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Hubble Interacting Galaxy Arp 148
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Name: Arp 148, VV 032, Mayall's Object, MCG+07-23-019
Description: Interacting Galaxies
Position (J2000): R.A.11 03 53.95 Dec. +40 50 59.90
Constellation: Ursa Major
Distance: 450 million light-years (150 million parsecs)
Instrument: WFPC2, ACS/WFC
Exposure Date(s): Oct. 9/10, 1995; Nov. 20, 2005; and April 27-29, 2007
Exposure Time: 10.3 hours
Filters: F336W (U), F450W (B), F606W (V), and F814W (I)
Image Credit: NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (U of Virginia, Charlottesville/NRAO/Stony Brook University)
Release Date: April 24, 2008
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ABOUT THIS IMAGE:

Arp 148 is the staggering aftermath of an encounter between two galaxies, resulting in a ring-shaped galaxy and a long-tailed companion. The collision between the two parent galaxies produced a shockwave effect that first drew matter into the center and then caused it to propagate outwards in a ring. The elongated companion perpendicular to the ring suggests that Arp 148 is a unique snapshot of an ongoing collision. Infrared observations reveal a strong obscuration region that appears as a dark dust lane across the nucleus in optical light. Arp 148 is nicknamed Mayall s object and is located in the constellation of Ursa Major, the Great Bear, approximately 500 million light-years away. This interacting pair of galaxies is included in Arp's catalog of peculiar galaxies as number 148.

From Wikipedia:

Mayall's Object (also classified under the Atlas of Peculiar Galaxies as Arp 148) is the result of two colliding galaxies located 500 million light years away within the constellation of Ursa Major. It was discovered by Nicholas U. Mayall of the Lick Observatory on 13 March 1940, using the Crossley reflector. When first discovered, Mayall's Object was described as a peculiar nebula, shaped like a question mark. Originally theorized to represent a galaxy reacting with the intergalactic medium, it is now thought to represent the collision of two galaxies, resulting in a new object consisting of a ring-shaped galaxy with a tail emerging from it. It is thought that the original collision between the two original galaxies created a shockwave that initially drew matter into the center which then formed the ring.

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.