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

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The Earth's core contributes significantly less heat to the surface compared to solar radiation, with calculations showing that the core transfers approximately 4.4 x 10^17 J over 9 hours. In contrast, solar energy incident on Earth during the same period amounts to about 1.07 x 10^22 J. This results in a ratio indicating that the heat from the Earth's core is only 0.004% of the solar energy received. The thermal conductivity of the crust and the temperature gradient were essential in determining the core's contribution. Overall, solar radiation overwhelmingly dominates the heat energy reaching the Earth's surface.
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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.
 
The book claims the answer is that all the magnitudes are the same because "the gravitational force on the penguin is the same". I'm having trouble understanding this. I thought the buoyant force was equal to the weight of the fluid displaced. Weight depends on mass which depends on density. Therefore, due to the differing densities the buoyant force will be different in each case? Is this incorrect?

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