Gases are everywhere, and understanding their behavior is crucial. The ideal gas law connects pressure , volume, temperature, and the number of gas particles, helping us predict how gases will act under different conditions.
But gases aren't always ideal. Real gases can behave differently, especially at high pressures or low temperatures. The molecular model of gases helps explain these behaviors, treating gas particles as tiny, fast-moving objects that collide with each other and container walls.
Ideal Gas Law and Molecular Model
Gas behavior and ideal gas law
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Ideal gas law relates pressure (P P P ), volume (V V V ), temperature (T T T ), and number of moles (n n n ) of a gas: P V = n R T PV = nRT P V = n RT
R R R is the ideal gas constant , which has a value of 8.314 J/(mol·K)
At constant temperature and number of moles, pressure is inversely proportional to volume (###Boyle 's_Law_0###)
Doubling the volume of a gas at constant temperature and moles will halve its pressure
At constant pressure and number of moles, volume is directly proportional to temperature (###Charles 's_Law_0###)
Increasing the temperature of a gas from 300 K to 600 K at constant pressure will double its volume
At constant volume and temperature, pressure is directly proportional to the number of moles (###Avogadro 's_Law_0###)
Adding more gas to a container at constant volume and temperature increases the pressure
Combined gas law relates pressure, volume, and temperature changes between two states: P 1 V 1 T 1 = P 2 V 2 T 2 \frac{P_1V_1}{T_1} = \frac{P_2V_2}{T_2} T 1 P 1 V 1 = T 2 P 2 V 2
Used to calculate changes in gas properties when multiple variables are changing simultaneously (pressure, volume, and temperature)
Mole and molecule conversions
One mole of a substance contains Avogadro's number (N A N_A N A ) of particles (atoms or molecules)
N A = 6.022 × 1 0 23 N_A = 6.022 \times 10^{23} N A = 6.022 × 1 0 23 particles per mole
Number of moles (n n n ) is related to the number of particles (N N N ) by: n = N N A n = \frac{N}{N_A} n = N A N
1 mole of carbon dioxide (C O 2 CO_2 C O 2 ) contains 6.022 × 1 0 23 6.022 \times 10^{23} 6.022 × 1 0 23 C O 2 CO_2 C O 2 molecules
Molar mass (M M M ) is the mass of one mole of a substance, expressed in grams per mole (g/mol)
Molar mass of water (H 2 O H_2O H 2 O ) is 18.02 g/mol
Mass (m m m ) of a substance is related to the number of moles (n n n ) by: m = n M m = nM m = n M
2 moles of sodium chloride (NaCl, molar mass 58.44 g/mol) has a mass of 116.88 g
Limitations of ideal gas law
Ideal gas law assumptions break down at high pressures, low temperatures, and near the point of condensation
High pressure: gas particles are close together, and intermolecular forces become significant
Low temperature: gas particles move slowly, and intermolecular forces become more important relative to kinetic energy
Real gases deviate from ideal behavior due to the finite volume of gas particles and intermolecular forces between them
Finite volume: gas particles occupy space, reducing the available volume for motion
Intermolecular forces: attractive forces between gas particles cause them to stick together, reducing pressure
Van der Waals equation corrects for non-ideal behavior: ( P + a n 2 V 2 ) ( V − n b ) = n R T \left(P + \frac{an^2}{V^2}\right)(V - nb) = nRT ( P + V 2 a n 2 ) ( V − nb ) = n RT
a a a accounts for intermolecular attraction, and b b b accounts for the finite volume of gas particles
Used for more accurate calculations of gas behavior under non-ideal conditions (high pressure or low temperature)
Molecular model of ideal gases
Gas particles are treated as point masses with negligible volume, moving randomly and independently
Particle size is much smaller than the average distance between particles
Collisions between particles and the container walls are elastic (no energy loss)
Kinetic energy is conserved during collisions, and no energy is transferred to or from the container walls
No intermolecular forces (attraction or repulsion) between gas particles
Gas particles do not interact with each other, only with the container walls during collisions
Average kinetic energy of gas particles is proportional to the absolute temperature: 1 2 m v r m s 2 = 3 2 k T \frac{1}{2}mv_{rms}^2 = \frac{3}{2}kT 2 1 m v r m s 2 = 2 3 k T
m m m is the mass of a gas particle, v r m s v_{rms} v r m s is the root-mean-square velocity , and k k k is the Boltzmann constant (k = R N A k = \frac{R}{N_A} k = N A R )
Higher temperature means higher average kinetic energy and faster particle motion
Mean free path is the average distance a gas particle travels between collisions
Longer mean free path indicates less frequent collisions and lower gas density
Statistical mechanics and gas behavior
Maxwell-Boltzmann distribution describes the probability distribution of particle speeds in an ideal gas
It shows that not all particles have the same speed, but rather a range of speeds centered around an average value
Equipartition theorem states that energy is equally distributed among all degrees of freedom in a system
Each degree of freedom (e.g., translational, rotational, vibrational) contributes 1 2 k T \frac{1}{2}kT 2 1 k T to the average energy per particle
Degrees of freedom represent the independent ways a molecule can store energy
Monatomic gases have 3 translational degrees of freedom, while diatomic gases have additional rotational degrees of freedom
Pressure in a gas results from the collective impact of particles colliding with the container walls
Higher particle velocity and more frequent collisions lead to higher pressure