SDP.81 : how do we see the gavitational lens?

  • Thread starter maajdl
  • Start date
  • Tags
    Lens
In summary, a recent news article discusses a photograph of a cosmic ring that confirms Einstein's prediction of gravitational lensing. The distance of the lens is known through spectroscopy analysis, which was also used to confirm a similar event in the case of PS1-10afx. The technology available at the time was not advanced enough to directly observe this phenomena, but there is no other known explanation for these types of images.
  • #1
maajdl
Gold Member
391
29
I just read this news:

http://www.space.com/29042-cosmic-ring-photo-rules-them-all.html

I wonder how we can know about the gravitational lens, how can we even be sure it is there?
Would that be only by analyzing the image of the supposed distant galaxi?
Which kind of analysis?
Or are there other footprints?
I am specially impressed by the fact that the distance of the lens is known.
How can that be knonw?
 
Astronomy news on Phys.org
  • #2
We can be sure that it's there alright, it's a photograph of something.
That 'something' very much matches what Einstein predicted, although he doubted the phenomena could be directly observed.
Optical technology at the time was well short of the resolution that is required.
There is no alternative explanation (that I know of), for these kind of images.
 
  • #3
Spectroscopy is one way to detect an intervening mass in a suspected lensing event. This was used to confirm a lensing event in the case of PS1-10afx, which was initially suspected to be a new class of supernovae. See http://arxiv.org/abs/1404.6014 for further details.
 
Last edited:

Related to SDP.81 : how do we see the gavitational lens?

1. How does gravitational lensing occur?

Gravitational lensing occurs when the gravity of a massive object, such as a galaxy or cluster of galaxies, bends the path of light from a more distant object behind it. This bending of light can create distorted or magnified images of the background object.

2. What is the significance of SDP.81 in studying gravitational lensing?

SDP.81 is a distant galaxy that has been observed to have a massive galaxy cluster in front of it, causing gravitational lensing. This allows scientists to study the effects of gravitational lensing on the light from the distant galaxy and gain a better understanding of the phenomenon.

3. How does SDP.81 help us understand the properties of dark matter?

Gravitational lensing is one of the main lines of evidence for the existence of dark matter, as it can only be explained by the presence of massive invisible matter. By studying the effects of gravitational lensing on SDP.81, scientists can gather information about the distribution and properties of dark matter in the galaxy cluster in front of it.

4. How can SDP.81 be used to test Einstein's theory of general relativity?

Einstein's theory of general relativity predicts the bending of light by massive objects. By observing the gravitational lensing of SDP.81, scientists can test the accuracy of this prediction and further validate the theory.

5. What future research is needed to further our understanding of gravitational lensing using SDP.81?

Future research could involve more detailed observations of SDP.81 and other similar gravitational lensing events, as well as theoretical studies and simulations to better understand the complex processes involved. Additionally, studying more distant and fainter objects could provide new insights into the properties of dark matter and the expansion of the universe.

Similar threads

  • Astronomy and Astrophysics
Replies
18
Views
3K
  • Science Fiction and Fantasy Media
Replies
13
Views
2K
Replies
5
Views
1K
Replies
18
Views
2K
  • Astronomy and Astrophysics
Replies
3
Views
2K
  • Introductory Physics Homework Help
Replies
15
Views
7K
Replies
2
Views
1K
  • Astronomy and Astrophysics
Replies
17
Views
6K
  • Astronomy and Astrophysics
Replies
7
Views
2K
Replies
2
Views
1K
Back
Top