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Consider the combustion of one mole of methane gas:

CH4(gas)+2O2(gas)CO2(gas)+2H2O(gas)

The system is at standard temperature (298K)and pressure 105Paboth before and after the reaction.

(a) First imagine the process of converting a mole of methane into its elemental constituents (graphite and hydrogen gas). Use the data at the back of this book to find ΔHfor this process.

(b) Now imagine forming a mole of CO2and two moles of water vapor from their elemental constituents. Determine ΔHfor this process.

(c) What is ΔHfor the actual reaction in which methane and oxygen form carbon dioxide and water vapor directly? Explain.

(d) How much heat is given off during this reaction, assuming that no "other" forms of work are done?

(e) What is the change in the system's energy during this reaction? How would your answer differ if theH2Oended up as liquid water instead of vapor?

(f) The sun has a mass of2×1030kgand gives off energy at a rate of 3.9×1026watts. If the source of the sun's energy were ordinary combustion of a chemical fuel such as methane, about how long could it last?

Short Answer

Expert verified

The data at the back of this book to find Hlocalid="1650341273731" Hfor this process. is

localid="1650341277027" (a)ΔHCH4(dissociation)=74.81kJ

Forming a mole of localid="1650341280022" H and two moles of water vapor from their elemental constituents is

localid="1650341283020" (b)ΔH=877.15kJ

For the actual reaction in which methane and oxygen form carbon dioxide and water vapor directly localid="1650341286125" (c)ΔH=802.34kJ

Heat is given off during this reaction, assuming that no "other" forms of work are done is

localid="1650341289419" (d)Q=802.34kJ

(e) If the water in vapor state localid="1650341292882" ΔU=-802.34kJIf the water in liquid statelocalid="1650341296979" ΔU=-890.36-(-4.95)=-885.41kJ

The sun's energy were ordinary combustion of a chemical fuel such as methane, could it last at

localid="1650341300797" (f)t=1652y

Step by step solution

01

Step1:Temperature Reaction(part a)

(a)Using the enthalpy of the reactants and products, we can calculate how much heat is emitted or absorbed by a chemical reaction. Consider the combustion of methane in the presence of oxygen at a constant temperature of 298°K:

CH4(gas)+2O2(gas)CO2(gas)+2H2O(gas)

(a) The enthalpy for the formation of methane from elemental carbon (solid) and hydrogen (gas) is calculated using the table at the back of Schroeder's book as follows:

2H2(gas)+C(solid)CH4(gas)

2ΔHH2+ΔHCΔHCH4

2(0)+(0)74.81

02

Step2:determine∆H(part b)

Similarly, the enthalpy for producing one mole of carbon dioxide from elemental carbon (solid) and oxygen (gas) isO2(gas)+C(solid)C2(gas)

localid="1650341326563" ΔHO2+ΔHCΔHCO2(0)+(0)393.51

Solocalid="1650341329756" ΔHfor the formation of methane is therefore:

localid="1650341332718" ΔHCO2ΔHCΔHO2=393.5100=393.51kJ

localid="1650341335575" ΔHCO2(formation)=393.51kJ

The enthalpy of forming two moles of vapor from elemental oxygen (gas) and hydrogen (gas) is as follows

localid="1650341339663" 2H2(gas)+O(gas)2H2O(gas)

localid="1650341342662" 2ΔHH2+ΔHO2ΔHH2O2(0)+(0)2(241.82)

Solocalid="1650341346216" ΔHAs a result, the formation of two moles of water is required.:

localid="1650341349932" 2ΔHH2OΔHOΔHH2=2(241.82)00=483.64kJ

localid="1650341353807" ΔH2H2O(formation)=483.64kJ

The enthalpy of producing one mole of CO2 and two moles of water is:

localid="1650341357759" ΔH=ΔH2H2O(formation+ΔHCO2(formation)=483.64+393.51

localid="1650341361917" ΔH=877.15kJ

03

Step3:Describe which methane and oxygen(part c)

(c)ΔHfor the reaction as a whole is;ΔH=ΔHprodΔHreact

where localid="1650341370451" ΔHprodis the enthalpy of producing one mole of CO2 and two moles of water. (calculated in (b)), and localid="1650341373459" ΔHreactis the enthalpy of methane dissociation (calculated in localid="1650341376617" (a)), It is worth noting that the enthalpy of oxygen dissociation is zero. so:

localid="1650341379957" ΔH=ΔHC2(formation)+ΔH2H2O(formation)ΔHCH4(dissociation)

localid="1650341383103" ΔH=393.51483.64+74.81=802.34kJ

04

Step4:how much heat is produced during this reaction (part d)

(d) The enthalpy at constant pressure is given by:

ΔH=Q+Wother

Because no other work is being done on the reaction, the amount of heat is therefore:

Q=ΔH=802.34kJ

05

Step5:During this reaction, the system energy(part e)

(e) If all four compounds in the main equation are gases and the temperature is the same on both sides, there will be no volume changeV=0because three moles of gas are present both before and after the reaction As a result, for one mole of methane, the entire change in enthalpy is due to a change in internal energy U.

ΔH=ΔU+PΔVΔU=ΔH=802.34kJ

If water is produced as a liquid rather than a vapor, the enthalpy for producing two moles of liquid water from elemental oxygen (gas) and hydrogen (gas) is:

2H2(gas)+O(gas)2H2O(liquid)

2ΔHH2+ΔHO2ΔHH2O2(0)+(0)2(285.83)

So ΔHas a result of the formation of methane:

2ΔHH2OΔHOΔHH2=2(285.83)00=571.66kJ

So, ΔHfor the reaction as a whole is:

ΔH=393.51571.66+74.81=890.36kJ

This time, the final volume is 13of the initial volume, Because the two moles of water have condensed into a liquid with a negligible volume in comparison to the gases. As a result, the environment is effective:

W=PΔV=RTΔn=RTnfni

As a result, the change in internal energy is discovered from:

ΔU=ΔHW

ΔU=890.36(4.95)=885.41kJ

The latent heat of vaporization should be the difference between this value and when the water is produced as vapor at 298K.

06

Step6:The sun been in existence (part f)

(f) Suppose the Sun with a mass of around 2×1033gand luminosity of3.839×1026watts Its energy source was the combustion of methane and oxygen. The molar weights of methane and molecular oxygen are approximately16mgand 32mg, respectively. The chemical reaction of methane consumption is as follows:

CH4(gas)+2O2(gas)CO2(gas)+2H2O(gas)

So, if the Sun is made up of one part methane and two parts oxygen, the mole ratio is:

nCH4nO2=12

The mass ratio is then:

mCH4mO2=mass of one mole of methane×nCH4mass of one mole of oxygen×nO2

mCH4mO2=16×132×2=14

As a result, the mass of methane in the Sun is:

mCH4=ratio of methane mass×Sun mass

mCH4=14+1×2×1033=4×1032g

As a result, the number of moles of methane in the Sun is:

nCH4=methane mass in the sunmass of one mole of methane

nCH4=4×103216=2.5×1031mol

07

Step7:How long can the sun last if it has a mass?(part f)

(f)Assuming that the water is produced as vapor, the Sun could generate a total energy of:

E=number of methane moles×energy of one mole consumption

where the energy of one mole consumption is substituted802.34kJ, so:

E=2.5×1031×802.34=2×1034kJ

so it would burn out after a time interval of:

Power=Ett=EPower

substitute, where Power=3.839×1026watts

t=2×1034kJ3.839×1026Js1=2×1037J3.839×1026Js1=5.2×1010s

t=1652y

We're pretty sure the Sun's power source isn't chemical reactions!

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Most popular questions from this chapter

Geologists measure conductive heat flow out of the earth by drilling holes (a few hundred meters deep) and measuring the temperature as a function of depth. Suppose that in a certain location the temperature increases by20Cper kilometer of depth and the thermal conductivity of the rock is 2.5W/mK. What is the rate of heat conduction per square meter in this location? Assuming that this value is typical of other locations over all of the earth's surface, at approximately what rate is the earth losing heat via conduction? (The radius of the earth is 6400km.)

Even at low density, real gases don’t quite obey the ideal gas law. A systematic way to account for deviations from ideal behavior is the virial

expansion,

PVnRT(1+B(T)(V/n)+C(T)(V/n)2+)

where the functions B(T), C(T), and so on are called the virial coefficients. When the density of the gas is fairly low, so that the volume per mole is large, each term in the series is much smaller than the one before. In many situations, it’s sufficient to omit the third term and concentrate on the second, whose coefficient B(T)is called the second virial coefficient (the first coefficient is 1). Here are some measured values of the second virial coefficient for nitrogen (N2):

T(K)
B(cm3/mol)
100–160
200–35
300–4.2
4009.0
50016.9
60021.3
  1. For each temperature in the table, compute the second term in the virial equation, B(T)/(V/n), for nitrogen at atmospheric pressure. Discuss the validity of the ideal gas law under these conditions.
  2. Think about the forces between molecules, and explain why we might expect B(T)to be negative at low temperatures but positive at high temperatures.
  3. Any proposed relation between P, V, andT, like the ideal gas law or the virial equation, is called an equation of state. Another famous equation of state, which is qualitatively accurate even for dense fluids, is the van der Waals equation,
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  4. Plot a graph of the van der Waals prediction for B(T), choosing aand bso as to approximately match the data given above for nitrogen. Discuss the accuracy of the van der Waals equation over this range of conditions. (The van der Waals equation is discussed much further in Section 5.3.)

An ideal diatomic gas, in a cylinder with a movable piston, undergoes the rectangular cyclic process shown in the given figure.

Assume that the temperature is always such that rotational degrees of freedom are active, but vibrational modes are "frozen out." Also assume that the only type of work done on the gas is quasistatic compression-expansion work.

(a) For each of the four steps A through D, compute the work done on the gas, the heat added to the gas, and the change in the energy content of the gas. Express all answers in terms of P1,P2,V1,andV2. (Hint: Compute ΔUbefore Q, using the ideal gas law and the equipartition theorem.)

(b) Describe in words what is physically being done during each of the four steps; for example, during step A, heat is added to the gas (from an external flame or something) while the piston is held fixed.

(c) Compute the net work done on the gas, the net heat added to the gas, and the net change in the energy of the gas during the entire cycle. Are the results as you expected? Explain briefly.

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  1. Consider a small portion (area = A) of the inside wall of a container full of gas. Show that the number of molecules colliding with this surface in a time interval Δtis role="math" localid="1651729685802" PAΔt/(2mvx¯), where width="12" height="19" role="math">Pis the pressure, is the average molecular mass, and vxis the average xvelocity of those molecules that collide with the wall.
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  3. If we now take away this small part of the wall of the container, the molecules that would have collided with it will instead escape through the hole. Assuming that nothing enters through the hole, show that the number Nof molecules inside the container as a function of time is governed by the differential equation
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