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Ch 20: The Micro/Macro Connection
Chapter 20, Problem 20

Liquid helium boils at 4.2 K. In a flask, the helium gas above the boiling liquid is at the same temperature. What are (a) the mean free path in the gas, (b) the rms speed of the atoms, and (c) the average energy per atom?

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Key Concepts

Here are the essential concepts you must grasp in order to answer the question correctly.

Mean Free Path

The mean free path is the average distance a particle travels between collisions with other particles. In gases, this concept is crucial for understanding how particles interact and move. It depends on factors such as the density of the gas and the size of the particles. At low temperatures, like in liquid helium, the mean free path can be significantly longer due to reduced particle density.
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Root Mean Square (RMS) Speed

The root mean square speed is a measure of the average speed of particles in a gas, calculated from the kinetic theory of gases. It is defined as the square root of the average of the squares of the speeds of all the particles. The RMS speed is directly related to the temperature of the gas, indicating that as temperature increases, the speed of the particles also increases, which is particularly relevant for helium at 4.2 K.
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Average Energy per Atom

The average energy per atom in a gas is derived from the kinetic theory and is proportional to the temperature of the gas. For a monatomic ideal gas, this energy can be calculated using the formula E = (3/2)kT, where k is the Boltzmann constant and T is the temperature in Kelvin. At 4.2 K, this relationship helps determine the energy distribution among helium atoms, which is essential for understanding their behavior in the gas phase.
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Related Practice
Textbook Question
Photons of light scatter off molecules, and the distance you can see through a gas is proportional to the mean free path of photons through the gas. Photons are not gas molecules, so the mean free path of a photon is not given by Equation 20.3, but its dependence on the number density of the gas and on the molecular radius is the same. Suppose you are in a smoggy city and can barely see buildings 500 m away. a. How far would you be able to see if all the molecules around you suddenly doubled in volume?
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Textbook Question
On earth, STP is based on the average atmospheric pressure at the surface and on a phase change of water that occurs at an easily produced temperature, being only slightly cooler than the average air temperature. The atmosphere of Venus is almost entirely carbon dioxide (CO₂), the pressure at the surface is a staggering 93 atm, and the average temperature is 470℃. Venusian scientists, if they existed, would certainly use the surface pressure as part of their definition of STP. To complete the definition, they would seek a phase change that occurs near the average temperature. Conveniently, the melting point of the element tellurium is 450℃. What are (a) the rms speed and (b) the mean free path of carbon dioxide molecules at Venusian STP based on this phase change in tellurium? The radius of a CO₂ molecule is 1.5 x 10⁻¹⁰ m.
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Textbook Question
1.0 mol of argon has 3100 J of thermal energy. What is the gas temperature in °C?
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Textbook Question
The rms speed of the atoms in a 2.0 g sample of helium gas is 700 m/s. What is the thermal energy of the gas?
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Textbook Question
A 6.0 m ✕ 8.0 m ✕ 3.0 m room contains air at 20℃. What is the room's thermal energy?
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Textbook Question
Consider a container like that shown in Figure 20.12, with n₁ moles of a monatomic gas on one side and n₂ moles of a diatomic gas on the other. The monatomic gas has initial temperature T₁ᵢ. The diatomic gas has initial temperature T₂ᵢ. b. Show that the equilibrium temperature is
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