If Kc = 0.405 at 40.°C and Kc = 0.575 at 90.°C, what is ΔH° for the reaction? RXN is simply x yields y and reverse
Van Hoff equation mate.
But do I need to rearrange it?
You have to solve for \(\Delta H^{\circ}\) of cause. But the van't Hoff equation is given by: \[\Large \frac{ d \ln(K) }{ dT }=\frac{ \Delta H^{\circ} }{ RT^{2} }\] Solve the differential equation we get \[\Large \ln(\frac{ K_{2} }{ K_{1} })=\frac{ - \Delta H^{\circ} }{ R } \times \left( \frac{ 1 }{ T_{2} }-\frac{ 1 }{ T_{1} } \right)\] Solve for standard enthalpy and we are there.
Can you help me solve for h? Can't you just use algebra instead of calculus?
I don't see what the problem is. The last part is just algebra (solving for \(\Delta H\))?
You don't have to solve the differential equation.. I've already done that for you.
Thanks.
Else let me fast show how I fast figure out how to solve the problem. We are interesting in some expression with \[\Large \frac{ \partial K }{ \partial T }\] We can relate the Gibbs free energy to the equilibrium constant from the known equation \[\Large \Delta G^{\circ}=-RT \ln(K)\]\[\Large \ln(K)=-\frac{ \Delta G^{\circ} }{ RT }\] Differentiation of ln K with respect to temperature \[\Large \frac{ d }{ dT }\ln(K)=-\frac{ 1 }{ R }\frac{ d }{ dT }\left( \frac{ \Delta G^{\circ} }{ T } \right)\] Using the Gibbs-Helmholtz expression we can evaluate the differential for Gibbs free energy. The Gibbs-Helmholtz expression is given by \[\Large \left( \frac{ \partial }{ \partial T } \frac{ \Delta G ^{\circ} }{ T } \right)_{p}=-\frac{ \Delta H ^{\circ} }{ T^2 }\] Substute we get the Van't Hoff equation \[\Large \Large \frac{ d \ln(K) }{ dT }=\frac{ \Delta H^{\circ} }{ RT^{2} }\] Now we need solve the equation. We choose to assume that \(\Delta H^{\circ}(T)\) is constant in the temperature interval [\(T_{1},T_{2}\)], we can then take \(\Delta H^{\circ}(T)\) out of the integral and treat it as a constant. Using separation of variables and integration in the respective intervals we get \[\Large \ln(T_{2})-\ln(T_{1})=\frac{ \Delta H^{\circ} }{ R }\int\limits_{T_{1}}^{T_{2}}T ^{-2} dT\] Solve the integral we get the solution I wrote \[\Large \ln(K_{2})-\ln(K_{1}) =\ \frac{ - \Delta H^{\circ} }{ R } \times \left( \frac{ 1 }{ T_{2} }-\frac{ 1 }{ T_{1} } \right)\] Solve for the standard enthalpy, \(\Delta H^{\circ}\) \[\Large \Delta H^{\circ}=-R\left( \frac{ \ln(K _{2})-\ln(K_{1}) }{\frac{ 1 }{ T_{2}}-\frac{ 1 }{ T_{1} } } \right)\]
Sorry in the 7th expression I wrote \[\large \ln(T_{2})-\ln(T_{1})\] I meant \[\large \ln(K_{2})-\ln(K_{1})\] It should however not totally destroy the mathematical context.
If you like to have fun with thermodynamics we can choose to change a bit in our approximations. In the previous method we chooses to assume that \[\Large \left( \frac{ \partial \Delta H^{\circ} }{ \partial T } \right)_{p}=\Delta C _{p}^{\circ}=0\] We can make a more exact calculation and this time assume that the change in standard heat capacity, \( \Delta C_{p}^{\circ}\) remains constant in the temperature interval [\(T_{1},T_{2}\)], so our approximation build on \[\Large \left( \frac{ \partial ^{2} \Delta H^{\circ} }{ \partial T^2 } \right)_{p}=\left( \frac{ \partial \Delta C _{p}^{\circ} }{ T } \right)_{p}=0\] Doing this we can solve the Van't Hoff equation to \[\ln(K_{2})-\ln(K_{1})=-\frac{ \Delta H^{\circ}(T_{1})- \Delta C_{p}^{\circ} T_{1} }{ R }\left( \frac{ 1 }{ T_{2} }-\frac{ 1 }{ T_{1} } \right)+\frac{ 1 }{ R } \Delta C_{p}^{\circ} \ln \left( \frac{ T_{2} }{ T_{1} } \right)\] This expression is more complex as we now take into account that the enthalpy is temperature dependent.
Correction! \[\large \left( \frac{ \partial \Delta C_{p}^{\circ} }{ \partial T } \right)_{p}\] Forgot a partial sign the mathematical expression of the second possible approximation.
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