A state function is a property that depends solely on the current state of a system, such as temperature, pressure, volume, internal energy, and entropy, rather than the path taken to reach that state. State functions are related through equations of state, like PV=nRT, and can be evaluated using differences (Δ) between states without needing to consider the process involved. While some calculations, like work done during variable pressure and volume changes, require calculus, the essential concept is that only a few state functions are needed to define a system's state. Gravitational potential energy can also be considered a state function, indicating a broader application beyond thermodynamics. Understanding state functions is crucial for grasping thermodynamic principles and their implications in various physical contexts.