Why should the Bullet Cluster focus light?

In summary, the Bullet Cluster is a system consisting of two galaxy clusters that exhibit gravity lensing. The mass of gas between the two clusters is much larger than the observable mass of the two galaxies, but it does not exhibit any lensing. The question is why do we expect the gas to act like a lens, since its shape can vary. However, it is important to note that coherence is not necessary for lensing to occur, as seen in the multiple images of the same object. The total mass of the cluster is what matters for lensing, not the distribution of matter. The gas in the cluster is not the main factor in determining the existence of dark matter, as the majority of the cluster's mass is dark matter.
  • #1
Earnest Guest
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In the Bullet Cluster, we have two well defined galaxy clusters that exhibit gravity lensing. Between them is a mass of gas (mostly hydrogen and helium) that is roughly eight to nine times the stellar (observable) mass of the two galaxies. The mass of gas doesn't exhibit any lensing. My question is, why do we expect the gas to act like a lens? For a lens to work, no matter how massive, it needs to focus the rays of light coming from behind it in a coherent way. Since this cloud could be shaped like a box, or a cone or have any shape at all, why are we so convinced that it can focus light? There's no question it can bend light, the question is how is it able to focus light.

Bullet X-Ray Contour.png


Here's the X-Ray contour map of the Bullet Cluster. From this it's easy to see that we're not dealing with a relaxed system (there's absolutely no symmetry). I don't see any possible way to de-project the surface brightness to a 3D density profile without an assumption of a relaxed system. Without a density profile, I don't see how you can make any predictions at all about how this mass should bend light. What am I missing?
 
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  • #2
Earnest Guest said:
Between them is a mass of gas (mostly hydrogen and helium) that is roughly eight to nine times the mass of the two galaxies.
Where does that number come from?
Most of the mass of the system is dark matter.
Earnest Guest said:
For a lens to work, no matter how massive, it needs to focus the rays of light coming from behind it in a coherent way.
It does not have to be coherent - we can see multiple images of the same object taking different ways around the galaxy.
 
  • #3
mfb said:
Where does that number come from?
Most of the mass of the system is dark matter.
Thanks for pointing that out. I updated the question to specify the observable (stellar) mass.
mfb said:
It does not have to be coherent - we can see multiple images of the same object taking different ways around the galaxy.
Yes, it does have to be coherent to focus. The multiple images are a result of the magnification factor and the distance from the actual object to the observer and the distance from the lens to the observer, but the light is still focused.

A glass marble and a class cube can have the same mass. One will act like a lens, the other won't.
 
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  • #4
Earnest Guest said:
Thanks for pointing that out. I updated the question to specify the observable (stellar) mass.
Yes, it does have to be coherent to focus. The multiple images are a result of the magnification factor and the distance from the actual object to the observer and the distance from the lens to the observer, but the light is still focused.

A glass marble and a class cube can have the same mass. One will act like a lens, the other won't.
You are misunderstanding gravitational lensing, I think. Light from a galaxy, say 8 billion light years from us shows gravitational lensing around a galactic cluster, for example, that is 4 billion light years from us. The distribution of matter in the galactic cluster is irrelevant; what matters is the total mass, which for the Einstein Rings acts the same as if that amount of gravity existed at the center of mass of the cluster.

Light passing THROUGH the cluster has the problem you describe but that has nothing to do with Einstein Rings.
 
  • #5
phinds said:
You are misunderstanding gravitational lensing, I think. Light from a galaxy, say 8 billion light years from us shows gravitational lensing around a galactic cluster, for example, that is 4 billion light years from us. The distribution of matter in the galactic cluster is irrelevant; what matters is the total mass, which for the Einstein Rings acts the same as if that amount of gravity existed at the center of mass of the cluster.

Light passing THROUGH the cluster has the problem you describe but that has nothing to do with Einstein Rings.
No, I'm pretty sure that the source of the gravity lensing must bend space the same way an optical lens does with light. There's LOTS of mass between the source of the photon and the observer, but if the space isn't curved in a coherent way (e.g. a sphere), then the light won't be magnified. If we could create a concave galaxy cluster then we would see the light scatter instead of focus.
 
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  • #6
Earnest Guest said:
No, I'm pretty sure that the source of the gravity lensing must bend space the same way an optical lens does with light. There's LOTS of mass between the source of the photon and the observer, but if the space isn't curved in a coherent way (e.g. a sphere), then the light won't be magnified. If we could create a concave galaxy cluster then we would see the light scatter instead of focus.
But it IS "curved" in a coherent way, just as I described. The lensing effect isn't THROUGH the cluster, it's AROUND it, so convexity/concavity is utterly irrelevant.
 
  • #7
phinds said:
But it IS "curved" in a coherent way, just as I described. The lensing effect isn't THROUGH the cluster, it's AROUND it, so convexity/concavity is utterly irrelevant.
Then could you please explain to me, like I'm five, how the Bullet Cluster demonstrates the existence of Dark Matter. If what you say is true, then the separation of gas from stellar material isn't going to be a factor and we should look outside of the combined cluster for any conclusions about the gravity well.
 
  • #8
Earnest Guest said:
Then could you please explain to me, like I'm five, how the Bullet Cluster demonstrates the existence of Dark Matter. If what you say is true, then the separation of gas from stellar material isn't going to be a factor and we should look outside of the combined cluster for any conclusions about the gravity well.
Most of the mass of the cluster, as with all clusters, is dark matter. The significance of the bullet cluster is that it shows the flaws in the so called "modified gravity" theories (MOND) that try to explain dark matter. It does this by showing that the dark matter masses of each of the two colliding galaxies went well past the intersection of the two galaxies and formed blobs on the other sides of the collision. In order to do that, it had to be shown that the dark matter was in fact forming those blobs. It did that because of gravitational lensing. That is, the only way to "see" the dark matter blobs was by gravitational lensing. This is completely explained in the Wikipedia article on the bullet cluster, which I recommend you read.

EDIT: better still, you should get clear about what gravitational lensing IS. Your concept of concavity/convexity of the galaxies doing the lensing seems to show that you have a fundamental misunderstanding of what it is / how it works.
 
  • #9
phinds said:
Most of the mass of the cluster, as with all clusters, is dark matter. The significance of the bullet cluster is that it shows the flaws in the so called "modified gravity" theories (MOND) that try to explain dark matter. It does this by showing that the dark matter masses of each of the two colliding galaxies went well past the intersection of the two galaxies and formed blobs on the other sides of the collision. In order to do that, it had to be shown that the dark matter was in fact forming those blobs. It did that because of gravitational lensing. That is, the only way to "see" the dark matter blobs was by gravitational lensing. This is completely explained in the Wikipedia article on the bullet cluster, which I recommend you read.

EDIT: better still, you should get clear about what gravitational lensing IS. Your concept of concavity/convexity of the galaxies doing the lensing seems to show that you have a fundamental misunderstanding of what it is / how it works.
I'm not sure you have the argument right (or perhaps I'm just misreading it). I've read a couple of articles about it now and you (or I) are missing an issue. The proponents of MOND claim that their modified gravity can bend light just as well as Dark Matter (better in some cases). The argument seems to be: well if that's the case, then how come the dust isn't bending light more because there's 9 times more of it? It's to that argument that my question is directed: yes, we all agree that there's 9 times more matter, but where's the argument saying a non-relaxed cloud of dust of any shape can bend the matter such that it's focused on a distant observer?

And yes, I agree with you about lensing if you take the observation out to a radius where the entire cluster appears to be a point mass, but we are drawing our contour maps (X-Ray and Weak Gravity) right through the heart of the cluster. If I place two black holes right next to each other and look directly between them, are you saying that I'll see a magnified image?
 
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  • #10
Earnest Guest said:
No, I'm pretty sure that the source of the gravity lensing must bend space the same way an optical lens does with light.
No it does not, and that approach won't lead anywhere.
 
  • #11
Earnest Guest said:
where's the argument saying a non-relaxed cloud of dust of any shape can bend the matter such that it's focused on a distant observer?
This seems to be a continuation of your belief that gravitational lensing is in some way similar to optical (glass lenses) lensing, but as mfb pointed out, that incorrect point of view will lead you to false conclusions. Gravitational lensing is not limited to Einstein Rings, which as I see you agree, occur around the periphery of a high-mass area of the cosmos. Light is "bent" (that is the local geodesics are not straight in the context of Euclidean Geometry, which space-time doesn't follow anyway) by any-shaped large mass and the resulting distortions can be detected.
 
  • #12
Earnest Guest said:
The proponents of MOND claim that their modified gravity can bend light just as well as Dark Matter (better in some cases).

Citation, please.

In MOND there is no dark matter, and since the bending of light is relativistic phenomenon, it can't be explained by any non-relativistic theory, like MOND. It's simply outside its domain of applicability.
 
  • #13
phinds said:
This seems to be a continuation of your belief that gravitational lensing is in some way similar to optical (glass lenses) lensing, but as mfb pointed out, that incorrect point of view will lead you to false conclusions. Gravitational lensing is not limited to Einstein Rings, which as I see you agree, occur around the periphery of a high-mass area of the cosmos. Light is "bent" (that is the local geodesics are not straight in the context of Euclidean Geometry, which space-time doesn't follow anyway) by any-shaped large mass and the resulting distortions can be detected.
I may indeed have an incorrect concept of bending of space. Could you please answer my previous question about the two black holes. If you tell me they'll magnify an image when I look between them, then I'll go back and do more reading.
 
  • #14
Earnest Guest said:
I may indeed have an incorrect concept of bending of space. Could you please answer my previous question about the two black holes. If you tell me they'll magnify an image when I look between them, then I'll go back and do more reading.
No, gravitational lensing never magnifies the image. That's a property of optical lensing and for the nth time, it just doesn't apply here.
 
  • #16
Try plotting the path of rays of light [assume they are all parallel] passing the cluster and see if they converge, diverge or remain parallel..
 
  • #17
Earnest Guest said:
I can see why this article gave you exactly the impression that you have because that's basically what it says. I believe this is a misrepresentation of what is actually happening. An optical lens magnifies the SIZE of an object. Gravitational lensing magnifies the amount of light that reaches the observer, and it presents multiple images which are separated much more that the size of the object. That is, the multiple images have an angular separation that is way bigger than the angular size of the object being lensed. BUT ... none of the images looks any bigger than the object and that's where the writer of the article misunderstood the physics and made the same mistake you are making. You will note that the article was written by a public affairs officer at NASA HQ, not by a scientist at a research center.

EDIT: you have GOT to get rid of this conflating of optical lensing and gravitational lensing or you are going to remain confused. There are zillions of things in physics that have absolutely nothing to do with gravitational lensing and optical lensing is one of them. It is very unfortunate, but understandable, that the term "lensing" is used because it causes exactly the confusion you have. Best to replace in your mind the term "gravitational lensing" with "gravitational gallumpfing" and study it as a new phenomenon completely unrelated to optical lensing.
 
  • #18
Chronos said:
Try plotting the path of rays of light [assume they are all parallel] passing the cluster and see if they converge, diverge or remain parallel..
How do you perform this exercise without knowing the density profile of the gas mass? If you don't have the density profile, then you can't create a mass profile. If you don't have a mass profile, there's no way to draw the geodesics, which is basically the question I have.
 
  • #19
phinds said:
I can see why this article gave you exactly the impression that you have because that's basically what it says. I believe this is a misrepresentation of what is actually happening. An optical lens magnifies the SIZE of an object. Gravitational lensing magnifies the amount of light that reaches the observer, and it presents multiple images which are separated much more that the size of the object. That is, the multiple images have an angular separation that is way bigger than the angular size of the object being lensed. BUT ... none of the images looks any bigger than the object and that's where the writer of the article misunderstood the physics and made the same mistake you are making. You will note that the article was written by a public affairs officer at NASA HQ, not by a scientist at a research center.
I posted the article because it was easy. There are volumes of information on the subject. Galaxy clusters are not my main focus, SNe IA are and I know enough about the subject to tell you without question that we couldn't detect most of the distant SNe Ia without the magnification that comes from a gravity lens.
 
  • #20
Earnest Guest said:
I posted the article because it was easy. There are volumes of information on the subject. Galaxy clusters are not my main focus, SNe IA are and I know enough about the subject to tell you without question that we couldn't detect most of the distant SNe Ia without the magnification that comes from a gravity lens.
Exactly. The magnification of the amount of light, not any magnification of the size of the object. For the final time, this has nothing to do with optical style lensing where the apparent size of the object is increased.
 
  • #21
phinds said:
Exactly. The magnification of the amount of light, not any magnification of the size of the object. For the final time, this has nothing to do with optical style lensing where the apparent size of the object is increased.
At what point did I say the apparent size was increased and are you going to answer my question about the two black holes? When you look between them, is the image going to be magnified or de-magnified?
 
  • #22
Earnest Guest said:
At what point did I say the apparent size was increased and are you going to answer my question about the two black holes?
You did not. Perhaps I was mislead by your belief that concavity/convexity (which are optical lensing properties) had something to do with gravitational lensing.
 
  • #23
You don't need a density profile, just assume the mass is a point source concentrated at the center.
 
  • #24
Chronos said:
You don't need a density profile, just assume the mass is a point source concentrated at the center.
That simplification only works at very large radii compared to the cluster. We're talking about the contours going right through the center of the cluster where you find the X-Ray and Weak Lensing data. To my knowledge, no one has made any claims about the characteristics of the bullet cluster from a distance you're suggesting.
 
  • #25
phinds said:
You did not. Perhaps I was mislead by your belief that concavity/convexity (which are optical lensing properties) had something to do with gravitational lensing.
I'm trying to make my point logically and step-by-step. Take two black holes. Put them relatively close to each other. Now look directly through the center point between the black holes at a distant SNe Ia. Are you going to see a image that is magnified or de-magnified?
 
  • #26
Earnest Guest said:
That simplification only works at very large radii compared to the cluster.
It is a perfectly valid approximation if you just want to understand the concept of gravitational lensing.

You don't need general relativity to understand masses sliding on inclined planes, and in the same way you don't need elaborate 3D models of clusters to understand the idea of gravitational lensing.
 
  • #27
mfb said:
It is a perfectly valid approximation if you just want to understand the concept of gravitational lensing.

You don't need general relativity to understand masses sliding on inclined planes, and in the same way you don't need elaborate 3D models of clusters to understand the idea of gravitational lensing.
I'm afraid you just haven't been following the conversation. In addition, I don't think you have a grasp of the concepts here. The Bullet Cluster doesn't have enough mass to create any strong lensing effects. The only effects are 'weak' lensing effects which can only be seen in a statistical blip in the shape of the stars inside the projected radius of the cluster.
 
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  • #28
You apparently missed the point of well intended posts here. Your misconceptions have been adequately addressed, so, I will refrain from further comments.
 
  • #29
Chronos said:
You apparently missed the point of well intended posts here. Your misconceptions have been adequately addressed, so, I will refrain from further comments.
From your comments, you also don't understand the difference between strong lensing and weak lensing. I suggest you go back and review the materials before trying to act as an 'advisor' on this subject again. There is simply no foundation for being able to simplify a weak lensing problem as a point source. You must perform a statistical analysis of all the galaxies in a region before you can draw a contour map. There's some good material on the Wiki pages about it.

https://en.wikipedia.org/wiki/Weak_gravitational_lensing
 
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  • #30
Earnest Guest said:
From your comments, you also don't understand the difference between strong lensing and weak lensing. I suggest you go back and review the materials before trying to act as an 'advisor' on this subject again. There is simply no foundation for being able to simplify a weak lensing problem as a point source. You must perform a statistical analysis of all the stars in a region before you can draw a contour map. There's some good material on the Wiki pages about it.

https://en.wikipedia.org/wiki/Weak_gravitational_lensing

Just as an aside, you have STILL never acknowledged your mistake in thinking that convexity/concavity has something to do with gravitational lensing and that there is a similarity with optical lensing. Do you still believe that it is true?
 
  • #31
Earnest Guest said:
From your comments, you also don't understand the difference between strong lensing and weak lensing. I suggest you go back and review the materials before trying to act as an 'advisor' on this subject again. There is simply no foundation for being able to simplify a weak lensing problem as a point source. You must perform a statistical analysis of all the stars in a region before you can draw a contour map. There's some good material on the Wiki pages about it.
https://en.wikipedia.org/wiki/Weak_gravitational_lensing
Earnest Guest said:
I'm afraid you just haven't been following the conversation. In addition, I don't think you have a grasp of the concepts here. The Bullet Cluster doesn't have enough mass to create any strong lensing effects. The only effects are 'weak' lensing effects which can only be seen in a statistical blip in the shape of the stars inside the projected radius of the cluster.

?
 
  • #33
The weak lensing effect extends out beyond the projected radius of the cluster which is causing the lensing.

And it is typically measured from the distortion of the shapes of galaxies (not individual stars) which are out beyond the cluster causing the lensing.
 
  • #34
phinds said:
Just as an aside, you have STILL never acknowledged your mistake in thinking that convexity/concavity has something to do with gravitational lensing and that there is a similarity with optical lensing. Do you still believe that it is true?
Take two black holes. Place them relatively close together. Now look at a distant SNe Ia that lies directly between the two black holes. Will this supernova appear to be magnified or de-magnified?
 
  • #35
This may be a case of "don't feed the argument". We've had plenty of calm peaceful friendly discussion of weak lensing (e.g. as used to map concentration of DM mass) here at PF since, as I recall, 2005. We don't need vituperation about who said what and who was wrong etc etc. It doesn't add any useful understanding. AFAICS. That is just my private opinion---I'm not a mentor (they do the moderating).
I'd give everybody a pass and lock the thread, if it were up to me.
 
<h2>1. Why is the Bullet Cluster important for studying dark matter?</h2><p>The Bullet Cluster is important for studying dark matter because it provides evidence for the existence of dark matter. The cluster is made up of two colliding galaxies, and the fact that the majority of the mass is found in the form of dark matter, rather than visible matter, supports the theory that dark matter exists.</p><h2>2. How does the Bullet Cluster focus light?</h2><p>The Bullet Cluster does not actually focus light. Instead, it acts as a gravitational lens, bending and magnifying the light from background galaxies as it passes through the cluster. This allows us to see objects that would otherwise be too faint to detect, providing valuable information about the distribution of dark matter within the cluster.</p><h2>3. What is the significance of the Bullet Cluster's dark matter distribution?</h2><p>The Bullet Cluster's dark matter distribution is significant because it provides further evidence that dark matter exists and makes up a large portion of the universe's mass. The fact that dark matter is concentrated in the center of the cluster, rather than being evenly distributed with visible matter, supports the theory that dark matter interacts differently with gravity than visible matter.</p><h2>4. How does studying the Bullet Cluster help us understand the universe?</h2><p>Studying the Bullet Cluster helps us understand the universe by providing insights into the nature of dark matter. By analyzing the distribution and behavior of dark matter in the cluster, scientists can gain a better understanding of its properties and how it affects the evolution of galaxies and the structure of the universe.</p><h2>5. What future research is being done on the Bullet Cluster?</h2><p>Future research on the Bullet Cluster includes using more advanced telescopes and techniques to study the cluster in greater detail and to search for smaller substructures within the cluster. Scientists are also studying other galaxy clusters to compare their dark matter distributions and further refine our understanding of dark matter and its role in the universe.</p>

Related to Why should the Bullet Cluster focus light?

1. Why is the Bullet Cluster important for studying dark matter?

The Bullet Cluster is important for studying dark matter because it provides evidence for the existence of dark matter. The cluster is made up of two colliding galaxies, and the fact that the majority of the mass is found in the form of dark matter, rather than visible matter, supports the theory that dark matter exists.

2. How does the Bullet Cluster focus light?

The Bullet Cluster does not actually focus light. Instead, it acts as a gravitational lens, bending and magnifying the light from background galaxies as it passes through the cluster. This allows us to see objects that would otherwise be too faint to detect, providing valuable information about the distribution of dark matter within the cluster.

3. What is the significance of the Bullet Cluster's dark matter distribution?

The Bullet Cluster's dark matter distribution is significant because it provides further evidence that dark matter exists and makes up a large portion of the universe's mass. The fact that dark matter is concentrated in the center of the cluster, rather than being evenly distributed with visible matter, supports the theory that dark matter interacts differently with gravity than visible matter.

4. How does studying the Bullet Cluster help us understand the universe?

Studying the Bullet Cluster helps us understand the universe by providing insights into the nature of dark matter. By analyzing the distribution and behavior of dark matter in the cluster, scientists can gain a better understanding of its properties and how it affects the evolution of galaxies and the structure of the universe.

5. What future research is being done on the Bullet Cluster?

Future research on the Bullet Cluster includes using more advanced telescopes and techniques to study the cluster in greater detail and to search for smaller substructures within the cluster. Scientists are also studying other galaxy clusters to compare their dark matter distributions and further refine our understanding of dark matter and its role in the universe.

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