The Magic of Phase Change
Imagine a beaker filled with exactly 90 g of liquid water, sitting on a hot plate. The temperature is a steady 100∘C (373 K). As you watch, the water begins to boil, transforming from a dense liquid into an expansive gas. This isn't just a physical transformation; it is a thermodynamic journey.
During this process, we are constantly pumping heat into the system. This heat is known as the enthalpy of vaporization, ΔHvap. But where does all this energy go? Does it all stay inside the water molecules, or is some of it spent doing something else? To answer this, we need to dive into the First Law of Thermodynamics and calculate the true change in the system's internal energy, ΔU.
Decoding the Moles
In the realm of chemistry, mass is just a stepping stone. The true currency of thermodynamics is the mole. The problem gives us the enthalpy of vaporization as 41 kJ/mol. This means it takes 41 kJ of energy to vaporize exactly one mole of water.
But we don't have one mole; we have 90 g. To find out how many moles we are dealing with, we divide the given mass by the molar mass of water (18 g/mol):
So, our system consists of exactly 5 moles of water undergoing a phase change.
The Chemical Equation of Phase Change
To understand the expansion work, we must look at the chemical equation for evaporation:
Initially, we have 5 moles of liquid water. Finally, we have 5 moles of water vapor. The change in the number of gaseous moles, denoted as Δng, is crucial because gases occupy significantly more volume than liquids.
Δng=ngas, products−ngas, reactants
This tells us that the system has generated 5 moles of new gas, which will push against the atmosphere, doing work.
The First Law of Thermodynamics
The First Law of Thermodynamics connects the heat added at constant pressure (Enthalpy, ΔH) to the change in internal energy (ΔU) and the expansion work done by the system (pΔV). For ideal gases, we can replace pΔV with ΔngRT. This gives us our master equation:
We want to find the internal energy change, so we rearrange the equation:
This equation tells a beautiful story: The change in internal energy is the total heat supplied minus the energy spent by the gas pushing the atmosphere away.
The Enthalpy of Vaporization
Before we plug numbers into our master equation, we need the total enthalpy change, ΔHtotal. The problem gives us the molar enthalpy, so we must scale it up for our 5 moles:
ΔHtotal=5 mol×41 kJ/mol=205 kJ
Because the universal gas constant R is given in Joules (8.314 J K−1mol−1), we must convert our enthalpy into Joules to avoid a catastrophic unit mismatch:
The Final Calculation
Now, we have all the pieces of the puzzle. Let's substitute them into our rearranged First Law equation:
The term (5×8.314×373) represents the expansion work. Calculating this gives:
Expansion Work=15505.61 J
Finally, we subtract this work from the total heat supplied:
ΔU=205000−15505.61=189494.39 J
The question asks us to round off to the nearest integer.
And there we have it! Out of the 205,000 J of heat we pumped into the water, about 15,505 J was spent pushing the atmosphere away to make room for the steam, leaving exactly 189,494 J to increase the internal energy of the water molecules.