14 The IDEAL GAS LAW. and KINETIC THEORY Molecular Mass, The Mole, and Avogadro s Number. Atomic Masses
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1 14 The IDEAL GAS LAW and KINETIC THEORY 14.1 Molecular Mass, The Mole, and Avogadro s Number Atomic Masses The SI Unit of mass: An atomic mass unit is de ned as a unit of mass equal to 1/12 of the mass of an atom of carbon-12 ( 12 6 C). It is equal to 1: kg (see below). Symbol: u (in some older texts: amu)
2 A Z X nomenclature: A is the mass number; Z is the atomic number; N is the neutron number: A=Z+N. For a given chemical element Z is xed, e.g. Z=6 for carbon, while N may vary, giving several isotopes. [WEBSITE: UPSCALE at UofT: - look for Nuclear Constants ] Let m be the mass of atom / molecule: m = () molar mass N A number of moles: n = N N A = m mass per mole Periodic Table on the inside back cover of text: carbon in nature: m (C) = 12:011 u N.B. m 12 6 C = 12 u (exactly) Molecular Mass: the sum of the masses of its component atoms, e.g. H 2 O:
3 2(1:00794 u) + 15:9994 u = 18:0153 u N.B. He, Ne, Ar, Xe are monatomic; while H 2, N 2, O 2 are diatomic, as gases in nature. The Mole and Avogadro s Number The SI Unit of amount of substance: A mole is de ned as the amount of substance of a system that contains as many elementary entities as there are atoms in 0:012 kilograms of carbon-12. The elementary entities must be speci ed and may be atoms, molecules, ions, electrons, other particles, or speci ed groups of particles. Symbol: mol Avogadro s number N A = 6: mol 1 [CODATA inside front cover] CAUTION: this SI Unit refers to a GRAM-MOLE of substance! One mole of carbon-12 has a mass of 12
4 grams, or kg. One mole of natural carbon has a mass of grams, or kg. ADDED CALCULATIONS (see Ex. 6 - later) m 12 6 C = 0:012 kg 6: = 1: kg m (1 u) = : kg = 1: kg If we use a kilogram-mole we must count 1000 times as many molecules: 6: = 6: m (H) = 1:00794 kg 6: = 1: kg which is slightly more than the mass of 1 1H, because of deuterium, 2 1 H. m (proton) = 1: kg Ex. 1: Hope Diamond - monatomic carbon
5 (44:5 carats) 0:2 g 1 carat = 8:9 g 8:9 g 1 mol 12:011 g = 0: 741 mol 0: 741 mol 6: atoms 1 mol = 4: atoms Rosser Reeves Ruby - Al 2 O 3 m (Al 2 O 3 ) = 2 (26:9815 u) + 3 (15:9994 u) = 101:96 u (138 carats) 0:2 g 1 carat = 138=5 g = 27: 6 g 27: 6 g 1 mol 101:96 g = 0: 271 mol 0: 271 mol 6: molecules 1 mol = 1: molecules 14.2 The IDEAL GAS LAW
6 Recollect Chapter 12 and Figures 12.3, 12.4, but now use the Kelvin scale instead of Celsius DRAW FIG PRESSURE versus TEMPERATURE at CONSTANT VOLUME The graph is a straight line which extrapolates to absolute zero. Also the pressure is proportional to the number of molecules, and inversely proportional to the volume (Boyle s Law). We assume that the density is low enough so that the molecules do not interact except during elastic collisions. GOOD SIMULATION ON WEB:
7 IDEAL GAS LAW: The absolute pressure P of an ideal gas is directly proportional to the Kelvin temperature T and the number of moles n of the gas and is inversely proportional to the volume of the gas: P V = nrt (14:1) where R is the universal gas constant and has the value 8.31 J= mol K 1 in SI units. If N is the total number of particles: N = nn A, so P V = nn A RNA T = NkT where Boltzmann s constant k = R NA = 1: J K 1 Then the ideal gas law is P V = NkT (14:2)
8 Ex. 2: Alveoli air sacs absolute pressure: P = 10 5 Pa radius: r = 0:125 mm, V = 4 3 r3 body temperature: T = 310 K h N = P kt V = (105 Pa) 43 (0: m) 3i (1: J K 1 )(310 K) = 1: Since air is 14% O 2, (85% N 2, 15% Argon), number of oxygen molecules =0:14N = 2: CEx. READ 3 - Beer Bubbles expand when they rise!-! Problem 22
9 CO 2 bubble at depth of 0.2 m: volume V 2 ; pressure P 2 = P 1 + gh, P 1 = P atm = 1: Pa Ideal gas law (or Boyle s law): P 1 V 1 = P 2 V 2 V 1 V = P 2 2 P = P atm+gh 1 1: P atm = 1+ gh P atm = 1+ (1000)(9:8)(0:2) 1: = i.e. a 2% increase in volume. Boyle s Law - TRSP FIG P _ 1=V P i V i = P f V f (14:3) Ex. 4: Scuba Diving - READ Charles Law (Gay-Lussac) V i T I = V f T f (14:4)
10 14.3 KINETIC THEORY of GASES The Distribution of Molecular Speeds TRSP FIG Maxwell-Boltzmann curves Kinetic Theory TRSP FIG The essence of this idea goes back to Newton:. Calculate the pressure due to molecules impacting the walls of a container of gas (assume square of side L). Consider motion along the x -direction: average force = final momentum initial momentum time between collisions = ( mv) (mv) 2L=v = mv2 L Total force: F = N mv 2 3 L
11 where v 2 is the square of the root-mean-square speed: v rms = v 21 2 Then P = F L 2 = N mv 2 rms 3 L 3 Since V = L 3, P V = 2 3 N 1 2 mv 2 rms (14:5) We see that the bracket is just the average translational kinetic energy KE = 1 2 mv2 rms : P V = 2 3 N KE Comparing with the ideal gas law, P V = NkT : KE = 1 2 mv2 rms = 3 2kT (14:6) THUS the absolute Kelvin temperature is expressed in terms of the mechanics of particles. They move faster when the temperature is hotter, and vice versa.
12 CEx.5 - A single particle does not have a temperature. Ex. 6: Speeds of Molecules (14:6)! v rms = 1 2KE 2 m Take T = 293 K: KE = 3 2 kt = 3 2 1: J K 1 (293 K) = 6: J () m = molar mass N A v rms (N 2 ) = 9 m= s v rms (O 2 ) = 9 m= s 2(6: J) 2 = 510: 28 g mol 1 =(6: mol 1 ) 2(6: J) 2 = 477: 32 g mol 1 =(6: mol 1 )
13 v rms (H 2 ) = 6 m= s 2(6: J) 2 =1911: 2 g mol 1 =(6: mol 1 ) CEx. 7 - Hydrogen escapes the atmosphere of Earth. The escape velocity is 2GM R 1 2 = 2(6: )(5: ) 2 6:3810 = 11182: m= s 6!Problem 32: At what temperature is v rms (H 2 ) of hydrogen equal to this escape velocity? 1911 m= s 1 T K = m= s! T = K = 10032: K ALT: (14:6)! T = mv2 rms 3k
14 ! 2 g mol 1 =(6: mol 1 )(11182: m= s) 2 3(1: J K 1 ) = K Brownian motion of pollen in water - Einstein in 1905 showed that this was due to impacts of molecules. The Internal Energy of a Monatomic Ideal Gas This is useful in Chapter 15. For a monatomic ideal gas: U = N A 32 kt, or since N A k = R: U = 2 3 nrt (14:7) *14.4 Di usion - READ IF INTERESTED- (MCAT?) [TRSP FIG ]
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