What is Gravitational lensing?

In summary, gravitational lensing is a phenomenon that occurs when light from a distant object is bent or distorted by the gravitational pull of a massive object in its path. This can cause the distant object to appear larger, brighter, or distorted, depending on the strength and position of the gravitational lens. It is a key concept in Einstein's theory of general relativity and has been observed in various astrophysical objects, providing valuable insights into the distribution of matter in the universe. Gravitational lensing has also been used as a powerful tool in astronomy to study galaxies, dark matter, and even the expansion of the universe.
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  • #2
In simplified terms, Einstein stated that gravity would bend space, so even light would follow the curved path near a massive object. For an observer, far away, it appears as if the light waves bend.
 
  • #3
how could it be so sure that the light is bent? because the observer can see it straightly where the light comes from(telescope or something).
Only when its seen laterally or in sidewise view it is possible to assure that light is bent.!
 
  • #5
Soundariya Raja said:
how could it be so sure that the light is bent? because the observer can see it straightly where the light comes from(telescope or something).
Only when its seen laterally or in sidewise view it is possible to assure that light is bent.!
I'm not usually fond of going just with Wikipedia, but they have a nice animation of what something passing through the "lens" might look like. https://en.wikipedia.org/wiki/Gravitational_lens
 
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  • #6
So this is my attempt at sketching out what is happening. I have greatly exaggerated the effect. As the light passes near a massive object, which has distorted the space, the light follows a curved path, near it then continues on. An observer would see images on either side of the front massive object.
https://flic.kr/p/WgNVyn
 
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  • #7
Soundariya Raja said:
how could it be so sure that the light is bent? because the observer can see it straightly where the light comes from(telescope or something).
Only when its seen laterally or in sidewise view it is possible to assure that light is bent.!

We can compare the apparent relative position of stars in the sky as a massive object (such as the Sun) passes near our line of sight to the star. As the massive object comes very close to our LOS, the apparent position of the star changes slightly as the light is bent. The measured change in the apparent position matches predictions by GR.
 
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  • #8
OH..WOW!..:woot: THANK YOU SCOTTDAVE, DRAKKITH!.."FOR THE ANIMATIONS" :biggrin:
NOW I COULD UNDERSTAND THE WHOLE THING.:smile:
 
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  • #9
I've just had a little experience with it, since I did a little undergraduate research semester on it. But one thing that's not been mentioned, and what excites me the most about it, is that it enables an observer to actually observe behind an occulting galaxy. Just from line of sight considerations, it might be natural to assume that when a galaxy occults another galaxy from view, the more distant object is unobservable.

Not so due to the the effects of gravitational lensing.

The nearer galaxy acts as a lens to send information from the more distant galaxy to the observer. Quite amazing, really.
 
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  • #11
mark! said:
True, but this lensing technique is also used to 'see' dark matter. But does ligt behave/interact the same way when it goes 'through' dark matter, unaffected whatsoever?
Dark matter does not interact with electromagnetic fields, so light can pass through dark matter as though it's not there at all.
The light is not absorbed or reflected or refracted in any form.
Sufficient quantity of dark matter has a gravitational field though, and that field does interact with light, changing it's apparent direction as seen by a remote observer This lensing is the same as that produced by concentrations of normal matter
 
  • #12
Isn't there some evidence that Eddington's calulations were incorrect?
 
  • #13
pmwelec said:
Isn't there some evidence that Eddington's calulations were incorrect?
What difference does it make? Surely, you are not going to dispute General Relativity.
 
  • #14
Soundariya Raja said:
how could it be so sure that the light is bent? because the observer can see it straightly where the light comes from(telescope or something).
Only when its seen laterally or in sidewise view it is possible to assure that light is bent.!

No, we only see light coming at us. (see lens) There is no sideways view of light.

390px-Lens1.svg.png


Suppose you take a Sherlock Holmes style magnifying glass and place a sticker in the middle of the glass. You can still see parts of an object that are behind the sticker. Light that would not have hit our eye gets bent and now it does get to our eye (or telescope, camera etc).

A lot of telescopes have a blockage in the middle of the tube. Makes a good image anyway.
220px-Newtonian_telescope2.svg.png

225px-Schmidt-Cassegrain-Telescope.svg.png
 

What is Gravitational Lensing?

Gravitational lensing is a phenomenon in which the light from a distant object is bent by the gravitational pull of a massive object, such as a galaxy or a cluster of galaxies, in its path. This results in the appearance of the object being distorted or magnified.

How does Gravitational Lensing occur?

Gravitational lensing occurs when the path of light from a distant object is bent due to the warping of space-time by a massive object. The more massive the object, the greater the bending of light and the stronger the gravitational lensing effect.

What are the types of Gravitational Lensing?

There are two main types of gravitational lensing: strong lensing and weak lensing. Strong lensing occurs when the light from a distant object is highly distorted, resulting in multiple images or an Einstein ring. Weak lensing occurs when the distortion is more subtle and can only be detected through statistical analysis of large numbers of galaxies.

What is the significance of Gravitational Lensing?

Gravitational lensing has significant implications in the study of astrophysics and cosmology. It allows us to study distant objects that would otherwise be too faint or small to be observed. It also provides evidence for the existence of dark matter, as the gravitational lensing effect cannot be fully explained by visible matter alone.

How is Gravitational Lensing studied?

Gravitational lensing is studied through various methods such as imaging, spectroscopy, and numerical simulations. Astronomers use telescopes to observe and analyze the distorted images of distant objects, while theorists use mathematical models to understand the underlying physics of gravitational lensing.

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