What Is Lattice Energy and How Do Gaseous Ions Exist Under Standard Conditions?

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SUMMARY

Lattice Energy is defined as the enthalpy change when one mole of an ionic compound is formed from its gaseous ions under standard conditions, specifically at a pressure of 1 bar. Gaseous ions can exist under standard conditions by extrapolating their behavior from ideal gas laws at low pressures. Ionization energy and electron affinity are not thermodynamic quantities, thus they remain independent of temperature and pressure. The discussion emphasizes the importance of understanding these concepts in relation to Born-Haber cycles, which involve the calculation of lattice energy and related thermodynamic properties.

PREREQUISITES
  • Understanding of Lattice Energy and its definition
  • Familiarity with the Ideal Gas Law
  • Knowledge of thermodynamic quantities such as enthalpy
  • Basic concepts of Born-Haber cycles
NEXT STEPS
  • Research the concept of Born-Haber cycles in detail
  • Learn about the Ideal Gas Law and its applications
  • Study the differences between thermodynamic and non-thermodynamic quantities
  • Explore the implications of ionization energy and electron affinity in chemical reactions
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Chemistry students, educators, and professionals interested in thermodynamics, ionic compounds, and the principles governing lattice energy and related concepts.

PFuser1232
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My A level Chemistry textbook defines Lattice Energy as "the enthalpy change when 1 mole of an ionic compound is formed from its gaseous ions under standard conditions"; a definition which I can't fully grasp because of the "standard conditions" part. How can gaseous ions exist under standard conditions?
 
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That's a hypothetical point of reference. More precisely you extrapolate the enthalpy of a gas of the ionic compound from it's ideal behaviour at very small pressure to the value at 1 bar. So effectively you calculate with a gaseous phase at infinitely small pressure, but (more so for entropy than enthalpy) you have to fix units.
 
DrDu said:
That's a hypothetical point of reference. More precisely you extrapolate the enthalpy of a gas of the ionic compound from it's ideal behaviour at very small pressure to the value at 1 bar. So effectively you calculate with a gaseous phase at infinitely small pressure, but (more so for entropy than enthalpy) you have to fix units.

What about temperature? How can gaseous ions exist at room temperature? Also, just to be clear, does this apply for ionisation energy and electron affinity as well?
 
MohammedRady97 said:
What about temperature? How can gaseous ions exist at room temperature? Also, just to be clear, does this apply for ionisation energy and electron affinity as well?

Before discussing this any further, I want to point out that this question is probably not too relevant for what you are about (I suppose Born Haber cycles), as the ionization enthalpy does depend only to a minor extent on temperature and pressure.
This having been said, let's go on:
In principle there is always a gaseous phase at equilibrium with a solid. At low temperatures it will behave like an ideal gas as pressure is very low. Hence it is an easy exercise to extrapolate the ideal gas law to any pressure and temperature you like.

Ionisation energy and electron affinity aren't thermodynamic quantities, so they are independent of temperature and pressure.
 
DrDu said:
Before discussing this any further, I want to point out that this question is probably not too relevant for what you are about (I suppose Born Haber cycles), as the ionization enthalpy does depend only to a minor extent on temperature and pressure.
This having been said, let's go on:
In principle there is always a gaseous phase at equilibrium with a solid. At low temperatures it will behave like an ideal gas as pressure is very low. Hence it is an easy exercise to extrapolate the ideal gas law to any pressure and temperature you like.

Ionisation energy and electron affinity aren't thermodynamic quantities, so they are independent of temperature and pressure.

So is my textbook wrong in defining (the first) electron affinity as "the enthalpy change when 1 mole of electrons is added to 1 mole of gaseous atoms to form 1 mole of gaseous 1- ions under standard conditions."?
 
No, that's a correct definition. As DrDu stated several times, we EXTRAPOLATE to standard conditions. Otherwise we would have numbers that are not comparable.
 
Borek said:
No, that's a correct definition. As DrDu stated several times, we EXTRAPOLATE to standard conditions. Otherwise we would have numbers that are not comparable.

Yes, I am quite familiar with this now. But I was referring to his statement regarding the fact that ionization energy and electron affinity are not thermodynamic quantities.
 
DrDu said:
Before discussing this any further, I want to point out that this question is probably not too relevant for what you are about (I suppose Born Haber cycles), as the ionization enthalpy does depend only to a minor extent on temperature and pressure.
This having been said, let's go on:
In principle there is always a gaseous phase at equilibrium with a solid. At low temperatures it will behave like an ideal gas as pressure is very low. Hence it is an easy exercise to extrapolate the ideal gas law to any pressure and temperature you like.

Ionisation energy and electron affinity aren't thermodynamic quantities, so they are independent of temperature and pressure.

What about bond energy and atomisation enthalpy? Are those quantities thermodynamic? Also, on what basis do I judge whether or not a quantity is thermodynamic?
 

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