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11/1 Week 11 Topics: • More on diffusion (Study guide 17. Section 13.8.) • Osmosis (Study guide 17. Sections 13.9 and 13.10.) • Heat capacity (Study guide 18. Section 14.2.) • Phase transformations (Study guide 18. Section 14.3) Next deadlines: Friday Nov. 14 — Quiz #9 (14–15); requires lab 14 Thursday Nov. 27 — Quiz #10 (16–17); requires lab 17 (on pretest page in Blackboard) Final exam: Thursday December 04, 11:30am to 1:30pm, TBA 11/2 More on diffusion (Sec. 13.8) We have seen that thermal agitation causes a typical molecule to undergo a random walk, so that after a time t it has diffused by a typical distance p √ 2 Rrms = R = 6Dt For a spherical molecule, the diffusion constant is given by D= kB T 6πηr where r is the molecule’s radius, and η is the viscosity of the fluid in which the molecule is moving. 11/3 How can D be determined? One way is to let the molecules diffuse through a porous membrane, and to measure the concentration of molecules as time goes by. (The concentration C is the number of moles per unit volume.) Let a container be separated in half by a porous membrane of thickness ∆x and area A. C2(0) = 0 V V C1(0) ∆x Initially, side 1 of the container contains all the molecules, and side 2 is empty; the initial concentration C1 (0) of side 1 is high, and C2 (0) = 0. 11/4 As time goes by, C1 (t) decreases and C2 (t) increases, until equilibrium is reached and the concentrations becomes equal. C1 C2 t The number of moles of molecules going through the membrane per unit time is given by Flux (J) across membrane = C1 − C 2 1 ∆n =D A ∆t ∆x (Fick’s law) 11/5 As a consequence of this equation, the time evolution of C1 is given by ¸¾ ½ · 1 2DA t C1 (t) = C1 (0) 1 + exp − 2 V ∆x As t → ∞, C1 → 12 C1 (0) and C2 → 12 C1 (0); we have equal concentrations. Because A, ∆x, and V are all known, D can be determined by a measurement of C1 as a function of time. But molecules generally don’t actually diffuse across the whole membrane area A, but only through the pores in the membrane, which have an “effective” area Aef f < A, e.g., Aef f = 0.04A in Lab 17. Then you have to multiply your measured D by the ratio A/Aef f (= 25 in Lab 17). See also Text p. 13-29 and exercise 13-13. 11/6 What can a measurement of D tell us? A measurement of D can be converted into a determination of the molecule’s molar mass M . The molar mass is the mass of NA = 6.02 × 1023 molecules: 4π NA ρr3 M = NA (ρV ) = 3 where ρ is the molecule’s density. But the molecule’s radius r is determined by the diffusion constant: kB T D= 6πηr kB T r= 6πηD ⇒ So we find µ kB T 4π NA ρ M= 3 6πηD ¶3 11/7 Molar masses calculated using measured values of D from the last equation are sometimes too high, due to the presence of so-called “bound” water or due to non-spherical shape. Both of these effects reduce the measured value of D. Example 1: In a given time, protein A diffuses 3 times as far as protein B. What is the ratio MA /MB of their molar masses? (Assume that the proteins are spherical and have the same density.) 11/8 Osmosis (Secs. 13.9 and 13.10) The term osmosis refers to the diffusion of solvent molecules across a semi-permeable membrane that allows the solvent to pass through, but prevents the passage of the larger solute molecules. Osmotic pressure Consider the flow of water — the solvent — in the following experiment: A B pure water water + solute 11/9 Water flows from A to B because its concentration is initially smaller in B than in A (a number of water molecules were removed by the larger solute molecules). A B At equilibrium, the concentrations of water have equalized, but a pressure difference (measured by the difference in levels) has developed. This pressure difference is called the osmotic pressure Π (upper case pi). 11/10 If the solution is dilute, the osmotic pressure is given by PB − PA = Π = RT C where n(solute) C= V is the solute’s concentration (the number of moles of solute molecules per m3 of solution), R = 8.315 J/(K · mol) is the ideal gas constant, and T is the temperature (in K). These relations give Π in units of pascals. 11/11 In the text, S.G. and quizzes, concentration is sometimes expressed as m/V = ξ (grams of solute per unit volume). Conversion relation is C = ξ/M where M is the molar mass (in grams/mole). (But mole fraction is not used on quizzes.) Example 2: (Similar to text, Example 13-12) Suppose that 1.00 g of ovalbumin is dissolved in 1.00 L (= 1.00 dm3 ) of water on one side of a semi-permeable membrane. If the experiment is carried out at 20◦ C, by how much does the level of water rise because of the osmotic pressure? (The molar mass of ovalbumin is 44.6 kg/mol.) 11/12 Some terminology The molarity C of a solution is the number of moles of solute molecules per litre (1 L = 1 dm3 = 10−3 m3 ) of solution. (Notice this definition of C differs from the previous, in terms of the volume unit.) The molality Cos of a solution is the number of moles of solute molecules per kilogram of solution. A solute molecule that cannot pass through the semi-permeable membrane is said to be osmotically active; otherwise it is said to be osmotically inactive. (Only the osmotically active molecules contribute to the osmotic pressure.) 11/13 At low concentrations, the relation between molarity and molality is C = Cos ρ, where ρ is in units of kg/dm3 , but molality is not needed on quizzes. For water at 20◦ C, ρ = 1.00 kg/dm3 , so that molality and molarity are equal. Take this case in all following. The osmolarity of a solution is the number of moles of osmotically active solute species per litre of solution. Depending on the chemistry of the solute molecules, the solution’s osmolarity may not be equal to its molarity. An important example is NaCl, which in a solution ionizes into Na+ and Cl− . The osmolarity of the solution is therefore twice its molarity. 11/14 Osmosis in biological cells (For now, we assume the cells are placed in solution of osmotically active solutes, which cannot diffuse through the cell membrane) The membrane of a biological cell is semi-permeable, and the cell’s interior (the lumen) contains osmotically active material. The lumen is typically 0.30 osmolar. If the cell is placed in an environment with the same osmolarity (isosmotic or isotonic), then the concentration of water inside and outside the cell is the same, and there is no flow of water — this is good. 11/15 If the cell is placed in an environment with a smaller osmolarity (hypotonic), then the concentration of water is larger outside the cell, and water flows in. The cell swells and may burst (or lyse) — bad. If the cell is placed in an environment with a larger osmolarity (hypertonic), then the concentration of water is larger inside the cell, and water flows out. The cell shrinks — this is also bad. 11/16 Thus, the ideal cell environment has the same osmolarity as the lumen. If the cell is placed in a nonideal environment, then its volume will increase or decrease according to C1 (cell)V1 = C2 (cell)V2 where C1 (cell) is the initial osmolarity of the cell, C2 (cell) the final osmolarity of the cell (which at equilibrium equals the osmolarity Cout of the environment, which doesn’t change), V1 is the cell’s initial volume, and V2 is its final volume. The relation above follows because the number of moles n of the lumen does not change, and Ci (cell) = n/Vi . 11/17 Example 2: Red blood cells of osmolarity 0.30 are placed in a dilute solution of 0.12 molar NaCl in water. What will happen to the cells? If their volume changes, what is the percentage change? 11/18 Things are different if cells are placed in a solution containing osmotically inactive solutes, which can diffuse across the membrane. In this case, an “isosmotic” solution is not necessarily “isotonic”. (See text example 13-16 and Self-Test IV (SG 17), #4) Example 3 A particular type of cell is impermeable to Na+ and Cl− ions, but permeable to glycerol and water. A solution of 0.15 molar NaCL is isotonic for this type of cell. Will a solution of 0.30 molar glycerol be isotonic, hypotonic or hypertonic for this kind of cell? 11/19 Study guide 18 Heat In this final study guide we examine the flow of heat and its relation to changes in temperature. We will look into: heat capacity, phase transitions, heat conduction, convection, heat radiation, and Newton’s law of cooling. 11/20 Heat capacity (Sec. 14.2) Heat is a form of thermal energy that can be transferred from one body to another (eg. from a burner to a coffee pot). We denote a quantity of heat by the symbol Q; its unit is the Joule. The transfer of heat typically comes with a change of temperature: T increases if a body absorbs heat. The heat capacity of a body is a measure of how much energy is required to raise its temperature by 1 degree. 11/21 Since the amount of required heat increases with the mass of the body, we have heat = (heat capacity)(change in temperature) = (mass)(specific heat capacity)(change in temperature) The specific heat capacity C is the body’s heat capacity per unit mass. In symbols, Q = mC∆T where m is the mass of the body. The unit of the specific heat capacity is the J/(kg · K). 11/22 The specific heat capacity depends on the body’s composition, and it may also depend on temperature (See Table 14-1, given below). Substance C (J/(kg · K)) Aluminum 886 Lead 127 Ice 2100 Water (20◦ C) 4186 Ethyl alcohol (20◦ C) 2500 A substance like lead has a low specific heat capacity, and raising its temperature requires only a small quantity of heat. A substance like water has a high specific heat capacity, and raising its temperature requires a large quantity of heat (this is why water takes a long time to boil). 11/23 Example: A bucket containing 1.0 kg of water at 90◦ C is placed in contact with another bucket that contains 2.0 kg of water at 20◦ C. Heat is observed to flow from the hot bucket to the cold bucket until a common equilibrium temperature is reached. What is the equilibrium temperature? How much heat was lost by the first bucket? How much heat was gained by the second bucket? 11/24 Phase transformations (Sec. 14.3) Sometimes the absorbtion of heat by a substance does not translate into an increase in temperature: the temperature might, in fact, stay constant. This occurs during a change of phase, for example, when ice turns into liquid water. heat added −20 o temperature 20o 0o 11/25 Instead of going into an increase of temperature, the absorbed heat goes into the molecular reorganization that takes place during a phase transformation. (For example, ice’s crystalline structure is destroyed and the water molecules become only loosely bound.) The heat required to fuel a phase change for 1 kg of a given substance is called the latent heat L (unit J/kg). The heat required to fuel a phase change for a mass m of that substance is therefore Q(phase transformation) = mL The latent heat depends on the substance, and on the type of phase transformation (see Table 14-2 of the textbook). 11/26 Several types of phase transformations can occur: fusion (or melting): from solid to liquid vaporization: from liquid to vapour condensation: from vapour to liquid solidification: from liquid to solid sublimation: directly from solid to vapour Fusion and vaporization require heat, while condensation and solidification give off heat. The latent heats for fusion and solidification are equal; the latent heats for vaporization and condensation are also equal. 11/27 Example: An ice cube is dropped into a glass of scotch to cool the drink down to 0◦ C from 20◦ C. Supposing that the glass contains 3.4 × 10−2 kg of scotch (about 1.5 oz) and the ice cube has an initial mass of 7.5 × 10−3 kg, calculate the final mass of the ice cube after the drink has cooled down. (The specific heat capacity of scotch is 2.8 × 103 J/(kg · K) and the latent heat of fusion of ice is 3.34 × 105 J/kg.)