Gravitational lensing anomaly?

In summary, the gravity of a luminous red galaxy has distorted the light from a more distant blue galaxy, leading to the blue-shifted appearance of the latter. This phenomenon is known as gravitational lensing, and can be used to study distant galaxies.
  • #1
Last_Exile
21
0
Hi,

The recent Astronomy Picture of the Day:

http://apod.nasa.gov/apod/ap111221.html

Has the following caption:

...the gravity of a luminous red galaxy (LRG) has gravitationally distorted the light from a much more distant blue galaxy.

I was under the impression that the more distant a galaxy is then the more red-shifted it becomes. So my question is how can the more distant galaxy be blue?

Thanks in advance.
 
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  • #2
Last_Exile said:
Hi,

The recent Astronomy Picture of the Day:

http://apod.nasa.gov/apod/ap111221.html

Has the following caption:

...the gravity of a luminous red galaxy (LRG) has gravitationally distorted the light from a much more distant blue galaxy.

I was under the impression that the more distant a galaxy is then the more red-shifted it becomes. So my question is how can the more distant galaxy be blue?

Thanks in advance.

Hello,

You appear to have a misconception with regards to redshift. Redshift does not mean becomes redder, it corresponds to a longer wavelength - moving to the "red" end of the spectrum so through the visible spectrum to eventually x rays, gamma rays.

Please see the following link for clarification:

http://en.wikipedia.org/wiki/Redshift

Extract: "In physics (especially astrophysics), redshift happens when light seen coming from an object is proportionally increased in wavelength, or shifted to the red end of the spectrum. More generally, where an observer detects electromagnetic radiation outside the visible spectrum, "redder" amounts to a technical shorthand for "increase in electromagnetic wavelength" — which also implies lower frequency and photon energy in accord with, respectively, the wave and quantum theories of light."
 
  • #3
Hmmm...

Wouldn't that still mean that the light appears redder to the observer?

http://www.setterfield.org/000docs/Redshift.htm


In the simplest terms, 'redshift' is a term used to describe the fact that the light seen from distant galaxies shows up a little differently than it does here on earth. Each element has a 'fingerprint' in light. This is how we know which elements are in which stars. There is a certain pattern of lines associated with each element which identifies it. However, as we get further and further out in space, these identifying lines, while keeping the same identifying patterns for each element, appear shifted somewhat to the red end of the spectrum -- thus causing the light to appear redder than it would be here on earth.

My emphasis.
 
Last edited by a moderator:
  • #4
Last_Exile said:
Hmmm...

Wouldn't that still mean that the light appears redder to the observer?

My guess is one of the side effects of gravitational lensing would be a change in wavelength. Thus the further galaxy (the blue one that's now an Einstein Ring) would appear blue-shifted to us simply because of the distortion caused by the gravitational lensing.
 
  • #5
The "color" of a galaxy relies on more than just its Doppler shift. A galaxy of mostly hot stars will be bluer than one with cooler stars or one that is dusty. It takes quite a sever doppler shift to cause a visible reddening of a galaxy. The light at the blue end of the spectrum that is shifted to the red is replaced by ultraviolet that shifts from being invisible to being blue.
 
  • #6
Thanks Janus, that does seem to make sense.

It would imply that the lensed galaxy, now appearing blue (and much further away) consisted of extremely hot stars whose ultra-violet radiation is now visible to us.

My faith in science is restored!
 

Related to Gravitational lensing anomaly?

What is gravitational lensing anomaly?

Gravitational lensing anomaly is a phenomenon in which light from a distant object is distorted and magnified by the gravitational pull of a massive object, such as a galaxy or a black hole, that lies in between the object and the observer.

How does gravitational lensing anomaly occur?

Gravitational lensing anomaly occurs due to the bending of space-time caused by the massive object's gravitational field. The light passing through this bent space-time gets distorted and can appear as multiple images or arcs around the massive object.

What is the importance of studying gravitational lensing anomaly?

Studying gravitational lensing anomaly can provide valuable insights into the distribution of dark matter in the universe, the properties of distant objects, and the nature of gravity itself. It also allows us to observe and study objects that would otherwise be too faint or far away to detect.

What are some examples of gravitational lensing anomaly?

Some famous examples of gravitational lensing anomaly include the Einstein Cross, a quasar that appears as four separate images due to the gravitational lensing effect of a galaxy, and the Cosmic Horseshoe, a galaxy that appears as a distorted ring due to the lensing effect of a massive galaxy cluster.

How is gravitational lensing anomaly detected and studied?

Gravitational lensing anomaly can be detected through observations of distorted or duplicated images of distant objects. It can also be studied through computer simulations and mathematical models that take into account the properties of the massive object and its gravitational field.

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