Edit: Bad example. Looking for a different galaxy.
Ya, I'll bet it was a "bad example" alright.
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Edit: Bad example. Looking for a different galaxy.
It seems to me that this statement and claim is "brainwashed" into every single first year *astronomy* student perhaps, but I'm not finding such literature related to *all* forms of scattering. Even if that *is* true of Compton scattering, that's just *one* type of scattering!
How about one of you now providing us with a 'non blurred' image of the most *distant* galaxies?
Ya, I'll bet it was a "bad example" alright.Too bad I missed it.
![]()
HubbleSite - NewsCenter - Tracing the Evolution of the First Galaxies in the Universe (09/13/2006) - Release Images
Here's a few. Which one is as "clear" and non-blurred as your close galaxy?
Deep field photo showing clear disk shaped galaxies:
File:HubbleDeepField.800px.jpg - Wikipedia, the free encyclopedia
We should be able to get that type of clarity if PC is true.
In other words *so much* inelastic scattering takes place between here and there, that some wavelengths simply don't make it at all, and *that* is how they determine that it's a "distant" galaxy.This abrupt drop-off in the flux is strongly characteristic of star-forming galaxies at high redshifts and occurs due to the absorption of light by the large amounts of neutral hydrogen in the universe at early times. Astronomers use the presence of this break to find high-redshift galaxies.
It seems to me that this statement and claim is "brainwashed" into every single first year *astronomy* student perhaps, but I'm not finding such literature related to *all* forms of scattering. Even if that *is* true of Compton scattering, that's just *one* type of scattering!
How about one of you now providing us with a 'non blurred' image of the most *distant* galaxies?
The most distant ones look a lot more blurry to me than your close up image of a nearby galaxy.
In other words *so much* inelastic scattering takes place between here and there, that some wavelengths simply don't make it at all, and *that* is how they determine that it's a "distant" galaxy.![]()
In other words *so much* inelastic scattering takes place between here and there, that some wavelengths simply don't make it at all, and *that* is how they determine that it's a "distant" galaxy.![]()
ESA Science & Technology: Young Galaxy in the Hubble Ultra Deep Field at Redshift 5.76
It looks like nothing more than a red smudge and that's not a even a 7 redshift.
I would say it is more like Michael did not do the basic research that someone with a scientific background would do.IOW, Michael was shown to be wrong in 1954.
Wrong, because you did not read what was cited.Right, because everything we know about scattering was already known in 1953 by one guy that apparently talked *exclusively* about Compton scattering.
The physics is farily simple and clearly valid.I haven't even been completely through the rebuttal paper, but already it's clearly bogus. Any loss of momentum of the photon would be transferred to the particle in question.
Actually what he showed was that it does not work for *for any scattering* including Brillouin scattering and Raman scattering.All he showed is that it does not work *for Compton scattering*.
In other words *so much* absorption takes place between here and there, that some wavelengths simply don't make it at all, and *that* is one way they determine that it's a "distant" galaxy.Here was my favorite line of the link I handed you:
In other words *so much* inelastic scattering takes place between here and there, that some wavelengths simply don't make it at all, and *that* is how they determine that it's a "distant" galaxy.This abrupt drop-off in the flux is strongly characteristic of star-forming galaxies at high redshifts and occurs due to the absorption of light by the large amounts of neutral hydrogen in the universe at early times. Astronomers use the presence of this break to find high-redshift galaxies.![]()
None of them because they are pixelatted.HubbleSite - NewsCenter - Tracing the Evolution of the First Galaxies in the Universe (09/13/2006) - Release Images
Here's a few. Which one is as "clear" and non-blurred as your close galaxy?
There is no known interaction that can degrade a photon's energy without also changing its momentum, which leads to a blurring of distant objects which is not observed. The Compton shift in particular does not work.
For example, Zwicky considered whether an integrated Compton Effect could account for the scale normalization of the above model:
... light coming from distant nebulae would undergo a shift to the red by Compton effect on those free electrons [in interstellar spaces] [...] But then the light scattered in all directions would make the interstellar space intolerably opaque which disposes of the above explanation. [...] it is evident that any explanation based on a scattering process like the Compton effect or the Raman effect, etc., will be in a hopeless position regarding the good definition of the images.[6]
Actually what he showed was that it does not work for *for any scattering* including Brillouin scattering and Raman scattering.
Read: The red shift in the spectra of distant galaxies Atkinson, Robert d'Escourt 1954
Robert d'Escourt explicitly states that he is no longer considering just Compton scattering. He is responding to Shelton's "not prepared to guess in detail" about the interaction by showing that any interaction with just changes in the forward velocity of the particle violates the conservation of momentum.
Did you take a look at the pixelation? The feature you are pointing to is only a few pixels in diameter.
Actually what he showed was that it does not work for *for any scattering* including Brillouin scattering and Raman scattering.
Oh man - you're so close to figuring this out now. You see and acknowledge wavelength dependence...
just take the next step to realising something wavelength dependent can't be a 'bit of' something wavelength independent and you'll be there...