Perseus dwarf galaxy
This object, [CGW2003] J031931.7+4131, is one of four dwarf galaxies that is part of a census of small galaxies in the tumultuous heart of the nearby Perseus galaxy cluster.
The galaxies appear smooth and symmetrical, suggesting that they have not been tidally disrupted by the pull of gravity in the dense cluster environment. Larger galaxies around them, however, are being ripped apart by the gravitational tug of other galaxies.
The image, taken by NASA/ESA’s Hubble Space Telescope in 2005, is an evidence that the undisturbed galaxies are enshrouded by a "cushion" of dark matter, which protects them from their rough-and-tumble neighborhood.
NASA, ESA and C. Conselice (University of Nottingham, U.K.)
About the Image
|Release date:||12 March 2009, 14:00|
|Size:||500 x 500 px|
About the Object
|Name:||Perseus Cluster, [CGW2003] J031931.7+4131|
|Type:||• Local Universe : Galaxy : Size : Dwarf|
• X - Galaxies Images/Videos
|Distance:||250 million light years|
Colours & filters
|555 nm||Hubble Space Telescope|
|814 nm||Hubble Space Telescope|