Lecture 22: Gases 1 Read: HW: BLB 10.1–10.5 BLB 10.2,19a,b,23,26,30,39,41,45,49 Sup 10:1–6 Know: • gases & gas laws • PV=nRT(!!!!) • partial pressures • density & molecular mass Exam #2: “NO SCORE”? Not a problem. Please talk with Mike Joyce in 210 Whitmore Fina l Exa m: Wednesday, December 17 @ 8 am; MUST register on elion for a final exam conflict or overload by Oct 26. See http://www.registrar.psu.edu/exams/exam_overload.cfm http://www.psu.edu/dus/handbook/exam.html#conflict Need help?? Get help!! TAs in CRC (211 Whitmore) and SI—hours on Chem 110 website; my office hours (Mon 12:30-2 & Tues 10:30-12 in 324 Chem Bldg [or 326 Chem]) Sheets Page 1 Lecture 22 Itʼs a gas, gas, gas gas molecules: • are constantly • are far apart (10 times as far as they are big; occupy < 0.1% of the total volume) • move in lines from collision to collision • move at higher temperatures • move at lower temperatures as a result: • expand in whatever volume is available • have pressure (collisions with walls) • mix completely with one another • can be easily compressed • when cooled, will eventually condense (compression may be necessary) • gases are described in terms of (T), (V), & # (P), (n) • all gases behave similarly at low • gases will mix in all proportions with other gases to form mixtures Sheets Page 2 Lecture 22 Pressure • pressure: force/unit area force: kg•m•s–2, Newton (N) unit area: m2 • SI unit for pressure: 1 N•m–2 = 1 Pa (Pascal) • standard atmospheric pressure**: 1 atm ≡ 1.013 × 105 Pa 1 atm = 760 torr (or mm Hg) [1 atm = 14.7 lb/in2] **real atmospheric pressure varies with altitude, temperature and weather • how big is one atm? 10 tons / m2! or 600 lbs/head Sheets Page 3 Lecture 22 Measuring pressure • barometer used to measure Patm by balancing forces; (Torricelli, early 1600ʼs) • measure P in terms of height of Hg 1 atm ≡ 760 torr “=” 760 mm Hg [know this conversion!] [factoid: 760 mm Hg = 10 m H2O] Sheets Page 4 Lecture 22 The ideal gas law • state of gas described by: P, V, T in K (degrees Kelvin), & n • STP: standard temperature (273.15 K) & pressure (1 atm) NOTE: STP for gases is not the same as standard state conditions used for ΔH!! (more in Chap 5) • absolute temperature in Kelvin (K): °C + 273.15 = K • Avagadro: V ∝ n V/n = constant* (P,T fixed) *proportionality constant is the same for ALL gases V n Sheets Page 5 Lecture 22 The ideal gas law (cont.) • Boyle: V ∝ 1/P PV = constant (T,n fixed) V P V 1 atm 2 atm • Charles: V ∝ T V/T = constant (P,n fixed) note: T in absolute T (K)! 1/P 4 atm V -273.15°C = 0 K T (°C) • All of these laws can be described by one equation: PV = nRT • R = gas constant; units of R are very, very important! L atm J R = 0.08206 R = 8.314 mol K mol K cal R =1.987 mol K Sheets Page 6 Lecture 22 Example: • for problems: given known quantities, solve for the unknown What is the volume (V) occupied by 1.00 mole of gas at exactly 0°C and 1 atm (STP)? V =? P = 1atm n = 1mol T = 0° + 273 = 273K 0.08206L atm R= mol K Sheets PV = nRT Page 7 Lecture 22 Example: The gas in a 750 mL vessel at 105 atm and 27°C is expanded into a vessel of 54.5 L and –10°C. What is the final pressure? 1L $ ! V1 = 750mL # = 0.75L " 1000mL &% V2 = 54.5L P1 = 105atm T2 = !10° + 273 = 263K T1 = 27° + 273 = 300K P2 = ? PV = nRT so P1V1 = nRT1 n is not changing & R is a constant, so... nR = Sheets P1V1 T1 Page 8 & nR = P2V2 T2 Lecture 22 Density and molecular weight Example: can derive d = PM/RT from PV=nRT where d = density M = molar mass You should derive this on your own! (see BLB pp 406– 407) Calculate the average molar mass of dry air if it has a density of 1.17 g/L at 21°C and 740.0 d = 1.17g / L torr. ! 1atm $ P = ( 740.0torr ) # = 0.974atm " 760torr &% d = PM / RT Sheets T = 21° + 273 = 294K M =? Page 9 Lecture 22 Example: What is the density of oxygen, in grams per liter, at 25°C and 0.850 atm? d = ? need g / L P = 0.850atm T = 25° + 273 = 298K M = 32g / mol Sheets Page 10 Lecture 22 Daltonʼs law of partial pressures • partial pressure: the pressure a gas would have if it was the only gas in the container • Daltonʼs law of partial pressures: total pressure is equal to the sum of partial pressures Ptot = P1 + P2 + P3 + ... P= Ptot Ptot ntot nRT V n RT n2RT n3RT = 1 + + + ... V V V RT = ( n1 + n2 + n3 + ...) V = n1 + n2 + n3 + ... Ptot = ntot RT V • mole fraction: ratio of na/ntot; dimensionless Xa = na/ntot X 1 = n1 / ntot n1RT P1 = V n P1 = 1 Ptot ntot note: mole fractions must sum n1 ! ntot RT $ P = to 1 1 n #" V &% tot P1 = X 1Ptot Sheets Page 11 Lecture 22 Example: Mix 5 moles of CO2, 2 moles of N2 and 1 mole of Cl2 in a 40 L container at 0°C. (a) What is the pressure in the container? (b) What is the partial pressure of each gas in the container? (c) What volume does each gas occupy in the container? nCO 2 = 5mol nN 2 = 2mol nCl 2 = 1mol Ptot = ntot RT V Ptot = ntot = 8mol X CO 2 = XN2 = X Cl 2 = [ check: ! X = 1.000 ] V = 40L T2 = 0° + 273 = 273K Ptot = ? therefore, PCO 2 = PN 2 = PCl 2 = [ check: ! P = P tot Sheets Page 12 = 4.48atm ] Lecture 22 Example: 3.0 L of He at 5.0 atm and 25°C are combined with 4.5 L of Ne at 2.0 atm and 25°C in a 10 L vessel at constant temperature. What is the partial pressure of the He in the 10 L vessel? He (initial): VHe = 3L PHe = 5.0atm T = 25° + 273 = 298K nHe = PHeVHe RT nHe = ntot = nHe + nNe ntot = therefore, X He = X Ne = note: do not need X Ne for problem Ne (initial): VNe = 4.5L [ check: ! X = 1.000 ] PNe = 2.0atm T = 25° + 273 = 298K nNe = PNeVNe RT nNe = Sheets on to next page… Page 13 Lecture 22 Ptot in 10L vessel: (final) Vtot = 10L Ptot = ?? ntot = 0.981mol T = 25° + 273 = 298K Ptot = ntot RT Vtot Ptot = Now we need to find PHe (final) PHe = Sheets Page 14 Lecture 22 Before next class: Read: HW: BLB 10.6–9 BLB 10:5,8,59,61,71,75,77,82,83,84 Sup 10:7–15 Know: • kinetic-molecular theory • effusion & diffusion • real gases (van der Waals) Answers: p. 7: 22.4 L p. 8: Pfinal = 1.27 atm p. 9: 29.0 g/mol p. 10: 1.11 g/L p. 12: (a) Ptot = 4.48 atm; (b) PCO2 = 2.80 atm, PN2 = 1.12 atm, PCl2 = 0.56 atm; (c) 40 L p. 13: 1.5 atm Sheets Page 15 Lecture 22 Lecture 23: Gases 2 Read: Read: HW: BLB 10.6–9 BLB 10.6–9 BLB 10:5,8,59,61,71,75,77,82,83,84 Sup 10:7–15 Know: • kinetic-molecular theory • effusion & diffusion • real gases (van der Waals) Exam #2: “NO SCORE”? Not a problem. Please talk with Mike Joyce in 210 Whitmore Fina l Exa m: Wednesday, December 17 @ 8 am; MUST register on elion for a final exam conflict or overload by Oct 26. See http://www.registrar.psu.edu/exams/exam_overload.cfm http://www.psu.edu/dus/handbook/exam.html#conflict Need help?? Get help!! TAs in CRC (211 Whitmore) and SI—hours on Chem 110 website; my office hours (Mon 12:30-2 & Tues 10:30-12 in 324 Chem Bldg [or 326 Chem]) Bonus deadline for BST #8: Intermolecular forces, Oct. 30 Sheets Page 1 Lecture 23 Collecting a gas over water Example: During a reaction, N2 is collected over H2O. How many milligrams of nitrogen were collected under these conditions? Pbar = 742 torr (=Ptot); V = 55.7 mL; T = 23°C (296 K) NOTE: Ptot = Pgas + PH2O vapor vapor pressure at 23°C = 21.07 torr (BLB Appendix B) PN 2 = PN 2 = nN 2 = PN 2V RT nN 2 = Sheets Page 2 Lecture 23 Kinetic-molecular theory (KMT) • PV = nRT explains how gases behave • KMT explains why gases behave they way they do; gives a view of gases on a molecular level The 5 key postulates of KMT 1. -line motion in random directions 2. molecules are —volume they occupy is small compared to the total volume 3. intermolecular forces—molecules are not “sticky” 4. collisions 5. mean kinetic energy ε ∝ T (in K) != 1 mu 2 2 ε = average kinetic energy of a molecule m = mass of molecule (in kg) u = root mean squared (rms) speed of a molecule (in m/s) Sheets Page 3 Lecture 23 Kinetic-molecular theory (cont.) • KMT provides molecular level explanation for why gases behave as they do • T ↑ at constant (V, n) ⇒ P T ↑, ε ↑, u ↑; thus: more collisions per unit time & and harder collisions, so P • V ↑ at constant (T, n) ⇒ P constant T means constant ε & u; thus, longer distances between collisions & fewer collisions per unit time with walls, so P Sheets Page 4 Lecture 23 Temperature & molecular speeds • some molecules move slowly & some molecules move quickly: mean speed is in middle of of molecular speeds • entire distribution (& mean) shift ↑ for higher temperature; that is, when T ↑, fewer molecules move slowly, more molecules move quickly, so average speed ↑ Temperature & kinetic energy T! = 1 mu 2 2 ε = average kinetic energy of a molecule m = mass of molecule (in kg) u = root mean squared (rms) speed of a molecule (in m/s) != 1 3RT mu 2 = 2 2N N = Avagadroʼs number • at a given T, all gases have same average KE, independent of m & u; that is as m↑, u Sheets Page 5 Lecture 23 Diffusion & effusion • from KMT: 3RT u= M u = rms speed M = molar mass (this is not m from previous page!) • thus, gases with lower molar mass have higher rms speed • Grahamʼs law of effusion: r1 = r2 M2 M1 • effusion: escape of gas through a pinhole • diffusion: spread of one gas throughout a space or second substance; even though diffusion is more complicated (due to gas molecular collisions), it still obeys Grahamʼs law Sheets Page 6 Lecture 23 Collisions & diffusion • diffusion: movement of molecules interrupted by collisions • rate of diffusion follows Grahamʼs Law: depends on molecular speed & therefore, [1/M]0.5 • at STP, molecules collide ~1010 times/s for each molecule! • this means that although molecular speeds are high at STP, molecules donʼt go very far net distance traveled << (speed × time) • mean free path (mfp): distance traveled between collisions (~50 nm at 1 atm); mfp↓ as density (& P) ↑ factoid: if there were no collisions, O2 would traverse this room (~20 m) in ~0.04 s. BUT, in the absence of drafts, it takes many, many days!!?! Sheets Page 7 Lecture 23 Before next class: Read: HW: BLB 10.6–9 BLB 10:5,8,59,61,71,75,77,82,83,84 Sup 10:7–15 Know: • kinetic-molecular theory of real gases • real gases (van der Waals) Answers: p. 2: 60.9 mg Sheets Page 8 Lecture 23
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