/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 80 Starting with \(2.50 \mathrm{~mo... [FREE SOLUTION] | 91Ó°ÊÓ

91Ó°ÊÓ

Starting with \(2.50 \mathrm{~mol}\) of \(\mathrm{N}_{2}\) gas (assumed to be ideal) in a cylinder at 1.00 atm and \(20.0^{\circ} \mathrm{C}\), a chemist first heats the gas at constant volume, adding \(1.52 \times 10^{4} \mathrm{~J}\) of heat, then continues heating and allows the gas to expand at constant pressure to twice its original volume. (a) Calculate the final temperature of the gas. (b) Calculate the amount of work done by the gas. (c) Calculate the amount of heat added to the gas while it was expanding. (d) Calculate the change in internal energy of the gas for the whole process.

Short Answer

Expert verified
(a) Final temperature is 1170.9 K. (b) Work done by gas is 12175.7 J. (c) Heat added while expanding is 42614.4 J. (d) Change in internal energy is 45638.7 J.

Step by step solution

01

Calculate Molecular Properties

We begin by identifying relevant properties of nitrogen gas. The specific heat capacity at constant volume for diatomic gases like nitrogen is 20.8 J/mol·°C, and at constant pressure is 29.1 J/mol·°C.
02

Heat Gas at Constant Volume

For heating at constant volume, the change in temperature \( \Delta T \) can be calculated using \( q = nC_v \Delta T \). Given that \( q = 1.52 \times 10^4 \text{ J} \), \( n = 2.50 \text{ mol} \), and \( C_v = 20.8 \text{ J/mol·°C} \), we solve for \( \Delta T \): \[ \Delta T = \frac{q}{nC_v} = \frac{1.52 \times 10^4}{2.50 \times 20.8} = 292.3 \text{ °C} \]The initial temperature \( T_1 = 20.0 \text{ °C} = 293.15 \text{ K} \). The new temperature \( T_2 \) is:\[ T_2 = T_1 + \Delta T = 293.15 + 292.3 = 585.45 \text{ K} \]
03

Expansion at Constant Pressure

As the gas expands at constant pressure and doubles in volume, use the ideal gas law. \( V_2 = 2V_1 \), so \( \frac{T_3}{T_2} = \frac{V_2}{V_1} = 2 \). Thus, \[ T_3 = 2 \cdot T_2 = 2 \cdot 585.45 = 1170.9 \text{ K} \]
04

Calculate Work Done by the Gas

The work done by the gas during expansion at constant pressure is given by \( W = P \Delta V \). Using the ideal gas law, \( \Delta V = V_2 - V_1 = \frac{nRT}{P} \); thus,\[ W = nR(T_3 - T_2) = 2.50 \times 8.314 \times (1170.9 - 585.45) \approx 12175.7 \text{ J} \]
05

Calculate Heat Added During Expansion

For constant pressure, the heat added is given by \( q = nC_p \Delta T \), where \( \Delta T = T_3 - T_2 \) and \( C_p = 29.1 \text{ J/mol·°C} \).\[ q = 2.50 \times 29.1 \times (1170.9 - 585.45) = 42614.4 \text{ J} \]
06

Total Change in Internal Energy

The change in internal energy, \( \Delta U \), is given by \( \Delta U = q_{cv} + q_{cp} - W \), where \( q_{cv} = 1.52 \times 10^4 \text{ J} \) and \( q_{cp} = 42614.4 \text{ J} \).\[ \Delta U = 15200 + 42614.4 - 12175.7 = 45638.7 \text{ J} \]

Unlock Step-by-Step Solutions & Ace Your Exams!

  • Full Textbook Solutions

    Get detailed explanations and key concepts

  • Unlimited Al creation

    Al flashcards, explanations, exams and more...

  • Ads-free access

    To over 500 millions flashcards

  • Money-back guarantee

    We refund you if you fail your exam.

Over 30 million students worldwide already upgrade their learning with 91Ó°ÊÓ!

Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Ideal Gas Law
The Ideal Gas Law is a fundamental equation in thermodynamics that describes how gases behave under various conditions of temperature (T), pressure (P), and volume (V). The law is expressed as \( PV = nRT \), where \( P \) is pressure, \( V \) is volume, \( n \) is the amount of gas in moles, \( R \) is the ideal gas constant (8.314 J/mol·K), and \( T \) is temperature in Kelvin.

This relationship helps determine how gases expand or contract when the temperature changes, or when they are compressed or allowed to expand. In the context of the exercise, the Ideal Gas Law was used to predict how the nitrogen gas behaves when it is first heated at constant volume and then allowed to expand at constant pressure. Understanding the interplay of these variables is key to predicting the behavior of an ideal gas in various scenarios, such as calculating the final temperature or the amount of work done by the gas.
Heat Transfer in Gases
When heat is transferred to a gas, it typically results in a change in temperature, depending on the conditions of the process. The heat transferred either increases the internal energy of the gas or does work by expanding against an external pressure.

In the specified exercise, the heat added during constant volume heating is calculated using the formula \( q = nC_v \Delta T \), where \( C_v \) is the specific heat at constant volume, \( n \) is the number of moles, and \( \Delta T \) is the change in temperature. This calculation provides insight into how the gas's temperature changes due to heat input.

Later, when the gas is allowed to expand at constant pressure, heat transfer is described by another formula: \( q = nC_p \Delta T \), where \( C_p \) is the specific heat at constant pressure. This part of the process shows how additional heat is used not just to increase internal energy but also to do work as the gas expands.
Work Done by Gas
Work done by an ideal gas is an important concept when the gas expands or contracts. The work \( W \) done by the gas during an expansion or compression at constant pressure is calculated using the relationship: \( W = P \Delta V \), or more specifically, in terms of temperature change: \( W = nR(T_3 - T_2) \).

In the given problem, part of the work done results from the gas doubling its volume during expansion. This process requires energy, which is provided by the added heat. The calculation of work allows us to see how much energy is used in expanding the gas against a constant pressure.
  • This process is essentially an energy conversion where heat energy is turned into mechanical work.
  • Knowing the work done is crucial in thermodynamics to analyze energy efficiency and changes within systems.
Internal Energy Change
The internal energy change \( \Delta U \) of a system is a central concept in thermodynamics that reflects the net change in the energy contained within the system. This change can be understood as the balance between heat added to the system and the work done by it.

Mathematically, it is expressed by the equation: \( \Delta U = q_{cv} + q_{cp} - W \), where \( q_{cv} \) is the heat at constant volume, \( q_{cp} \) is the heat added at constant pressure, and \( W \) is the work done by the system. In the context of the exercise, the total change in internal energy combines the effects of heating and expansion.
  • This balance highlights the first law of thermodynamics, which states that energy cannot be created or destroyed.
  • Understanding \( \Delta U \) is essential for analyzing how energy flows into and out of systems during various processes.

One App. One Place for Learning.

All the tools & learning materials you need for study success - in one app.

Get started for free

Most popular questions from this chapter

If deep-sea divers rise to the surface too quickly, nitrogen bubbles in their blood can expand and prove fatal. This phenomenon is known as the bends. If a scuba diver rises quickly from a depth of \(25 \mathrm{~m}\) in Lake Michigan (which is freshwater), what will be the volume at the surface of an \(\mathrm{N}_{2}\) bubble that occupied \(1.0 \mathrm{~mm}^{3}\) in his blood at the lower depth? Does it seem that this difference is large enough to be a problem? (Assume that the pressure difference is due only to the changing water pressure, not to any temperature difference, an assumption that is reasonable, since we are warm-blooded creatures.)

An ideal gas at 4.00 atm and \(350 \mathrm{~K}\) is permitted to expand adiabatically to 1.50 times its initial volume. Find the final pressure and temperature if the gas is (a) monatomic with \(C_{p} / C_{V}=\frac{5}{3},\) (b) diatomic with \(C_{p} / C_{V}=\frac{7}{5}\).

The gas inside a balloon will always have a pressure nearly equal to atmospheric pressure, since that is the pressure applied to the outside of the balloon. You fill a balloon with helium (a nearly ideal gas) to a volume of \(0.600 \mathrm{~L}\) at a temperature of \(19.0^{\circ} \mathrm{C}\). What is the volume of the balloon if you cool it to the boiling point of liquid nitrogen \((77.3 \mathrm{~K}) ?\)

At an altitude of \(11,000 \mathrm{~m}\) (a typical cruising altitude for a jet airliner), the air temperature is \(-56.5^{\circ} \mathrm{C}\) and the air density is \(0.364 \mathrm{~kg} / \mathrm{m}^{3} .\) What is the pressure of the atmosphere at that altitude? The molar mass of air is \(28.8 \mathrm{~g} / \mathrm{mol}\).

One way to improve insulation in windows is to fill a sealed space between two glass panes with a gas that has a lower thermal conductivity than that of air. The thermal conductivity \(k\) of a gas depends on its molar heat capacity \(C_{V},\) molar mass \(M,\) and molecular radius \(r\). The dependence on those quantities at a given temperature is approximately \(k \propto C_{V} / r^{2} \sqrt{M}\). The noble gases have properties that make them particularly good choices as insulating gases. Noble gases range from helium (molar mass \(4.0 \mathrm{~g} / \mathrm{mol}\), molecular radius \(0.13 \mathrm{nm}\) ) to xenon (molar mass \(131 \mathrm{~g} / \mathrm{mol}\), molecular radius \(0.22 \mathrm{nm}\) ). (The noble gas radon is heavier than xenon, but radon is radioactive and so is not suitable for this purpose.) The rate of effusion-that is, the leakage of a gas through tiny cracks-is proportional to \(v_{\mathrm{rms}}\). If there are tiny cracks in the material that's used to seal the space between two glass panes, how many times greater is the rate of He leakage out of the space between the panes than the rate of Xe leakage at the same temperature? A. 370 times B. 19 times C. 6 times D. No greater; the He leakage rate is the same as for Xe.

See all solutions

Recommended explanations on Physics Textbooks

View all explanations

What do you think about this solution?

We value your feedback to improve our textbook solutions.

Study anywhere. Anytime. Across all devices.