Why is Far-UV spectrum unobservable

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In summary, the far-UV spectrum is difficult to observe due to the strong absorption of hydrogen and interstellar dust at these wavelengths. This is why the optical and UV emissions from AGN are mainly from the accretion disk, which is often obscured by dust torii. Additionally, the Earth's atmosphere is highly effective at blocking UV light, making it necessary to use space-based telescopes to observe the UV spectrum.
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PianoDentist
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Hi

couldn't find a similar thread so thought i'd make one. I keep seeing around the web that the far-UV spectrum is unobservable (context is looking at the spectra of AGN) but no-one seems to explain why.

I think that its something to do with hydrogen strongly absorbs at these wavelengths so all the dust between us and what we're looking at intercepts all the radiation at these wavelengths.

But I am not sure if this is the case and I am not sure why hydrogen/ or interstellar dust would absorb strongly at these far UV frequencies.

if anybody can explain why the far-uv is unobservable that would be greatly appreciated!
 
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I am inferring this from the literature on AGN I've read but I am by no means confident in what I am saying: I think the optical & UV comes mainly from the accretion disk, which is generally obscured by the dust torii that surround it if it's observed sideways. The jets get in the way for compact objects that are at smaller inclination angles wrt the jet axis. So I think that's why it might by difficult to resolve disk UV emission specifically from other structures like the NLR clouds.

"The physics of AGN at all scales" (Springer) might have the answer to your question.
 
  • #3
Earths atmosphere is extremely efficient at blocking UV light - which is good because it keeps the sun from sterilizing the surface of the earth. Life on Earth was limited to the oceans until the atmosphere became oxygenated and the ozone layer formed. To observe the universe in the UV spectrum requires space based telescopes. See http://www.britannica.com/EBchecked/topic/613577/ultraviolet-telescope for discussion.
 

FAQ: Why is Far-UV spectrum unobservable

Why is the Far-UV spectrum unobservable?

The Far-UV spectrum (wavelengths between 100-200 nanometers) is unobservable because these wavelengths are absorbed by Earth's atmosphere. Specifically, the ozone layer in the stratosphere blocks most of the Far-UV radiation from reaching the surface.

Can we observe the Far-UV spectrum from space?

Yes, some space-based telescopes, such as the Hubble Space Telescope, are able to observe the Far-UV spectrum since they are above Earth's atmosphere. However, these telescopes have limited capabilities and cannot observe the full range of Far-UV wavelengths.

What type of radiation is present in the Far-UV spectrum?

The Far-UV spectrum is composed of ionizing radiation, which has enough energy to break chemical bonds. This type of radiation is harmful to living organisms, which is why Earth's atmosphere blocks it from reaching the surface.

Are there any natural sources of Far-UV radiation?

Yes, the sun is a natural source of Far-UV radiation. However, most of this radiation is absorbed by Earth's atmosphere before it reaches the surface. Other sources include stars and other astronomical objects.

How do scientists study the Far-UV spectrum if it is unobservable?

Scientists use specialized instruments and telescopes, such as the Hubble Space Telescope, to observe the Far-UV spectrum from space. They also use computer simulations and laboratory experiments to study the properties and effects of Far-UV radiation.

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