Einstein ring and Einstein Cross

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In summary, an Einstein ring is a phenomenon where light from a distant object, such as a galaxy, is bent around a massive foreground object due to gravitational lensing, creating a ring-like image. An Einstein Cross is a specific case of gravitational lensing where a single distant source appears as four distinct images surrounding the lensing mass, typically seen in situations where the alignment of the source, lens, and observer is nearly perfect. Both phenomena illustrate the effects of gravity on light and provide insights into the distribution of dark matter in the universe.
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Why does an Einstein ring sometimes appear and sometimes an Einstein Cross appear?

Some say it is due to the distribution of the mass of the galaxy in front, while others say it is due to alignment. What is right? Are both correct?

If it is due to the galaxy's mass distribution, I wonder if it can be affected by the type of galaxy and the angle between the galaxy's rotation axis and the Earth. I also wonder if the distribution of dark matter could also affect this.
Why does an Einstein ring sometimes appear and sometimes an Einstein Cross appear?

Some say it is due to the distribution of the mass of the galaxy in front, while others say it is due to alignment. What is right? Are both correct?

If it is due to the galaxy's mass distribution, I wonder if it can be affected by the type of galaxy (like an Elliptical Galaxy, Spiral galaxy) and the angle between the galaxy's rotation axis and the Earth. It's the same principle as how the shape of the dot behind the glass looks different depending on the glass model.

I also wonder if the distribution of dark matter could also affect this.
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You get a ring from a circularly symmetric mass distribution lensing light from an object more or less directly behind it. You get a cross (or at least you can) from an elliptical mass distribution like a galaxy seen edge on. So yes, if you have two identical disc-shaped galaxies lensing light from two identical sources, you could get a cross from one and a ring from the other depending on the orientations of the lensing galaxies.

Dark matter affects light paths the same as normal matter.
 
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Ibix said:
You get a ring from a circularly symmetric mass distribution lensing light from an object more or less directly behind it. You get a cross (or at least you can) from an elliptical mass distribution like a galaxy seen edge on. So yes, if you have two identical disc-shaped galaxies lensing light from two identical sources, you could get a cross from one and a ring from the other depending on the orientations of the lensing galaxies.

Dark matter affects light paths the same as normal matter.
So, is it wrong to say that it is due to alignment?
And can I get a source for your claim?
 
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hongseok said:
So, is it wrong to say that it is due to alignment?
The exact shape will depend on alignment, yes. You'll only get a perfect ring around a perfectly symmetric source perfectly aligned with a perfectly symmetric lens, but you'll get things like the ring illustration in your OP from nearly symmetric situations. I don't think alignment can turn a ring into a cross, although you can certainly have crosses from nearly symmetric situations that can be very ring-like.
hongseok said:
And can I get a source for your claim?
Which one?
 
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hongseok said:
And can I get a source for your claim?
If it's just the point about alignment, all orbits around spherically symmetric sources lie in a plane. A source, a lens and an observer that are not colinear define a plane, and only light emitted in this plane can reach the observer. Light emitted in any other direction has a path that lies in a plane that doesn't include the observer. So you will get at most two images, one each side of the lens, that smear into a ring if the source, lens and observer become colinear. Thus alignment can't create a cross from a spherical lens.

Elliptical sources are harder to reason about, but there's detail here: https://lweb.cfa.harvard.edu/~dfabricant/huchra/ay202/lectures/lecture12.pdf. If you can program in python (or anything else where someone's written a numerical integrator) you can get lensing patterns from the weak field metric for arbitrary lens mass distributions if you really want.
 
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FAQ: Einstein ring and Einstein Cross

What is an Einstein ring?

An Einstein ring is a phenomenon that occurs when light from a distant object, such as a galaxy or star, is bent around a massive object, like a galaxy or black hole, located between the light source and the observer. This bending of light, predicted by Einstein's theory of general relativity, creates a ring-like appearance of the distant object.

How is an Einstein ring formed?

An Einstein ring is formed through a process called gravitational lensing. When the source, lens, and observer are perfectly aligned, the light from the source bends around the lensing object due to its gravitational field and converges towards the observer, forming a ring. The degree of alignment and mass of the lens determine the size and shape of the ring.

What is an Einstein Cross?

An Einstein Cross is a specific type of gravitational lensing effect where a single distant object, such as a quasar, appears as four distinct images arranged in a cross-like pattern around a foreground massive object, typically a galaxy. This occurs due to the gravitational field of the lensing galaxy bending the light from the quasar at multiple points.

Why are Einstein rings and Einstein Crosses important in astronomy?

Einstein rings and Einstein Crosses are important because they provide a natural laboratory for studying the distribution of dark matter, the mass of galaxies, and the expansion of the universe. They also allow astronomers to observe extremely distant objects that would otherwise be too faint to detect, thereby providing insights into the early universe.

Can Einstein rings and Einstein Crosses be observed with amateur telescopes?

Observing Einstein rings and Einstein Crosses typically requires powerful telescopes due to their faintness and the need for high resolution. Professional observatories and space telescopes like the Hubble Space Telescope are often used to capture these phenomena. However, some brighter and more prominent examples might be observable with advanced amateur telescopes under ideal conditions.

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