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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.)

Short Answer

Expert verified

Rate of heat conduction and the rate at which the earth loses heat via conduction

QΔt=0.05W

QtotalΔt=2.573×1013

Step by step solution

01

Calculation of ratio

Because the rock that makes up the Earth's crust has a thermal conductivity and there is a temperature differential between a point underground and the Earth's surface, the Earth loses energy through heat conduction. We've calculated the following using Schroeder's values:ΔT=20Kper Δx=1000mand kt=2.5WK1, the rate of heat conduction in an area of 1m2is, therefore:

localid="1651746825640" QΔt=ktAΔTΔx=2.5×1×201000=0.05W/m2

localid="1651746839506" QΔt=0.05W/m2

02

Calculation of heat

Even if the rate of heat loss for a square metre is fairly low, if we assume that this figure applies to the entire Earth, the total heat loss is:

QtotalΔt=Loss per meter square×Total area of earth

QtotalΔt=0.05×4πr2=0.05×4π6400×1032

QtotalΔt=2.573×1013W

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Most popular questions from this chapter

At the back of this book is a table of thermodynamic data for selected substances at room temperature. Browse through the CPvalues in this table, and check that you can account for most of them (approximately) using the equipartition theorem. Which values seem anomalous?

Calculate the rms speed of a nitrogen molecule at room temperature.

Calculate the total thermal energy in a liter of helium at room temperature and atmospheric pressure. Then repeat the calculation for a liter of air.

Uranium has two common isotopes, with atomic masses of 238 and 235. one way to separate these isotopes is to combine the uranium with fluorine to make uranium hexafluoride gas, UF6, then exploit the difference in the average thermal speeds of molecules containing the different isotopes. Calculate the rms speed of each molecule at room temperature, and compare them.

In Problem 1.16 you calculated the pressure of the earth’s atmosphere as a function of altitude, assuming constant temperature. Ordinarily, however, the temperature of the bottommost 10-15 km of the atmosphere (called the troposphere) decreases with increasing altitude, due to heating from the ground (which is warmed by sunlight). If the temperature gradient |dT/dz|exceeds a certain critical value, convection will occur: Warm, low-density air will rise, while cool, high-density air sinks. The decrease of pressure with altitude causes a rising air mass to expand adiabatically and thus to cool. The condition for convection to occur is that the rising air mass must remain warmer than the surrounding air despite this adiabatic cooling.

a. Show that when an ideal gas expands adiabatically, the temperature and pressure are related by the differential equation

dTdP=2f+2TP

b. Assume that dT/dzis just at the critical value for convection to begin so that the vertical forces on a convecting air mass are always approximately in balance. Use the result of Problem 1.16(b) to find a formula for dT/dzin this case. The result should be a constant, independent of temperature and pressure, which evaluates to approximately 10°C/km. This fundamental meteorological quantity is known as the dry adiabatic lapse rate.

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