Hubble image archive

Hubble Interacting Galaxy UGC 5101

UGC 5101 is a peculiar galaxy with a single nucleus contained within an unstructured main body that suggests a recent interaction and merger. UGC 5101 is thought to contain an active galactic nucleus an extremely bright, compact core - buried deep in the gas and dust. A pronounce...

Date
Jan 1, 2008
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2008-16-2301-image
By

UGC 5101 is a peculiar galaxy with a single nucleus contained within an unstructured main body that suggests a recent interaction and merger. UGC 5101 is thought to contain an active galactic nucleus an extremely bright, compact core - buried deep in the gas and dust. A pronounced tail extends diagonally to the top-right of the frame. A fainter halo of stars surrounds the galaxy and is visible in the image, due to Hubble s ability to collect and detect faint light. This halo is probably a result of the earlier collision. UGC 5101 is about 550 million light-years away from Earth.

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.

Credits

NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)

Image Details

About The Object
Object NameUGC 5101
Object DescriptionInteracting Galaxies
R.A. Position09h 35m 51.67s
Dec. Position61° 21' 14.0"
ConstellationUrsa Major
Distance500 million light-years (150 million parsecs)
About The Data
Data DescriptionHST Proposal: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
InstrumentHST>ACS/WFC
Exposure DatesJanuary 28, 2002, Exposure Time: 38 minutes
FiltersF435W (B) and F814W (I)

Google Preferred Sources

See more from Space Telescope in Google

Choose Space Telescope as a preferred source to make our mission news, visual reporting, and independent explainers easier to find in Google Search.