NGC 3256 is an impressive example of a peculiar galaxy that is actually the relict of a collision of two separate galaxies that took place in a distant past. The telltale signs of the collision are two extended luminous tails swirling out from the galaxy. NGC 3256 belongs to the Hydra-Centaurus supercluster complex and provides a nearby template for studying the properties of young star clusters in tidal tails. The system hides a double nucleus and a tangle of dust lanes in the central region. The tails are studded with a particularly high density of star clusters.
This image is part of a large collection of 59 images of merging galaxies taken by the Hubble Space Telescope and released on the occasion of its 18th anniversary on 24th April 2008.
NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
About the Image
|Release date:||24 April 2008, 15:00|
|Size:||3640 x 3640 px|
About the Object
|Name:||NGC 3256, VV 65|
|Type:||• Local Universe : Galaxy : Type : Interacting|
• X - Galaxies Images/Videos
|Distance:||100 million light years|
Colours & filters
|435 nm||Hubble Space Telescope|
|Hubble Space Telescope|
|814 nm||Hubble Space Telescope|