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This is a tricky concept. I'm not sure I grasp it entirely myself, but I'll give it a go.Nothing can move through space faster than the speed of light. However, there is no mechanism (that we know of) that prevents space between two object from expanding at an arbitrary rate, such that the distance between the objects increases faster than the speed of light.It appears that space is expanding all around us such that extremely distant objects (galaxies) appear to be moving away from us at speeds approaching the speed of light. If the distance between us and them is increasing faster than light can traverse the space, we can't (and won't ever) observe them.There are a few other reasons we may not be able to see distant galaxies:1) They are so far away that not enough light can reach us (too dim).2) They are so far away that other things get the way and block the light.3) They are space between us and them is expanding at nearly the speed of light, and the light gets redshifted so far that we cannot observe it4) They are so far away that the light hasn't had enough time to reach us (the universe has only been transparent for a little over a dozen billion years, so something 100 billion light years away won't be visible for quite some time, even if the other problems don't manifest.)Hope that helps.
Hello Chiral, you say ''the Universe has only been transparent for a little over a dozen billion years, so something 100 billion light years away won't be visible for quite some time''Can I ask why it would not be visible for some time if you state the universe is transparent?Can we not see through transparent things?
Quote from: Thebox on 18/02/2016 22:49:09Hello Chiral, you say ''the Universe has only been transparent for a little over a dozen billion years, so something 100 billion light years away won't be visible for quite some time''Can I ask why it would not be visible for some time if you state the universe is transparent?Can we not see through transparent things?A long time ago, the universe was very densely filled with very hot matter, and was therefore not transparent. Then, because it takes light a year (time) to travel a light year (distance), if an object is 100 billion light years away, it would take light 100 billion years for its light to reach us. Since light has only been able to travel through the universe for 13 billion years, there is no hope of seeing the light from such a distant object.
Interesting idea, would hot matter not give off light?
Quote from: Thebox on 18/02/2016 23:17:19Interesting idea, would hot matter not give off light? Yes. It is now what we call the cosmic microwave background. It was visible light when it was emitted, but has been redshifted so much that it now registers as microwaves.
does this CBMR you mention have substance, or is it just a Physical presence like Electromagnetic radiation?
Quote from: TheBoxdoes this CBMR you mention have substance, or is it just a Physical presence like Electromagnetic radiation?CMBR is electromagnetic radiation, with a peak in the microwave part of the spectrum (160 GHz).See: http://en.wikipedia.org/wiki/Cosmic_microwave_background..although I wouldn't really call electromagnetic radiation a "Physical presence", like (say) atoms or molecules.
Am I correct in thinking that cosmic background microwave radiation remains present in space without what we refer to as light
Quote from: Thebox on 19/02/2016 12:11:40Am I correct in thinking that cosmic background microwave radiation remains present in space without what we refer to as lightmicrowaves are electromagnetic radiation just like light, but much closer in frequency to radio waves. As such they do not depend on the presence of light or dark but propagate independantly.
does the cbmr ''fill'' the visual universe space
Quote from: Thebox on 19/02/2016 13:44:59 does the cbmr ''fill'' the visual universe spaceAs far as I am aware it is detected in every direction, but in varying intensities.
Quote from: Colin2B on 19/02/2016 16:33:44Quote from: Thebox on 19/02/2016 13:44:59 does the cbmr ''fill'' the visual universe spaceAs far as I am aware it is detected in every direction, but in varying intensities.Interesting, how do we distinguish the difference between the CBMR and electromagnetic radiation emitted from stars etc? In a rephrased form, how do we know that CBMR is not the detection of light propagating through space if it is detected as ''light''?
By physical presence I perceive that to be things that exist without solidity such as light or gravity.
how do we distinguish the difference between the CBMR and electromagnetic radiation emitted from stars etc?
Quote from: TheBoxBy physical presence I perceive that to be things that exist without solidity such as light or gravity.- By "Physical", I interpret something that can be touched and felt*. - By "presence", I interpret something that is here, and stationary relative to me.But:- Light cannot be touched or felt, so I would call it non-physical.- Light cannot be stationary relative to me, so I would call it non-presence.- If I were to make up a description of light, I prefer "non-physical non-presence".The same could be effectively said for gravitational waves and neutrinos - if they could be stationary, they would be definitely non-touchable.*Dictionary.com has 8 possible meanings for physical; part of one meaning does allow for energy as a subject for non-biological sciences Quotehow do we distinguish the difference between the CBMR and electromagnetic radiation emitted from stars etc?By their spectrum.- CMBR has an effective temperature of 2.7K, so its spectrum has a peak in the microwave band, and not much at Infra-Red. - Our Sun has a surface temperature of 5500K, so it has a peak in the visible band, with lots of infra-red, a bit of ultraviolet, and a moderate amount of microwaves.- Other stars, galactic dust and gas clouds have different temperatures and composition, each with their own spectrum.By measuring the radiation in space at multiple wavelengths, and by modeling the distribution of gas in the galaxy, it is possible to subtract out the effect of stars and dust clouds, leaving the contribution of the CMBR. A description of the process and sample images of each step may be found here: http://abyss.uoregon.edu/~js/ast123/lectures/lec23.html http://en.wikipedia.org/wiki/Cosmic_microwave_background#Data_reduction_and_analysis