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Hubble Interacting Galaxy NGC 6670 (2008-04-24)
 

 

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Description NGC 6670 is a gorgeous pair of overlapping edge-on galaxies resembling a leaping dolphin. Scientists believe that NGC 6670 has already experienced at least one close encounter and is now in the early stages of a second. The nuclei of the two galaxies are approximately 50,000 light-years apart. NGC 6670 glows in the infrared with more than a hundred billion times the luminosity of our Sun and is thought to be entering a starburst phase. The pair is located some 400 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.

About the object
Object name NGC 6670 , NGC 6670A/B, VII Zw 812
Object description Interacting Galaxies
Position (J2000) 18 33 37.38
+59 53 21.2
Constellation Pavo
Distance 400 million light-years (100 million parsecs)
About the data
Data description The Hubble image was created using HST data from proposal 10592: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
Instrument ACS/WFC
Exposure date(s) October 30, 2001
Exposure time 38 minutes
Filters F435W (B) and F814W (I)
Date
Source https://hubblesite.org/newscenter/archive/releases/2008/16/image/ad/ (direct link)
Author NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
Permission
(Reusing this file)
Public domain This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.
The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.
For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.
Hubble 01.jpg
Other versions

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Photo's description:
NGC 6670 is a gorgeous pair of overlapping edge-on galaxies resembling a leaping dolphin. Scientists believe that NGC 6670 has already experienced at least one close encounter and is now in the early stages of a second. The nuclei of the two galaxies are approximately 50,000 light-years apart. NGC 6670 glows in the infrared with more than a hundred billion times the luminosity of our Sun and is thought to be entering a starburst phase. The pair is located some 400 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. About the object Object name NGC 6670 , NGC 6670A/B, VII Zw 812 Object description Interacting Galaxies Position (J2000) 18 33 37.38 +59 53 21.2 Constellation Pavo Distance 400 million light-years (100 million parsecs) About the data Data description The Hubble image was created using HST data from proposal 10592: A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University) Instrument ACS/WFC Exposure date(s) October 30, 2001 Exposure time 38 minutes Filters F435W (B) and F814W (I) Date 24 April 2008 Source http://hubblesite.org/newscenter/archive/releases/2008/16/image/ad/ (direct link) Author NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University) Permission (Reusing this file) Public domainPublic domainfalsefalse
Licensing:
Public Domain


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EXIF data:
File name hubble_interacting_galaxy_ngc_6670__2008-04-24_.jpg
Size, Mbytes 6.9747158203125
Mime type image/jpeg




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