How Does Earth's Core Contribute to Surface Heat Compared to Solar Radiation?

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SUMMARY

The Earth's core contributes a mere 0.004% of the solar intensity at the surface, as calculated by comparing the heat transferred from the core to the energy received from the Sun. The heat transfer from the Earth's interior to the surface was determined using the formula dQ/dt = kA(dT/l), yielding a total of 4.4x1017 J over 9 hours. In contrast, the energy incident from solar radiation during the same period was calculated to be 1.07x1022 J. This stark difference highlights the dominance of solar energy in heating the Earth's surface.

PREREQUISITES
  • Understanding of thermal conductivity and heat transfer equations.
  • Familiarity with the concept of solar irradiance.
  • Basic knowledge of the Earth's geometry and surface area calculations.
  • Ability to perform unit conversions and dimensional analysis.
NEXT STEPS
  • Explore the principles of heat transfer in geology, focusing on thermal conductivity.
  • Research solar irradiance calculations and their implications for climate science.
  • Investigate the Earth's energy balance and the role of geothermal energy.
  • Learn about the methods for measuring and modeling Earth's surface temperatures.
USEFUL FOR

Students in earth sciences, physicists studying energy transfer, and climate scientists analyzing the contributions of geothermal heat versus solar radiation.

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Homework Statement


The temperature within the Earth's crust increases about 1.0 C∘ for each 30 m of depth. The thermal conductivity of the crust is 0.80 W/C∘⋅m.
A)Determine the heat transferred from the interior to the surface for the entire Earth in 9.0h .
B)Compare this heat to the amount of energy incident on the Earth in 9.0h due to radiation from the Sun.

Homework Equations


dQ/dt = kA(dT/l)

The Attempt at a Solution


I have solved the first part.
surface area of Earth = 4pir^2 = 4pi(6.378x10^6 m)^2 = 5.1x10^14 m^2
dQ/dt = kA(dT/l)
dQ/dt = (.80 J/smC)(5.1x 10^14 m^2)(1 C/ 30m)
dQ/dt = 1.36x10^13 J/s

9h is 9h(3600 s/h) = 32400 s

32400s(1.36x10^13 J/s) = 4.4x10^17 J

The second part I am having a hard time understanding. I'm not really sure I even know what they are asking
 
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Well, I take it they want you to estimate solar irradiance, right ?
Don't worry about more than one or two decimals of accuracy...
And pay attention to the fact that values such as in the table here are for perpendicular incidence.
 
part b of the problem asks you to compare energy into the surface from the core and compare it to the sun,
energy from the sun:
1300 W/m^2 *(4*pi*(6.37*10^6)^2)* .5 (only half the Earth is hit per second) = 3.32*10^17 W sun.
3.32*10^17 W * 32400 s = 1.07*10^22 J
now create a ratio:
Jcore/Jsun = (4.4*10^17)/(1.07*10^22)

the Earth's core only adds .004% of the suns solar intensity to the surface.
 

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