The Reality of Heating Things Up
Imagine you have a block of silver, and you start heating it up. You might intuitively think that adding a certain amount of heat will always raise its temperature by the exact same amount. But nature is a bit more complicated than that!
As the silver gets hotter, its atoms vibrate more intensely, and it actually becomes slightly harder to raise its temperature further. This means its heat capacity, Cp, isn't a constant number—it increases with temperature.
In our problem, the molar heat capacity is given by the temperature-dependent function:
Cp=23+0.01T
We need to find the total heat added at constant pressure. In thermodynamics, the heat exchanged at constant pressure is exactly what we call the change in enthalpy, ΔH.
The Master Equation
Kirchhoff's Law
Because the heat capacity is constantly changing as the temperature rises, we cannot just use the simple formula ΔH=nCpΔT. That elementary formula only works if the heat capacity is perfectly constant!
Instead, we have to use the power of calculus to account for the continuous change. We need to add up all the infinitesimal amounts of heat required for each tiny increase in temperature.
This means we need to integrate. The total enthalpy change is the integral of the number of moles,
n, times the molar heat capacity,
Cp, with respect to temperature:
ΔH=∫T1T2nCpdT
The Calculus of Heat
Let's set up our integral with the given values. We are given that we have 3 moles of silver, so n=3.
We are heating the silver from an initial temperature of 300 K to a final temperature of 1000 K. These will serve as the lower and upper limits of our definite integral.
Substituting our temperature-dependent function for
Cp, we get a clear mathematical path forward:
ΔH=∫30010003(23+0.01T)dT
Now for the fun part—performing the integration! We can pull the constant 3 outside the integral to keep our calculation clean.
Inside, we integrate term by term. The integral of the constant 23 is simply 23T. For the second term, we use the power rule, making the integral of 0.01T equal to 20.01T2.
Putting this together, we are ready to apply our limits:
ΔH=3[23T+20.01T2]3001000
Crunching the Numbers
It's time to apply the upper and lower limits. A quick tip here: instead of calculating the whole expression twice, you can apply the limits to each term individually.
For the first term, we have 23(1000−300). For the second term, we have 0.005(10002−3002).
Watch out for silly mistakes here—it is the difference of the squares, not the square of the difference!
ΔH=3[23(1000−300)+0.005(10002−3002)]
Let's crunch these numbers carefully. 1000−300 is 700, and 23×700 gives us 16100.
Now for the squares: 10002 is 1,000,000, and 3002 is 90,000. Subtracting those gives us 910,000.
Multiplying
910,000 by
0.005 gives us
4550. So, inside our brackets, we have:
ΔH=3[16100+4550]
We are almost at the finish line! Adding the terms inside the bracket gives us 20650.
Multiplying this by the 3 moles we left outside gives us exactly 61950 J.
Looking at our options, they are all in kilojoules. Dividing by 1000, we get 61.95 kJ, which is incredibly close to 62 kJ. This matches our first option perfectly!