Analyzing the Setup
Imagine two identical cylindrical vessels standing side-by-side on a flat table.
Both vessels have the same cross-sectional area A and are filled with an incompressible liquid of density ρ.
Initially, a closed valve prevents any flow between them, keeping the liquid in the left vessel at a height h1 and the liquid in the right vessel at a height h2.
Because the heights are different, there is a pressure imbalance at the bottom.
Once the valve is opened, gravity will naturally drive the fluid from the higher column to the lower column until the levels equalize at a common height h.
Finding the Equalized Height
Since the liquid is incompressible, the total volume of the liquid is conserved throughout the process.
Let's write down the conservation of volume:
Dividing both sides by the area A, we find the final equalized height h is simply the arithmetic mean of the initial heights:
Gravitational Potential Energy of a Fluid Column
To calculate the work done by gravity, we must find the change in the gravitational potential energy of the system.
For a continuous, uniform fluid column of height H, the mass is distributed uniformly.
We can treat the entire mass m=ρAH as if it were concentrated at its center of mass, which lies exactly at its geometric midpoint:
Therefore, the gravitational potential energy U of a single column of height H is:
U=mgycm=(ρAH)g(2H)=21ρAgH2
This is a beautiful and powerful result: the potential energy of a uniform fluid column is proportional to the square of its height.
Calculating Initial and Final Potential Energies
Initially, the two columns are separate. The total initial potential energy Ui is the sum of their individual potential energies:
Ui=21ρAgh12+21ρAgh22=21ρAg(h12+h22)
In the final state, both vessels are filled to the equalized height h. The total final potential energy Uf is:
Now, substituting h=2h1+h2 into this expression:
Uf=ρAg(2h1+h2)2=41ρAg(h1+h2)2
Work Done by Gravity
According to the work-energy theorem, the work done by gravity W is equal to the loss in gravitational potential energy of the system:
Let's substitute our expressions for Ui and Uf:
W=21ρAg(h12+h22)−41ρAg(h1+h2)2
To simplify this algebraically, let's factor out 4ρAg:
W=4ρAg[2(h12+h22)−(h1+h2)2]
Expanding the terms inside the bracket:
W=4ρAg[2h12+2h22−(h12+h22+2h1h2)]
W=4ρAg[h12+h22−2h1h2]
Recognizing the perfect square identity h12+h22−2h1h2=(h1−h2)2, we arrive at the final elegant formula:
This positive work done by gravity represents the energy released as the fluid levels equalize, which is typically dissipated as heat due to viscous friction within the fluid.