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Fayl:Hubble Interacting Galaxy NGC 1614 (2008-04-24).jpg

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Asl fayl (3 373 × 3 373 piksel, fayl hajmi: 9,38 MB, MIME tipi: image/jpeg)

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Taʼrif

The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one-sided curved extension of one of these arms to the lower right, and a long, almost straight tail that emerges from the nucleus and crosses the extended arm to the upper right. The galaxy appears to be the result of a tidal interaction and the resulting merger of two predecessor systems. The system has a nuclear region of quasar-like luminosity, but shows no direct evidence for an active nucleus. It is heavily and unevenly reddened across its nucleus, while infrared imaging also shows a ridge of dust. The linear tail to the upper right and extended arms to the lower right are likely the remains of an interacting companion and the tidal plume(s) caused by the collision. NGC 1614 is located about 200 million light-years away from Earth in the constellation of Eridanus, the River.

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 1614, Arp 186, Mrk 0617, II Zw 015
Object description Interacting Galaxies
Position (J2000) 04 33 59.99
+08 34 42.8
Constellation Eridanus
Distance 200 million light-years (50 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) August 13, 2002
Exposure time 33 minutes
Filters F435W (B) and F814W (I)
Sanasi
Manba http://hubblesite.org/newscenter/archive/releases/2008/16/image/bq/ (direct link)
Muallif NASA, ESA, the Hubble Heritage (STScI/AURA)-ESA/Hubble Collaboration, and A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University)
Ruxsat
(Bu faylning takror foydalanilishi)
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.

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tasvirlangan obyekt

24 aprel 2008

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Sana/VaqtMiniaturaOʻlchamlariFoydalanuvchiIzoh
joriy18:48, 2008-yil 27-aprel18:48, 2008-yil 27-aprel dagi versiya uchun tasvir3 373 × 3 373 (9,38 MB)とある白い猫{{Information |Description=The galaxy system NGC 1614 has a bright optical center and two clear inner spiral arms that are fairly symmetrical. It also has a spectacular outer structure that consists principally of a large one-sided curved extension of one

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