Solving a Thermodynamics Problem

In summary, the problem involves finding the value of 'h' in a thermodynamics question, given the pressure at point X and the dimensions of fluid A (water) and B (mercury). The main equation used is absolute pressure = gauge pressure + atmospheric pressure, where gauge pressure is calculated using the formula rho*g*h. By setting the calculated gauge pressure for water equal to the gauge pressure for mercury at the same point, the value of 'h' can be determined. After solving for 'h', the final answer is 1.145m.
  • #1
brittt
4
0
Kinda lost...please help !

Hello,

There's this basic problem in thermodynamics that I'm stuck on. The question is

Fluid 'A' is water and 'B' is mercury. Determind the value of 'h' if the pressure at 'X' is 138 kN/m2 and 'a' is 1.5m
rhow = 1000 kg/m3
rhom = 13600 kg/m3

The main equation used is:
Absolute pressure = Gauge pressure + atmospheric pressure
Gauge pressure = rho * g * h

The value that you're supposed to get is 1.145m. Please help, I'm stuck on it for hours now and I'm sure its somethin basic that I've forgotten.

Here's a figure that might help with the problem:

http://s155.photobucket.com/albums/s300/br1ttt/?action=view&current=thermo.jpg

Many thanks,
-Brittt
 
Last edited:
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  • #2
You have atmospheric pressure outside, you have pressure X that's a bit higher in the vessel. Now just find the height difference (h-a) that corresponds to the pressure difference according to the formula you already wrote above.
 
  • #3
The given info is where you need to start. At X you have a given static pressure. Then you travel down the U tube to the bottom of dimension A. At that point, for the water you have the combination of the pressure at X and the rho*g*a contribution. That will give you a new static pressure at that point. At the point that coincides with the bottom of dimensions A and H, the pressure has to be equal. So you take your new pressure that you just calculated and set that equal to the rho*g*h for the mercury to calculate h.
 
  • #4
FredGarvin said:
The given info is where you need to start. At X you have a given static pressure. Then you travel down the U tube to the bottom of dimension A. At that point, for the water you have the combination of the pressure at X and the rho*g*a contribution. That will give you a new static pressure at that point. At the point that coincides with the bottom of dimensions A and H, the pressure has to be equal. So you take your new pressure that you just calculated and set that equal to the rho*g*h for the mercury to calculate h.

If i calculate as per your instructions, it would be:
X + rho * g * a
138 + 1000 * 9.81 * 1.5
14853 N/m2

Now,
14853 = rho * g * h
h = 14853 / rho * g
h = 14853 / (13600 *9.81)
Therefore, h = 0.111328

But the solution is 1.145m :(

Thanks for trying to help...any other ideas?

Cheers,
-Brittt
 
  • #5
Aero Stud said:
You have atmospheric pressure outside, you have pressure X that's a bit higher in the vessel. Now just find the height difference (h-a) that corresponds to the pressure difference according to the formula you already wrote above.

In order to find the height difference, we need to know both the a and h, and 'h' is what we're expected to calculate.
 
  • #6
You have 138 KN/m^2=138,000 N/m^2 or 138 kPa. Put it in what you wrote already and you get the answer.

p.s. Your drawing doesn't make clear which material is where, so at first I thought you have water only in the ball so it didn't matter.
 
  • #7
The pressure at X is in kPa, NOT Pa. Your units are incorrect by a factor of 1000.

[tex]h=\frac{138x10^3 + (9.81*1000*1.5)}{9.81*13.6x10^3}[/tex]
 

1. What is the first step in solving a thermodynamics problem?

The first step in solving a thermodynamics problem is to clearly define the system and its boundaries. This will help determine the relevant variables and equations that need to be considered.

2. How do you determine the direction of heat transfer in a thermodynamics problem?

The direction of heat transfer can be determined by using the Second Law of Thermodynamics. This law states that heat will naturally flow from a higher temperature to a lower temperature.

3. What are the key equations used in solving a thermodynamics problem?

The key equations used in solving a thermodynamics problem include the First Law of Thermodynamics (energy conservation), the Second Law of Thermodynamics (entropy), and the ideal gas law (for ideal gas systems).

4. How do you handle non-ideal systems in thermodynamics problems?

Non-ideal systems can be more challenging to solve in thermodynamics problems. In these cases, additional equations and assumptions may be needed, such as equations of state for non-ideal gases or accounting for non-ideal processes like friction or turbulence.

5. Are there any common mistakes to avoid when solving a thermodynamics problem?

One common mistake to avoid when solving a thermodynamics problem is not properly tracking units throughout the calculations. It is important to consistently use the same units and convert them as needed to ensure accurate results. Additionally, it is important to carefully consider the assumptions made in the problem and make sure they are valid for the given scenario.

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