TOPIC 5: CHEMICAL ENERGETICS Flashcards

1
Q

[Units]
Enthalpy change, ΔH

A

kJ/mol or J/mol

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2
Q

[Recall]
Exothermic VS Endothermic

A

ΔH < 0 VS ΔH > 0
Heat released VS Heat absorbed
Surrounding temp increase VS Surrounding temp decrease
Products energetically more stable VS products energetically less stable

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3
Q

IMPT THINGS FOR THERMOCHEMICAL EQN / SOLVING QNS

A
  1. STATE SYMBOL
  2. MULTIPLY BY MOLE RATIO
  3. 3SF
  4. SIGN ( + / - )
  5. UNITS
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4
Q

[Definition]
Standard state

A

The standard state of a substance at a specified temperature is its pure form at 1 bar ( = 10^5 Pa), and 1 mole/dm^3 for solutions.

*Temperature usually 298K (25°C)

*NOT the stp in Gaseous State

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5
Q

[Definition]
Standard enthalpy change of formation

A

The standard enthalpy change of formation is the ENERGY CHANGE when 1 MOLE of a substance in its standard state is formed from its constituent elements in their standard states, at a specified temperature, usually 298K.

*Standard enthalpy change of formation of ELEMENTS in their standard states is ZERO

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6
Q

[Definition]
Standard enthalpy change of combustion

A

The standard enthalphy change of combustion is the ENERGY RELEASED when 1 MOLE of a substance is burnt in excess oxygen, with all reactants and products in their standard states, at a specified temperature, usually 298K.

*Standard enthalpy change of combustion of O2 (g) / H2O (l) / CO2 (g) is ZERO
O2 cos cannot combust further
H2O and CO2 cos they’re products of combustion

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7
Q

[Definition]
Standard enthalpy change of neutralisation

A

The standard enthalpy change of neutralisation is the ENERGY RELEASED when 1 MOLE of water is formed in the neutralisation reaction between an acid and a base, all in their standard states, at a specified temperature, usually 298K.

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8
Q

[Recall]
Why is the enthalpy change of neutralisation between a strong acid and base almost the same for all?

What is the general value of enthalpy change?

Why are reactions with weak acid / base slightly less exothermic than usual?

A

Complete dissociation, so the reactions between them are effectively the reaction between the aqueous H+ and OH- ions.

-57.0 kJ/mol

Do not dissociate completely, so energy is absorbed to dissociate the undissociated weak acid or base, so less exothermic.

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9
Q

[Defintion]
Bond Energy

A

Bond energy is the AVERAGE ENERGY REQUIRED to break 1 MOLE of a covalent bond between two atoms in the gaseous state.

*2 x ΔHat = BE

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10
Q

What is bond dissociation energy?

A

The energy required to break 1 mole of a PARTICULAR COVALENT BOND in a specific molecule in the gaseous state

*Bond dissociation energy may differ even for the exact same type of bond as the strength is also influenced by its neighbouring atoms

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11
Q

[Formulas]
Heat change & Enthalpy change

A

q = -mcΔT / q = -CΔT

ΔH = q / n = (-mcΔT)/(no. of moles of limiting reagent)

***Values are ALL about the WATER / SOLUTION, NOT the solid / substance
e.g. mass of solution, c of solution etc

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12
Q

[Definition] Specific Heat Capacity

A

The specific heat capacity, c, is definied as the amount of heat energy required to raise the temperature of 1g of the substance by 1K.

Unit of c: J g⁻¹ K⁻¹

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13
Q

[Definition] Heat Capacity

A

Heat capacity, C, is defined as the amount of heat required to raise the temperature of a certain mass of a substance by 1K.

Unit of C: J K⁻¹

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14
Q

Assumptions / Sources of errors in calorimetry experiments

A

Assumed negligible heat loss / heat gain from surrounding air / calorimeter

Density of solution is same as that of water

Incomplete combustion

Wick also burns and releases some heat

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15
Q

[Definition]
Hess’ Law

A

Hess’ Law states that the enthalpy change of a reaction is determined only by the initial and final states and is independent of the reaction pathway taken.

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16
Q

3 Ways of Presenting Hess’ Law

A

Energy Cycle & Energy Level Diagram & Algebraic Method

17
Q

[Recall]
Common Hess’ Law applications for combustion, formation and bond energy

A

ΔHr (combustion) =
∑mΔHc (reactants) - ∑nΔHc (products)

ΔHr (formation) =
∑mΔHf (products) - ∑nΔHf (reactants)

ΔHr (bond energy) =
∑BE (bonds broken) - ∑BE (bonds formed)

18
Q

Why is experimental value of enthalpy change of bond broken different from that of the theoretical value?

A

The bond energies given in the data booklet are the average bond energies of that particular covalent bond in different types of molecules. Thus, these values may not apply to the specific molecules in this reaction.

19
Q

[Definition]
Standard enthalpy change of atomisation (element & compound)

A

The standard enthalpy change of atomisation, for an ELEMENT is the ENERGY REQUIRED to form 1 MOLE of gaseous atoms from the element, all in their standard states, at a specified temperature, usually 298K.

The standard enthalpy change of atomisation, for a COMPOUND is the ENERGY REQUIRED to form gaseous atoms from 1 MOLE of the compound, all in their standard states, at a specified temperature, usually 298K.

*2 x ΔHat = BE

20
Q

[Definition]
Lattice energy

A

Lattice energy of a compound is the ENERGY RELEASED when 1 MOLE of a solid ionic compound is formed from its consitutent gaseous ions.

21
Q

[Factors]
Factors affecting lattice energy

A
  1. Charge
  2. Size

|LE|∝|(q⁺ * q⁻) / (r⁺ + r⁻)|

22
Q

[Definition]
Ionisation Energy (first and second)

A

The FIRST ionisation energy is the ENERGY REQUIRED to REMOVE 1 MOLE of electrons from 1 MOLE of gaseous atoms to form 1 MOLE of singly charged gaseous cations.

The SECOND ionisation energy is the ENERGY REQUIRED to REMOVE 1 MOLE of electrons from 1 MOLE of singly charged gaseous cations to form 1 MOLE of doubly charged gaseous cations.

*IE ALWAYS positive (aka endothermic)

23
Q

[Definition]
Electron affinity (first and second)

A

The FIRST electron affinity is the ENERGY CHANGE when 1 MOLE of electrons is added to 1 MOLE of gaseous atoms to form 1 MOLE of singly charged gaseous anions.

The SECOND electron affinity is the ENERGY CHANGE when 1 MOLE of electrons is added to 1 MOLE of singly charged gaseous anions to form 1 MOLE of doubly charged gaseous anions.

*1st EA usually negative (aka exothermic)
- more energy released from attraction than repulsion
*2nd EA usually positive (aka endothermic)
- more energy required to overcome repulsion than attraction

24
Q

[Recall]
Purpose of Born-Haber Cycle

A
  1. Impossble to generate measurable quantities
  2. Impossible to harness the ions to react with each other
  3. Impossible to measure chg in temp
25
Q

[Defintion]
Standard enthalpy change of hydration

A

The standard enthalpy change of hydration of an ion is the ENERGY RELEASED when 1 MOLE of free gaseous ions in its standard state is dissolved in water to give a solution of INFINITE DILUTION, at a specified temperature, usually 298K.

26
Q

[Factors]
Factors affecting standard enthalpy change of hydration

A

Charge density

|ΔHhyd|∝|q/r|

The higher the charge density, the stronger the ion-dipole interactions, the more exothermic it will be

27
Q

[Definition]
Standard enthalpy change of solution

A

The standard enthalpy change of solution of a substance is the ENERGY CHANGE when 1 MOLE of a substance is completely dissolved in a solvent to give a solution of infinite dilution, at a specified temperature, usually 298K.

*Substance usually ionic compound
*Solvent usually water

28
Q

[Formula]
Standard enthalpy change of solution

A

ΔHsol = -LE + ΔHhyd (cation) + ΔHhyd (anion)

29
Q

[Definition]
Entropy

A

Entropy, S, is a measure of the RANDOMNESS or DISORDER in a system, reflected in the number of ways that the energy of a system can be distributed through the motion of its particles.

ΔS = S (final) - S (initial)
ΔS > 0 (more ways to distribute energy)
ΔS < 0 (less ways to distribute energy)

30
Q

[Factors]
Factors affecting entropy

A
  1. Change in temperature
    - Temp increase, Average KE & range of energies increase, more ways energy can be distributed among the particles, entropy increases
  2. Change in phase
    - entropy of solid < liquid < gas
    - When melt / vaporize / sublime, particles in final state move more freely and more disordered, increase number of ways the particles and energy can be distributed, entropy increases
  3. Change in number of particles
    - more particles more ways the particles and energy can be distributed, entropy increases
  4. Mixing of particles (assuming ideal gas)
    - Volume of gas increase, more ways to distribute particles and their energy, entropy increases
31
Q

[Formula]
Gibbs Free Energy

A

ΔG = ΔH - TΔS

*ΔG < 0 (thermodynamically feasible & spontaneous)
*ΔG = 0 (equilibrium & no net reaction)
- during change in state
*ΔG > 0 (themodynamically not feasible & not spontaneous)

32
Q

[Recall]
Limitations of the use of ΔG to predict spontaneity of reaction

A
  1. All must be in their standard states
  2. Temperature must be achievable
  3. Kinetics considerations (may be spontaneous but not instaneous - not at observable rate)
33
Q

[Units]
Entropy change, ΔS

A

Jmol⁻¹K⁻¹ or kJmol⁻¹K⁻¹

34
Q

[Units]
Gibbs free energy, G

A

kJmol⁻¹ or Jmol⁻¹