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Energy matters. Unit 1. a) Reaction rates. Reaction rates. From standard grade you should remember that a reaction can be speeded up by; Decreasing particle size Increasing concentration Increasing temperature. Following the course of a reaction. - PowerPoint PPT Presentation
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Energy matters Unit 1
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Page 1: Energy matters

Energy matters

Unit 1

Page 2: Energy matters
Page 3: Energy matters

Reaction rates

• From standard grade you should remember that a reaction can be speeded up by;

• Decreasing particle size

• Increasing concentration

• Increasing temperature

Page 4: Energy matters

Following the course of a reaction

• In general to measure the rate of a reaction we must choose some measurable quantity which changes as the reaction proceeds.

e.g mass of reactants in a flask, volume of gas produced, colour intensity, concentration of reagent

Page 5: Energy matters

Following the course of a reaction

• If we react marble chips (Calcium carbonate) with hydrochloric acid we can monitor the course of the reaction.

CaCO3(s) + 2HCl(aq) CaCl2(aq) + CO2(g) + H2O(l)

Page 6: Energy matters

Marble chips & acid

• As we are producing a gas, it will escape from the vessel causing the total mass to drop.

• If we measure this change in mass over a fixed period of time we can calculate the rate of the reaction.

Marble chips

Balance

Cotton woolHCl(aq)

Page 7: Energy matters

Time (s) Total mass of flask (g)

Decrease in mass (g) or Mass of CO2

produced

0

30

60

90

120

150

180

210

240

270

300

149.00

147.75

147.08

146.60

146.26

145.94

145.68

145.48

145.32

145.19

145.08

-

1.25

1.92

2.40

2.76

3.06

3.32

3.52

3.68

3.81

3.92

Page 8: Energy matters

Decrease in mass (g) -

00.5

11.5

22.5

33.5

44.5

0 50 100 150 200 250 300 350

Time (seconds)

Decre

ase in

mass

(g)

Page 9: Energy matters

Average rate of reaction

• It is difficult to measure the actual rate at any one instant since the rate is always changing.

• We can calculate average rate over a certain period of time.

Average reaction rate = Change in mass of product Time taken for change

Page 10: Energy matters

Example

• Calculate average rate of reaction between 30 and 60 seconds.

Average reaction rate = Change in mass of product

Time taken for change

Average reaction rate = 1.92 - 1.25

30

Average reaction rate = 0.022gs-1

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Collision theory

• For a chemical reaction to occur, the reactants must collide.

• Any factor that increases the number of collisions per second is likely to increase reaction rate.

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Particle size

• More collisions occur if the particle size of a solid reactant is decreased, since its overall surface area is increased.

• Powdered marble (calcium carbonate) reacts much faster than marble chips.

Page 13: Energy matters

Concentration

• If concentration is increased, there are more reactant particles.

• The more particles there are in one space, the more collisions.

Page 14: Energy matters

Raising temperature

• Raising the temperature at which a reaction takes place does more than merely raise the number of collisions.

• Temperature is a measure of the average kinetic energy of particles in a substance.

• Therefore at higher temperatures, particles have greater kinetic energy and they collide with more force.

Page 15: Energy matters

Collisions

• Not all collisions cause a reaction to occur e.g. nitrogen & oxygen particles in the air.

• The colliding particles must have a minimum amount of kinetic energy for a reaction to occur.

• This minimum kinetic energy is called the Activation energyActivation energy (EA)

Page 16: Energy matters

Activation energy

• Activation energy required varies from one reaction to another.

• If the activation energy of a reaction is high, only few particles will have enough energy to successfully collide.

• Conversely, a reaction with low activation energy will be very fast.

Page 17: Energy matters

Kinetic energy• At a given temperature (T1) individual molecules of

a gas have widely different kinetic energies.

• Most molecules will have energy near to the average energy but some will be well below average, and some well above.

Page 18: Energy matters

Activation energy

• The shaded area represents the all of the molecules which have kinetic energy greater than the activation energy.

• The shaded area represents the portion of molecules that will react

EA

Page 19: Energy matters

Temperature• Distribution of energy changes when the temperature

changes.• A small rise from T1 to T2 considerably increases the

number of particles capable of reacting.• Hence increasing the reaction rate.

T2

 

Kinetic energy

Page 20: Energy matters

Catalysts

• Substance that alters rate of reaction without being used up.

• Homogeneous catalyst: Same state as the reactants.

• Heterogeneous catalyst: Different state as the reactants.

Page 21: Energy matters

Heterogeneous catalyst

• The catalyst has a large surface area.• Catalysis occurs at certain points on the

catalyst called ‘active sites’. • At these sites reactant molecules are

adsorbed onto the surface of the catalyst.• At least 1 reactant is held in place on active

site, making collision more likely.

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Catalyst poisoning

• Occurs when reactants or impurities become preferentially adsorbed or even permanently attached to the catalyst surface.

• Hence reducing number of active sites and therefore rendering the catalyst as useless.

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Industrial catalystCatalystCatalyst ProcessProcess ImportanceImportance

Vanadium(v) oxide

Contact Manufacture of H2SO4

Iron Haber Manufacture of ammonia

Platinum Oxidation of ammonia

Manufacture of nitric acid

Nickel Hydrogenation Manufacture of margarine

Page 25: Energy matters

Enzymes

• Biological catalyst.

• Examples of enzymes:– Amylase, catalyses the hydrolysis of starch.– Catalase, catalyses the decomposition of

hydrogen peroxide. Catalyase is found in the blood, preventing build up of hydrogen peroxide in the body.

Page 26: Energy matters

Enzymes continued

• Enzymes are highly specific. • Enzymes work best at their

optimum temperature & pH.• Optimum temperature for

human enzymes will be 37°C.

• Greatly exceeding either of these will result in the protein being denatured.

Page 27: Energy matters

Industrial enzymesEnzymeEnzyme ProcessProcess

Lipase Enhance flavour of cheese, ice-cream &

chocolate

Rennin Cheese production

Protease Tenderising meat

Amylase Desizing (removing starch from fabric)

Page 28: Energy matters
Page 29: Energy matters

Potential energy• Potential energy is the energy

possessed by the reactants.

• In an exothermic reaction, the products have less potential energy than reactants.

Page 30: Energy matters

Potential energy

• In an endothermic reaction, the opposite is true. Reactants must absorb energy from their surroundings.

• Products have more energy than the reactants.

Page 31: Energy matters

Enthalpy

• The difference in potential energy between reactant and product is called the enthalpy enthalpy changechange (ΔH)

• Enthalpy changes are normally quoted in kJ mol-1

Page 32: Energy matters

Activation energy

• The rate of reaction depends on the height of the Ea barrier.

• Rate of reaction does not depend on the enthalpy change ( )

HH

Page 33: Energy matters

Catalyst• Catalysts provide alternative reaction

pathways.

• Thus lowering the activation energy.

Energy

Reaction pathway

Page 34: Energy matters

Activated complex

• When reactants change into products, they pass through a very unstable state known as the activated activated complexcomplex. (Situated at the maximum potential energy).

• The activated complex is a highly energetic arrangement of atoms that exists for a short time.

• The activated complex loses this energy by either forming products or reforming as reactant particles.

Page 35: Energy matters

Activated complex

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Page 37: Energy matters

Density

• The amount of material packed into a given volume.

• Density values are much larger for Solid & liquid elements.

• Density increases down each group.• Across the period from L to R,

density increases towards the centre of the period, then decreases again towards the noble gases.

Page 38: Energy matters

Atomic size: Groups• Atomic size is measured in covalent

radius. This is the distance from the nucleus to the outer electrons.

• As you move down a group the atomic radius increases.

• This is due to the increased number of occupied electron shells.

Page 39: Energy matters

Atomic radius: Periods• Across a period atomic number and electron number

increase by one.

• Although the number of outer electrons is increasing across the period, the atomic radius decreases.

• This is due to the increasing attraction between the nucleus and the outermost electrons.

Page 40: Energy matters

Ionisation energies

• The attraction between the nucleus and the outer electrons means that energy is required to remove electrons from the atom.

• Ionisation energy is a measure of the nuclear attraction for outer electrons.

Page 41: Energy matters

First ionisation energy

• Energy required to remove an electron from one mole of free atoms in a gaseous state.

• K(g) K+(g) + e-

Page 42: Energy matters

Second ionisation energy

• Energy required to remove an electron from one mole of ions with a charge of 1+ in the gaseous state.

• K+(g) K2+(g) + e

Page 43: Energy matters

Third ionisation energy

• Energy required to remove an electron from 1 mole of ions with 2+ charge in the gaseous state.

• K2+ K3+(g) + e

Page 44: Energy matters

Ionisation energies• The first ionisation energy decreases as

you go down a group.• This is due to the increasing atomic radius.• As the radius increases, the attraction

between the nucleus and the outermost electrons decreases.

• Screening / Shielding effect.• Therefore the energy required to remove

that electron decreases.

Li

Na

K

e-

e-

e-

Page 45: Energy matters
Page 46: Energy matters

Bonding, structure and properties of

compounds

Page 47: Energy matters

Metallic Bonding

Covalent bonding

Polar covalent bonding

Ionic bonding

Page 48: Energy matters

Metallic Lattice

Page 49: Energy matters
Page 50: Energy matters

Covalent molecular

Page 51: Energy matters

Carbon atoms

Covalent bonds

Covalent network

Page 52: Energy matters

Electronegativity

• The greater the difference in electronegativity between two elements, the less likely they are to share electrons and form covalent bonds.

• Caesium fluoride is the compound with the greatest degree of ionic bonding.

Page 53: Energy matters

• Formed when atoms of different electronegativities bond to form a covalent compound.

• Bonding electrons are not shared equally.

• The atom with the greater share of electrons becomes slightly negative (δ-)

• The other atom becomes slightly positive (δ+)

• These molecules have a permanent dipole.

Polar covalent bonding

Page 54: Energy matters

Polar covalent bonding

Page 55: Energy matters

Ionic bonding

• Different elements have different attraction for bonding electrons, (electronegativity values).

• One atom may attract electrons very strongly and another atom may attract them very weekly and lets them go.

Page 56: Energy matters
Page 57: Energy matters

Ionic bonding

Page 58: Energy matters

Summary

Page 59: Energy matters
Page 60: Energy matters

Intermolecular forces of attraction

Page 61: Energy matters

Covalent molecular

Page 62: Energy matters

Intermolecular interactions

• Van der Waal forces are a result of electrostatic attraction between temporary dipoles and induced dipoles caused by movement of electrons in atoms and molecules.

• All covalent molecules interact by van der Waals bonding, as all molecules possess temporary dipoles.

Page 63: Energy matters

Halogens

• All halogen have 1 unpaired electron in the outer shell. Therefore form 1 pure covalent bond. E.g. F2, Cl2, Br2, I2

• These molecules interact only weakly by van der Waals’ mechanism, this makes them very volatile. (Fluorine & chlorine are gaseous).

Page 64: Energy matters

                                          

Permanent dipole

A molecule can be described as polar if it has a permanent dipole. A permanent dipole is due to a difference in electronegativity between the atoms involved in a covalent bond.

Page 65: Energy matters
Page 66: Energy matters

Symmetry

• Some molecules have a symmetrical arrangement of polar bonds.

• This cancels out the polarity over the molecule as a whole.

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Page 68: Energy matters

Polar or Non-polar?

Page 69: Energy matters

Boiling point• Polar molecules have higher boiling

points than non-polar molecules with similar molecular mass.

Page 70: Energy matters

Hydrogen bonds• Bonds consisting of a hydrogen atom bonded to an

atom of a strongly electronegative element such as fluorine, oxygen or nitrogen.

Page 71: Energy matters

Water molecules

Page 72: Energy matters

Ice

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Page 74: Energy matters

Glycerol Sulphuric Acid

Phosphoric Acid

Page 75: Energy matters

Covalent molecular

Page 76: Energy matters

Carbon atoms

Covalent bonds

Covalent network

Page 77: Energy matters

Diamond

Page 78: Energy matters

Fullerenes• Discrete covalently

bonded molecules

• Consisting of pentagonal & hexagonal panels.

Page 79: Energy matters

Graphite

Page 80: Energy matters

Bonding, structure & properties of elements

Page 81: Energy matters

Groups 1,2 & 3• Not enough electrons to achieve full outer shell.

• Elements contribute electrons to a common ‘pool’ of delocalised electrons.

• This binds the resultant positive ions.

• Bonding is less directional, therefore metals are more ductile & malleable.

• Delocalised electrons, therefore conduct electricity.

Page 82: Energy matters

Metallic Bonding

Page 83: Energy matters

1 exception: Boron• Structure made up of

B12 groups, interbonded with other groups.

• This results in an element almost as hard as diamond.

Page 84: Energy matters

Group 4

• Standard structure: Infinite 3D network or lattice, e.g. diamond, silicon.

• Therefore exceptionally hard & rigid.

• No discrete molecules, each atom joined to another.

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Diamond

Page 86: Energy matters

Graphite

Page 87: Energy matters

Fullerenes• Discrete covalently

bonded molecules

• Consisting of pentagonal & hexagonal panels.

Page 88: Energy matters

Phosphorus (group 5)

• Phosphorous bonds to 3 other phosphorous atoms to form tetrahedral P4 molecules.

• Fewer electrons in P4 than S8 make van der Waals forces weaker in phosphorous, therefore lower m.p.

Page 89: Energy matters

Group 6

• Oxygen: 2 unpaired electrons, therefore forms 2 pure covalent bonds.

• Intermolecular interactions are weak van der Waals, therefore volatile & gaseous.

Page 90: Energy matters

Sulphur

• Sulphur atoms can bond to more than one other sulphur, forming an 8 member ring.

• Van der Waals forces strong enough to make sulphur a solid at room temperature.

Page 91: Energy matters

Groups 5, 6 & 7

• Intra molecular forces (bonds within molecules) are covalent.

• Intermolecular forces are very weak van der Waals forces.

• Therefore most elements are volatile even if solid at room temperature.

• This is due to the little energy required to break intermolecular forces in order to melt/boil.

Page 92: Energy matters

Bonding in elements: Noble gases

• There are no covalent or ionic bonds between atoms in group 8.

• Uneven distribution of electrons within the atom produce temporary (or transient) dipoles on the atom.

Page 93: Energy matters

Solvent action

• In general polar solvents dissolve polar substances and ionic substances.

Page 94: Energy matters

Non polar solvents…(e.g hexane)

• Dissolve non polar solvents

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Page 96: Energy matters

The Avagadro constant

• 1 mole of any element contains the same number of atoms.

• This number is known as the Avagadro constant.

• This constant is given the symbol (L) after the first person to calculate a numerical value.

Page 97: Energy matters

Avagadro constant (L)

• One mole of any substance contain L, 6.02x1023 formula units.

Page 98: Energy matters

Formula units• For metals & monatomic species e.g. Noble

gases, a formula unit is an atom.

• Thus 4g helium

40g of calcium

197g of gold

Contain L Contain L (6.02x10(6.02x102323) ) atomsatoms

Page 99: Energy matters

Covalent substances• A formula unit is a molecule• The total number of atoms can be found by

multiplying L by the number of atoms in the molecule.

Quantity of substance

Number of molecules

No. of atoms per molecule

Total No. of atoms

2g of Hydrogen, H2

18g of Water, H2O

30g of ethane, C2H6

L

L

L

2

3

8

2L

3L

8L

Page 100: Energy matters

Ionic compounds• Formula unit consists of a ratio of ions

expressed by ionic formula.

Quantity of substance No. of formula

units

No. of +ve and –ve ions

Total No. of ions

58.5g of Na+Cl-

74g of Ca2+ (OH-)2

342g of (Al3+)2(SO42-)3

L

L

L

LNa+ and LCl-

LCa2+ and 2LOH-

2L Al3+ and 3L SO4

2-

2L

3L

5L

Page 101: Energy matters

Example 1

• How many molecules are there in 8.8g of CO2?

1 mole of CO2 contains L molecules

44g of CO2 contains L molecules

1g of CO2 contains L/44 molecules

8.8g of CO2 contains L/44 x 8.8 molecules

= 1.204 X 10= 1.204 X 102323 molecules molecules

Page 102: Energy matters

Example 2

• What mass of Nitrogen gas contains 18.06x1022 atoms of Nitrogen?

6.02x1023 molecules of N2 1 mole

6.02x1023 molecules of N2 28g

1 molecule of N2 28/L

18.06x1022 molecules of N2 28/L x 18.06x1022

= 8.4g

Therefore 8.4g of N2 gas contains 18.06x1022 molecules

4.2g of N2 gas contains 18.06x1022 atoms

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Page 104: Energy matters

Molar volume

• The volume occupied by one mole of gas at specific temperature and pressure.

• At room temperature and pressure, i.e. 20°C and 1 atmosphere pressure, the molar volume of any gas is approximately 24 litres mol-1

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Molar volume

• Volume of gas changes if the temperature and/or pressure changes.

• Therefore you must specify at what temperature and pressure the volume is being measured.

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Mass

Volume Density

Page 107: Energy matters

GFM

DensityVmol

Density in g l-1Molar volumeIn litres mol-1

Page 108: Energy matters

Example 1

(a) D = GFM / Vmol

= 20.2 / 24

= 0.84 g l= 0.84 g l-1-1

(b) V = GFM / Vmol

= 17 / 24

= 0.71 g l = 0.71 g l -1-1

• Calculate the density in g l-1 of the following gases at room temperature. The molar volume under these conditions is 24 litres mol-1.

(a) Neon (b) Ammonia

Page 109: Energy matters

Gas Formula Density (gl-1) Molar volume (litres mol-1)

Methane CH4 0.65

Oxygen O2 1.33

Nitrogen N2 1.15

Carbon dioxide

CO2 1.81

Argon Ar 1.63

24.6

24.0

24.3

24.3

24.5

Page 110: Energy matters

V

n Vmol

Volume of gasIn litres

No. of moles

Molar volumeIn litres mol-1

Page 111: Energy matters

Example 2

• The molar volume at 0°C and 1 atmosphere pressure is 22.4 litres mol-1, Calculate

(a) The volume of 0.025 mol of oxygen

(b) The no. of moles of nitrogen in 4.48 litres under these conditions.

(a) Volume of oxygen V = n X Vmol= 0.025 X 22.4= 0.56 litres

= 560cm= 560cm33

Page 112: Energy matters

(b) No. of moles of Nitrogen in 4.48 litres under these conditions?

No. of moles of nitrogen, n = V/Vmol

= 4.48/22.4

= 0.2 moles= 0.2 moles

Page 113: Energy matters
Page 114: Energy matters

Example 1• Calculate (i) the volume of oxygen required for the

complete combustion of 100cm3 of ethane and (ii) the volume of each product.

2C2H6(g) + 7O2(g) 4CO2(g) + 6H2O(g)

2 mol 7 mol 4 mol 6 mol2 vol 7 vol 4 vol 6 vol

Simplified ratio1 vol 3.5 vol 2 vol 3 vol

(i) 100cm3 of ethane requires 350cm350cm33 O O22 and (ii) produces 200cm200cm33 CO CO22 and 300cm300cm33 H H22O.O.

Page 115: Energy matters

Example 2• A mixture of 20cm3 propane and 130cm3 Oxygen was

ignited and allowed to cool. Calculate the volume and composition of the resulting gaseous mixture.

C3H8(g) + 5O2(g) 3CO2(g) + 4H2O(l)

1 mol 5 mol 3 mol 4 mol1 vol 5 vol 3 vol -

20cm3 propane requires 5 x 20 = 100cm3 Oxygen. Oxygen in excess by 30cm3 (130cm3 – 100cm3)CO2 formed = 3 x 20 = 60cm3

Resulting gas mixture = 30cm30cm33 O O22 and 60cm and 60cm33 COCO22..


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