Space.com says intergalactic hydrogen gas absorbs all optical light

In summary: The caption on the photo says "since all the optical light has been absorbed by intergalactic hydrogen gas, leaving only infrared light."Based on the article, it seems that the photo is of a distant GRB. The photo has been labeled as evidence that the expansion of space is the more likely explanation for the disappearance of optical light. The article also mentions that neutral hydrogen is an excellent absorber of visible light and that this is why we see a drop-off in light when radiation is more intense than Lyman alpha.
  • #1
thenewmans
168
1
What? Is there any truth to this? The caption on a space.com photo of the oldest object ever found says, "… since all the optical light has been absorbed by intergalactic hydrogen gas, leaving only infrared light." I'm thinking the expansion of space is a more likely explanation.

http://bit.ly/2smLUp - photo with caption

I found it in this article.
http://www.space.com/scienceastronomy/091028-most-distant-grb.html
 
Astronomy news on Phys.org
  • #2
Considering we 'see' stars, it doesn't seem correct that all optical light has been absorbed.

Is the photo caption referring to Milky Way stars in the foreground, as opposed to GRB which is far away?

I wonder how the EM signature of GRB 090423 compares with others, and how much of the 'color' is due to redshift vs scatter or absorption.
 
Last edited:
  • #3
From the Gemini Observatory website

http://www.gemini.edu/furthestgrb
“Our infrared observations from Gemini immediately suggested that this was an unusually distant burst, these images were the smoking gun." said Edo Berger, a leader in the scientific team that made the discovery and professor at Harvard Smithsonian Center for Astrophysics. "The visible light was completely absorbed by hydrogen gas in the early universe, but the GRB was brightly glowing in the infrared images from Gemini."
 
  • #4
The theory is that at present most of the intergalactic medium is ionized hydrogen, which let's most of the light through, but for a period in the early history of the universe, there would have been more neutral hydrogen gas around, which would absorb light. This is called the "Gunn-Peterson effect", and shows up as a "trough" feature in the spectra of the most distant quasars and galaxies.

For a summary, see http://en.wikipedia.org/wiki/Gunn-Peterson_trough" in Wikipedia.
 
Last edited by a moderator:
  • #5
Wow, you guys are great. That wikipedia page says it starts at about z=6. Ned Wright's calculator says that's about 12.7 billion years ago. So that GRB is well within that. Thanks.
 
  • #6
What I *think* they meant is that anything that we'd be seeing on Earth now as visible light now, would have been extreme UV when it was produced and the neutral hydrogen would have absorbed all of that. Any light that the original object produced would end up as infrared by the time it gets to earth.
 
  • #7
Also neutral hydrogen isn't a huge absorber of visible light. If you shine light through a hydrogen balloon most of it makes it through. It is a major absorber of extreme UV since if you have neutral hydrogen and shine extreme UV in it, it will knock off the electrons and ionize the hydrogen.

At z=8.2, anything that ends up as light on Earth is going to start out as UV.
 
  • #8
That seems to be what happened...

http://gcn.gsfc.nasa.gov/gcn3/9219.gcn3

Lyman alpha is the amount of energy that it takes to take a hydrogen atom from the ground state to the next higher state. Once you start exposing hydrogen atoms to radiation that's more intense than Lyman-alpha, you start breaking up the atom and so the amount of radiation that the hydrogen let's through drops dramatically. For radiation that less intense than Lyman-alpha, all you end up doing is jiggling the atom so the hydrogen really doesn't block that much radiation.

So we know what frequency you get this drop-off. If you see the drop-off in infrared, you then get a redshift. Get the redshift, you get a distance.
 

1. What is intergalactic hydrogen gas?

Intergalactic hydrogen gas refers to the hydrogen gas that exists between galaxies in our universe. It is the most abundant element in the universe and is present in the form of gas clouds that are spread out in the vastness of space.

2. How does intergalactic hydrogen gas absorb light?

Intergalactic hydrogen gas absorbs light through a process called Lyman-alpha absorption. This occurs when photons of light from a distant source, such as a star or galaxy, pass through the hydrogen gas clouds. The hydrogen atoms in the gas absorb the photons, causing them to lose energy and preventing them from reaching our telescopes.

3. Why does intergalactic hydrogen gas absorb all optical light?

Intergalactic hydrogen gas absorbs all optical light because it is made up of neutral hydrogen atoms that can only absorb a specific wavelength of light known as the Lyman-alpha line. This wavelength falls within the ultraviolet range, which is invisible to our eyes, making the gas appear to absorb all optical light.

4. How does this absorption affect our observations of the universe?

This absorption can affect our observations of the universe by making it difficult to see distant objects in the optical range. It can also distort the light from these objects, making it more challenging to study their properties and understand their evolution.

5. Is intergalactic hydrogen gas always present in space?

Yes, intergalactic hydrogen gas is always present in space. It is estimated that about 90% of the atoms in the universe are hydrogen, and a significant portion of these atoms exist as intergalactic gas. The amount of gas can vary in different regions of space, but it is always present.

Similar threads

Replies
4
Views
1K
  • Sci-Fi Writing and World Building
Replies
15
Views
3K
  • Other Physics Topics
Replies
0
Views
737
Replies
2
Views
3K
  • Quantum Physics
Replies
1
Views
2K
Replies
7
Views
10K
Replies
59
Views
10K
  • MATLAB, Maple, Mathematica, LaTeX
Replies
4
Views
2K
Back
Top