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Where does the radiated energy difference come from?

2007-10-05 07:20:54 · 4 answers · asked by Anonymous in Science & Mathematics Physics

This is a geothermodynamics Q.

2007-10-05 07:21:38 · update #1

BTW Does anybody know what the difference is in an energy rate of some kind and where I can find the info?

2007-10-05 09:46:02 · update #2

4 answers

Yes, but not by much. The excess consists of heat energy from below the surface, consisting of heat from radioactive decay as well as heat left over from the gravitational energy of the original agglomeration of the earth's matter.

2007-10-05 07:24:47 · answer #1 · answered by Anonymous · 3 1

Ever drill an oil well. It's hot down there. If the earth didn't radiate more energy than it absorbed from the sun the surplus added to the heat coming up through the ground would make things pretty unpleasant.

2007-10-05 18:25:01 · answer #2 · answered by Nomadd 7 · 1 0

Currently, thanks to global warming, the earth absorbs more energy than it radiates back to space. The total forcing is on the order of 1-1.5W per square meter if I am not mistaken.

According to

http://en.wikipedia.org/wiki/Geothermal_gradient

the average geothermal heat flow is 63mW per square meter, which would be roughly one twentieth of the total current climate forcing.

It always amuses me how fervent geothermal energy pundits get a kick out of putting solar energy down as "not concentrated enough" and such... 200W/m^2 is not good enough, yet their own average of 63mW/m^2 will save mankind... yeah, right.

Note: I do know the difference between averages and peak sources... it is the pundits who don't and like to compare apples with oranges to convince people who don't take the time to look up the reality behind their propaganda.

2007-10-05 14:43:02 · answer #3 · answered by Anonymous · 0 2

Hi,

no, it does not radiate more energy than it absorbs.

All energy on the earth can be traced back to the sun at one (1) point or another.

REgards,
Chas.

2007-10-05 14:24:18 · answer #4 · answered by Chas. 3 · 1 3

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