Q.At 298 K, Kp for the reaction N2O4(g) ⇌ 2NO2(g) is 0.98. Predict whether the reaction is spontaneous or not.
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🔒 Start your 14-day free trial to unlock the full solution →Concept understanding — Gibbs Free Energy from K
Gibbs Free Energy from K — The Bridge Between Thermodynamics and Equilibrium
Imagine you're pushing a heavy box across a rough floor. You push hard, but the box barely moves. The potential to move is there — you're applying force — but the actual motion is tiny. That's the difference between thermodynamic spontaneity (the push) and equilibrium (where the box sits, barely budging).
Gibbs Free Energy (ΔG) tells you the push — whether a reaction can happen. The equilibrium constant K tells you how far it actually goes before stopping. The equation that links them is one of the most powerful in chemistry:
ΔG∘=−RTlnK
Let's unpack this from the ground up.
Step 1: What is ΔG?
Gibbs Free Energy change (ΔG) measures the maximum useful work a reaction can do at constant temperature and pressure. More practically:
- If ΔG<0: the reaction is spontaneous (it can happen on its own).
- If ΔG>0: the reaction is non-spontaneous (it needs energy input).
- If ΔG=0: the system is at equilibrium — no net change.
But here's the catch: ΔG depends on how much reactant and product you have at any moment. It's not a fixed number.
Step 2: Standard vs. Non-standard Conditions
Chemists define a standard state (pure substances at 1 bar, 1 M concentration for solutions, 25°C usually). Under those conditions, the free energy change is called ΔG∘ (standard Gibbs free energy change).
But real reactions rarely start at standard conditions. So we have:
ΔG=ΔG∘+RTlnQ
where Q is the reaction quotient (ratio of products to reactants at that instant, raised to their stoichiometric coefficients).
R is the gas constant (8.314 J/mol·K), T is temperature in Kelvin. The ln is natural log.
Step 3: At Equilibrium — The Key Insight
At equilibrium, the reaction has no net tendency to go forward or backward. That means:
ΔG=0
And the reaction quotient Q becomes exactly the equilibrium constant K.
So plug into the equation:
0=ΔG∘+RTlnK
Rearrange:
ΔG∘=−RTlnK
That's it. This single equation connects a thermodynamic property (ΔG∘) with a concentration-based constant (K).
Step 4: What This Tells You
| ΔG∘ value | K value | Meaning |
|---|---|---|
| Negative (<0) | K>1 | Products favoured at equilibrium |
| Zero (=0) | K=1 | Equal amounts at equilibrium |
| Positive (>0) | K<1 | Reactants favoured at equilibrium |
A negative ΔG∘ does not mean the reaction is fast — only that it's thermodynamically favourable. Kinetics (activation energy) is a separate story.
Step 5: A Concrete Example
Consider the reaction: N2(g)+3H2(g)⇌2NH3(g)
At 25°C, ΔG∘=−33.3 kJ/mol. Using R=8.314 J/mol⋅K:
−33,300=−(8.314)(298)lnK …
The key idea is that the standard Gibbs free energy change ΔG∘ is related to the equilibrium constant by ΔG∘=−RTlnKp. A negative ΔG∘ indicates a spontaneous reaction under standard conditions.
Step 1: Write the relation and substitute the given values.
R=8.314 J mol−1K−1, T=298 K, Kp=0.98.
Step 2: Compute lnKp. Since 0.98<1, ln(0.98) is negative.
ln(0.98)≈−0.0202.
Step 3: Calculate ΔG∘. …
The spontaneity of a reaction is determined by the sign of ΔG∘ (standard Gibbs free energy change), which is related to the equilibrium constant Kp by ΔG∘=−RTlnKp. Here, Kp=0.98<1, so lnKp is negative, making ΔG∘ positive — the reaction is non-spontaneous under standard conditions at 298 K.
The question asks whether the reaction N2O4(g)⇌2NO2(g) is spontaneous at 298 K, given Kp=0.98. The key is to connect the equilibrium constant to Gibbs free energy.
Spontaneity under standard conditions (1 bar pressure for gases, 1 M concentration for solutions, pure solids/liquids) is governed by the sign of ΔG∘. A negative ΔG∘ means the forward reaction is spontaneous; a positive ΔG∘ means it is non-spontaneous (the reverse reaction is spontaneous). The relationship is:
ΔG∘=−RTlnKp
Here, R is the gas constant (8.314 J/mol·K), T is the temperature in Kelvin, and Kp is the equilibrium constant in terms of partial pressures. This formula comes from the thermodynamic condition for equilibrium: at equilibrium, ΔG=0, and ΔG=ΔG∘+RTlnQ, where Q is the reaction quotient. Setting Q=Kp at equilibrium gives the equation above.
Now, let's work through the calculation step by step.
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Identify the given values.
T=298 K, Kp=0.98, R=8.314 J mol−1K−1.
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Compute lnKp.
Since Kp=0.98, which is slightly less than 1, ln(0.98) is a small negative number.
ln(0.98)≈−0.0202
(You can verify: e−0.0202≈0.98.)
- Plug into the formula.
ΔG∘=−(8.314)(298)ln(0.98)
First compute RT: 8.314×298≈2477.6 J/mol.
Then:
ΔG∘=−2477.6×(−0.0202)=+50.0 J/mol
More precisely, 2477.6×0.0202≈50.05, so ΔG∘≈+50 J/mol.
- Interpret the sign. ΔG∘ is positive (about +50 J/mol). Under standard conditions, a positive ΔG∘ means the forward reaction is non-spontaneous. The reverse reaction (2 NO₂ → N₂O₄) would be spontaneous. …
Showing the 12 most recent of 17 on this concept.
- TG EAPCET 2026Set eng-2026-05-09-AN1 markMCQQ.The ΔfHΘ of BaCO3 (s), BaO (s) and CO2(g) is respectively −1216.3, −553.5 and −393.5 kJ mol−1. What is the value of x (in kJ mol−1) in the following reaction? BaCO3 (s) Δ BaO (s) + CO2(g) −x (A) −269.3 (B) 269.3 (C) 2163 (D) −2163
›Reveal solutionSolution
ΔrHΘ=ΔfH(BaO)+ΔfH(CO2)−ΔfH(BaCO3)=+269.3 kJ mol−1, so x=269.3.
For BaCO3(s)→BaO(s)+CO2(g):
ΔrHΘ=[ΔfH(BaO)+ΔfH(CO2)]−ΔfH(BaCO3)
ΔrHΘ=[(−553.5)+(−393.5)]−(−1216.3)=−947.0+1216.3=+269.3 kJ mol−1 …
- TG EAPCET 2026Set eng-2026-05-10-AN1 markMCQQ.The transition temperature of sulphur is (A) 369 ∘C (B) 369 K (C) 133 K (D) 133 ∘C
›Reveal solutionSolution
The transition temperature of sulphur (rhombic to monoclinic) is a well‑known constant of 369 K (≈ 96 °C). The correct option is (B).
The question asks for the transition temperature of sulphur. This refers to the temperature at which the solid phase changes from the rhombic (α‑sulphur) to the monoclinic (β‑sulphur) form. This is a classic fact from solid‑state chemistry and phase diagrams. The key is to recall the value and its correct unit — many students confuse the Celsius and Kelvin scales.
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Recall the known value
The rhombic‑to‑monoclinic transition for sulphur occurs at 96 °C under standard pressure. This is a standard datum in textbooks.
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Convert to Kelvin
Since Kelvin = Celsius + 273.15, we have:
96+273.15≈369 K
(Often rounded to 369 K.)
- Match with the options
- (A) 369 °C → far too high (sulphur melts at ~115 °C).
- (B) 369 K → matches the conversion. …
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- TG EAPCET 2026Set eng-2026-05-11-FN1 markMCQQ.The difference between energy of an activated complex and the average energy of reactants is called? (A) Threshold energy (B) Lattice energy (C) Activation energy (D) Kinetic energy
›Reveal solutionSolution
The question asks for the term that describes the energy difference between the activated complex (transition state) and the average energy of reactants. That term is activation energy, so the correct option is (C).
The key concept here is reaction energy profiles and the transition state theory. In a chemical reaction, reactants must overcome an energy barrier to form products. The highest-energy, unstable arrangement along the reaction path is called the activated complex (or transition state). The energy required to go from the average energy of the reactants up to that peak is precisely the activation energy — it’s the “hump” that must be surmounted.
Let’s break down why each option fits or doesn’t:
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Understanding the definition
The difference between the energy of the activated complex and the average energy of the reactants is, by definition, the minimum energy that reactants must acquire to react. This is the activation energy (Ea). It is always positive for an endothermic or exothermic reaction (except in barrierless reactions, where it’s zero).
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Why not (A) Threshold energy?
Threshold energy is a related but distinct concept from collision theory: it is the minimum kinetic energy that colliding molecules must have for a reaction to occur. While it is numerically equal to activation energy in some simple models, the question specifically asks for the difference between the energy of the activated complex and the average energy of reactants — that is the textbook definition of activation energy, not threshold energy. Threshold energy is defined relative to the ground state of reactants, not their average energy.
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Why not (B) Lattice energy? …
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- TG EAPCET 2026Set ap-2026-05-04-FN1 markMCQQ.What is the enthalpy change (in kJ mol−1) for the following reaction? CCl4(g) → C(g) + 4Cl(g) (ΔvapHΘ(CCl4) = 30.5 kJ mol−1 ; ΔfHΘ(CCl4) = −135.5 kJ mol−1 ; ΔaHΘ(C) = 715.0 kJ mol−1 ; ΔaHΘ(Cl2) = 242 kJ mol−1) (A) 1304 (B) 326 (C) 1033 (D) 1199
›Reveal solutionSolution
The enthalpy change for atomising CCl4(g) into gaseous atoms is found by reversing its formation from atoms and adding the atomisation enthalpies of C and Cl2. The result is 1304 kJ mol−1, option (A).
The reaction CCl4(g) → C(g) + 4Cl(g) is the complete atomisation of gaseous carbon tetrachloride. We are not measuring this directly — we build it from known thermodynamic data using Hess’s law.
The key idea: the standard enthalpy of formation ΔfHΘ of a compound is the enthalpy change when it is made from its elements in their standard states. For CCl4(l), the standard state of carbon is graphite (C(s)) and of chlorine is Cl2(g). But our target starts from CCl4(g) and ends with gaseous atoms. So we need to:
- start with CCl4(g),
- break it down into its elements in standard states (reverse of formation),
- then atomise those elements into gaseous atoms.
We are given ΔvapHΘ for CCl4 — that tells us the liquid-to-gas step, because the formation enthalpy given is for the liquid, not the gas. Let’s work through it.
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Convert liquid CCl4 to gaseous CCl4
The given ΔfHΘ(CCl4)=−135.5 kJ mol−1 is for the liquid. Our target reaction starts with the gas, so we must first vaporise it:
CCl4(l)→CCl4(g), ΔH=+30.5 kJ mol−1 (endothermic).
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Reverse the formation of CCl4(g) from its elements
The formation reaction is:
C(s)+2Cl2(g)→CCl4(l), ΔH=−135.5 kJ mol−1.
But we need the gas, so combine step 1:
C(s)+2Cl2(g)→CCl4(g), ΔH=−135.5+30.5=−105.0 kJ mol−1.
Reversing this gives:
CCl4(g)→C(s)+2Cl2(g), ΔH=+105.0 kJ mol−1.
-
Atomise carbon
C(s)→C(g), ΔaHΘ(C)=715.0 kJ mol−1.
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Atomise chlorine …
- TG EAPCET 2025Set eng-2025-05-02-FN1 markMCQQ.When electromagnetic radiation of wavelength 310 nm falls on the surface of a metal having work function 3.55 eV, the velocity of photoelectrons emitted is x×105 ms−1. The value of x is (Nearest integer) (me=9×10−31 kg) (A) 2 (B) 4 (C) 5 (D) 6
›Reveal solutionSolution
The photoelectric effect gives the kinetic energy of emitted electrons as the photon energy minus the work function. Using the given wavelength and work function, the electron velocity is found to be about 4×105 m/s, so the nearest integer x is 4.
Concept & Intuition
This is a classic photoelectric effect problem. When light of a certain frequency (or wavelength) hits a metal, each photon can transfer its energy to an electron. If the photon’s energy exceeds the metal’s work function (the minimum energy needed to free an electron), the excess becomes the electron’s kinetic energy. The kinetic energy then determines the electron’s speed via K=21mv2. The key is to convert all units consistently — here, photon energy is in joules (from wavelength) and work function is given in electronvolts, so we must convert eV to joules.
Step-by-step solution
- Find the photon energy in joules The energy of a photon is E=λhc, where h=6.63×10−34 J⋅s, c=3×108 m/s, λ=310 nm=310×10−9 m.
E=310×10−9(6.63×10−34)(3×108)=3.1×10−71.989×10−25≈6.416×10−19 J.
- Convert the work function to joules Work function ϕ=3.55 eV. Since 1 eV=1.6×10−19 J,
ϕ=3.55×1.6×10−19=5.68×10−19 J.
- Compute the kinetic energy of the photoelectron By Einstein’s photoelectric equation:
K=E−ϕ=(6.416−5.68)×10−19=0.736×10−19 J.
- Relate kinetic energy to velocity K=21mev2, with me=9×10−31 kg. v2=me2K=9×10−312×0.736×10−19…
- TG EAPCET 2025Set eng-2025-05-04-AN1 markMCQQ.At 298 K the equilibrium constant for the reaction M(s) + 2Ag+(aq) → M2+(aq) + 2Ag(s) is 1015. What is the EcellΘ (in V) for this reaction? (F2.303RT)=0.06 V (A) 0.45 (B) 0.90 (C) 0.225 (D) 1.10
›Reveal solutionSolution
The key idea is to relate the equilibrium constant to the standard cell potential using the Nernst equation at equilibrium. The result is EcellΘ=0.45 V, which corresponds to option (A).
We are given a reaction between a metal M and silver ions, with an enormous equilibrium constant (1015). That tells us the reaction strongly favors products — so the standard cell potential must be positive and fairly large. The bridge between K and EΘ is the Nernst equation at equilibrium, where the cell potential is zero and the reaction quotient equals K.
- Recall the fundamental relation At equilibrium, the Nernst equation becomes:
EcellΘ=n0.0591logK(at 298 K, using F2.303RT=0.0591 V)
But here they give F2.303RT=0.06 V (a rounded value), so we use:
EcellΘ=n0.06logK
where n is the number of moles of electrons transferred in the balanced reaction.
- Determine n The reaction is:
M(s)+2Ag+(aq)→M2+(aq)+2Ag(s)
Each Ag⁺ gains one electron to become Ag, and two Ag⁺ ions are reduced, so total electrons transferred = 2. Also, M loses two electrons to become M²⁺. Hence n=2.
- Plug in the numbers
- TG EAPCET 2025Set ap-2025-04-29-AN1 markMCQQ.At T(K) 10 L of an ideal gas was expanded to 12 L against a pressure of 2 atm irreversibly. What is the work done by the gas? (A) −4 atm L (B) Zero (C) −240 atm L (D) −4 J
›Reveal solutionSolution
For an irreversible expansion against a constant external pressure, the work done by the gas is calculated using the external pressure and the change in volume. The work done is −4 atm L.
When a gas expands or contracts, it does work on its surroundings or has work done on it by the surroundings. The amount of work done depends on the path taken by the process.
For an irreversible process, especially when the expansion or compression occurs against a constant external pressure, the work done is determined by this external pressure, not the internal pressure of the gas. This is because the system (the gas) is not in equilibrium with its surroundings throughout the process. The external pressure is the opposing force that the gas must overcome to expand.
The work done (W) by a gas during an irreversible expansion or compression against a constant external pressure (Pext) is given by:
W=−PextΔV
where ΔV=V2−V1 is the change in volume.
The negative sign indicates that if the gas expands (ΔV>0), it does work on the surroundings, and W is negative. If the gas is compressed (ΔV<0), work is done on the gas by the surroundings, and W is positive.
Here, the gas is expanding, so we expect the work done by the gas to be negative.
-
Identify the given values:
- Initial volume, V1=10 L
- Final volume, V2=12 L
- External pressure, Pext=2 atm
- The process is irreversible.
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Calculate the change in volume (ΔV):
The change in volume is the final volume minus the initial volume.
ΔV=V2−V1=12 L−10 L=2 L
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Apply the formula for work done in an irreversible process: …
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- TG EAPCET 2025Set ap-2025-04-30-FN1 markMCQQ.The equilibrium constant for the reaction M(s) + 2Ag+(aq) → M2+(aq) + 2Ag(s) is 1015. What is the Gibbs energy change (ΔrGΘ in KJ mol−1) for this reaction? (FRT×2.303=0.06V;F=96500C mol−1). (A) −86850 (B) −96500 (C) −86.85 (D) −96.5
›Reveal solutionSolution
The key is linking the equilibrium constant to the standard Gibbs energy via ΔrGΘ=−RTlnK, and then using the given relation RT/F×2.303=0.06 V to compute the numerical value. The answer is -86.85 kJ mol⁻¹, which is option (C).
The problem gives you the equilibrium constant K=1015 for a redox reaction and asks for ΔrGΘ in kJ mol⁻¹. The direct thermodynamic link is the equation ΔrGΘ=−RTlnK. But here they’ve supplied a specific value for FRT×2.303=0.06 V, which is a hint that you can avoid plugging in R and T separately — just use this conversion factor.
Notice that lnK=2.303log10K, so ΔrGΘ=−RT×2.303log10K. And since FRT×2.303=0.06 V, you have RT×2.303=0.06F. This lets you compute ΔrGΘ directly in joules, then convert to kJ.
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Write the standard relation:
ΔrGΘ=−RTlnK=−RT×2.303log10K.
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Substitute log10K=log10(1015)=15:
ΔrGΘ=−RT×2.303×15.
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Use the given: RT×2.303=0.06×F, where F=96500 C mol⁻¹. So:
ΔrGΘ=−(0.06×96500)×15 J mol⁻¹.
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Compute stepwise:
0.06×96500=5790 J mol⁻¹.
Then 5790×15=86850 J mol⁻¹. …
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- TG EAPCET 2024Set eng-2024-05-10-FN1 markMCQQ.The standard enthalpy of combustion of C (graphite), H2(g) and CH3OH(l) respectively are −393, −286 and −726 kJ mol−1. What is the standard enthalpy of formation of methanol? (A) −726 kJ mol−1 (B) −239 kJ mol−1 (C) −96 kJ mol−1 (D) +96 kJ mol−1
›Reveal solutionSolution
Use Hess’s law: the enthalpy of formation of methanol is found by combining the combustion enthalpies of its elements and the combustion enthalpy of methanol. The result is −239 kJ mol−1, option (B).
The key idea here is Hess’s law: enthalpy change for a reaction is the same whether it happens directly or in steps. We want the enthalpy of formation of methanol, i.e., the enthalpy change for:
C(graphite)+2H2(g)+21O2(g)→CH3OH(l)
We are given combustion enthalpies, which are enthalpies of complete burning in oxygen. So we can think of building the formation reaction from combustion steps.
- Write the target formation reaction
C(s)+2H2(g)+21O2(g)→CH3OH(l)ΔHf∘=?
- Write the given combustion reactions
- Combustion of C(graphite):
C(s)+O2(g)→CO2(g)ΔH=−393 kJ/mol
- Combustion of H₂:
H2(g)+21O2(g)→H2O(l)ΔH=−286 kJ/mol
- Combustion of methanol:
CH3OH(l)+23O2(g)→CO2(g)+2H2O(l)ΔH=−726 kJ/mol
- Reverse the methanol combustion — because we want methanol as a product, not a reactant. Reversing changes the sign:
CO2(g)+2H2O(l)→CH3OH(l)+23O2(g)ΔH=+726 kJ/mol
- Add the combustion of C and 2× combustion of H₂ to the reversed methanol combustion, so that CO₂ and H₂O cancel.
- C combustion:
C(s)+O2(g)→CO2(g)ΔH=−393
- 2 × H₂ combustion:
2H2(g)+O2(g)→2H2O(l)ΔH=2×(−286)=−572
- Reversed methanol combustion:
- TG EAPCET 2023Set eng-2023-05-13-FN1 markMCQQ.Enthalpy of formation of CO(g), CO2(g) are −110, −393 kJmol−1 respectively. The enthalpy of combustion of CO (in kJmol−1) is (A) −283.0 (B) −110.5 (C) 504 (D) −221.2
›Reveal solutionSolution
The enthalpy of combustion of CO is found by applying Hess’s law: the combustion reaction is CO + ½O₂ → CO₂, and its enthalpy equals ΔH_f(CO₂) − ΔH_f(CO) = −393 − (−110) = −283 kJ mol⁻¹, so the correct option is (A).
The key idea is that enthalpy of combustion is just the enthalpy change when one mole of a substance burns completely in oxygen. For CO, the combustion reaction is:
CO(g)+21O2(g)→CO2(g)
We are given the standard enthalpies of formation:
- ΔH_f°(CO) = −110 kJ mol⁻¹
- ΔH_f°(CO₂) = −393 kJ mol⁻¹
Since enthalpy is a state function, we can use Hess’s law: the enthalpy change for a reaction equals the sum of the enthalpies of formation of products minus the sum for reactants.
- Write the target reaction
CO(g)+21O2(g)→CO2(g)
- Apply the formation enthalpy formula For any reaction:
ΔHrxn=∑ΔHf∘(products)−∑ΔHf∘(reactants)
Here, the only product is CO₂, and the only reactant with a non-zero formation enthalpy is CO (O₂ is an element in its standard state, so its ΔH_f° = 0).
- Plug in the numbers
ΔHcomb=ΔHf∘(CO2)−ΔHf∘(CO)
- TG EAPCET 2023Set ap-2023-05-10-AN1 markMCQQ.At 27∘C, the osmotic pressure of 0.5M solution of sucrose (in bar) is (R=0.083Lbarmol−1K−1) (A) 12.45 (B) 24.90 (C) 84.63 (D) 7.61
›Reveal solutionSolution
Osmotic pressure is a colligative property given by π=iCRT. For a non-electrolyte like sucrose, i=1, so π=CRT. At 27∘C (300K) with C=0.5M and R=0.083Lbarmol−1K−1, the osmotic pressure is 12.45bar, which corresponds to option (A).
Osmotic pressure is one of the four colligative properties — properties that depend only on the number of solute particles, not on their identity. The key formula is π=iCRT, where i is the van't Hoff factor (number of particles per formula unit in solution). Sucrose is a non-electrolyte; it dissolves as intact molecules, so i=1. That means the formula simplifies directly to π=CRT.
The temperature must be in Kelvin. 27∘C converts to T=27+273=300K. The concentration is given as 0.5M, which means 0.5 moles per litre. The gas constant R is provided in units of Lbarmol−1K−1, so the answer will come out directly in bar — no unit conversion needed.
- Write the formula: π=CRT.
- Substitute the values: C=0.5, R=0.083, T=300.
- Multiply: π=0.5×0.083×300.
- First, 0.5×300=150.
- Then, 150×0.083=12.45. …
- TG EAPCET 2022Set ap-2022-07-30-FN1 markMCQQ.The equilibrium constant Kc of the following reaction is 9 at a temperature T. A(g) + B(g) ⇌ C(g) + D(g) Assuming that the initial concentration of all the gases is 1 mole, what will be the concentration of A and C, respectively, at equilibrium? (A) 0.5 ; 1.5 (B) (1−103);(1+103) (C) 0.5 ; 0.5 (D) 1.5 ; 1.5
›Reveal solutionSolution
The symmetric equilibrium (Kc=9, all start at 1) gives x=0.5, so [A]=0.5 and [C]=1.5 — option (A).
Idea. Equal moles on both sides mean the total moles are unchanged, so we work directly with concentrations. Let x react.
ICE table. Start: [A]0=[B]0=[C]0=[D]0=1 M. Let x of A and B react:
[A]=1−x,[B]=1−x,[C]=1+x,[D]=1+x.
Equilibrium expression.
Kc=[A][B][C][D]=(1−x)2(1+x)2=9.
Solve. Take the positive square root (all concentrations positive for 0<x<1):
1−x1+x=3⇒1+x=3(1−x)⇒1+x=3−3x⇒4x=2⇒x=0.5.
Concentrations.
[A]=1−0.5=0.5 M,[C]=1+0.5=1.5 M. …
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