbers of neutrons but the same number of protons
AVERAGE ATOMIC WEIGHT
Atomic Weight=
Isotope 1
% Abundance Isotope 2
( Mass of Isotope 1 )+(
)(Mass of Isotope 2)
(% Abundance
)
100
100
AVERAGE ATOMIC WEIGHT MEASUREMENT
-
Spectrometer measures atomic and molecular weights
As well as % abundancies of different isotopes
PERIODIC TABLE OF ELEMENTS
-
Systematic organization of elements
-
Arranged in order of atomic number
Periods – Horizontal rows
Elements – order of increasing atomic number
Groups – vertical columns (elements with similar properties)
Non-metals and metals – divided by steplike line
19 – Atomic Number
K – Atomic Symbol
39.0983 – Atomic Weight
-
Repeating pattern of properties and reactivity:
Element  nonreactive gas  soft reactive metal  element  etc.
SOME GROUPS IN PERIODIC TABLE
GROUP
1
2
16
17
18
IONS AND IONIC COMPOUNDS
NAME
Alkali Metals
Alkaline Earth Metals
Chalcogens
Halogens
Noble Gases
ELEMENTS
Li, Na, k, Rb, Cs, Fr
Be, Mg, Ca, Sr, Ba, Ra
O, S, Se, Te, Po
F, Cl, Br, I, At
He, Ne, Ar, Kr, Xe, Rn
COMMON CATIONS
COMMON ANIONS
IONIC COMPOUNDS
-
Charge on cation becomes subscript on anion
Charge of anion becomes subscript on cation
If these subscripts are not in lowest whole number ratio – divide them by greatest common
factor
MOLECULES AND MOLECULAR COMPOUNDS
CHEMICAL FORMULAS
-
Molecular – structure
E.g. H2O2
-
Empirical – simplest form
E.g. HO
Week 2 – Lectures and Slides
Lecture 4 – Introduction to Chemistry
NOMENCLATURE – IONIC COMPOUNDS
NAMES OF CATIONS
-
-
-
Cations of metal – same name as metal
 Na+ = Sodium ion
 Zn2+ = Zinc ion
 Al3+ = aluminium ion
Transition metals can form cations with different charges
 Roman numerals indicate charges
 Exception = Ag+ and Zn2+
 Cu+ = copper (I) ion and Cu2+ = copper (II) ion
 Co2+ = cobalt (II) ion and Co3+ = cobalt (III) ion
Cations of Non-metals – names end in —ium
 NH4+ = ammonium ion
 H3O+ = hydronium ion
NAMES OF ANIONS
-
-
-
-
-
Monoatomic anions: Replace end of name with –ide
 H- = hydride ion
 O2- = oxide ion
 N3- = nitride ion
Few simple polyatomic anions also end in –ide
 OH- = hydroxide ion
 CN- = cyanide ion
 N3- = azide ion
 O22- = peroxide ion
Oxyanions – end in –ate or –ite (–ite oxyanion has same charge as –ate, but one less oxygen)
 NO3- = nitrate ion and NO2- = nitrite ion
 SO42- = sulfate ion and SO32- = sulphite ion
 ClO3- = chlorate ion and ClO2- = chlorite ion
Note when to use prefixes per—and hypo—
 ClO4- = perchlorate ion
 ClO3- = chlorate ion
 ClO2- = chlorite ion
 ClO- = hypochlorite ion
Oxyanions with H+ - add prefix hydrogen or dihydrogen
 PO43- = phosphate ion
 HPO32- = hydrogen phosphate ion
 H2PO2- = dihydrogen phosphate ion
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NAMES AND FORMULAE OF IONIC COMPOUNDS
Ionic Compound
CaBr2
NaHSO4
Mg(OH)2
TiCl2
Co2O3
FeO
Fe2O3
Ions Involved
Ca2+ and 2 BrNa+ and HSO4Mg2+ and 2 OHTi2+ and 2 Cl2 Co3+ and 3 O2Fe2+ and O22 Fe3+ and 3 O2-
Name
Calcium Bromide
Sodium Hydrogen Sulfate
Magnesium Hydroxide
Titanium(II) Chloride
Cobalt(III) Oxide
Iron(II) Oxide
Iron(III) Oxide
ACID NOMENCLATURE
NOMENCLATURE – MOLECULAR COMPOUNDS
-
-
Name of element farther to the left in periodic table or lower in same group – written first
Prefix used to denote number of atoms of each element in the compound (mono- not used
on first element listed)
Ending of second element = —ide
 CO2 = carbon dioxide
 CCl4 = carbon tetrachloride
If prefix ends with a or o and name of element begins with vowel – two successive vowels
often elided into one
 N2O5 = dinitrogen pentoxide
 CO = carbon monoxide
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Lecture 1 – Stoichiometry
BALANCING CHEMICAL EQUATIONS
-
CH4 (g) + O2 (g)  CO2 (g) + H2O (g)
Balanced version = CH4 (g) + 2O2 (g)  CO2 (g) + 2H2O (g)
LHS = 1C, 4H, 4O & RHS = 1C, 4H, 4O
TYPES OF REACTIONS ACCORDING TO CHEMICAL REACTIVITY
-
Combination – Reactants combined to form one product
A + B  AB
-
Decomposition – Reactant is split into two or more products
AB  A + B
-
Combustion – Reactant reacts with oxygen
A + O2  CO2 + H2O
COMBINATION
2Mg (s) + O2 (g)  2MgO (s)
-
Ribbon of Mg metal surrounded by oxygen gas in the air
Intense white flame produced as Mg atoms react with O 2
Reaction forms MgO (white, ionic solid)
DECOMPOSITION
-
Inflation of car air bags:
2NaN3 (s)  2Na (s) + 3N2 (g)
-
Production of Lime:
CaCO3 (s)  CaO (s) + CO2 (g)
COMBUSTION
-
O2 from air is used as a reactant
CH4 (g) + 2O2 (g)  CO2 (g) + 2H2O (g)
C3H8 (g) + 5O2 (g)  3CO2 (g) + 4H2O (g)
FORMULA AND MOLECULAR WEIGHT
-
Formula Weight = sum of atomic weights for atoms in chemical formula
E.g. for Na the formula weight is the atomic weight (23.0 u)
If substance is a molecule – formula weight also called molecular weight
Molecular Weight = sum of atomic weights of atoms in a molecule
E.g. for C6H12O6 (glucose) the molecular weight is 180.0 u
PERCENTAGE COMPOSITION OF A COMPOUND
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% Element =
-
( Number of atoms)( Atomic weight)
x 100
Formula weight of compound
Example:
% C ∈C 6 H 12 O6=
( 6 ) ( 12.0 u )
72.0 u
x 100=
x 100=40.0 %
180.0u
180.0 u
AVOGADRO’S NUMBER AND MOLAR MASS
-
NA = 6.02x1023 mol-1
1 mole = number of atoms found in exactly 12g of 12C
6.02x1023 (Avogadro’s Number) carbon atoms in 12g 12C
Therefore:
 1 mol 12C atoms = 6.02x1023 atoms
 1 mol CO2 molecules = 6.02x1023 molecules
 1 mol CO22- ions = 6.02x1023 ions
MOLAR MASS
-
Molar Mass (Mr) = mass of 1mol of a substance (i.e. g/mol)
Molar mass of an element = atomic weight (from periodic table)
Formula weight (in u) = Molar mass (in g/mol) – are the same number
CONVERTING MASS, MOLES AND NUMBERS
-
Mass (g) > (Use molar mass) > Moles (mol) > (Use NA) > Formula units (-)
(Mass / Molar mass) = Moles
Number of molecules = NA x Moles
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Week 3
Lecture 2 – Stoichiometry
Empirical Formulas from Analyses
-
EXAMPLE:
o 73.9% Hg and 26.1% Cl by weight – can work out molar ratio
o Means that 100g of the substance contains 73.9g Hg and 26.1g Cl
o Covert masses to moles:
o Hg, 1 mol = 200.6g
o Cl, 1 mol = 35.5g
o Molar ratio:
o Hg: 73.9g x 1mol/200.6g = 0.368 mol
o Cl: 26.2g x 1 mol/35.5g = 0.735 mol
o Hg: 0.368 mol/0.368 mol = 1.00
o Cl: 0.735 mol/0.368 mol = 1.997 ~ 2.00
o Empirical formula = HgCl2
Finding Molecular formula from Empirical
formula
-
Calculate empirical formula weight – formula weight calculated from empirical formula
Obtain a whole number multiple by diving molecular weight by empirical formula weight
Use this multiple to multiply through subscripts in empirical formula
EXAMPLE – MESITYLENE:
o C3H4 w/ molecular weight of 121.0 amu
o 3 x 12 + 4 x 1 = 40 amu
o (Experimental M. wt) / (empirical formula weight) = 121 amu/40 amu = 3.02 ~ 3.0
o Multiple = 3.0, so molecular formula = C9H12
Lecture 3.1 – Stoichiometry
Quantitative Information from Balanced
Equations
-
Coefficients in balanced equation represent both rea=lative numbers of molecules and
realative numbers of moles
Therefore, they also represent relative masses
2H2 + O2  2H2O = 2 moles of H, 1 mole of O and 2 moles of H2O = 2x2.0g + 32.0g  2x18.0g
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Multiplying an Equation Through by a
Common Multiple
-
Can multiply coefficients in a balanced equation by any multiple – still has correct ratio of
moles
EXAMPLE:
o Zn (s) + 2HCL (aq)  ZnCl2 (aq) + H2 (g)
o 1 mole + 2 moles  1 mole + 1 mole
IF WE HAVE S MOLES OF ZN (X2):
o
2 moles + 4 moles  2 moles + 2 moles
IF WE HAVE 0.5 MOLES OF ZN (X0.5):
o
0.5 moles + 1 mole  0.5 moles + 0.5 moles
Masses of products and Reactants in
Balanced Equation
-
Can work out how many grams of water will be produced by burning given amounts of H 2
and O2 together
EXAMPLE – COMBUSTION OF BUTANE:
2 C4H10 (l) + 13 O2 (g)  8CO2 (g) + 10 H2O (l)
2 moles + 13 moles  8 moles + 10 moles
2 x 58.0 g(m.m. C4H10) 8 x 44.0 g(m.m.CO2)
General Plan for Stoichiometry Calculations
-
MASS REACTANT  (n = M/Mr)  MOLES REACTANT  (Stoichiometric Factor)  MOLES
PRODUCT  (x molar mass)  MASS PRODUCT
How Many Grams of CO2 will be Obtained by
Burning 1.00g of C4H10?
1. GRAMS OF REACTANT  MOLES OF REACTANT
Conversion factor: 1 = 1 mol/58.0 g
1.00g x 1mol/58g = 0.0172 mol
2. MOLES OF REACTANT  MOLES OF PRODUCT
2 moles C4H10  8 moles CO2
Moles CO2 = 0.0172 x 8/2 = 0.0688 moles
3. MOLES OF PRODUCT  GRAMS OF PRODUCT
0.0688 moles CO2 = 0.0688 mol x 44.0 g/1 mol
4. GRAMS OF CO2 = 3.03g
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Lecture 3.1 – Stoichiometry
Limiting Reactants
-
-
-
Limiting reactant = Reactant that is completely used up in a reaction
EXAMPLE:
o 2 Bd + 1 Ch = Bd2Ch
o If we have 12Ch and 8Bd, we can only make 4Bd 2Ch
o Bd = limiting reactant
EXAMPLE:
o 2H2 + O2  2H2O
o 2 mol + 1 mol  2 mol
o If we have 4mol H2 and 1 mol O2 – only make 2mol H2O with 2 mol H2 left over
o O2 = limiting reactant
Same general stoichiometry calculations plan applies to limiting reactants
Reaction to Study
-
-
2Al + 3Cl2  Al2Cl6
QUESTION: mix 5.40 g of Al with 8.10g of Cl2 – what mass of Al2Cl6 can form?
Mass of reactants  Moles of reactant  Moles of product  Mass of products
1. COMPARE ACTUAL MOLE RATIO OF REACTANTS TO THEORETICAL MOLE RATIO:
 If (mol Cl2)/(mol Al) = 3/2 – even
No limiting reagent, because both are used up in reaction
 If (mol Cl2)/(mol Al) > 3/2 – more Cl than Al, Cl in excess
Al = limiting Reagent
 If (mol Cl2)/(mol Al) < 3/2 – more Al, Al in excess
Cl = limiting Reagent
2. CALCULATE MOLES OF EACH REACTANT:
 5.40g Al = 1mol/27.0g = 0.200 mol Al
 8.10g Cl2 = 1mol/70.9g = 0.114 mol Cl2
3. FIND MOLE RATIO OF REACTANTS:
 (mol Cl2)/(mol Al) = (0.114 mol)/(0.200 mol) = 0.57
 0.57 < 2/3
4. LIMITING REAGENT = Cl2
Grams of Cl2  Moles of Cl2  (1mol Al2Cl6/3mol Cl2)  moles of Al2Cl6  Grams of Al2Cl6
1.
2.
1 mol Al 2Cl 6
=0.0380 mol Al 2 cl 6
3 mol Cl 2
266.4 g Al 2 Cl 6
0.0380 mol Al 2Cl 6 X
=10.1 g Al 2 Cl 6
mol
0.114 mol Cl 2 X
3. 10.1 g of Al2Cl6
Lecture 3.2 – Stoichiometry
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Limiting Reactants Continued
-
Cl2 = limiting reactant
AL WAS PRESENT IN EXCESS, BUT HOW MUCH?
 Find how much Al was required
 Find how much Al is in excess
1. 2Al + 3Cl2  products
2. 0.200 mol of Al and 0.114 mol for Cl2 (LR)
3.
0.114 mol Cl 2 X
2mol Al
=0.0760 mol Al required
3 mol Cl 2
4. Excess Al = Al available – Al required
5. = 0.200 mol – 0.0760 mol
6. = 0.124 mol Al in excess
Percentage Yield
Percentage yield=
-
Actual yeild ( g ) X 100 %
Theorectical yield( g)
Theoretical yield = quantity of product that forms if all limiting reagent reacts – calculated
quantity
Actual yield = less than theoretical yield – measured quantity
Find Theoretical yield: with moles, Mr and n = m/Mr
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Week 4 – Solution Stoichiometry
Lecture 1 – Solution Stoichiometry
Introduction
Aqueous Reactions and solution Chemistry
-
Chemical reactions in water are important – life occurs in water and chemical reactions in the
environment occur mainly in water
General properties of aqueous Solutions
-
Electrolytic Properties: NaCl dissolved in water produces solution that conducts electricity,
whereas table sugar (sucrose C12H22O11) does not.
Demonstration of electrical conductivity of an electrolyte:
 Bulb glows in presence of electrolyte
 Does not glow in pure water
 Circuit contains a cathode and an anode in solution (Na + towards cathode and Cltowards anode)
 Electrolyte produces ions that conduct electric current
Distribution of Charge on the Water
Molecule
-
Water molecule = polar
Means that hydrogens have partial (+) charges and oxygen has partial (–) charge
Oxygen is more electronegative than hydrogen – therefore angular shape ( V )
Due to shape of the molecule H and O get charges (+/-)
Partial positive charges (δ+) attracted to negative charges
Partial negative charges (δ-) attracted to positive charges
Structure of water around anions and
cations
-
Each anion surrounded by partial positive (+) charges from waters
Each cation surrounded by partial negative (-) charges from waters
O attracted to cation
H attracted to anion
Ionic Compounds
-
Ionic compounds dissolve in water – tend to dissociate completely
NaCl (s) + H2O (l)  Na+ (aq) (Cation) + Cl- (aq) (Anion)
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-
 side surrounds Na – attracted to +
 H side surrounds Cl – attracted to –
Starts from edge of solid and water molecule attracts ion by ion until whole solid dissolved
Molecular Compounds
-
-
Most do not dissociate when dissolved in water
Methanol (molecular compound) + H2O  Methanol dissolved in water
 Methanol molecule not ionized
 Homogenous and spread throughout water
 + and – attracts slight but not complete (?)
Intermolecular interacts between + part of water and – part of Methanol molecule
Molecular Compounds that ionize in water
-
Some molecular compounds dissociate (ionize) in water – mainly acids
Strong acids: Hydrochloric acid
HCl (aq)  H+ (aq) + Cl- (aq)
Dissociate completely – Strong electrolyte
Single arrow shows equilibrium well to the right
Weak acids: Acetic acid
HC2H3O2 (aq)  H+ (aq) + C2H3O2- (aq)
Dissociate only partially – Weak electrolyte
Double arrow shows equilibrium does not lie completely to right
Strong and Weak Electrolytes
-
-
Strong electrolytes = completely ionized in water
 E.g. NaOH
 NaOH (aq)  Na+ (aq) + OH- (aq)
 Single arrow used to indicates complete ionization
Weak electrolytes = partially ionized in water
 E.g. Acetic Acid – only ionizes to small extent
 HC2H3O2 (aq)  H+ (aq) + C2H3O2- (aq)
 Indicated by double arrow
Lecture 2 – Precipitation Reactions
-
Ppt = insoluble solid formed by a reaction in solution
E.g. Mix clear AgNO3 and NaI solutions  produces yellow AgI (s) ppt
Soluble Ionic Compounds
-
Table given in tests
COMPOUNDS CONTAINING
EXCEPTIONS
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NO3C2H3O2ClBrISO42-
None
None
Ag+ Hg22+ Pb2+
Ag+ Hg22+ Pb2+
Ag+ Hg22+ Pb2+
Sr2+ Ba2+ Hg22+ Pb2+
Insoluble Ionic Compounds
COMPOUNDS CONTAINING
S2OHCO32PO43-
EXCEPTIONS
Alkali metal cations: NH4+ Ca2+ Sr2+ Ba2+
Alkali metal cations: NH4+ Ca2+ Sr2+ Ba2+
Alkali metal cations: NH4+
Alkali metal cations: NH4+
Ionic Equations
-
MOLECULAR EQUATION – do not show as ions
 Pb(NO3)2 (aq) + 2KI (aq)  PbI2 (s) + 2KNO3 (aq)
COMPLETE IONIC EQUATIONS – show all ions
 Pb2+ + 2NO3- + 2H+ + 2I-  Pbl2 (s) + 2K+ + 2NO3NET IONIC EQUATION – omit ions that do not change during reaction
 In e.g. those ions are NO3- and K+
 Pb2+ (aq) + 2I- (aq)  PbI2 (s)
EXAMPLES:
What is the net ionic reaction that corresponds to the molecular reaction below?
Ca(NO3)2 (aq) + Na2CO3 (aq)  CaCO3 (s) + 2 NaHO3 (aq)
1. Write out complete ionic equation and then remove spectator ions
Ca2+ + 2NO3- + 2Na+ + CO32-  CaCO3 (s) + 2Na+ + 2NO32. Net ionic equation =
Ca2+ (aq) + CO32- (aq)  CaCO3 (s)
Acid-Base Reactions
ACIDS
-
Acids = substance that ionize aq solutions to form protons (H+ (aq) ions)
Proton donator
HCl, HNO3 are monoprotic acids – they ionize to give only one proton per acid molecule:
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-
 HNO3 (aq)  H+ (aq) + NO3- (aq)
H2SO4 is a diprotic acid – gives two protons
 H2SO4 (aq)  2H+ (aq) + SO42- (aq)
 H2SO4 – only first ionization is complete
BASES
-
Substance that accept protons
Proton acceptor
Common bases are OH- compounds for group 1 cations (NaOH, KOH) or heavier Group 2
(Ba(OH)2)
These produce hydroxide (OH- (aq)) ion in solution
 NaOH (aq)  Na+ (aq) + OH- (aq)
Bases react with proton (net ionic reaction below)
 H+ (aq) (acid) + OH- (aq)(base)  H2O (l)(water)
Lecture 3 – Concentrations
Concentration of Solutions
-
Molarity – used to express concentrations of solutions
Molarity=
-
Moles Solute( substance dissolved ∈ solution)
Volume of Solution∈litres
Units = mole/litre = M
EXAMPLE: WHAT STRENGTH SOLUTION IS OBTAINED IF WE DISSOLVE 0.250 MOL CUSO 4 IN
A 250ML FLASK
250 ml = 0.250 litre
Molarity=
-
Moles Solute
0.250 moles
=
=1.00 M
Volume of Solution∈litres 0.250 litres
EXAMPLE: WHAT MOLARITY SOLUTION DO WE OBTAIN IF WE DISSOLVE 4.82 G CUSO 4 IN A
200ML FLASK
200ml = 0.200 litre
Molar mass CuSO4 = 4.82 g / 159.5 g = 0.0302 moles
Molarity=
0.0302moles
=0.151 M
0.200 litres
Expressing the concentration of an
Electrolyte
-
-
A 1.00 M SOLUTION OF NaOH IS ALSO 1.00 M IN Na+ IONS AND OH- IONS
NaOH (aq)  Na+ (aq) + OH- (aq)
1 Molar
1 Molar 1 Molar
A 1.00 M SOLUTION OF H2SO4 IS 1.00 M IN SO42- BUT 2.00 M IN H+
H2SO4 (aq)  2H+ (aq) + SO42- (aq)
1 molar
2 molar 1 molar
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-
A 1.00 M SOLUTION OF Na3PO4 IS 1.00 M IN PO43- BUT 3.00 M IN Na+. WHAT ABOUT A 0.1
M SOLUTION
Na3PO4 (aq)  3 Na+ (aq) + PO43- (aq)
1 M x 0.1
3 M x 0.1 1 M x 0.1
Interconverting Molarity, Moles and Volume
-
-
EXAMPLE: CALCULATE NUMBER OF MOLES HNO3 IN 2.0L OF 0.200 M HNO3
1. Molarity = moles/litres
2. 0.200 M = moles/2.0 L
3. Moles = (0.200 mol/1 L) x 2.0 L = 0.40 moles
EXAMPLE: HOW MANY GRAMS OF Na2SO4 ARE REQUIRED TO MAKE 0.350L OF 0.500 M
Na2SO4?
1. Moles = 0.350 L x 0.500 mol/L = 0.175 moles
2. 0.175 moles Na2SO4
3. Molar Mass Na2SO4 = 142.0 g/mol
4. Grams = 0.175 mol x 142.0 g/mol = 24.9 g
Dilution
-
-
Take volume of solution and place it in a larger container and make it more dilute by adding
water
- MOLES = MOLARITY x LITRES
In diluting a solution – number of moles of dissolved substance stays the same
Moles before dilution = moles after dilution
-
M=
MCONC x VCONC = MDIL x VDIL
Example: How many ml of 3.00 M H2SO4 needed to make 450 ml of 0.100 M H2SO4
1. Mconc x Vconc = Mdil x Vdil
2. 3.0 M x Vconc = 0.100 M x 450 ml
3. Vconc = 15.0 ml
Moles
Volume
Lecture 4 – Solution Stoichiometry
-
Able to convert from gras to moles and use M = moles / volume to convert from moles to
molarity
EXAMPLE: 1 LITRE OF 0.5 M Cu SO4
(0.5 mol / 1 litre) x 1 litre = 0.5 mol
Example: 79.8 g of CuSO4
79.8 g x (1 mole / 159.5 g)
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General Plan for Stoichiometry Calculations
– Solutions
-
Mass Reactant > Moles Reactant > Moles Product > Mass Product or Volume Product
EXAMPLE: HOW MANY GRAMS OF CA(OH)2 NEEDED TO NEUTRALIZE 25.0 ML OF 0.100 M HCL
1. 2HCl + Ca(OH)2  CaCl2 + 2H2O
2 mol 1 mol
1 mol 2 mol
Will need 1 mole of Ca(OH)2 to neutralize 2 moles HCl
2. Mole HCl = 0.100 M x 0.025 L = 0.0025 moles
2HCl + Ca(OH)2  CaCl2 + 2H2O
2 mol 1 mol
1 mol 2 mol
3. Factor = moles we have / moles in equation = 0.0025 / 2 = 0.00125
Moles of Ca(OH)2 = 0.00125 x 1 = 0.00125 mol
4. Grams = 74.2g x 0.00125 mol = 0.0926 g
EXAMPLE: WHAT VOLUME OF 0.30 M HCL SOLUTION IS NEEDED TO COMPLETELY REACT 3.5 G OF
CA(OH)2
1. 2HCl + Ca(OH)2  CaCl2 + 2H2O
2. Number of moles of Ca(OH)2 = 3.5 g / 74.1 g = 0.047 mol
Moles of HCl = 0.047 x 2 = 0.094 mol
3. Molarity = moles / volume
0.30 = 0.094 / volume
4. Volume = 0.094 / 0.30 = 0.3 L (310ml)
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Lecture 1 – Thermodynamics
14.1: The Nature of Energy
-
Energy = capacity to do work (w) or transfer heat (q)
Work = energy used to cause an object with mass to move
Heat = energy that causes temperature of an object to increase
FORMS OF ENERGY
-
Different forms of energy are interconvertible
Kinetic Energy
1
2
Ek= m v
2
-
m = mass, v = velocity
Potential Energy
Ep=mgh
-
m = mass, h = height relative to reference point, g = gravitional constant (9.81 ms -2)
Electrostatic Potential Energy
Eel=
-
kq 1 q 2
r
k = constant (8.99 x 109 JmC-2), r = distance between charges (q1 & q2)
UNITS OF ENERGY
-
SI unit for energy is joule (J)
1 cal = 4.184 J
1000 cal = 1 x 103 cal = 1 kcal
1 kcal = 4184 J = 4.184 kJ
REACTION SYSTEM AND SURROUNDINGS
-
System = just reaction and contents
Surroundings = exterior environment and glassware (excluding of contents)
Universe = whole thing
System + Surroundings = Universe
IS MATTER
TRANSFERABLE?
IS ENERGY
TRANSFERABLE?
OPEN
Yes
CLOSED
No
ISOLATED
No
Yes
Yes
No
14.2: The First Law of Thermodynamics
-
Also known as Law of Conservation of Energy
1st Law = energy is conserved
Energy cannot be created or destroyed – rather there is a set amount in universe which can
be converted from one from to another, or transferred from one place to another
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INTERNAL ENERGY (U)
-
Sum of all kinetic and potential energy
Not possible to measure absolute value of U – possible to measure change in U (ΔU)
∆ U =U Final −U Initial
-
Internal energy = example of state function: values of Uinitial and Ufinal are fixed and not
dependent on how change comes about
Initial State = reactants
Final State = products
System:
ΔU > 0
Net GAIN of energy
Surroundings – Loss of energy
ΔU < 0
Net LOSS of energy
Surroundings – Gain in energy
RELATING ΔU TO HEAT AND WORK
-
System undergoes chemical or physical change – change in internal energy can be
determined from extent of heat and work exchanged with the surroundings
Δ U =q+ w
-
Q = heat transferred, w = work performed
Sign conventions (with respect to system):
q
+ Heat GAINED
- Heat LOST
- + Energy enters
- - Energy leaves
w
+ Work done ON system
- Work done BY system
ENDOTHERMIC AND EXOTHERMIC PROCESSES
-
Endothermic = system gains (absorbs) heat (+q)
Exothermic = system loses heat (-q)
14.3: Enthalpy
-
Many reactions described as isobaric
Isobaric = constant pressure of atmosphere, Patm
Work (w) that accompanies such reactions is generally mechanical in nature – resulting in
change in volume of system
This is pressure-volume (P-V) work
- ΔV
Vf < Vi
+ ΔV
Vf > Vi
System
COMPRESSED
System EXPANDS
Work done ON
system
Work done BY
system
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+w
-w
w=−P ∆ V
-
Where P-V is the only form of work – transfer of heat is accounted for by Enthalpy (H):
∆ H=∆ U + P ∆ V
∆ H= ( q+ w ) +(−w)
ΔH = qp
-
Sign Conventions:
+ ΔH + qp
- ΔH - qp
Heat GAINED by system
Heat LOST by system
Process is ENDOTHERMIC
Process is EXOTHERMIC
Lecture 2 – Thermodynamics
14.4 Enthalpy of Reaction
-
Enthalpy (H) is also a state function – therefore enthalpy of rection (ΔrxnH) depends only one
initial and final states
-
Thermochemical equation = balanced equation when Δ rxnH takes place
Example:
ΔrxnH = Hproducts – Hreactants
2H2 (g) + O2 (g)  2H2O (g) ΔH = - 483.6 kJ
1. Enthalpy is an extensive proterty
H2 (g) + 0.5 O2 (g)  H2O (g) ΔH = - 241.8 kJ
2. Reverse equation = opposite sign
2H2O (g)  2H2 (g) + O2 (g) ΔH = + 483.6 kJ
3. States of matter influence magnitude
2H2 (g) + O2 (g)  2H2O (l) ΔH = - 571.6 kJ
Lecture 3 – Thermodynamics
14.5: Calorimetry
-
Value of ΔH can be determined experimentally
Calorimeter = experimental device used to do this
HEAT CAPACITY AND SPECIFIC HEAT CAPACITY
-
All substances change temperature when subjected to heat transfer
Magnitude of this change differs from substance to substance
Temperature change experienced by an object = determined by heat capacity (C)
Heat capacity = amount of heat required to change temperature (ΔT) of object by 1 K or 1 ᵒC
For pure substances – also consider molar heat capacity (C m) and Specific Heat Capacity (C)
Specific Heat Capacity = amount of heat required to change the temperature of 1 gram of a
substance by 1 K or 1 ᵒC
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-
C = J / (g.ᵒC)
Magnitude of ΔT is independent of units
ᵒC  K = +273
Specific heat capacity helps limit evaporation in water, so biological lifeforms are not harmed
by sharp increases/decreases in temperature
CONSTANT PRESSURE CALORIMETRY
-
Pressure controlled (kept constant) – ΔH can be readily measured (ΔH = qp)
Simple coffee-cup calorimeter (CCC) used in lab to obtain informative results
Example of an isolated system – Styrofoam prevents (limits) heat exchange with greater
surroundings
qrxn = -qsoln
qsoln = Csoln x Msoln x ΔT
-
Small part of the result in solution ΔT is partly from surroundings (minimal)
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Week 6
Lecture 4
14.6 Hess’s Law
-
Enthalpies of reaction for which experimental data is not available can be calculated using
Hess’s Law
∆ H 1=( ∆ H 2+∆ H 3+ ∆ H 4 )
∆ H=∆ Hf −∆ Hi
Lecture 5
14.7 Enthalpies of Formation
-
Standard state – form of a substance when P = 1bar and T = 298K (25ᵒC)
When all reactants and products are in their standard states – most stable state
Graphite = most stable form of carbon
Standard enthalpy change indicated as ΔHᵒ
Enthalpy of formation (ΔfH) = enthalpy change associated with formation of a substance
from its constituent elements
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-
Standard enthalpy of formation of a compound (ΔfHᵒ) – defined as enthalpy change for the
formation of 1 mole of a substance from its constituent elements with all species in their
standard states
2C (graphite) + 3H2 (g) + ½ O2 (g)  C2H5OH (l)
ΔfHᵒ = -277.7 kJmol-1
Important considerations:
-
-
If an element exists in more than one form under standard conditions – most stable form is
selected
E.g. thus O2 is used instead of O or O3 and graphite instead of diamond
By definition, formation reactions involved formation of 1 mole of a substance; enthalpies of
formation are therefore reported in units of kJ per mole (kJmol -1)
USING ENTHALPIES OF FORMATION TO CALCULATE ENTHALPIES OF REACTION
-
-
Can apply Hess’s Law order to determine ΔrxnHᵒ - need to use the individual formation
reactions for each species
Can make use of following relationship – which holds since any reaction can be broken down
into a series of formation reactions
ΔrxnHᵒ = ∑nΔfHᵒ (products) - ∑mΔfHᵒ (reactants)
∑nΔfHᵒ (products) = sum of enthalpies of formation of products
∑mΔfHᵒ (reactants) = sum of enthalpies of formation of reactants
Quantity and amount of moles needs to be taken into consideration
Lecture 6
14.8 Spontaneous Processes
-
Can calculate ΔU and ΔH
Important consideration is the extent of a reaction (how likely is it to take place)
Spontaneous process = one in which change occurs in a particular direction and without ongoing
external intervention
-
-
Occurs under given set of conditions
Reactions may be described as spontaneous irrespective of rate at which they occur
 Gas expanding into a vacuum – instantaneous
 Nail rusting – days to weeks
Temperature and pressure can influence whether or not a reaction is spontaneous
Examples:
 falling brick, rusting nail, gas expanding into a vacuum
 2Na(s) + Cl2(g)  2NaCl(s)
Non-spontaneous = reverse of spontaneous and do require work
-
Does not occur under given set of conditions
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REVERSIBLE AND IRREVERSIBLE PROCESSES
-
-
-
Reversible
 No net change to surroundings
 Restoring system causes requires no work
Irreversible
 Change in the surroundings
 Restoring system rewires work
Under given set of conditions = spontaneous processes are irreversible and take place in a
particular direction
Entropy – important for determining whether reaction will be spontaneous or not
Entropy = characteristic system that gives us indication of extent to which energy is
disordered
Entropy ΔS = amount of disorder in a system
14.10 The molecular Interpretation of
Entropy
MOLECULAR MOTIONS AND ENERGY
-
-
Molecules can undergo three kinds of motion:
 Translational – entre molecule moves
 Vibrational – atoms and bonds move
 Rotational – molecule spins
When molecule heated – motion (and Ek) increases
Refer to molecules as having motional energy
BOLTZMANN’S EQUATION AND MICROSTATES
-
-
Microstate is a single arrangement of positions and kinetic energies of a given set of
molecules (system)
For any system, entropy (S) related to total number of microstates (W)
S = K ln W
ΔS = k ln (Wfinal)/(Winitial)
Number of microstates available in system increases with increase in volume, temperature
and number of independent particles
MAKING QUALITIES PREDICTIONS ABOUT ΔS
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Increase in disorder / entropy (+ΔS)
THIRD LAW OF THERMODYNAMICS
-
If temperature if a system decreased to such a point
S
L
(W
-
S
Solvent
that all molecular
motion is
halted
G
then a
single
microstate
= 1) is
essentially
achieved
Solution
2NH (g)  N (g) + 3H (g)
3
2
2
Temperature
at which this is achieved = Absolute zero
(0K)
- Entropy of a pure crystalline system at 0K is zero (S = 0)
-
Pure crystalline solid heated – entropy increases from 0:
1. At std temperature (298K) Sᵒ for pure elements is not zero
2. In general Sᵒ (g) > Sᵒ (L) > Sᵒ (s)
3. Value of Sᵒ usually increases with increasing molar mass
4. Value of Sᵒ usually increase with increasing number of atoms
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Week 7
Lecture 7
14.9 Entropy and the Second law of
Thermodynamics
SECOND LAW OF THERMODYNAMICS
-
Spontaneous (irreversible) process characterized by overall increase in entropy of universe
ΔunivS = [ΔsysS + ΔsurrS] > 0
-
If no change in entropy of universe – dealing with reversible process:
ΔunivS = [ΔsysS + ΔsurrS] = 0
-
To determine whether reaction is spontaneous or not – consider ΔunivS
ΔsysS = readily determined using this equation:
ΔrxnHᵒ = ∑nΔfHᵒ (products) - ∑mΔfHᵒ (reactants)
-
For isothermal (constant temperature) process at equilibrium (forward and backwards rates
are the same) following relationship useful alternative to calculate ΔsysS
ΔsysS = (qrev) / T
-
qrev = heat transferred if process reversible
T = temperature (K) at which process occurs
ENTROPY CHANGES IN SURROUNDINGS
-
To calculate ΔsurrS:
ΔsurrS = (-qsys) / T = (-ΔHsys) / T
-
Surroundings and system = equal magnitude and opposite signs
If we know ΔH of system we can find ΔS of surroundings
14.11 Entropy Changes in Chemical
Reactions
-
Can measure ΔH using calorimetry
No easy method to measure ΔS
Absolute values of entropy (S) can be determined
Standard molar entropies (Sᵒ) for substances in their standard state reported in units of
Jmol-1K-1
Examples in table 4.6
Observations:
 At standard temperature (289K) Sᵒ for pure elements is not zero
 In general, Sᵒ (g) > Sᵒ (l) > Sᵒ (s)
 Value of Sᵒ usually increases with increasing molar mass
 Value of Sᵒ usually increases with increasing number if atoms
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-
Entropy is a sate function – ΔrxnS = Sfinal – Sinitial
Change in entropy for a chemical reaction calculated by:
ΔSᵒ = ∑nSᵒ (products) - ∑mSᵒ (reactants)
-
These are the absolute entropies of the products and reactants
ΔH = kJ and is therefore much larger than ΔS (J)
Lecture 8
14.12 Gibbs Free Energy
-
Reaction spontaneity depends on both enthalpy and entropy
Expressed in state function: Gibbs Free Energy (G)
G = H – TS
ΔG = ΔH – TΔS
-
T = constant under isothermal conditions
From entropy considerations:
ΔunivS = ΔsysS + ΔsurrS
-
Substitute so RHS is only in terms of system
ΔunivS = ((-ΔsysH) / T) + ΔsurrS
-
Cross multiply by -T:
-TΔunivS = ΔsysH – TΔsurrS
-
Compare this to
ΔG = ΔH – TΔSthat
-
Therefore:
ΔG = -TΔunivS
- ΔG
Forward reaction is spontaneous
Backward reaction is not spontaneous
Reaction is in equilibrium
Forward reaction is not spontaneous
Backward reaction is spontaneous
ΔG = 0
+ ΔG
-
Change in Gibbs free energy for a reaction can be calculated if changes in enthalpy and
entropy for same reaction are known
Change in Gibbs free energy for a reaction can also be calculated, as for enthalpy, using
standard Gibbs free energies of formation:
-
ΔGᵒ = ∑nΔfGᵒ (products) - ∑mΔfGᵒ (reactants)
ΔGᵒ = 0 – substance that only contains one atom type and is already in standard stable state
(e.g.O2)
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Lecture 9
14.13 Gibbs (Free) Energy and Temperature
ΔG = ΔH – TΔS
+ΔH – Endothermic
-ΔH – Exothermic
+ΔS – increase in disorder
ΔG = +ΔH – (T(+ΔS))
ΔG = +
Spontaneous at HIGH values of
T
ΔG = -ΔH + TΔS
ΔG = Spontaneous at ALL values of T
-ΔS – Decrease in disorder
ΔG = +ΔH – (T(-ΔS))
ΔG = +
Not spontaneous at ALL values
of T
ΔG = -ΔH – (T(-ΔS))
ΔG = Spontaneous at LOW values of
T
Gibbs (Free) Energy and the Equilibrium
Constant
ΔG
- (Spontaneous)
0
+ (Not spontaneous)
K
>1
=1
<1
Species Favoured
Products
50:50 (equally favoured)
Reactants
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Week 8
Kinetics - Lecture 1
-
Change = transformation of reactants to products
Reaction can be classified as spontaneous regardless of how long it takes (ms or
days/months/years)
Chemical Kinetics = area of chemistry that deals with speed (rate) of a reaction
15. 1 Factors That Affect Reaction Rates
-
Reactions involve breaking and forming bonds
Rate at which these take place depend on nature of reactants
Factors influence rate of chemical reaction:
o Physical state of reactants
 Larger surface area = faster reaction
 Smaller surface area = slower reaction
o Concentration of reactants
 More atoms = more likely to collide
 Higher concentration = quicker reaction
o Reaction temperature
 Higher temperature = speeds up reactions – more kinetic energy and
movement
 Lower temperature = slows down reactions
o Presence of a catalyst
 Lowers activation energy
 Catalyst is not used up during reaction
 Rate increases
15.7 Catalysts
-
-
Homogenous catalysis = same phase as reacting molecules
E.g. 2H2O2 (aq)  2H2O (l) + O2 (g)
o In absence of catalyst this reaction = extremely slow
o Including bromide:
o 2Br- (aq) + 2H+ (aq) + 2H2O2 (aq)  Br2 (aq) + 2H2O (l)
o Br2 (aq) + 2H2O2 (aq)  2Br- (aq) + 2H+ (aq) + O2 (g)
o Bromide ions (together with H+) catalyse this reaction
o Br2 (aq) = intermediate – produced in reaction 1 and consumed in reaction 2
Heterogenous catalysis = different phase than reacting molecules
o Catalyst is usually a solid
o Reactants may be gas or liquid
o Reactant molecules first absorb to catalyst surface (which is highly reactive)
o Then reaction proceeds to yield product molecules – which later desorb from surface
o Absorption  Reaction  Desorption
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15.2 Reaction Rates
-
-
Speed = extent of change in a given time interval
Measurable change with time = concentration (M/s or M s -1)
AB
 A used up and B formed
 At the end, there is the same number of total mol in reaction vessel as at the start of
the reaction
 Reaction rate can be expressed relative to disappearance of reactant (A) or the
appearance/formation of product (B)
−Change∈concentraion of A
Change∈time
Change∈concentraion of B
Average rate of appearance of B=
Change∈time
Average rate of disapperance of A=
Rates are always expressed as positive quantities
CHANGE IN RATE WITH TIME
-
E.g. in lecture notes
Average rate decreases with increasing time
Concentration of reactants decreases – resulting in a decrease in the number of collisions
Can determine the instantaneous rate – rate of reaction at a particular time
Instantaneous Rate=
ΔConcentration( M )
Δ time
Instantaneous rate= tangent of concentration(Y) against time(X) graph
REACTION RATES AND STOICHIOMETRY
-
AB
o Reaction stoichiometry is 1:1
o
-
−∆[ A] ∆ [B]
=
∆t
∆t
2A  B + C
o Reaction stoichiometry is 2:1 (A:B or A:C)
o
o
-
Rate=
−∆ [ A ]
∆ [ B]
∆ [ C]
=2×
∨2 ×
∆t
∆t
∆t
−1 ∆ [ A ] 2 ∆ [ B ] 2 ∆ [ C ]
Rate=
=
∨
2 ∆t
2 ∆t
2 ∆t
Rate=
aA+bBcC+dD
o
Rate=
−1 ∆ [ A ] −1 ∆ [ B ] 1 ∆ [ C ] 1 ∆ [ D ]
=
=
=
a ∆t
b ∆t c ∆t
d ∆t
Kinetics - Lecture 2
15.3 Concentration and Rate Laws
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-
Rate law = equation that shows how rate of reaction depends on concentration of all
reactants
For general equation: a A + b B  c C + d D
Rate Law is:
Rate = k[A]m[B]n
k = rate constant/coefficients
Exponents (m and n) = reaction orders
REACTION ORDERS: EXPONENTS IN THE RATE LAW
-
Exponents (m and n) – indicate how reaction rate is affected by concentration of each
reactant
Values of m and n must be determined experimentally
Exponent (m or n)
0
Meaning
Zero order
1
First order
2
Second order
-
Interpretation
Rate independent of reactant
concentration
Rate directly proportional to
concentration
Rate changes as square of
concentration
Overall reaction order = sum of orders
UNITS OF RATE CONSTANTS
-
Rate constant does not depend on concentration
It is affected by temperature and presence of catalyst
Units of rate constant, k, depend on overall order of reaction
Rate Equation
Rate = k
Rate = k[A]
Rate = k[A][B]
Rate = k[A]2
Rate = k[A][B]2
Overall Reaction Order
0
1
2
Units of k (t in seconds)
Ms-1
s-1
M-1 s-1
3
M-2 s-1
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Week 9
Kinetics – Lecture 3
15.4 The Change of Concentration with Time
(Integrated Rate Equations)
-
Integrated form of rate equation – used to find reaction rate at different times
AB
o Differential form of reaction rate (for disappearance of A) is:
o
Rate=
−d [ A ]
dt
ZERO-ORDER REACTIONS
-
Rate independent of concentration
Rate=
t
−d [ A ]
0
k [ A ] =k
dt
t
∫ d [ A ] =∫−k dt
0
0
[ A ]t −[ A ] 0=−k (t−0)
[ A ]t =−kt + [ A ] 0
-
Linear graph (y = mx + c)
FIRST-ORDER REACTIONS
-
Rate directly proportional to concentration
Rate=
−d [ A ]
1
k [ A ] =k [ A ]
dt
t
t
∫ [ A1 ] d [ A ] =∫ −k dt
0
0
ln [ A] t−ln [ A ]0 =−k (t−0)
ln [ A] t=−kt+ ln [ A ]0
-
Linear graph (y = mx + c) – ln[A]
Slope – [A]
ln
[ A ]t
=−kt
[ A ]0
[ A ]t =[ A ]0 e−kt
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SECOND-ORDER REACTIONS
-
Rate directly proportional to square of concentration
Rate=
−d [ A ]
2
=k [ A ]
dt
t
t
∫ 1 2 d [ A ] =∫ −k dt
0 [A]
0
−1 −1
−
=−k (t−0)
[ A ]t [ A] 0
1
1
=−kt+
[ A ]t
[ A ]0
-
Linear graph (y = mx + c)
HALF-LIFE
-
Half-life of a reaction (t1/2) = time required for concentration of reactant to reach one-half if
its initial value
1
[ A ]t 1 = [ A] 0
2
2
-
Zero-Order
o [A]t = -kt + [A]0
o
t1 =
2
-
2k
First-Order
o Half-life is constant
o
ln [ A ] t=−kt+ ln [ A ] t
o
t1 =
2
-
[ A ]0
ln 2
k
Second-Order
o
1
1
=kt+
[ A ]t
[ A ]0
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o
t1 =
2
1
k [ A ]0
15.5 Temperature and Rate
-
Rates of most chemical reactions increase with
increasing temperature
The faster rate at higher temperature – due to increase in rate constant with increasing
temperature
Exponential relationship
Reaction rates affected by both concentration of reactants and by temperature
Collison model – molecules must collide in order to react
Greater the number of collisions = greater reaction rate
Not all collisions lead to reaction
Molecules also need to be orientated in a certain way for collisions to result in reaction –
Orientation Factor
ARRHENIUS EQUATION
-
Increase in reaction rate with increasing temperature does not show a linear dependence
Exponential relationship given by Arrhenius equation:
k = Ae-Ea/RT
-
k = rate constant
Ea = Activation energy
R = gas constant (8.314 J/K mol)
T = temperature (K)
A = frequency factor – relates to frequency of favourably-orientated collisions (changes very
little with temperature – can be considered a constant)
Arrhenius equation predicts that as activation barrier increases, the reaction rate
decreases
DETERMINING ACTIVATION ENERGY
-
-
Arrhenius equation can be re-worked into a linear form
o
ln k =
−E a
+ ln A
RT
o
ln k =
−E a 1
∙ + ln A – Linear form (negative (-) slope)
R T
Two different reaction temperatures:
o Assume A is constant
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o
ln k 1−ln k 2=ln
k 1 Ea 1
1
= (
−
)
k2 R T 2 T 1
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Week 10
Electronic Structure
Limitations of the Bohr Model
-
Only works for atoms/ions with single electron (e.g. H or He +)
Cannot account for more numerous lines in multi-electron atoms
However is does make two important postulates:
o Electrons exist only in discrete energy levels
o Energy is involved in moving electron from one level to another – energy absorbed
as photons to excite electron from one level to a higher energy level and energy is
emitted as photons when an electron drops to a lower energy level
The wave Behaviour of Matter
-
Louis de Broglie – matter also had a wave property
For any particle:
λ=
-
-
h
mv
v – velocity
v – frequency
λ – wavelength
m – mass
h – Planck’s constant (6.626 x 10-34)
How to get to this equation:
1. E = hv
2. E = mv2
3. hv = mv2
4. λ = v/v
5. λ = hv/mv2
Quantity mv = momentum
Electron thus is not only a particle, but also a wave
Confirmed in that electrons can be diffracted by crystals
Since electrons are waves – inappropriate to treat them as particles (as in Bohr model)
Schrodinger Wave Equation
Ӈψ = Eψ
-
-
Same account of e in H atom as Bohr
Gives correct account of heavy atoms
ψ2 – measure of e- density in various regions around the nucleus
Orbitals and Quantum Numbers
-
Solution to Schrodinger wave equation leads to set of wavefunctions that yields 4 types of
quantum numbers
Single quantum number yielded by Bohr model
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-
-
-
These numbers are:
O PRINCIPLE QUANTUM NUMBER (n)
 Values 1, 2, 3,…
 This corresponds to quantum number in Bohr model
O AZIMUTHAL/ ANGULAR MOMENTUM QUANTUM NUMBER (l)
 Values of 0 to n-1 for each value of n
 Corresponding orbitals = 0 – s; 1 – p; 2 – d; 3 – f
O MAGNETIC QUANTUM NUMBER (ml)
 Values -l to +l for each value of l
O SPIN QUANTUM NUMBER (ms)
 Values + ½ or – ½
 Each value of ml – there are two values of ms
 Leads to occupation of each orbital by two electrons of opposite spin
These quantum numbers lead to the shells (different n values) and subshells (different values
of l) that lead to our modern understanding of chemistry
Number of orbitals in each sub-shell = determined by m l
Only two electrons of opposite spin can occupy each orbital = determined by m s
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Representation of Orbitals
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Many-electron Atom
-
PAULI EXCLUSION PRINCIPLE – no two electrons in an atom can have all four quantum
numbers (n, l, ml, ms) the same
Result of this is that each orbital can hold a max of two electrons, with m s = + ½ or – ½
Failure of Bohr Model for Many-electron Atoms
-
For H-atom – all subshells within same shell have the same energy
Bohr model works for H-atom – generates single quantum number (n), which predicts only
energy of shells and not the existence of subshells
Many-electron atom – subshells within single shell do not have same energy
Cause of failure of the Bohr model when applied to multi-electron atom
Electron Configurations
-
Electron configuration = way in which electrons are distributed among various orbitals
Orbitals filled in order of increasing energy – two electrons of opposite spin per orbital
Orbital diagram:
o Each orbital represented by a box
o Half arrow up (spin up) = positive spin (m s = + ½ )
o Half arrow down (spin down) = negative spin (m s = - ½ )
o
Electrons
Indicates number of
having
electrons in sub-shell
opposite
spins are
spin-paired
when in the
same orbital
Hund’s Rule
-
Orbitals that have same energy = degenerate
-
HUND’S RULE = for degenerate orbitals, lowest energy attained when number of electrons
with same spin is maximized
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Uncertainty Principle
-
If electron is a wave – cannot state position with any accuracy
HEISENBERG postulated: UNCERTAINTY PRINCIPLE – we cannot precisely know exact
momentum of an electron and also its location in space
Condensed Electron Configurations
-
Abbreviate electron configuration by only writing noble gas before element (e.g. [Ne]) and
electrons in outermost occupied shell (valence shell)
Transition Metals
-
-
Row ended by Ar marks beginning of 4th row (n = 4)
In this row = first row of transition elements
This is where the 3d orbital is being filled
4s = lower in energy than 3d orbital
Therefore 3d orbital does not fill right away
First two electrons for K and Ca go into this orbital
K = [Ar] 4s1
Ca = [Ar] 4s2
After 4s is filled then 3d starts to fill up
E.g. Mn = [Ar] 4s2 3d5
Lanthanoids and Actinoids
-
Filling up f orbital
Although energies of 4f and 5d are very close – electrons also occupy 5d orbitals
La = [Xe] 6s2 5d1
Lu = [Xe] 6s2 4f14
Electron Configurations and The Periodic Table
-
Each group of elements in periodic table has characteristic electronic configuration
E.g. Halogens have characteristic configuration of ns2 np5 of highest energy occupied shell
Valence electrons determine chemical properties of elements and occupy highest energy
shell
Electron Configuration of ions
-
Add or subtract n number of electrons from last orbital depending on +n or –n
Electron Configurations of Transition Metal
Cations
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-
S orbital filled before d-subshell
However, when cations formed – d-subshell is lower in energy and therefore any valence
electrons left occupy the d-subshell
Atomic Numbers (Z)
-
Each element produces X-rays of a distinct frequency
This frequency increases with atomic number
Atomic number = number of protons in a nucleus
This concept allowed correct placement of certain elements on periodic table
E.g. Ar (Z = 18) and K (Z = 19) but atomic weight Ar > K
Core and Valence Electrons
-
Valance electrons in 3s shell experience small net positive charge
Core electrons shield valence electrons from nucleus
Effective Nuclear Charge
-
Many-electron atom – each electron is simultaneously attracted to nucleus and repelled by
other electrons
Generally – valence electrons screened from nucleus by core electrons (~S, where S is
screening constant = number of core electrons)
Effective nuclear charge = approximate charge experienced by valence electrons
Thus, effective nuclear charge (Zeff) experienced by valence electrons is given by:
Zeff = Z – S
E.g. Na: Zeff = 11 – 10 ~ 1+ (because of electrons in higher shells are less good at shielding
nucleus – charge experienced by Na+ is actually +2.5)
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Week 11
Periodic Properties of Elements
Development of Periodic Table
-
Elements in same group generally have similar chemical properties
Effective Nuclear Charge
-
Zef
-
Nuclear charge that electron experiences depends on both
factors
-
Effective nuclear charge = Zeff = Z – S
-
Many-electron atom – electrons both attracted to nucleus and
repelled by other electrons
Z = atomic number
S = screening constant (close to number of inner e -s
Zef increases across a period – nuclear charge increases while number of core
electrons remains the same
Zef increases only slightly down a group – larger electron cores are less able to
screen outer electrons
Atomic and Ionic Size
-
Bonding atomic radius = half of distance between covalently bonded nuclei
Size increases down a group – number of shells and electrons are increasing
Size decreases across a period – increase in Zef causes electrons to pull closer to nucleus
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Ion Sizes
-
Radius when cation formed – cations are
smaller because fewer electrons relative to
protons (repulsions reduced)
-
Radius when anion is formed – anions are
larger because more electrons relative to
protons (repulsions increased)
-
For series of ions which are isoelectronic (same number of electrons) – radius of ion
decreases as nuclear charge increases (electrons more strongly attracted to nucleus)
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Ionization Energy
-
IE = energy required to remove an electron from an atom in the gas phase
-
More energy required to remove each successive electron
-
1st IE = energy required to remove first electron
2nd IE = energy required to remove second electron
When all valence electrons removed – ionisation energy increases drastically
IE decrease down a group – outer electrons further from nucleus and are easier to remove
IE increases across a period – Zef increases, therefore electrons are held more tightly and
difficult to remove
EXCEPTIONS:
o
o
Group 3: IE lower (electrons easier to remove) – these elements have only one
electron in p subshell
Group 6: IE lower – these elements have 4 electrons in p subshell (repulsion of
paired electrons is unfavourable and makes these electrons easier to remove)
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Electron Affinity
-
EA = energy change when an atom gains an electron in the gas phase
EA does not change significantly down a group
EA increases across a period (becomes more -ve/exothermic) – Zef increases, therefore
increased attraction for extra electron
EXCEPTIONS:
o
o
Group 2: +ve EA – electrons would have to go into previously empty p subshell
Group 5: EAs less -ve than expected – half filled p subshell and would have to start
pairing electrons
Main Group Ions
-
Elements from groups 1 and 2 – tend to form cations with noble gas configuration (i.e.
oxidation number = group number)
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-
Elements from group 6 and 7 – tend to form anions with noble gas configuration
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