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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 93atm, and the average temperature is localid="1648638013375" 470°C. 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 localid="1648638019185" 450°C. 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 CO2molecule islocalid="1648638027654" 1.5×10-10m.

Short Answer

Expert verified

a.The root mean square speed is638m/s.

b.Mean free path of carbon dioxide is2.6nm.

Step by step solution

01

Calculation for root mean square speed (part a)

a.

The average translational kinetic energy is

ϵavg=32kBT.......1

ϵavg=12mvrms2.......2

Equating 1and 2

12mvrms2=32kBT

vrms=3kBTm...3

The molecular mass of carbon dioxide ism=40u.

Converting this tokg,

we get the mass of one molecule of oxygen by,

m=40u×1.66×10-27kg1u=73×10-27kg....3

TK=TC+273

=450°C+273

=723K

Substitute all values in below equation,

localid="1648638355268" vrms=3kBTm

localid="1648638366804" =31.38×10-23J/K(723K)73×10-27kg

localid="1648638394867" role="math" vrms=638m/s

02

Calculation for NV (part b)

(b) The ideal gas law,

pV=NkBT

NV=pkBT.........4

WherekBis Boltzmann's constant and inSIunit its value is,

kB=1.38×10-23J/K

The pressure is given in localid="1648638535433" atm.

So we need to convert it into Pascal by,

localid="1648638696043" p=(93atm)1.013×105Pa1atm=94.2×105Pa

localid="1648638706189" NV=94.2×105Pa1.38×10-23J/K(723K)

localid="1648638716592" NV=9.4×1026m-3

03

Calculation for mean free path part (b) solution

b.

The average distance traveled by the molecule between collisions is known as the mean free path.

Substitute all values,

λ=142π(N/V)r2

=142π9.4×1026m-31.5×10-10m2

λ=2.6nm

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Most popular questions from this chapter

Uranium has two naturally occurring isotopes. U238 has a natural abundance of 99.3% andU235 has an abundance of 0.7%. It is the rarer U235that is needed for nuclear reactors. The isotopes are separated by forming uranium hexafluoride, role="math" UF6, which is a gas, then allowing it to diffuse through a series of porous membranes. UF6235 has a slightly larger rms speed than UF6238 and diffuses slightly faster. Many repetitions of this procedure gradually separate the two isotopes. What is the ratio of the rms speed of UF6235 to that ofUF6238?

Consider a container like that shown in Figure 20.12, with n1moles of a monatomic gas on one side and n2moles of a diatomic gas on the other. The monatomic gas has initial temperature T1i. The diatomic gas has initial temperatureT2i .
a. Show that the equilibrium thermal energies are

E1f=3n13n1+5n2E1i+E2iE2f=5n23n1+5n2E1i+E2i

b. Show that the equilibrium temperature is

Tf=3n1T1i+5n2T2i3n1+5n2

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b. What is the final thermal energy of each gas?

c. How much heat energy is transferred, and in which direction?

d. What is the final temperature?

Scientists studying the behavior of hydrogen at low temperatures need to lower the temperature of 0.50molof hydrogen gas from 300K to 30K. How much thermal energy must they remove from the gas?

An experiment you're designing needs a gas with γ=1.50. You recall from your physics class that no individual gas has this value, but it occurs to you that you could produce a gas with γ=1.50by mixing together a monatomic gas and a diatomic gas. What fraction of the molecules need to be monatomic?

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