Primera detección de un anillo de materia oscura en un cúmulo de galaxias


The ring of dark matter
 
This Hubble Space Telescope composite image shows a ghostly "ring" of dark matter in the galaxy cluster ZwCl0024+1652.

The ring-like structure is evident in the blue map of the cluster's dark matter distribution. The map is superimposed on a Hubble image of the cluster. The ring is one of the strongest pieces of evidence to date for the existence of dark matter, an unknown substance that pervades the universe.

Astronomers suggest that the dark-matter ring was produced from a collision between two gigantic clusters.

Dark matter makes up the bulk of the universe's material and is believed to make up the underlying structure of the cosmos.

The Hubble observations were taken in November 2004 by the Advanced Camera for Surveys. Thanks its exquisite resolution, astronomers saw the detailed cobweb tracery of gravitational lensing in the cluster.

Ring of dark matter around ZwCl0024+1652
 
The ring of dark matter illustrated in blue around ZwCl0024+1652.

The galaxy cluster ZwCl 0024+17
 
This image shows the galaxy cluster ZwCl 0024+17 (ZwCl 0024+1652) as seen by Hubble’s Advanced Camera for Surveys.

The image displays faint faraway background galaxies that had their light bent by the cluster's strong gravitational field. By mapping the distorted light and using it to deduce how dark matter is distributed in the cluster, astronomers spotted the ring of dark matter.

One of the background galaxies is located about two times further away than the yellow cluster galaxies in the foreground, and has been multiple-imaged into five separate arc-shaped components, seen in blue.

Gravitationaly lensed galaxies
 
This amazing video shows us some spectacular examples of faint background galaxies that had their light bent by the cluster’s strong gravitational field. One of them, located about two times farther away than the yellow cluster galaxies in the foreground, has been multiple-imaged into five separate arc-shaped pieces. Hubble’s high resolution can even show the details of this background galaxy.


 
An illustration showing two views of interacting galaxy clusters.

The galaxy cluster ZwCl0024+1652
 
This image shows the galaxy cluster ZwCl0024+1652 as seen in the Digitized Sky Survey 2 (DSS2).

The image is a colour composite from Digitised Sky Survey 2 (DSS2) images. The field of view is 3.0 degrees. The cluster of galaxies is in the centre of the image.

Panning on the galaxy cluster
 
Panning on the galaxy cluster ZwCl0024+1652



Release date: 17 mayo 2007