![]() |
#1
|
|||
|
|||
![]()
Well Double-A prompted me to go with this posts(thoughts of) Double-A
the universe is expanding,at an accelerating rate and you can add that to these other reasons for the color red. Let me start with a very hot star our eyes pick up its intensity as blue" and a cool star as "red,but here is the reality the hot star is radiating more in the red part of the spectrum than is a cool star that appears red.Hmmm I could almost end this post with that information. Just about all galaxies are moving away from us,and that means longer wave lengths and that means more red photons. Another reason for red is dust. For us to view another galaxy we must look through the dust of our galaxy. This reddens the light. Seems to me the composition,and structure of dust particles must show themselves in the red spectrum(good reasons for this) Most galaxies are very far from us,and as their recessional velocity gets greater with increase distance they appear "highly red shifted" I think I red(not sure) that more luminous galaxies are redder because they contain more metals. We know that star formation has slowed down that means more old stars in this spacetime than new ones Stars redden as they age. Well I( seemed to run out of thoughts on reddening. So let me leave asking this question. Can the inverse square law that photons obey result over spacetime more red photons? Bert |
#2
|
|||
|
|||
![]()
photons?
Certainly, Or preferably mine. _______ Blog, or dog? Who knows. But if you see my lost pup, please ping me! A HREF="http://journals.aol.com/virginiaz/DreamingofLeonardo"http://journal s.aol.com/virginiaz/DreamingofLeonardo/A |
#3
|
|||
|
|||
![]() photons? Certainly, Or preferably mine. I'll be Graviton If you wish! _______ Blog, or dog? Who knows. But if you see my lost pup, please ping me! A HREF="http://journals.aol.com/virginiaz/DreamingofLeonardo"http://journal s.aol.com/virginiaz/DreamingofLeonardo/A |
#4
|
|||
|
|||
![]()
Well I'm looking at my red sun glasses,and the reason they are red is
only red light can go through the glass. What if space has this same feature??? Bert |
#5
|
|||
|
|||
![]()
Can the
inverse square law that photons obey result over spacetime more red photons? Could be! _______ Blog, or dog? Who knows. But if you see my lost pup, please ping me! A HREF="http://journals.aol.com/virginiaz/DreamingofLeonardo"http://journal s.aol.com/virginiaz/DreamingofLeonardo/A |
#6
|
|||
|
|||
![]()
In ,
G=EMC^2 Glazier typed: Well I'm looking at my red sun glasses,and the reason they are red is only red light can go through the glass. What if space has this same feature??? Bert You already know this, but a little reminder: Red shifting is not the same as red filtering. Hope Moby is well. I played with one of his wild cousins a few years back, we had fun. Jo |
#7
|
|||
|
|||
![]() |
#8
|
|||
|
|||
![]()
Hi Jo Just wanted to list the many ways light can go to red. Moby is
doing well. He knows how to keep time,and if I'm late with his Epswich clams he gets very festy. Likes to be lifted up and down out of the water(dunked),and won't let go of my fingers. Have to keep his tank under the air-conditioner for he likes cold water,and hate's the sun. Bert |
#9
|
|||
|
|||
![]() "G=EMC^2 Glazier" wrote in message ... Well I'm looking at my red sun glasses,and the reason they are red is only red light can go through the glass. What if space has this same feature??? Bert I dunno Bert, but it is good for the libido to look at the world with rose colored glasses even if the universe does not return the favor. BV. |
#10
|
|||
|
|||
![]()
Double-A wrote:
(G=EMC^2 Glazier) wrote in message ... Well I'm looking at my red sun glasses,and the reason they are red is only red light can go through the glass. What if space has this same feature??? Bert That's an interesting thought, but I believe they can tell by the shifting of spectral lines for elements such as hydrogen in the light that it has been Doppler shifted and not merely filtered through red space dust. Certainly, and the Doppler shift of each component could likely be identified. Suppose we're looking at a star that's receding from us: the bright emission lines from excited atoms in its atmosphere will appear at slightly lower frequencies than in a standard spectrum, all of them by the same amount. Now suppose that the star had gone through an episode of coughing up red dust -- however unlikely that may be -- in an expanding cloud whose trailing edge (that we have to look through to see the star) is actually approaching us. We must be calling the dust "red" because it absorbs a lot of blue and green light, showing a spectrum with dark bands in those regions, so we'd only be able to see the emission lines in the red area, or elsewhere between gaps in the pattern. But this "reddening" is quite independent of the red-shift in the bright spectrum. Anyway, assuming that we can identify the 'signature' of the absorbing material, we'll see the dark bands at slightly *higher* frequencies than normal. From this we could deduce that the dust is approaching us while the star is receding. This may be a rather silly example, but the principle that different sets of spectral features can show different red- or blue-shifts is important in the study of close binary systems, stars with turbulent atmospheres, planetary nebulae (& other kinds), star-systems containing disks or vortices of gas, and other situations where various different types of material are in motion. -- Odysseus |
|
Thread Tools | |
Display Modes | |
|
|