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

1.0 mol of argon has 3100 J of thermal energy. What is the gas temperature in °C?

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Key Concepts

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

Thermal Energy

Thermal energy refers to the total kinetic energy of the particles in a substance due to their motion. In gases, this energy is directly related to the temperature, as higher thermal energy indicates faster-moving particles. The relationship between thermal energy and temperature is crucial for understanding how energy is distributed among particles in a gas.
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Ideal Gas Law

The Ideal Gas Law is a fundamental equation in thermodynamics that relates pressure, volume, temperature, and the number of moles of a gas. It is expressed as PV = nRT, where P is pressure, V is volume, n is the number of moles, R is the ideal gas constant, and T is temperature in Kelvin. This law helps in calculating the temperature of a gas when its thermal energy and amount are known.
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Temperature Conversion

Temperature conversion is the process of changing temperature values from one scale to another, such as from Kelvin to Celsius. The conversion from Kelvin to Celsius is done using the formula °C = K - 273.15. Understanding this conversion is essential for accurately interpreting temperature readings in different contexts, especially in thermodynamic calculations.
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Related Practice
Textbook Question
A mad engineer builds a cube, 2.5 m on a side, in which 6.2-cm-diameter rubber balls are constantly sent flying in random directions by vibrating walls. He will award a prize to anyone who can figure out how many balls are in the cube without entering it or taking out any of the balls. You decide to shoot 6.2-cm-diameter plastic balls into the cube, through a small hole, to see how far they get before colliding with a rubber ball. After many shots, you find they travel an average distance of 1.8 m. How many rubber balls do you think are in the cube?
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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
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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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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