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CHEMISTRY 161 Chapter 5. Classification of Matter. solid liquid gas. 1. Gases. substances that exist in the gaseous phase under normal atmospheric conditions. T = 25 o C p = 1 atm. HF, HCl, HBr, HI CO, CO 2 CH 4 , NH 3 , H 2 S, PH 3 NO, NO 2 , N 2 O
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CHEMISTRY 161 Chapter 5
Classification of Matter solid liquid gas
1. Gases substances that exist in the gaseous phase under normal atmospheric conditions T = 25oC p = 1 atm
HF, HCl, HBr, HI CO, CO2 CH4, NH3, H2S, PH3 NO, NO2, N2O SO2
Jupiter (H2, He) Io (SO2)
Helix Nebula Orion Nebula
2. Pressure Ar EXP I molecules/atoms of gas are constantly in motion
Standard Atmospheric Pressure 760 mm at 273 K at sea level Torricelli barometer 1 atm = 760 mm Hg = 760 torr pressure of the atmosphere is balanced by pressure exerted by mercury
SI units force pressure = area p = F / A [p] = Nm-2 = kg m-1 s-2 = Pa
pressure measurement manometer
3. Gas Laws 3.1. pressure p versus volume V 3.2. temperature T versus volume V 3.3. volume V versus amount n p, V, T, n
3.1. Boyle’s Law pressure – volume relationship (temperature is constant) Boyle (1627-1691)
p ∞ 1/V EXP II
p ∞ 1/V p = const/V p × V = const p1× V1 = const p2× V2 = const p1× V1 = p2× V2
3.2. Gay-Lussac’s Law temperature – volume relationship (pressure is constant) Gay-Lussac (1778-1850)
V ∞ T EXP III
V ∞ T V = const’ ×T V/T = const’ V1 / T1 = const’ V2 / T2 = const V1 / T1 = V2 / T2
3.3. Avogadro’s Law amount – volume relationship (pressure and temperature are constant) Avogadro (1776-1856)
n ∞ V n = const’’ × V n/V = const’’ n1 / V1 = const’’ n2 / V2 = const’’ n1 / V1 = n2 / V2
SUMMARY 3.1. Boyle’s Law 3.2. Gay-Lussac’s Law 3.3. Avogadro’s Law p ∞ 1/V V ∞ T n ∞ V
1. IDEAL GAS EQUATION (1) p ∞ 1/V V ∞ 1/p (2) V ∞ T V ∞ T (3) n ∞ V V ∞ n V ∞ T × n / p p × V = const × n × T
p × V = const × n × T p × V = R × n × T p × V = n × R × T ideal gas equation
p × V = n × R × T [R] = [p] × [V] / [n] / [T] m3 mol K Pa = N/m2 [R] = N × m / mol / K [R] = J / mol / K
[R] = J / mol / K R = 8.314 J / mol / K ideal gas constant
2. MOLAR VOLUME What is the volume of 1 mol of a gas at 273.15 K (0oC) and 1 atm (101,325 Pa)? standard temperature and pressure (STP) p × V = n × R × T V = 22.4 l EXP IV
p × V = n × R × T V = 22.4 l Vm = 22.4 l the molar volume at standard pressure and temperature is independent on the gas type
3. STOICHIOMETRY NaN3(s) → Na(s) + N2(g) How many liters of nitrogen gas are produced in the decomposition of 60.0 g sodium azide at 80oC and 823 torr? • Balancing • Mole ratios • Convert grams into moles • Convert moles into liters
4. DENSITY CALCULATION ς = m / V p × V = n × R × T V = n × R × T / p relate the moles (n) to the mass (m) via the molecular weight (M) m = n × M n = m / M ς = p × M / (R × T)
5. DALTON’S LAW pure gases gas mixtures (atmospheres) Dalton (1801)
DALTON’S LAW the total pressure of a gas mixture, p, is the sum of the pressures of the individual gases (partial pressures) at a constant temperature and volume p = pA + pB + pC + …. EXP V
p × V = n × R × T pA× V = nA× R × T pA = nA× R × T / V pB× V = nB× R × T pB = nB× R × T / V p = pA + pB p = (nA + nB) × R × T / V p × V = n × R × T
p × V = (nA + nB) × R × T pA = nA× R × T / V pA / p = nA /(nA + nB) = xA mole fraction x < 1 pA = xA × p
2 KClO3→ 2 KCl + 3 O2 EXP VI/VII
SUMMARY 1. ideal gas equation p × V = n × R × T R = 8.314 J / mol / K 2. molar volume Vm = 22.4 l
3. Density of gases ς = p × M / (R × T) 4. Dalton’s Law n p = Σ pi i=1
1. Kinetic Molecular Theory of Gases macroscopic (gas cylinder) microscopic (atoms/molecules) Maxwell (1831-1879) Boltzmann (1844-1906)
Kinetic Energy of Gases physical properties of gases can be described by motion of individual gas atoms/molecules each macroscopic and microscopic particle in motion holds an energy (kinetic energy)
Assumptions of the Kinetic Theory of Gases • gases are composed of atoms/molecules which are • separated from each other by a distance l much more than their • own diameter d d = 10-10 m l = 10-3 m….. few m molecules are mass points with negligible volume l
2. gases are constantly in motion in random reactions and hold a kinetic energy gases collide and transfer energy (billiard ball model)
3. gases atoms/molecules do not exert forces on each other (absence of intermolecular interactions) F(inter) = 0 p(inter) = 0
2.Distribution of Molecular Speeds Maxwell-Boltzmann distribution
3.Real Gases p × V = n × R × T (n = 1) deviation of ideal gas law at high pressures p ≈ 90 atm
North America Nebula p << 10-10 atm
ideal gas law p V = n R T real gas law (van der Waals equation) (p + (a n2 / V2) ) (V – n b) = n R T corrected volume (volume occupied by molecules) corrected pressure (additional pressure/force from attraction)