Wien's Law & Earth Emission Spectra: Investigating the discrepancy

In summary, a conversation about emission spectra of the Earth revealed discrepancies between the expected temperature and peak emission according to Wien's displacement law and the actual observations. Possible explanations include a non-black body emission from the atmosphere due to molecular rotational and vibrational modes, as well as the emission temperature being that of the atmosphere rather than the surface.
  • #1
natski
267
2
Hi,

I have found several links using google to emission spectra of the Earth:

http://lasp.colorado.edu/~bagenal/1010/SESSIONS/13.Light.html
http://www.xylenepower.com/
http://spaceguard.esa.int/NScience/n...y/emission.htm

All of which indicate a temperature of 280K and peak clearly at around 18microns. However, Wien's displacement law indicates that the peak from thermal emission of the Earth should be at around 10 microns.

Many of these websites are indeed specifically about Wien's law and yet these two values do not correlate at all. What is going on?

Natski
 
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  • #2
natski said:
Hi,

All of which indicate a temperature of 280K and peak clearly at around 18microns. However, Wien's displacement law indicates that the peak from thermal emission of the Earth should be at around 10 microns.

Many of these websites are indeed specifically about Wien's law and yet these two values do not correlate at all. What is going on?
How did one determine it should be 10 microns?

This figure from the first link cited shows about 18 microns.

http://lasp.colorado.edu/~bagenal/1010/graphics/earth_ir_emission.gif
 
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  • #3
Zealous crackpots seeking validation on the net, natski. Is a common affliction.
 
  • #4
From Wien's displacement law 280K would give a peak at about 10 microns. I don't know how they came up with that graph but the theoretical black body line should not be 280K if it peaks at 18 microns.
 
  • #5
I used the calculator here -

http://hyperphysics.phy-astr.gsu.edu/hbase/wien.html#c3

And 280K corresponds to a wavelength of 10.35 microns - peak, but

a peak wavelength of 18 microns correspond to 161 K.


What's up with that?

Does this imply that the blackbody approximation is not valid?
 
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  • #6
http://wxpaos09.colorado.edu/radiation/background.html" page and a couple of others I found show the peak in the correct place. All I can assume is they've taken the emission spectrum from something else and drawn the theoretical curve on and assumed it was the Earth's temperature of ~280K.
 
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  • #7
Looking at the absorbtivity plot on the page cited by Kurdt in the previous post, there is a conspicuous peak at around 18 microns for CO2 and a band where absorption by water for wavelengths above 18 microns.

The absorption in the atmosphere seems dominated by H2O with some contribution from CO2. Does this imply the emission is also dominated by H2O?
 
  • #8
I'm by no means an expert Astro, but from what I can gather it is this NASA image that they have adapted.

http://origins.jpl.nasa.gov/habitable-planets/invest12.html

I don't think its a true Earth spectrum but an ideal spectrum of an Earth like planet which the ESA will be looking for with projects like DARWIN and NASA with their origins project.
 
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  • #9
I think the emission spectra that peaks at 18 microns is correct, despite the fact it disagrees with Wien's law. The reason for this is that my supervisor, who specializes in atmospherics, showed me the bible of atmospherics and in it the Earth spectra was also peaking at 15-18 microns, labeled as 300K. (I will post the name of the book soon, just looking for it now)

I thought at first this could be due a doppler shift or something but these observations should not have a moving observer. The book in question makes very little reference to Wien's law however.

Another possible explanation is that this emission temperature is the temperature of the atmosphere and not the surface. Perhaps a surface temp of 300K implies an atmospheric temp of 200K which implies an emission peak at 18 microns?

Natski
 
  • #10
natski said:
Another possible explanation is that this emission temperature is the temperature of the atmosphere and not the surface. Perhaps a surface temp of 300K implies an atmospheric temp of 200K which implies an emission peak at 18 microns?
According to the emission spectrum on the page (Investigation Twelve: Detect giant planets by direct imaging, and study their properties.) cited by Kurdt, there is a peak at approximately 18 microns, and the broadening would have to do with the fact that there is a temperature distribution as well as doppler effect. Perhaps it implies that the atmosphere does not emit as a black body, since the molecules have rotational modes as well as vibrational modes (?). Ostensibly the emission is characteristic of a particular mode of a particular molecular species.
 

1. What is Wien's Law?

Wien's Law is a scientific principle that states that the wavelength of the peak emission of thermal radiation from a blackbody is inversely proportional to its temperature. In other words, as the temperature of an object increases, the wavelength of its peak emission decreases.

2. How is Wien's Law related to Earth's emission spectra?

Wien's Law can be applied to the Earth's emission spectra, which is a graph showing the amount of thermal radiation emitted by the Earth at different wavelengths. By using Wien's Law, scientists can determine the temperature of the Earth's surface based on the wavelength of its peak emission.

3. What is the discrepancy in Wien's Law when applied to the Earth's emission spectra?

The discrepancy in Wien's Law when applied to the Earth's emission spectra is that the calculated temperature of the Earth's surface is much lower than the actual temperature measured by satellites. This is because the Earth's atmosphere absorbs and re-emits thermal radiation, causing a shift in the peak emission wavelength.

4. How do scientists investigate the discrepancy in Wien's Law and the Earth's emission spectra?

Scientists use advanced technology, such as satellites and spectrometers, to measure and analyze the Earth's emission spectra. They also use computer models to simulate the effects of the Earth's atmosphere on thermal radiation. By comparing the data from these methods, scientists can better understand and account for the discrepancy in Wien's Law.

5. What are the implications of the discrepancy in Wien's Law and Earth's emission spectra?

The discrepancy in Wien's Law and Earth's emission spectra has important implications for studying the Earth's climate and global warming. By accurately understanding and correcting for this discrepancy, scientists can improve their understanding of the Earth's energy balance and better predict future climate changes.

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