So, we know that the Gibbs Free Energy (\(\Delta G\)) is vital for determining spontaneity, but what about when conditions deviate from the ideal or ‘standard’? The 'standard' conditions refer to a specific set of pre-defined conditions: a temperature of 298K, 1 atm pressure, and all solutes at 1 M concentration. Under these conditions, the value of Gibbs Free Energy change (\(\Delta G^\circ\)) gives a baseline from which we can predict the behavior of substances. But reactions often occur under nonstandard reaction conditions, so we need to adjust our approach.
When conditions are nonstandard, concentrations, pressures, or temperatures will differ from the 'ideal' ones. Consequently, the actual Gibbs Free Energy (\(\Delta G\)) can still be determined by calculating deviations from standard state properties. This adjusted value tells us how far a system is from equilibrium under the given nonstandard conditions, informing us whether and in which direction a reaction will spontaneously proceed. Thus, assessing the reaction under both standard and nonstandard conditions paints a more accurate picture of the chemical process.