Hubble helps astronomers map dark matter in Abell 1689
This NASA/ESA Hubble Space Telescope image shows the distribution of dark matter in the centre of the giant galaxy cluster Abell 1689, containing about 1,000 galaxies and trillions of stars.
Dark matter is an invisible form of matter that accounts for most of the universe's mass. Hubble cannot see the dark matter directly. Astronomers inferred its location by analyzing the effect of gravitational lensing, where light from galaxies behind Abell 1689 is distorted by intervening matter within the cluster.
Researchers used the observed positions of 135 lensed images of 42 background galaxies to calculate the location and amount of dark matter in the cluster. They superimposed a map of these inferred dark matter concentrations, tinted blue, on an image of the cluster taken by Hubble's Advanced Camera for Surveys. If the cluster's gravity came only from the visible galaxies, the lensing distortions would be much weaker. The map reveals that the densest concentration of dark matter is in the cluster's core.
Abell 1689 resides 2.2 billion light-years from Earth. The image was taken in June 2002.
About the Image
|Release date:||11 November 2010, 17:00|
|Size:||3840 x 3936 px|
About the Object
|Type:||• Early Universe : Galaxy : Grouping : Supercluster|
• Early Universe : Cosmology : Phenomenon : Dark Matter
• X - Cosmology Images/Videos
Colours & filters
|475 nm||Hubble Space Telescope|
|625 nm||Hubble Space Telescope|
|775 nm||Hubble Space Telescope|
|850 nm||Hubble Space Telescope|
Notes: A map of the dark matter in Abell 1689 has been added to this image in blue.