NGC 3256
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.
Credit: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
| Id: | heic0810ar |
|---|---|
| Type: | Observation |
| Release date: | 24 April 2008, 15:00 |
| Related releases: | heic0810 |
| Size: | 3640 x 3640 px |
About the Object
| Name: | NGC 3256, VV 65 |
|---|---|
| Type: | Local Universe : Galaxy : Type : Interacting |
| Distance: | 100 million light years |
| Constellation: | Vela |
| Category: | Anniversary Galaxies |
Coordinates
| Position (RA): | 10 27 52.70 |
|---|---|
| Position (Dec): | -43° 54' 15.64" |
| Field of view: | 3.02 x 3.02 arcminutes |
| Orientation: | North is 95.3° left of vertical |
Colours & filters
| Band | Wavelength | Telescope |
|---|---|---|
| Optical B | 435 nm |
Hubble Space Telescope
ACS |
| Optical Pseudogreen (B+I) |
Hubble Space Telescope
ACS | |
| Infrared I | 814 nm |
Hubble Space Telescope
ACS |