Exploring Redshift Anomalies: Shape Distortion and Non-Visible Light Experiments

In summary, the conversation revolves around crude experiments investigating red shift anomalies and seeking input for corrections and improvements. The experiments involve using telescopes and spectography to determine velocity fields and redshift values of various astronomical objects, as well as testing for the effects of object shape on perceived redshift values. The conversation also touches on the importance of understanding optics and using diagrams to explain concepts.
  • #1
codex34
22
0
Anyone interested in going over some crude experiments and having a look to see if anything stands out as incorrect or impracticle?

I'm not interested in any discussion as to the validity of doing the experiments, kindly keep that nonsense to yourself, I'm only interested in any input to correct, improve on them, or extend them for non visible or polarized light.

These experiments represent an attempt to investigate red shift anomolies through experiment rather than to use statistical probability to simply ignore them.
The experiments are quite simple, they test primarily for shape distortion of redshift values, that is, to determine whether object shape has any bearing on perceived redshift value, shape being determined to be both perceived visible shape and non perceived - non visible shape which include but are not limited to components such as jets, rings, or any other observations that are not included in the visible light spectrum.

Experiment 1
A telescope is set up to determine the velocity field of a star in a polar region using long slit spectography.
After determining the velocitiy field, the slit, prism/grating, and detection equipment is fixed in place to prevent further adjustment or tampering.
Each week a further velocity field is measured for a period of 3 to 12 months.
Testing should also be performed on astronomical objects of differing shapes.

Experiment 2
A telescope is set up to determine the redshift value of an edge on galaxy.
The spectrographic equiptent is modified to rotate both the prism/grating and detection equiptment together about an axis that runs from the center of the collimating lens/mirror to the center of the prism/grating (ie, the optical axis).
The redshift value is determiined and compared to the already known value.
After determining the redshift value, the prism/grating and detection equpitment assembly is rotated about the aforementioned axis in 5° steps with a redshift value being determinied for each step.
The experiment should continue for a full 360° sample of values.

Experiment 3
A telescope is set up to determine the velocity fiields of an edge on galaxy.
The telescope is set up similarily to experiment 2 using a long slit.
The long slit is allowed to rotate independantly of the prism/grating and detection equpitment assembly.
Determine a velocity field as normal.
The experiment is then split into three sub experiments.
1) Rotate the slit only and determine the velocity fields over 360° in 5° steps.
2) Rotate the prism/grating and detection equpitment assembly but keep the slit fixed and determine the velocity fields over 360° in 5° steps.
3) Rotate the prism/grating and detection equpitment assembly and slit at the same time, and determine the velocity fields over 360° in 5° steps.

Experiment 4
A telescope is set up to determine the redshifts of multiple objects.
This experiment requires more expensive equipment, either a convex collimating mirror or equivelant concave collimating lens.
The experiment is however quite simple, instead of collimating light from a point behind the ideal focal point, light is collimated from a point before the ideal focal point.
A known, fairly close proximity object is used to calibrate the initial observation to a known reshift value.
Then larger and smaller objects have their redshift value determined and the results collated.
 
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  • #2
Have you done any work in spectroscopy before?
 
  • #3
Only as an amature, which is why I'm asking for help, that and not being able to find any results for similar experiments.
I have come across folks that simply dismiss these as invalid because they know for sure what the results would be, yet have never supplied any observational evidence for their claims. I know what the results should be, there's really no harm in making sure.

I also find a lot of folks I talk to don't really understand optics that well and when presented with my diagrams choose the basic understanding they were taught.
So with that in mind maybe you could view these diagrams :- http://homepage.ntlworld.com/papermodels/reflectors/ , and answer a simple question: Red or Blue?
 
  • #4
codex34 said:
Only as an amature, which is why I'm asking for help, that and not being able to find any results for similar experiments.
I have come across folks that simply dismiss these as invalid because they know for sure what the results would be, yet have never supplied any observational evidence for their claims. I know what the results should be, there's really no harm in making sure.

I also find a lot of folks I talk to don't really understand optics that well and when presented with my diagrams choose the basic understanding they were taught.
So with that in mind maybe you could view these diagrams :- http://homepage.ntlworld.com/papermodels/reflectors/ , and answer a simple question: Red or Blue?

I went to that website and looked at everything there. I am unable to connect any image with redshift spectroscopy. You ask "and answer a simple question: Red or Blue?" Is this some kind of joke?

Bobbywhy
 
  • #5
codex34 said:
Only as an amature, which is why I'm asking for help, that and not being able to find any results for similar experiments.
I have come across folks that simply dismiss these as invalid because they know for sure what the results would be, yet have never supplied any observational evidence for their claims. I know what the results should be, there's really no harm in making sure.

I also find a lot of folks I talk to don't really understand optics that well and when presented with my diagrams choose the basic understanding they were taught.
So with that in mind maybe you could view these diagrams :- http://homepage.ntlworld.com/papermodels/reflectors/ , and answer a simple question: Red or Blue?

I don't understand the point of the pictures. They just show parallel light at focus and non-parallel light out of focus. They have nothing to do with spectroscopy.
 
  • #6
The point of the pictures is an attempt to attain you level of understanding of optics.
The images in blue are an exageration of the caustic curve produced by effectively (Non)parallel light. The red images are you standard ideal optics taught at a basic level.

Caustics have everything to do with spectroscopy, maybe you just didn't understand the idea behind the experiments? I thought it was plain to see.
Ok, consider this, we send a divergent light source through a prism and obtain a spectrum one meter away, now we increase the divergence by 0.001 arcsecond and obtain a second spectrum, what happens to the second spectrum, does it stay the same as the first, or does it broaden and by how much?
My interest lies not with spectrum broadening within the apperatus, as this has surely been taken into account with telescopic design, my interest lies in what happens to the spectrum when a distant object with irregular shape produces a more complex caustic.

No-one, as yet, can provide me with an answer, hence the attempt at designing basic experiments to provide an answer.
 
  • #7
I haven't done any spectroscopy so can't input much. I like the premise of your experiment. After your explanation I can relate to what your asking. Unfortunately your knowledge on spectrography far exceeds mine lol
You have probably thought of this but multiple shapes can be mapped in a lab. Develop how complex objects affects on your caustic regions in the lab then pick close stellar objects see how they compare. Then work at increasingly further distances. Thats about the extent I can suggest lol
 
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  • #8
One thing that would be interesting is how the caustic regions are affected by cosmic dust on route?
Another consideration would be gravitational lensing effects.
 
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  • #9
codex34 said:
Only as an amature, which is why I'm asking for help, that and not being able to find any results for similar experiments.
I have come across folks that simply dismiss these as invalid because they know for sure what the results would be, yet have never supplied any observational evidence for their claims. I know what the results should be, there's really no harm in making sure.

I also find a lot of folks I talk to don't really understand optics that well and when presented with my diagrams choose the basic understanding they were taught.
So with that in mind maybe you could view these diagrams :- http://homepage.ntlworld.com/papermodels/reflectors/ , and answer a simple question: Red or Blue?

I've looked at all the diagrams you referred to. Will you please explain your request to "answer a simple question: Red or Blue?" I do not get how to answer it because I cannot figure out what you are referring to. Thank you.

Cheers, Bobbywhy
 
  • #10
codex34 said:
The point of the pictures is an attempt to attain you level of understanding of optics.
The images in blue are an exageration of the caustic curve produced by effectively (Non)parallel light. The red images are you standard ideal optics taught at a basic level.

Caustics have everything to do with spectroscopy, maybe you just didn't understand the idea behind the experiments? I thought it was plain to see.

Do they? Why have my books on spectroscopy never mentioned them?

Ok, consider this, we send a divergent light source through a prism and obtain a spectrum one meter away, now we increase the divergence by 0.001 arcsecond and obtain a second spectrum, what happens to the second spectrum, does it stay the same as the first, or does it broaden and by how much?

I believe the focal plane is moved backwards, so you would have to move your sensor backwards to attain proper focus. Nothing happens to the spectrum. Unless I'm misunderstanding what you mean by a "divergent light source".

My interest lies not with spectrum broadening within the apperatus, as this has surely been taken into account with telescopic design, my interest lies in what happens to the spectrum when a distant object with irregular shape produces a more complex caustic.

No-one, as yet, can provide me with an answer, hence the attempt at designing basic experiments to provide an answer.

I have never seen these caustics in anything I've seen or read on spectroscopy, so I couldn't tell you.
 
  • #11
codex, this is from your opening post on 7 February:

“I'm not interested in any discussion as to the validity of doing the experiments, kindly keep that nonsense to yourself, I'm only interested in any input to correct, improve on them, or extend them for non visible or polarized light.”

It is rather unusual for a scientist to say this because if another experienced scientist studied your experiments and wanted to offer some constructive suggestions, you have already decided in advance that his comments are “nonsense”. This indicates a lack of openness to evaluation by other experts. We who work in science do not commonly encounter this approach.

It is especially unusual since you say in post #3 on 22 February: “Only as an amature (sic), which is why I'm asking for help, that and not being able to find any results for similar experiments.” By claiming to be an amateur one would expect a more open-minded request for help. You further state “I know what the results (of these experiments) should be, there's really no harm in making sure.” So, will you please explain how you know what the results should be, what those results are, and what observational evidence you have accumulated? Will you supply some peer-reviewed journal reference article or some textbook that describes the results of these experiments?

The website you referred readers here to on 22 February did not contain the file: redshiftexperiments...25-Feb2013 04:16 2.4K
It was added to the site on 25 February.

I have read the document “Redshift Experiments” carefully and it has become clear why you label yourself as “an amature" (sic). Clearly you are. Clarity and simplicity in writing is essential for accurate and effective communication. Is English your first language? Notwithstanding all the misspelled words there appears to be some fundamental misunderstandings in your ideas about redshift measurements of distant objects. If you had simply posted this document in your opening post it would have simplified the process of communicating your ideas. In the document I found eleven declarative statements and nine specific questions. I’ve taken the liberty to separate them into two lists and to correct most of the spelling errors. This effort is intended to assist us to grasp your proposed experiments and to attempt to formulate useful answers to your questions. If I’ve made any mistakes in transcribing the document, please inform me soon. I’ve commented on a few statements.

Statements:

S1. Optically we cannot resolve the light from the edges of distant objects so we use the term effectively parallel.
S2. Light from distant objects is NOT perfectly parallel.
S3. Effectively parallel is not true parallel, an angular component exists in ALL incident light.
S4. The prism, or grating, is based on and set up for parallel light, but light isn't parallel.
S5. Optically we need to know what happens to the spread of the spectrum of light for parallel, convergent, and divergent light.
S6. When light is not parallel, which is always the case, we do not obtain a true focal point, we obtain a caustic curve either in front or behind the 'ideal' focal point.
S7. Since the angular component is based on angular diameter, it is logical to assume the caustic curve is directly proportional to the angular diameter.
S8. It isn't a secret that redshift values are directly proportional to magnitude, and that magnitude is proportional to angular diameter.
S9. The angular diameter V's redshift comparisons support a need to investigate the interaction of angular component and the instruments used for observations.
S10. An investigation is needed to calculate the degree of spread in redshift in the instrumentation compared to the angular component of incident light.
S11. Until such an investigation is carried out and the findings made public, ALL redshift based theory is merely speculation.

Questions:
Q1. So what happens when we use a prism, or diffraction grating, to split light?
Q2. What degree of angular component is needed, in convergent or divergent light, to affect the result spread of the spectrum?
Q3. What would happen if we set up our instruments for a nearby star and then compare that spectrum to a spectrum of an object with a different angular component?
Q4. Do we expect the angular component to somehow magically not alter the spread or position of the spectrum produced?
Q5. What happens to the spread of the spectrum if the light becomes more, or less, divergent, or convergent?
Q6. Wouldn't even the smallest angular difference move the spread of the spectrum?
Q7. If the difference in caustic curvature moves the spread of the spectrum, then isn't it also logical that some portion of the shift in the spectrum comparisons are directly proportional to the angular diameter?
Q8. What about object shape?
Q9. How does shape change the observed change in the spectrum?
++++++++++++++++++++++++++++++++++++++++++++++++++++++
my comments on a few statements:

S1. Only about ten nearby stars can be resolved as more than point sources. Stars more distant do appear as point sources.
S4. In modern spectrometers the light rays impinging on the prism or grating are parallel because they have passed through the collimator element.
S8. Measured redshift values are not proportional to magnitude of the object as you claim. Redshifts are proportional to the relative difference between the observed and emitted wavelengths of an object. And magnitude of the distant object is not proportional to angular diameter as you claim. The apparent magnitude of a celestial body is a measure of its brightness as seen by an observer on Earth, adjusted to the value it would have in the absence of the atmosphere. There is no connection between angular diameter and magnitude.
S11. You claim that your “investigations” should be done and the findings made public. You also claim that “until then, ALL redshift based (sic) theory is merely speculation.” This is a massive, sweeping claim that affects thousands of astrophysicists and astronomers world-wide. Is this a “personal theory”? Is there any supporting literature, any studies, any empirical evidence you can offer to support your claims?

Cheers, Bobbywhy
 
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  • #12
Quoting from Redshiftexperiments from the link:


Light from distant objects is NOT perfectly parallel.
Optically we cannot resolve the light from the edges of distant objects so we use the term effectively parallel.
Effectively parallel is not true parallel, an angular componant exists in ALL incident light.

True.

So what happens when we use a prism, or diffraction grating, to split light?
The prism, or grating, is based on and set up for parallel light, but light isn't parallel.

This is incorrect. The prism and grating do not care whether the light is parallel or not. The incoming light is typically collimated prior to the prism/grating anyways.

Optically we need to know what happens to the spread of the spectrum of light for parallel, convergent, and divergent light.

The light is parallel, so no we don't.

What would happen if we set up our instruments for a nearby star and then compare that spectrum to a spectrum of an object with a different angular componant?
Do we expect the angular componant to somehow magically not alter the spread or position of the spectrum produced?

That is exactly what we expect. Because it doesn't happen.

What happens to the spread of the spectrum if the light becomes more, or less, divergent, or convergent?
Wouldn't even the smallest angular difference move the spread of the spectrum?

No. The spectral lines may become a little wider or blurrier if your light isn't parallel when it enters the grating/prism, but there is no shift in the lines.

How does shape change the observed change in the spectrum?

It doesn't. The spectrum remains exactly the same.
It isn't a secret that redshift values are directly proportional to magnitude, and that magnitude is proportional to angular diameter.

If by this you mean that redshifted stars/galaxies are dimmer, then overall that's true because they are further away and get redshifted by expansion. But there is no direct relation between redshift and magnitude.

An investigation is needed to calculate the degree of spread in redshift in the instrumentation compared to the angular componant of incident light.
Until such an investigation is carried out and the findings made public, ALL redshift based theory is merely spectulation.

This is nonsense. Spectroscopy is used for a wide range of subjects, including a great many here on Earth. If the spectrum were affected by the angular component of the incoming light we would notice it immediately.
 
  • #13
Drakkith said:
But there is no direct relation between redshift and magnitude.

So what is this? or have I mis-interpreted it?
http://ssg.astro.washington.edu/elsst/images/miRedshift.png

This is incorrect. The prism and grating do not care whether the light is parallel or not.
And yet they take every precaution to eliminate light with any angle of incidence as it seriously effects the resulting spectrum. What exactly do you think diffusers are for?
Try placing 2 bulbs at different distances to a prism, the spectrum of one is broader than another? Why are they different if the prism does not care?

Drakkith said:
If the spectrum were affected by the angular component of the incoming light we would notice it immediately.

But would you? Think about it for more than the time it takes you to reply, how the hell would you be able to, try to devise a single experiment that would allow you to notice it.

@Bobbywhy
Comments on your comments.
S1 - exactly, we are ignoring angular componant within light because we can't optically resolve it, is it there?

S4 - collimators are desgined how? Are they part of the X²/4 curve? Is that curve based on parallel light? So if light does not pass through a SINGLE focal point how does it magically become parallel if it wasn't parallel when entering the mirror? Collimators are mostly solid and mathematically based on parallel light ideal models.

S8 - power per unit area? No Angular Diameter to Redshift Relationships and magnitude to redshift relationships? Google them.

S11 - My personal opinion is irrelevant, such experiments have never been attempted so you can only spectulate at what the outcome of such experiments would be, we both know what they should be, according to current theory, but should current theory object to such experiments being performed?
It is not a personal theory, it is curiosity arisen from reading a paper on measuring redshift velocity fields in which an edge on galaxy produced a velocity field when the slit was along the major axis of the galaxy but no velocity field could be produced when the slit was 90° to the major axis - why? You really need to think about that. Why does the light behave differently? It shouldn't matter what orientation the slit has, so long as light enters the slit we can obtain a redshift and therefore a velocity field. If you go back to the experiments, this is the first one suggested. Is the slit orientation to circluar objects and face on galaxies arbitary?
Is there some angular componant within light, interacting with the curve used for telescopic reflectors, something optic fibres and diffusers can't get rid of?

The obvious suspect is the non parallel componant which you agree exists but fail to see that collimators can't put right, unless your using a different collimator for every object...

And that's where you run into real trouble, real big trouble, if an objects shape affects redshift observations and if it is due to an interection between the incoming non parallel light and the x²/4 curve then all redshift observations themselves need looking at, big ifs yes but I repeat myself, try to devise a single experiment that would allow you to notice it. Can we even measure such small distances and angles with our current technology?

You can even go back to hubbles first observations and question them.
If a large angular diameter object has a large angular componant which results is a broadened spectrum, and we compare that to objects with smaller angular components which result in a reduced broadening of the spectrum then we can only conclude that objects with smaller angular components have a greater redshift, agreed?
And if we completely ignore the angular componant, thinking collimators somehow magically produce parallel light from non parallel light, we can only conclude what?

All based on a small curiosity as to why slit orientation has ANY effect on velocity fields.
(if you have a satisfactory answer let me know)

This is a massive, sweeping claim that affects thousands of astrophysicists and astronomers world-wide.
Test it, it can either be something or nothing, if something then we learn something new, if nothing then we learn something more about something we thought we knew.

Even though I am crap at explaining myself and my spell checker is offf, I am talking to a chap from chile via email who thinks this is of some interest, so hopefully he might be able to perform the first experiment at least, if he gets the time, maybe.

Here is a good question for you, if redshift is velocity related then the BBT fails at around z=1000, if redshift has angular relationships, what z value would be the maximum?
 
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  • #14
codex34 said:
So what is this? or have I mis-interpreted it?
http://ssg.astro.washington.edu/elsst/images/miRedshift.png

You have misunderstood it. Redshift in itself doesn't cause the reduction in magnitude, it is the increasing distance that does so. But since redshift is also related to distance thanks to expansion you have both reduced magnitude and increased redshift as objects get further away. If objects at the same distance where receding at different velocities their redshift and magnitude would not match up like this graph shows.

And yet they take every precaution to eliminate light with any angle of incidence as it seriously effects the resulting spectrum.

Yes, as it broadens the spectral lines. That's it. It has no effect on redshift measurements.

Try placing 2 bulbs at different distances to a prism, the spectrum of one is broader than another? Why are they different if the prism does not care?

If you aren't using a slit then of course it will be. But this has nothing to do with the prism. It has to do with the angular size of the light bulbs. The bigger looking bulb produces a broader spectrum unless you use a slit.

But would you? Think about it for more than the time it takes you to reply, how the hell would you be able to, try to devise a single experiment that would allow you to notice it.

Easy. Measure a near point source and then an extended source in a lab.

S4 - collimators are desgined how? Are they part of the X²/4 curve? Is that curve based on parallel light? So if light does not pass through a SINGLE focal point how does it magically become parallel if it wasn't parallel when entering the mirror? Collimators are mostly solid and mathematically based on parallel light ideal models.

Obviously no collimator is perfect, but the light will be as close to perfectly parallel as it's going to get. I don't see the issue here. It is trivial to build a collimator to work with an optical system to produce parallel light. How did it become parallel? The mirror or lens made it that way. What's the issue? Even a bad collimator will merely cause blurred spectral lines.

S11 - My personal opinion is irrelevant, such experiments have never been attempted so you can only spectulate at what the outcome of such experiments would be, we both know what they should be, according to current theory, but should current theory object to such experiments being performed?
It is not a personal theory, it is curiosity arisen from reading a paper on measuring redshift velocity fields in which an edge on galaxy produced a velocity field when the slit was along the major axis of the galaxy but no velocity field could be produced when the slit was 90° to the major axis - why? You really need to think about that. Why does the light behave differently? It shouldn't matter what orientation the slit has, so long as light enters the slit we can obtain a redshift and therefore a velocity field. If you go back to the experiments, this is the first one suggested. Is the slit orientation to circluar objects and face on galaxies arbitary?

When the slit takes in light from a large slice oriented along the major axis of the edge on galaxy, it captures light from many different stars, all moving at different speeds and directions relative to ourselves. When it is oriented the other way, along the minor axis, and the slice is only over a small section all the stars visible in that small slice are moving with approximately the same velocity relative to us.

Face on galaxies do not have stars orbiting in a plane parallel to our line of sight, so there are no major differences in their velocity away from or towards us.

The obvious suspect is the non parallel componant which you agree exists but fail to see that collimators can't put right, unless your using a different collimator for every object...

There is no obvious suspect here other than your own understanding of optics. A spectrometer simply doesn't work the way you imagine it to.
You can even go back to hubbles first observations and question them.
If a large angular diameter object has a large angular componant which results is a broadened spectrum, and we compare that to objects with smaller angular components which result in a reduced broadening of the spectrum then we can only conclude that objects with smaller angular components have a greater redshift, agreed?

No. A broadened spectrum has absolutely nothing to do with redshift.

And if we completely ignore the angular componant, thinking collimators somehow magically produce parallel light from non parallel light, we can only conclude what?

Magically? No. They use plain old reflection and refraction to produce parallel light.
 
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  • #15
codex34, Since you’ve said in post number 13 “It is not a personal theory, it is curiosity arisen from reading a paper on measuring redshift velocity fields...” I ask you: Why have you hidden that from everyone here? Why have you not posted the reference to that paper which seems to be driving this entire thesis of yours?

You have also written “And if we completely ignore the angular componant, thinking collimators somehow magically produce parallel light from non parallel light, we can only conclude what?”

There is no magic involved in the operation of an optical collimator’s function in a spectrometer. I’ve found this which seems to describe the exact nature of your thesis. See the website below, especially “Application 2: Collimating Light from a Point Source” and “Application 4: Focusing an Extended Source to a Small Spot”
http://www.newport.com/Focusing-and-Collimating/141191/1033/content.aspx

Even considering that a slightly imperfect formation of parallel light rays may be sent to the wavelength division element, this would NOT result in an erroneous redshift measurement. It would only cause a slight “broadening” of the spectral lines.

p.s. Since you say your spell checker is off, here’s a list of misspelled words from your post #13 that I’ve spelled correctly just to help you get them right the next time:

component
designed
speculate
circular
arbitrary
component
fibers
component
interaction
Hubble’s
component
components
components
component
off
Chile

Cheers, Bobbywhy
 

1. What is redshift in experiments?

Redshift in experiments refers to the phenomenon of light or other electromagnetic waves shifting towards the red end of the spectrum. This shift occurs when an object is moving away from the observer and is commonly used to measure the distance and velocity of objects in the universe.

2. How is redshift measured in experiments?

Redshift is typically measured using a spectrometer, which separates the different wavelengths of light. The amount of redshift is determined by comparing the observed wavelength of a known spectral line to the expected wavelength of that line. The difference between the two is known as the redshift value.

3. What can redshift tell us about the universe?

Redshift can provide valuable information about the expansion of the universe and the distance of objects from Earth. It can also be used to study the composition and movement of galaxies, as well as the presence of dark matter and dark energy.

4. How does redshift affect the interpretation of experimental data?

Redshift must be taken into account when interpreting experimental data, especially in studies of distant objects. The redshift value can impact the accuracy of measurements and must be accounted for in calculations and comparisons with other data.

5. Can redshift be used to study the evolution of the universe?

Yes, redshift is an important tool for studying the evolution of the universe. By measuring the redshift of different objects at various distances, scientists can gain a better understanding of how the universe has changed over time and how it may continue to evolve in the future.

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