Warning: foreach() argument must be of type array|object, bool given in /var/www/html/web/app/themes/studypress-core-theme/template-parts/header/mobile-offcanvas.php on line 20

(a) Under what condition will the enthalpy change of a process equal the amount of heat transferred into or out of the system? (b) During a constant- pressure process, the system releases heat to the surroundings. Does the enthalpy of the system increase or decrease during the process? (c) In a constant-pressure process, \(\Delta H=0\). What can you conclude about \(\Delta E, q\), and \(w\) ?

Short Answer

Expert verified
(a) The enthalpy change of a process will equal the amount of heat transferred into or out of the system under constant pressure conditions, i.e., \(\Delta H = q_p\). (b) During a constant-pressure process when the system releases heat to the surroundings, the enthalpy of the system decreases since \(q_p < 0\). (c) In a constant-pressure process with \(\Delta H=0\), we can conclude that \(\Delta E=-P\Delta V\), \(q=0\), and \(w=-P\Delta V\).

Step by step solution

01

Part a: Condition when enthalpy change equals heat transferred

At constant pressure, the enthalpy change (\(\Delta H\)) of a process is given by \(\Delta H = q_p\), where \(q_p\) represents heat transferred into or out of the system at constant pressure. The condition we seek is the one where \(\Delta H = q_p\) always holds true.
02

Part b: Change in enthalpy during a constant-pressure process

Given that heat is released to the surroundings during the constant-pressure process, it implies that \(q_p < 0\). Since \(\Delta H = q_p\) at constant pressure, the enthalpy of the system must decrease during the process as \(\Delta H < 0\).
03

Part c: Inference about \(\Delta E\), \(q\), and \(w\) at constant pressure when \(\Delta H = 0\)

In a constant-pressure process, the enthalpy change (\(\Delta H\)) is related to the change in internal energy (\(\Delta E\)), heat transfer (\(q\)), and work (\(w\)) performed by the system as follows: \[\Delta H = \Delta E + P\Delta V = q_p\] Given that \(\Delta H = 0\), we have: \[0 = \Delta E + P\Delta V\] We can rearrange the equation to obtain the relationship between \(\Delta E\) and \(P\Delta V\): \[\Delta E = -P\Delta V\] Since the process occurs at constant pressure, heat transfer (\(q\)) and work (\(w\)) are related as: \[q = \Delta E + w\] Substituting \(\Delta E = -P\Delta V\) and the work is given by \(w = -P\Delta V\) (since work is done by the system): \[q = -P\Delta V - (-P\Delta V) = 0\] Thus, at constant pressure when \(\Delta H = 0\), we can conclude that \(\Delta E = -P\Delta V\), \(q = 0\), and \(w = -P\Delta V\).

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 Vaia!

Key Concepts

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

constant-pressure process
In a constant-pressure process, the pressure of the system remains unchanged throughout the entire process. This consistency in pressure is a common scenario in many real-world applications. Imagine boiling water in an open pot - the pressure above the water is constantly atmospheric pressure.
At constant pressure, any change in the system is described by the behavior of its properties rather than changes in pressure. One key relationship that emerges is that the change in enthalpy (\(\Delta H\)) of the system equals the heat exchanged (\(q_p\)) between the system and its surroundings. This is represented mathematically as:\[\Delta H = q_p\]
  • Heat added to the system leads to an increase in enthalpy.
  • Heat lost from the system results in a decrease in enthalpy.
Under these conditions, the system's enthalpy becomes the straightforward measure of the heat exchanged, simplifying calculations and insights into the system's thermal dynamics.
heat transfer
Heat transfer refers to the movement of thermal energy from one part of a system to another, or to the surrounding environment. It's a key driver of change in a thermodynamic system, directing the flow of energy.
During constant-pressure processes, where pressure remains the same, heat transfer can significantly influence the system. The direction and magnitude of heat transfer determine how the system's enthalpy changes:
  • If the system gains heat (positive heat transfer), enthalpy increases.
  • If the system loses heat (negative heat transfer), enthalpy decreases.
This relationship is crucial because it allows us to predict and analyze the behavior of a system undergoing thermal changes without varying its pressure. Mastering the concept of heat transfer in these processes enables us to predict system states and transformations effectively.
internal energy
Internal energy (\(\Delta E\)) is a measure of the total energy contained within a system, encompassing both the kinetic and potential energies of its particles. In thermodynamics, understanding internal energy is essential for analyzing how systems exchange energy through work and heat.
In constant-pressure processes, the relationship between internal energy change and other forms of energy exchange is captured by the equation:\[\Delta E = q + w\]where \(q\) is the heat transfer and \(w\) is the work done by the system. When enthalpy (\(\Delta H\)) is zero, it indicates a balance where the system's pressure-volume work (\(P\Delta V\)) aligns with any internal changes:
  • If \(\Delta H = 0\), then \(\Delta E = -P\Delta V\)
  • This implies that the energy lost in the form of expansion work is compensated by the internal energy change, with no net heat transfer (\(q = 0\)).
This balance is a fascinating aspect of thermodynamics, revealing how internal adjustments can occur while maintaining overall energy equilibrium.

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

Suppose that the gas-phase reaction \(2 \mathrm{NO}(g)+\mathrm{O}_{2}(g) \longrightarrow\) \(2 \mathrm{NO}_{2}(g)\) were carried out in a constant-volume container at constant temperature. (a) Would the measured heat change represent \(\Delta H\) or \(\Delta E\) ? (b) If there is a difference, which quantity is larger for this reaction? (c) Explain your answer to part (b).

Limestone stalactites and stalagmites are formed in caves by the following reaction: $$ \mathrm{Ca}^{2+}(a q)+2 \mathrm{HCO}_{3}^{-}(a q) \longrightarrow \mathrm{CaCO}_{3}(s)+\mathrm{CO}_{2}(g)+\mathrm{H}_{2} \mathrm{O}(l) $$ If \(1 \mathrm{~mol}\) of \(\mathrm{CaCO}_{3}\) forms at \(298 \mathrm{~K}\) under 1 atm pressure, the reaction performs \(2.47 \mathrm{~kJ}\) of \(P-V\) work, pushing back the atmosphere as the gaseous \(\mathrm{CO}_{2}\) forms. At the same time, \(38.95 \mathrm{~kJ}\) of heat is absorbed from the environment. What are the values of \(\Delta H\) and of \(\Delta E\) for this reaction?

At one time, a common means of forming small quantities of oxygen gas in the laboratory was to heat \(\mathrm{KClO}_{3}\) : $$ 2 \mathrm{KClO}_{3}(s) \longrightarrow 2 \mathrm{KCl}(s)+3 \mathrm{O}_{2}(g) \quad \Delta H=-89.4 \mathrm{~kJ} $$ For this reaction, calculate \(\Delta H\) for the formation of (a) \(1.36\) \(\mathrm{mol}\) of \(\mathrm{O}_{2}\) and (b) \(10.4 \mathrm{~g}\) of \(\mathrm{KCl}\). (c) The decomposition of \(\mathrm{KClO}_{3}\) proceeds spontaneously when it is heated. Do you think that the reverse reaction, the formation of \(\mathrm{KClO}_{3}\) from \(\mathrm{KCl}\) and \(\mathrm{O}_{2}\), is likely to be feasible under ordinary conditions? Explain your answer.

Without referring to tables, predict which of the following has the higher enthalpy in each case: (a) \(1 \mathrm{~mol} \mathrm{CO}_{2}(s)\) or \(1 \mathrm{~mol} \mathrm{CO} 2(g)\) at the same temperature, (b) \(2 \mathrm{~mol}\) of hydrogen atoms or \(1 \mathrm{~mol}\) of \(\mathrm{H}_{2}\), (c) \(1 \mathrm{~mol} \mathrm{H}_{2}(g)\) and \(0.5 \mathrm{~mol} \mathrm{O}_{2}(g)\) at \(25^{\circ} \mathrm{C}\) or \(1 \mathrm{~mol} \mathrm{H}_{2} \mathrm{O}(g)\) at \(25^{\circ} \mathrm{C}\), (d) \(1 \mathrm{~mol} \mathrm{~N}_{2}(g)\) at \(100^{\circ} \mathrm{C}\) or \(1 \mathrm{~mol} \mathrm{~N}_{2}(g)\) at \(300^{\circ} \mathrm{C} .\)

The Sun supplies about \(1.0\) kilowatt of energy for each square meter of surface area \(\left(1.0 \mathrm{~kW} / \mathrm{m}^{2}\right.\), where a watt \(\left.=1 \mathrm{~J} / \mathrm{s}\right)\). Plants produce the equivalent of about \(0.20 \mathrm{~g}\) of sucrose \(\left(\mathrm{C}_{12} \mathrm{H}_{22} \mathrm{O}_{11}\right)\) per hour per square meter. Assuming that the sucrose is produced as follows, calculate the percentage of sunlight used to produce sucrose. $$ \begin{array}{r} 12 \mathrm{CO}_{2}(g)+11 \mathrm{H}_{2} \mathrm{O}(l) \longrightarrow \mathrm{C}_{12} \mathrm{H}_{22} \mathrm{O}_{11}+12 \mathrm{O}_{2}(g) \\ \Delta H=5645 \mathrm{~kJ} \end{array} $$

See all solutions

Recommended explanations on Chemistry 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.

Sign-up for free