Examples of Gases:
Monoatomic (Noble gases): He, Ne, Ar, Kr, Xe, Rn
Molecular (homonuclear diatomics): H2, O2, N2, F2, Cl2
Other gases: CH4, NO2, NO, N2O, CO2, NH3, HCl
Vapors (liquids with boiling points above room temperature): H2O, HNO3
Volume: Gases occupy the full volume of their containers, filling any available space.
Interdependence: Gas volume, pressure, and temperature are related; changing one affects the others.
Density: Gases have low densities and viscosities compared to solids and liquids.
Miscibility: Gases are highly miscible and can form homogeneous mixtures with other gases.
Physical vs. Chemical Properties: Gases can have similar physical properties but very different chemical properties.
Pressure Equations: Pressure (P) = Force (F) / Area (A)
Pressure Units:
1 atm = 760 mm Hg = 760 torr = 1.013 × 10^5 Pa = 101.3 kPa = 1.013 bar
Example Calculation:
Atmospheric pressure at 29.12 inches of mercury converts to 739.6 torr.
Barometers: Measure atmospheric pressure; invented by E. Torricelli in the 17th century.
Manometers: Instrument for measuring gas pressure in a closed volume using a U-tube containing mercury.
Closed-end U-tube: Measures absolute pressure, Pgas = PΔh.
Open-end U-tube: Measures relative pressure, can indicate whether gas pressure is above or below atmospheric pressure.
Definition: At constant temperature, volume (V) is inversely proportional to pressure (P) for a given amount of gas: P1V1 = P2V2.
Graphical Representation: Plotting V vs. P shows a hyperbolic relationship.
Definition: At constant pressure, volume of a gas is directly proportional to its absolute temperature (T): V/T = constant.
Key Point: Absolute zero is the temperature at which a gas would theoretically occupy zero volume.
Definition: Volume of a gas is directly proportional to the number of moles (n) of the gas at constant temperature and pressure: V/n = constant.
Implication: More gas means a larger volume under the same conditions.
Combination of earlier laws leads to: PV = nRT, where R = ideal gas constant.
Common Values:
R = 0.0821 L·atm/(K·mol)
R = 62.36 L·torr/(K·mol)
Standard Conditions: At STP (0℃ and 1 atm), 1 mole of an ideal gas occupies 22.41 L.
Gas Density and Molar Mass: Relates density to molar mass using equations involving P, V, T, and R.
Gases consist of numerous particles in random motion.
Gas particles have negligible volume and negligible intermolecular forces.
Collisions between gas particles and with container walls are elastic.
Pressure Variation: Pressure depends on collision frequency and particle speed; increasing temperature raises pressure due to increased particle motion.
Effusion: Escape of gas particles through orifices.
Diffusion: Spreading of gas particles in space due to thermal motion.
States that the rate of effusion is inversely proportional to the square root of the gas's molar mass.
Deviate from ideal behavior due to molecular volume and intermolecular forces, particularly at high pressures and low temperatures.
Adjusts the ideal gas law to account for non-ideal behavior with parameters specific to the particular gas.