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Gases Solid Liquid Gas States of Matter Definite Definite Condensed Fluid volume Shape Phase Definite No Condensed Fluid Volume definite Phase shape No No Much definite definite lower volume shape density Gases at room temperature – can be cooled and compressed into the liquid phase Vapor – gas formed by evaporation or sublimation Properties of Gases 1. Gases can be compressed into smaller volumes ↑ P causes ↓ V therefore: ↑ P causes ↑density 2. Gases exert pressure on surroundings. So to confine a gas, pressure must be exerted on it. (Newton’s third law: for every action, there is an equal and opposite reaction) 3. Gases expand without limits, therefore a gas will completely fill the container it occupies 4. Gases diffuse into one another. Gases mix completely, i.e. gases are miscible. 5. The amount of gas can be known if the pressure, temperature and volume are known. Pressure – force / unit area Units: pounds / square inch (psi) Newtons / m2 (Pascals) Atmospheres (atm) mm Hg Torr 1 atm = 14.7 psi = 1.01 x 105 Pa = 760 mm Hg = 760 Torr = 33.8 ft water To measure pressure a. Barometer – the force of the atmosphere pushes the liquid up the tube. 1 atmosphere pushes a column of mercury 760 mm, water 33.8 feet b. and c. Manometer – the pressure of a gas is known by comparing it with the atmosphere Patm at sea level > Patm at higher elevations As your elevation increases, the mass of air above you decreases, thus less pressure Gas Laws Boyle’s Law ↑ P causes ↓ V V is proportional to 1/P PV = constant so ………………..P1V1 = P2V2 Charles’ Law ↑ T causes ↑ V This is why a balloon in a hot car pops By extending this idea, ↓ T causes ↓ V All volumes approach zero at the same temperature – Absolute Zero Zero temperature corresponds to zero motion and zero volume Absolute Zero = -273.15º C = 0 K Kelvin Temperature = Celsius Temperature + 273.15 Mathematically: T is proportional to V, but you MUST use the Kelvin scale V1 = V2 T1 T2 Combined Gas Law P1V1 = P2V2 T1 T2 If temperature is constant: P1V1 = P2V2 (Boyle’s Law) If pressure is constant: V1 / T1 = V2 / T2 (Charles Law) If volume is constant: P1 / T1 = P2 / T2 Standard Temperature and Pressure (STP) T = 0º C = 273.15 K P = 1 atm = 760 mm Hg = 101.15 kPa Avogadro’s Law, 1811 At the same temperature and pressure, equal volumes of all gases contain the same number of molecules (or moles, n) Mathematically Stated ↑ n causes ↑ V If you put more gas into a container, it gets bigger Therefore: n is directly proportional to V V1 / n1 = V2 / n2 Ideal Gas Law Combining all gas laws P1V1 / n1T1 = P2V2 / n2T2 = constant = R = 0.08206 (lit atm) / (mol K) PV = nRT You must be careful of units when using the ideal gas law! Standard Molar Volume For all ideal gases, at STP If n = 1 mole, then V = 22.4 L Kinetic Theory of Gases Defines the behavior and assumptions of an ideal gas The particles are small, moving in constant, random, straight-line motion. Newton’s First Law of Motion – Any object with mass (inertia) will move in a straight line at a constant speed unless acted on by a force. Gases are mostly empty space; the particles are separated by large distances. The particles are considered “point masses” with no appreciable volume. The particles themselves occupy no volume; the volume of the gas is the result of the motion of particles and collisions with the container. Particles collide in perfectly elastic collisions. The collisions are with each other and the walls of the container. Elastic collisions – no net loss of energy in the collision, like billiard balls There are no forces between the particles Temperature is a measure of the average kinetic energy of the particles. Substances with higher molecular weight will move with a lower average velocity at the same temperature. KE = ½ mv2 Deviations from the ideal gas behavior Under high pressure, the particles are squished close together and the volume of the particles themselves affects the total volume. This results in a measured volume which is higher than expected At low temperatures, the particles are moving slowly, and the attractions between the particles become significant. This gives a pressure that is smaller than expected, because the particles are slowing down as they are drawn to each other. Polar molecules exert attractive forces on each other – therefore polar gases will deviate from ideal behavior Close to the condensation point (boiling point), molecules exert attractive forces on each other – therefore the gas will deviate from ideal behavior Diffusion and Effusion Effusion – the escape of a gas through a small opening due to random motion of particles Diffusion – mixing of gases with each other due to random motion of particles Both effusion and diffusion will happen faster for a lighter molecule which will have a larger velocity at the same temperature