Problem 37
Question
(a) Oxygen \(\left(\mathrm{O}_{2}\right)\) has a molar mass of 32.0 \(\mathrm{g} / \mathrm{mol}\) . What is the average translational kinetic energy of an oxygen molecule at a temperature of 300 \(\mathrm{K} ?\) (b) What is the average value of the square at a of its speed? (c) What is the root-mean-square speed? (d) What is the momentum of an oxygen molecule traveling at this speed? (e) Suppose an oxygen molecule traveling at this speed bounces back and forth between opposite sides of a cubical vessel 0.10 \(\mathrm{m}\) on a side. What is the average force the molecule exerts on one of the walls of the container? (Assume that the molecule's velocity is perpendicular to the two sides that it strikes.) (f) What is the aver- age force per unit area? (g) How many oxygen molecules traveling at this speed are necessary to produce an average pressure of 1 \(\mathrm{atm} ?\) (h) Compute the number of oxygen molecules that are actually contained in a vessel of this size at 300 \(\mathrm{K}\) and atmospheric pressure. (i) Your answer for part (h) should be three times as large as the answer for part (g). Where does this discrepancy arise?
Step-by-Step Solution
VerifiedKey Concepts
Translational Kinetic Energy
This means that at a higher temperature, each molecule will have a higher kinetic energy. For example, to find the average kinetic energy of an oxygen molecule at \( 300 \, \text{K} \), we calculate:
\[ \text{Average kinetic energy} = \frac{3}{2} \times 1.38 \times 10^{-23} \, \text{J/K} \times 300 \, \text{K} = 6.21 \times 10^{-21} \, \text{J} \].
Understanding this can help you predict how 'energetic' a gas's molecules are, impacting their speed and how they interact with other molecules and their container walls.
Root-Mean-Square Speed
To find the root-mean-square speed, we initially calculate the average of the square of the velocity, \( \langle v^2 \rangle \), using :
\[ \langle v^2 \rangle = \frac{3 k_B T}{m} \].
In this calculation, \( m \) is the mass of one molecule of the gas. For oxygen, converting the molar mass (32.0 g/mol) into kilograms, and using Avogadro's number, gives us the mass of a single molecule.
Plugging in the numbers, \( \langle v^2 \rangle \approx 5.99 \times 10^5 \, \text{m}^2/\text{s}^2 \).
The \( v_{rms} \) is then:
\[ v_{rms} = \sqrt{\langle v^2 \rangle} \approx 774 \, \text{m/s} \].
This speed increases with increased temperature, indicating more rapid motion as heat rises.
Ideal Gas Law
This equation links pressure \( P \), volume \( V \), and number of moles \( n \) of a gas to its temperature \( T \), with \( R \) being the universal gas constant, \( 8.31 \, \text{J/(mol} \cdot \text{K)} \).
The ideal gas law helps in estimating the number of gas molecules present in any given volume under specified conditions. For instance, with a cubic vessel at \( 0.001 \, \text{m}^3 \) volume and assessing the situation at atmospheric pressure (\( 1.013 \times 10^5 \, \text{N/m}^2 \)) and a temperature of \( 300 \, \text{K} \), it computes approximately \( 3.23 \times 10^{22} \) molecules.
We assume that these molecules have random, constant speeds and lack interactions, conditions that the ideal gas law utilizes to make real-world gas behavior predictable despite these simplifications.
Molecular Momentum
The oxygen molecule at root-mean-square speed (\( 774 \, \text{m/s} \)) and calculated mass gives \( p \approx 4.12 \times 10^{-26} \, \text{kg} \cdot \text{m/s} \).
When these molecules collide with a container wall, they exert a force dependent on their momentum change. Each bounce involves altering the momentum, causing a force that's twice the impulse over the period taken for a molecule to travel to the opposite wall and back.
This fundamental concept illustrates how gases apply force, translating their energetic, kinetic interactions into measurable quantities like pressure.
Pressure Calculation
Given the recurring impact of molecules, their momentum exchange establishes an average force, which when divided by the wall area (\( 0.01 \, \text{m}^2 \) for a side of the cubic vessel), provides the pressure.
In the example provided, a single molecule's cycle of striking the walls results in an average force determined by its momentum: \( F \approx 3.20 \times 10^{-22} \, \text{N}\).
This results in pressure on the order of \( 3.20 \times 10^{-20} \, \text{N/m}^2 \), much less than standard atmospheric pressure.
To achieve higher pressures akin to 1 atm, many more molecules or higher velocities are necessary, illuminating the aggregate effect of countless molecular collisions in creating significant pressure.