Perseus Dwarf Galaxy

This object, [CGW2003] J031910.4+4129, 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 in 2005 by NASA/ESA’s Hubble Space Telescope, is an evidence that the undisturbed galaxies are enshrouded by a "cushion" of dark matter, which protects them from their rough-and-tumble neighborhood.

Credit:

NASA, ESA and C. Conselice (University of Nottingham, U.K.)

About the Image

NASA press release
Id:heic0903c
Type:Observation
Release date:12 March 2009, 14:00
Related releases:heic0903
Size:500 x 500 px

About the Object

Name:[CGW2003] J031910.4+4129, Perseus Cluster
Type:Local Universe : Galaxy : Size : Dwarf
Distance:250 million light years
Constellation:Perseus
Category:Galaxies

Image Formats

r.titleLarge JPEG
134.1 KB
r.titleScreensize JPEG
243.2 KB

Coordinates

Position (RA):3 19 10.43
Position (Dec):41° 29' 36.57"
Field of view:0.42 x 0.42 arcminutes
Orientation:North is 85.1° right of vertical


Colours & filters

BandWavelengthTelescope
Optical
V
606 nm Hubble Space Telescope
ACS
Infrared
I
814 nm Hubble Space Telescope
ACS

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