Understanding Osmotic Pressure: Equation and Explanation

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In summary, osmotic pressure is a way of thinking about the effect of solutes. It's not much different from hydrostatic pressure- given a semi-permeable membrane, one can interchange one for the other, and compensate for one gradient with another.
  • #1
john16O
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can anyone explain osmotic pressure along with its equation because I am having a hard time with this concept. Thank you!
 
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  • #2
Osmotic pressure is a way of thinking about the effect of solutes. It's not much different from hydrostatic pressure- given a semi-permeable membrane, one can interchange one for the other, and compensate for one gradient with another.

As it happens, I'm currently working through "Water Movement Through Lipid Bilayers, Pores, and Plasma Membranes" by Alan Finkelstein (1987).

What equation are you referring to?
 
  • #3
(pie)=nRT --> van't Hoff equation
 
  • #4
Oh, ok. Here goes... hoping my tex skills are up to the challenge:

First, let's start by writing down the chemical potential of water: this is the amount of energy required to add a molecule (or a mole) of water to a solution:

[tex]\mu_{W} =\mu^{(0)}_{W} + RT ln X_{W} + P\overline{V_{W}} [/tex]

Where [itex]\mu^{(0)}_{W}[/itex] is the chemical potential defined at STP, [itex]X_{W}[/itex] the mole fraction of water, [itex]\overline{V_{W}}[/itex] the partial molar volume, R the gas constant, P the hydrostatic pressure, T the temperature.

If we have two compartments separated by a water-permeable membrane, such that one has solute and the other does not, both compartments are at internal equilbrium, then [itex]\mu(1)_{W} = \mu(2)_{W}[/itex]. Substituting that big expression about for [itex]\mu_{W}[/itex], with the knowledge that X_W(2) is 1 (pure water) and that a hydrostatic pressure difference must exist to oppose the flow of water across the membrane, we get

[tex]\Pi\equiv[P(1) - P(2)] = -\frac{RT}{\overline{V_{W}}} lnX_{W}(1)[/tex]

Now, for a dilute solution ln(X) = X, and doing a few other manipulations of X into n you end up with the van't Hoff expression.

How's that?

Edit: oops, made an error in tex formatting.
 
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  • #5
wow!, thank you so much, you have defiantly cleared it up for me. thank you again!
 

1. What is osmotic pressure?

Osmotic pressure is the force that drives water molecules to move from a region of low solute concentration to a region of high solute concentration, across a semi-permeable membrane. It is a measure of the concentration gradient between two solutions.

2. What is the equation for osmotic pressure?

The equation for osmotic pressure is π = iMRT, where π is the osmotic pressure, i is the van't Hoff factor (a measure of the number of particles per molecule), M is the molar concentration, R is the gas constant, and T is the temperature in Kelvin.

3. How does osmotic pressure affect cells?

Osmotic pressure plays a crucial role in maintaining the balance of water and solutes inside cells. If the osmotic pressure outside the cell is higher than inside, water will move out of the cell, causing it to shrink. Conversely, if the osmotic pressure inside the cell is higher, water will move into the cell, causing it to swell and potentially burst.

4. How is osmotic pressure measured?

Osmotic pressure can be measured using an osmometer, which is a device that measures the pressure required to stop the movement of water across a semi-permeable membrane. This pressure is directly proportional to the osmotic pressure of the solution being measured.

5. What factors affect osmotic pressure?

Osmotic pressure is affected by the concentration of solutes, temperature, and the properties of the semi-permeable membrane. Higher solute concentrations, higher temperatures, and membranes with larger pores or lower permeability will result in higher osmotic pressures.

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