The Temperature at Equilibrium[1] equation, T = ΔHrxn/ΔSrxn, estimates the temperature at which a process has reached equilibrium. This equation is derived from the Gibbs Free Energy and disorder laws (ΔG and ΔS). The inputs are as follows:
· T is temperature in Kelvin (K)
· ΔHrxn is the change in enthalpy over time with units of kilojoules per mole (kJ/mol)
· ΔSrxn is the change in entropy over time with units of kilojoules per mole*K (kJ/mol*K)
When entered into the calculator, ΔHrxn and ΔSrxn must have units of kJ/mol (or kJ/mol*K for ΔSrxn) in order to cancel out correctly. Due to the division, the kJ and moles will cancel, leaving only Kelvin (K) left as units for temperature.
We know the Gibbs Free Energy equation:
ΔGrxn = ΔHrxn - TΔSrxn
When ΔGrxn equals zero, we know the reaction has reached equilibrium. So, if we're trying to find the temperature at equilibrium, we can substitute zero for ΔGrxn:
0 = ΔHrxn - TΔSrxn
And after rearranging the substituted equation above, we get the Temperature at Equilibrium equation:
T = ΔHrxn/ΔSrxn
Whitten, et al. "Chemistry" 10th Edition. Pp. 594
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