Atomisation Enthalpy Solution: Definition, Enthalpy of Transition Elements, Examples

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Jasmine Grover

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Atomisation Enthalpy may be defined as the change in enthalpy which occurs primarily due to the breakage of one mole of bonds to form atoms in the gas phase. Chemical reactions are carried out in the lab under constant atmospheric pressure. Enthalpy, a thermodynamic concept, was established to examine reactions under constant pressure because internal energy was developed largely for volatile processes. 

Key Terms: Enthalpy, Atomization, Solution Enthalpy, Bond Enthalpy, Atmospheric Pressure, Diatomic Molecule, Molecule, Mean Bond Enthalpy, Vaporisation, Sublimation


Enthalpy of Atomization: Definition

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Before we can comprehend the enthalpy of atomization, we must first understand the number 'Enthalpy' H and how it came to be. The process of converting into atoms is known as ‘atomization’.

  • Chemical reactions occur in the laboratory under constant pressure, i.e., atmospheric pressure.
  • Because internal energy U, was designed primarily for constant volume reactions, enthalpy was developed to analyse constant pressure processes.
  • Every reaction requires energy to be absorbed or released. As a result, enthalpy influences temperature (H). 
  • Every natural process results in the creation of new objects. Some recognized human activity consumes energy, while others cause energy evolution. 
  • As a result, there is always a change in enthalpy when activities are completed. This enthalpy shift can be attributed to atomization enthalpy, solution enthalpy, or other factors.
  • Heat change may occur in various chemical reactions, including combustion, atomization, hydration, solution, neutralisation, and phase transitions, including vaporisation and fusion.

Enthalpy of Atomization of d-Block Elements

Enthalpy of Atomization of d-Block Elements


Enthalpy of Atomization: Reactions

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The enthalpy of atomization (ΔaH0) changes the enthalpy that happens when one mole of bonds is entirely broken to generate atoms in the gas phase. As an example, consider the atomization of a methane molecule.

C (g) → C (g) + 4H (g)\(\Delta\)aH0 = 1665.0 kJ mol-1

The Enthalpy of Atomization equals the enthalpy of bond dissociation for diatomic substances. As an example, consider the atomization of a hydrogen molecule.

H2 (g) → 2H (g); ΔaH0 = 435.0 kJ mol-1


Heat of Atomization

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The process of converting into atoms is referred to as atomization. It is the heat change in breaking one mole of a material's bonds into its atoms under normal circumstances (298K and 1 bar). The enthalpy of atomization is represented by the symbol \(\Delta\)aH0.

For molecular structures containing two atoms (diatomic molecule), consider the following scenario:

H2 (g) heat → H (g) + H (g) \(\Delta\)aH0 = +435.0 kJ mol-1

Dihydrogen is a diatomic molecule, and the energy given will be used to break the link, allowing the atoms to exist as gaseous particles. As a result, the Enthalpy of Atomization is never equal to zero. 

  • The heat of atomization is also known as the Heat Dissociation Enthalpy in the case of H2.
  • The Enthalpy of atomization equals the Enthalpy of bond dissociation in this case. Bond dissociation enthalpy is the change in enthalpy required in a gaseous state to break a mole of material's covalent bonds into its atoms. 
  • For all diatomic compounds, the Enthalpy of atomization equals the bond dissociation energy (Ex- Cl2, O2).
  • For polyatomic compounds, the enthalpy change of atomization is not the same as the energy of bond dissociation. For example, take methane,

CH4 (g) + C(g) + 4H(g) ΔaH0 = 1665 kJ mol-1

  • Even though the length and energy of the C-H bond are the same, the energy required to break the C-H bond varies. In this situation, the enthalpy change for the reaction 4H is 1665 kJ mol-1.
  • Mean bond enthalpy is employed in this case. Bond enthalpy is the average or means bond dissociation energy or bond enthalpy required to break a certain bond. The atomization energy of H2 is also known as the Heat Dissociation Enthalpy.
  • A bond's enthalpy fluctuates based on its chemistry. 
  • For common compounds such as Cl2, the atomization's bond dissociation enthalpy or heat is 242.5 kJ mol-1, and I2 is 242.5 kJ mol-1.

Enthalpy of Atomization of Transition Elements

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D-block elements are known to have greater boiling and melting points. The metallic bonding energy of a higher melting point element is larger. The atomization enthalpy determines the energy of metallic bonding. 

  • As the number of unpaired electrons in the d-orbital grows, so does atomization energy. 
  • The enthalpy of atomization of transition elements increases as the number of unpaired electrons increases. 
  • As the number of unpaired electrons grows, so do interatomic interactions. 
  • While travelling from left to right in a period, an increase in unpaired electrons is noticed when electron pairing occurs, melting temperatures in the second portion of the transition series fall.
  • For example, the melting point of cobalt is 1768K, while iron's melting point is 1808K. Iron has a higher enthalpy of atomization than copper due to the number of electrons in its d-orbitals. 
  • Iron's electronic configuration is 3d64s2, and 3d74s2 is cobalt’s electronic configuration. In total, there are three unpaired electrons. Because there are more unpaired electrons in iron, the enthalpy of atomization is higher.

Solution Enthalpy

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The enthalpy change, denoted by solH0, is the enthalpy change that happens when one mol of a chemical is entirely dissolved in a solvent. For example, the enthalpy of ionic chemical dissolution in water.

Solution Enthalpy

Solution Enthalpy


Different Transition Enthalpy

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Some energy is released or absorbed when a material undergoes a phase transition, which occurs when the phase of a substance transforms from one form to another. Energy is necessary when, for example, ice melts into water. 

Phase Transition

Phase Transition

Standard Enthalpy of Vaporisation

A form of heat transfer that occurs during the phase shift to a gaseous state is the standard enthalpy of vaporisation. Heat shifts and phase transitions are both connected. The enthalpy of vaporisation is the heat required to generate vapours from one mole of a liquid at constant temperature (boiling point) under normal conditions (1 bar pressure). The vaporisation enthalpy is denoted by \(\Delta\) H¯ vap o. For example, 

Nitrogen - 5.39 kJmol-1

NaCl - 170.0 kJmol-1

Vaporisation enthalpies also show the degree of intermolecular forces. The attraction forces are stronger when the enthalpy of vaporisation is larger. Because acetone has far weaker dipole-dipole interactions than water, it takes less heat to form vapours of its 1 mole.

Standard Enthalpy of Vaporisation of Zinc

Standard Enthalpy of Vaporisation of Zinc

Standard Enthalpy of Sublimation

The standard enthalpy of sublimation, subH0, is the change in enthalpy that occurs when one mole of a solid substance sublimes at constant temperature and pressure (1bar).

Enthalpy of Sublimation and Fusion

Enthalpy of Sublimation and Fusion

Enthalpy of Transition

Few reactions have enthalpies that cannot be determined directly. As a result, data on other enthalpies can be utilised to predict specific enthalpies indirectly. Hess' law may be used to calculate how allotropic rhombic sulphur transforms to monoclinic sulphur and graphite changes to diamond. The enthalpy of transition is difficult to compute. The heat of transition for allotropic elemental changes may be added using combustion enthalpy data. As an example, consider diamond and graphite. By subtracting the combustion of carbon in diamond form from the combustion of carbon in graphite due to this allotropic shift, the enthalpy of transition can be calculated.

Enthalpy of Phase Transition

Enthalpy of Phase Transition


Things to Remember

  • The enthalpy of atomization changes the Enthalpy when a mole of a substance in the gaseous state is broken down into its component atoms.
  • The enthalpy of the solution, also known as the enthalpy of dissolution or heat of solution, is the enthalpy change that occurs when a material is dissolved in a solvent under constant pressure, resulting in infinite dilution.
  • At constant temperature, the enthalpy of a solution is generally given as kJ/mol.
  • The enthalpy of combustion is the heat exchange that occurs when one mole of a substance is completely burnt or oxidised in oxygen.
  • The enthalpy change that occurs when one mole of a gaseous ionic compound dissociates into ions is the ionic compound's lattice enthalpy.
  • Bond enthalpy is the energy released when one mole of bonds is formed from isolated atoms in the gaseous state.

Sample Questions

Ques. Which of the elements among Sc and Zn have the greatest atomization enthalpy? How is the energy of atomization calculated? (2 marks)

Ans. Sc and Zn are elements in the third periodic table of the pf group. The amount of metallic bonding determines the atomization enthalpy of an element. The higher the metallic bonding of an element, the larger its atomization enthalpy. When the pressure remains constant, the change in Enthalpy is proportional to the change in the system's internal energy. As a result, the enthalpies of fusion and vaporisation equal the Enthalpy of atomization.

Ques. Why do greater atomization enthalpies characterise transition elements? What causes endothermic atomization enthalpy? (2 marks)

Ans. Transition elements have higher enthalpies of atomization because they have d- orbitals. The electrons in these d-orbitals are unpaired. Unpaired electrons improve interatomic interactions and, therefore, the heat of atomization. Transition enthalpies are greater in d-block elements with more unpaired electrons. The initial ionisation energy is defined as the energy necessary to remove one electron from each mole of free gaseous atoms of that element. Positive (endothermic) atomization and ionisation enthalpies remain.

Ques. What is the definition of Enthalpy of atomization? Is the bonding enthalpy the same as the atomization enthalpy? (2 marks)

Ans. Atomization enthalpy is the enthalpy change that occurs when a complex's bonds disintegrate, and component atoms are reduced to individual atoms. Ordinary atomization enthalpy is the enthalpy transition that occurs when 1 mol of material is entirely dissociated via atoms under normal circumstances (298.15 K, 1 bar). Atomization enthalpy is the enthalpy change that occurs when one mole of gaseous atoms is generated from atomic matter (atH). On the other hand, bond enthalpy/bond energy/bond dissociation enthalpy is the amount of energy required to break one mole of bond and produce separate atoms in a gaseous state.

Ques. Why does acetone have a lower enthalpy of evaporation than water? How do you calculate the Enthalpy of transition? (2 marks)

Ans. Acetone is a dipole-dipole organic compound with lower dipole-dipole interactions. The hydrogen bonding in water is stronger. The higher the forces of attraction, the more energy is required to generate vapours. At 1000°C, the standard Enthalpy of evaporation for water is 40.63 KJ mol-1, while the standard Enthalpy of evaporation for acetone is 31.3 KJ mol-1. The heat change that occurs during the interconversion of allotropic forms of elements such as carbon (as graphite and diamond) or sulphur (as monoclinic and rhombic) is referred to as the Enthalpy of transition. This Enthalpy of transition may be calculated indirectly using their respective enthalpy of combustion.

Ques. What are the differences between hydration and lattice energies? (5 marks)

Ans. Mentioned below are the differences between the two:

  • The amount of energy required to split one mole of crystal lattice into its constituent ions is called lattice energy. 
  • Ionic substances are naturally crystalline. They are made up of two pieces from distinct blocks. For example, NaCl Sodium belongs to the 1st group of the s block, while Cl belongs to the 17th group of the p block. 
  • The energies of these two elements' electrons differ greatly since they belong to different valence shells. However, both elements form ions and create strong ionic bonds. 
  • Some energy is released when creating an ionic bond, which results in the production of a crystal lattice. The lower the energy, the greater the stability. 
  • Every bond creation leads to a loss of energy. More energy is released during ionic bond formation. As a result, it is the most stable bonding. Lattice energy is the name given to released energy. 
  • The amount of energy released by component ions to produce one mole of the crystal lattice is also known as lattice energy. The energy required to break the crystal lattice into component ions is the same. 
  • The amount of energy released to split one mole of crystal lattice into its component ions in water is hydration energy. 
  • Because water provides the needed energy, the lattice energy is referred to as hydration energy; if another solvent is employed, it is referred to as solvation energy. The Born Haber Cycle may be used to compute hydration energy.

Ques. Why must the lattice enthalpy be less than the hydration enthalpy for the ionic component to dissolve in water? (3 marks)

Ans. They complement one another because the lattice dissociation enthalpy and the hydration enthalpy are components of the same overall process. The more complicated version is an application of Hess' Law, in which we measure the amount of energy required to break a solid ionic compound into its gaseous ions (which is generally endothermic, so a positive value) and then measure the amount of energy given off when the ion is bonded to a water molecule or group of water molecules (generally exothermic, so negative). Because the lattice dissociation enthalpy is the minimal amount of energy required to break up the solid, the energy released by ion hydration must be larger than the lattice energy keeping the solid together. The action can be seen as a group of water molecules “ripping" the ions off the material. They can't accomplish that if they aren't "strong" enough (releasing enough energy to overcome the lattice); thus, the solid stays together and doesn't melt.

Ques. Does hydration enthalpy contribute to lithium's maximum electrode potential (E°)? Also, why should hydration energy be larger than lattice energy for solubility? (3 marks)

Ans. Enthalpy of hydration is one of the heat changes considered in the computation of electrode potential. Because Li+ is so tiny, it has a very high enthalpy of hydration. As a result, the normal Li+/Li reduction potential is -3.05V. Caesium is the most powerful reducing agent in the gaseous form. Cs+ is less hydrated in an aqueous solution, contributing less to the electrode potential calculation. The hydration energy is the energy released when an ionic solid is dissolved in any solvent, usually water, whereas the lattice energy is the energy content of the lattice system. If salt is soluble, it has broken apart into ions, which means it is dissolved, and the dissolved energy is used to break the lattice, and we get ions. As a result, the hydration energy must be larger than the lattice energy for solubility.

Ques. What is the difference between Enthalpy of formation and lattice energy in this Born-Haber cycle? (4 marks)

Ans. The standard Enthalpy of formation consists of all the energy processes in a crystalline material's Born-Haber cycle. It is assumed that the elements begin in their most stable states at ambient temperature (298 K) and one atmosphere of standard pressure (760 torr). The earliest forms of the elements in caesium fluoride are solid for caesium and gas for fluorine.

  • Each element must first break apart and exchange electrons to produce ions, taking multiple processes. These phases either involve or generate energy, and one of the energy-producing steps is lattice energy. 
  • The energy gained when gaseous forms of ionised elements join together is lattice energy. If we started with already ionised elements, it would be the same as the Enthalpy of creation, but elements do not normally come as ions. 
  • Because they begin as neutral or molecules, extra procedures must be taken to prepare the elements for ionisation before reaching the lattice formation stage. 
  • We have distinct energy values for standard Enthalpy of formation and lattice energy. 
  • We have a crystalline solid and molecular gas as native forms of the components that make up our material.

Ques. Explain and offer arguments for (4 marks)
a) Why the electron gain enthalpies of noble gases are not negative?
b) Why are the initial ionisation enthalpies of nitrogen greater than those of oxygen?

Ans. (a) Noble gases have the most stable electronic configuration because they follow the octet rule. Even though they have a stable structure, gaining one electron requires a lot of energy, and their configuration becomes similar to group 1, which is extremely reactive. It has a positive electron gain enthalpy because of the high energy demand.

(b) Nitrogen's outermost electron configuration is homogenous, which increases its stability. Because of the greater stability in the electrical structure, it is more difficult to lose an electron from the outermost shell of nitrogen. Nitrogen, as a result, has a larger initial ionisation enthalpy than oxygen.

Explain and offer arguments for

Ques. Why is the usual enthalpy change of halogen atomisation half the bond energy of a halogen molecule? (2 marks)

Ans. The enthalpy of atomization is the change in enthalpy that happens when all atoms in a chemical substance are entirely separated (either a chemical element or a chemical compound). The symbols atHo is widely used to represent this. Because atomization breaks all bonds in the molecule and creates none, the enthalpies of atomization are always positive. The corresponding standard enthalpy at 298.15 K (or 25 degrees Celsius) and 101.3 kPa is known as the standard enthalpy of atomization. Because atomization involves the conversion of molecules into atomic form, which takes half a mole, and the standard enthalpy of the reaction deals with a full mole, the standard enthalpy of atomization is half that of the reaction's enthalpy.

Ques. What accounts for alkali metals' low atomisation enthalpy? (2 marks)

Ans. When the atoms require energy input to be separated, the enthalpies of atomization are considered positive. The introduction of extra electron shells causes the atomic radii of alkali metals to expand from top to bottom in a group. Because atoms with larger radii attract each other with less force than atoms with smaller radii, it is easier to separate larger atoms with less energy input, and hence alkali metals have a low atomization enthalpy.

Ques. Why do metals in the second and third transition series have greater atomisation enthalpies than metals in the first? (2 marks)

Ans. In the first transition sequence, only the d orbital is filled. In the second and third transition series, electrons are filled in both d and f orbitals. Nuclear screening is less effective for f orbital electrons than for d orbital electrons. As a result, the nuclear attraction felt by the outermost electrons in the second and third transition series is substantially greater. As a result, extracting an electron from metals in the second and third transition series becomes more difficult, requiring more energy. As a result, the greater the enthalpy.

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