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Problem 1.49. Consider the combustion of one mole of H2with1/2 mole ofO2 under standard conditions, as discussed in the text. How much of the heat energy produced comes from a decrease in the internal energy of the system, and how much comes from work done by the collapsing atmosphere? (Treat the volume of the liquid water as negligible.)

Short Answer

Expert verified

Short Answer :

The quantity of heat produced by the collapsing atmosphere accounts for 1.31 percent of the total, with the remaining 98.69 percent coming from the system's increased internal energy.

Step by step solution

01

Given Information : 

One mole of H2

1/2 mole of O2

02

Explanation

The enthalpy change for reaction where one mole of hydrogen molecules combines with half a mole of oxygen molecules to produce water is ΔH=-2.86×105J, assuming that reactant gases and the resulting water are both at 25°Cand 1atmpressure. Because the water will be in the form of vapour at first, it will need to release heat in order to condense into a liquid and then cool to room temperature. This results in a decrease in the thermal energy U of the system because U depends on the temperature difference, Tf<Ti. As well, the atmosphere will fill in the volume originally occupied by the reactant gases, doing work PVon the system. The enthalpy change is the total heat emitted by the system as a result of these two mechanisms.

03

Explanation 

The energy resulting from the PV work is (assuming that the volume of the liquid water is negligible compared to the initial volume) is:

W=PΔV=PVf-Vi=-PVi

the final volume volume of the water and we neglect it Vf=0, since it is very small, the reactant gases and the resulting water are both at 25°Cand 1atmpressure, so the work (from ideal gas law) is therefore:

W=-PVi=-nRT

where n=0.5mol(H)+1mol(O)=1.5mol,R=8.31J·K-1·mol-1 and T=25°C=298°K, so:

W=-1.5×8.31×298=-3.7×103J
04

Explanation

The change in enthalpy in the reaction is given by:

ΔH=ΔU+W→ΔU=ΔH-W

Substitute, so:

ΔU=-2.86×105+3.7×103=-2.823×105J

The work, PΔV, contribution is:

WΔU=-3.7×103-2.823×105=0.0131WΔU=1.31%

The contribution of amount of heat come from the work done by the collapsing atmosphere is 1.31%, where the rest for 98.69% comes from the increase of internal energy of the system.

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Most popular questions from this chapter

Your 200 g cup of tea is boiling-hot. About how much ice should you add to bring it down to a comfortable sipping temperature of 65°C? (Assume that the ice is initially 65°C. The specific heat capacity of ice isrole="math" localid="1650146844935" 0.5cal/g°C.

Estimate the average temperature of the air inside a hot-air balloon (see Figure 1.1). Assume that the total mass of the unfilled balloon and payload is 500 kg. What is the mass of the air inside the balloon?

Measured heat capacities of solids and liquids are almost always at constant pressure, not constant volume. To see why, estimate the pressure needed to keep Vfixed as Tincreases, as follows.

(a) First imagine slightly increasing the temperature of a material at constant pressure. Write the change in volume,dV1, in terms of dTand the thermal expansion coefficient βintroduced in Problem 1.7.

(b) Now imagine slightly compressing the material, holding its temperature fixed. Write the change in volume for this process, dV2, in terms of dPand the isothermal compressibility κT, defined as

κT≡−1V∂V∂PT

(c) Finally, imagine that you compress the material just enough in part (b) to offset the expansion in part (a). Then the ratio of dPtodTis equal to (∂P/∂T)V, since there is no net change in volume. Express this partial derivative in terms of βandκT. Then express it more abstractly in terms of the partial derivatives used to define βandκT. For the second expression you should obtain

∂P∂TV=−(∂V/∂T)P(∂V/∂P)T

This result is actually a purely mathematical relation, true for any three quantities that are related in such a way that any two determine the third.

(d) Compute β,κT,and(∂P/∂T)Vfor an ideal gas, and check that the three expressions satisfy the identity you found in part (c).

(e) For water at 25∘C,β=2.57×10−4K−1andκT=4.52×10−10Pa−1. Suppose you increase the temperature of some water from 20∘Cto30∘C. How much pressure must you apply to prevent it from expanding? Repeat the calculation for mercury, for which (at25∘C)β=1.81×10−4K−1andκT=4.04×10−11Pa−1

Given the choice, would you rather measure the heat capacities of these substances at constant vor at constant p?

Heat capacities are normally positive, but there is an important class of exceptions: systems of particles held together by gravity, such as stars and star clusters.
aConsider a system of just two particles, with identical masses, orbiting in circles about their center of mass. Show that the gravitational potential energy of this system is-2times the total kinetic energy.
bThe conclusion of part aturns out to be true, at least on average, for any system of particles held together by mutual gravitational attraction:

U¯potential=−2U¯kinetic

Here each Urefers to the total energy (of that type) for the entire system, averaged over some sufficiently long time period. This result is known as the virial theorem. (For a proof, see Carroll and Ostlie (1996), Section 2.4.) Suppose, then, that you add some energy to such a system and then wait for the system to equilibrate. Does the average total kinetic energy increase or decrease? Explain.

cA star can be modeled as a gas of particles that interact with each other only gravitationally. According to the equipartition theorem, the average kinetic energy of the particles in such a star should be 32KT, whereT is the average temperature. Express the total energy of a star in terms of its average temperature, and calculate the heat capacity. Note the sign.
dUse dimensional analysis to argue that a star of mass Mand radius Rshould have a total potential energy of -GM2/R, times some constant of order 1.
eEstimate the average temperature of the sun, whose mass is 2×1030kgand whose radius is 7×108m. Assume, for simplicity, that the sun is made entirely of protons and electrons.

A battery is connected in series to a resistor, which is immersed in water (to prepare a nice hot cup of tea). Would you classify the flow of energy from the battery to the resistor as "heat" or "work"? What about the flow of energy from the resistor to the water?

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