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Chapter 5: Gases. Pressure KMT Gas Laws Effusion and Diffusion Stoichiometry Real Gases Gas Mixtures. Properties of a Gas. State of Matter Compressible since molecules are far apart. Takes the shape and volume of container. Forms homogeneous mixtures with other gases.
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Chapter 5: Gases Pressure KMT Gas Laws Effusion and Diffusion Stoichiometry Real Gases Gas Mixtures
Properties of a Gas • State of Matter • Compressible since molecules are far apart. • Takes the shape and volume of container. • Forms homogeneous mixtures with other gases. • Pressure is a gas property which tells us about the amount of gas present.
PRESSURE • Pressure = Force/Area • Devices to measure pressure: manometer and barometer • Pressure Units (see p 181) • pascal = N/m2 = kg/(m s2) SI derived unit • 1 mm Hg = 1 torr • 1 std atm = 1 atm = 760 torr = 760 mm Hg = 1.01325E+05 Pa = @100kPa
GAS LAWS • These are empirical laws (based on expts rather than derived from theory) that define mathematical relationships between any two gas properties (P, V, T, n). • For example: If T and n are held constant, what happens to V if you increase P? • V will decreases: Boyle’s Law relates V vs P: V α 1/P or PV = k at constant n and T (Fig 5.5, 5.6).
GAS LAWS (2) • If P and n are held constant, what happens to V if you increase T? • V will increase: Charles’ Law relates V vs T (K): V α T or V/T = b at constant n and P (Fig 5.8, 5.9). • If P and T are held constant, what happens to V if n increases? • V will increase: Avogadro’s Law relates V vs n: V α n or V/n = a at constant P and T.
Figure 5.17 The Effects of Increasing the Temperature of a Sample of Gas at Constant Pressure
Figure 5.18 Increased Volume due to Increased Moles of Gas at Constant Temperature and Pressure
IDEAL GAS LAW PV = nRT • Combine Boyle, Charles and Avogadro’s Laws • Equation of state for ideal gas; hypothetical state • Note universality of equation; I.e. identity of the gas is not needed. • Limiting law (in the limit of high T and low P~1 atm); this means that as T increases and P decreases, real gases start to behave ideally.
IDEAL GAS LAW • R = Universal Gas Constant = PV/nT • 0.0821 (L-atm)/(mol-K) = 8.3145 J/(mol-K) • Note units of P = atm, V = L, T = K, n = #mol • STP = Standard Temperature and Pressure means 1 atm AND 273.15 K • Molar volume of a gas = Volume of one mole of gas at STP = 22.42 L (see T5.2)
OTHER • Use P, T and d to find molar mass (M) of gas. • Start with IGL: PV = nRT divide by VRT to get • n/V = P/RT then multiply by M to get • n (M)/V = d = MP/RT or M = dRT/P • Eqn 5.1
Problems • 19, 21, 34, 36, 42, 56, 62
STOICHIOMETRY of GAS PHASE REACTIONS • Use IGL to find # mol gas in stoichiometric problems • Law of Combining Volumes (Gay-Lussac) • Problems: 54, 58
MIXTURES of IDEAL GASES • DALTON’S LAW • Law of Partial Pressures • PTOTAL = P = ∑ Pi at constant T and V • Pi = niRT/V = partial pressure of a gas • xi = mole fraction = ni/nTOTAL = Pi/PTOTAL
Fig 5.12 The Partial Pressure of each Gas in a Gas Mixture in a Container Depends on n = #mol of that Gas
MIXTURES of IDEAL GASES • COLLECTING GASES OVER WATER • PTOTAL = P = Pg + Pw
Fig 5.13 The Production of O2 by Thermal Decomposition of KCIO3
Problems • 67, 72, 76
KINETIC MOLECULAR THEORY OF GASES (1) • Gas molecules are far apart form each other and their volumes are • They move constantly, rapidly and randomly in all directions and at various speeds. • There are no intermolecular forces between gas molecules except when they collide. Collisions are elastic.
Figure 5.19 Collisions with Walls and other Particles Cause Changes in Movement
Figure 5.20 A Plot of the Relative Number of O2 Molecules that Have a Given Velocity at STP
KINETIC MOLECULAR THEORY (2) • MEASURED PRESSURE OF A GAS IS DUE TO COLLISIONS WITH WALL. • COLLISIONS ARE ELASTIC. • THE AVERAGE KINETIC ENERGY OF A MOLECULE IS PROPORTIONAL TO T (K). • EXPLAINS MACROSCOPIC PROPERTIES LIKE P, T, V, v AND EMPIRICAL GAS LAWS.
KINETIC MOLECULAR THEORY (QUANT.) • Average kinetic energy = [(3/2) RT] α T • KE depends on T only • i.e. KE does not depend on identity of gas (M) • Root mean square velocity • urms = √(3RT/M) where R = 8.314 J/(K-mol) • As T increases, urms [dec, stays the same, inc] • As M increases, urms [dec, stays the same, inc]
Figure 5.21 A Plot of the Relative Number of N2 Molecules that Have a Given Velocity at 3 Temperatures
Figure 5.23 Relative Molecular Speed Distribution of H2 and UF6
EFFUSION AND DIFFUSION • Diffusion: Mixing of gases • Diffusion rate is a measure of gas mixing rate • Diffusion distance traveled α (1/√M) • Effusion • Passage of gas through orifice into a vacuum • Graham’s Law describes • Effusion rate α urms α(1/√M) α (1/T) • or Effusion time αM α (1/T)
Problems • 78, 80, 82, 88
REAL GASES • IDEAL: PV= nRT • van der Waals Eqn of State • PeffVeff = P’V’ = (Pobs + n2a/V2) (Vobs - nb) = nRT • 1st term corrects for non-zero attractive intermolecular forces • 2nd term corrects for non-zero molecular size • a and b values depend on the gas’s identity – loss of universality in gas law
KMT OF GASES (1-revisited) • GAS MOLECULES are FAR APART FROM EACH OTHER and THEIR VOLUMES ARE NOTNEGLIGIBLE. (b ≠ 0) • THEY MOVE CONSTANTLY, RAPIDLY and RAMDONLY IN ALL DIRECTIONS AND AT VARIOUS SPEEDS. • THERE ARE (NO) INTERMOLECULAR FORCES EXCEPT FOR COLLISIONS. (a ≠ 0)
Figure 5.25 Plots of PV/nRT versus P for Several Gases (200K)
Table 5.3 Values of the van der Waals Constants for Some Common Gases