Hubble image archive
Hubble Interacting Galaxy NGC 520
NGC 520 is the product of a collision between two disk galaxies that started 300 million years ago. It exemplifies the middle stages of the merging process: the disks of the parent galaxies have merged together, but the nuclei have not yet coalesced. It features an odd-looking ta...
- Date
- Jan 1, 2008
- Mission
- Hubble Space Telescope
- Archive ID
- hubblesite-images-2008-16-2342-image
NGC 520 is the product of a collision between two disk galaxies that started 300 million years ago. It exemplifies the middle stages of the merging process: the disks of the parent galaxies have merged together, but the nuclei have not yet coalesced. It features an odd-looking tail of stars and a prominent dust lane that runs diagonally across the center of the image and obscures the galaxy. NGC 520 is one of the brightest galaxy pairs on the sky, and can be observed with a small telescope toward the constellation of Pisces, the Fish, having the appearance of a comet. It is about 100 million light-years away and about 100,000 light-years across. The galaxy pair is included in Arp's catalog of peculiar galaxies as Arp 157.
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 B. Whitmore (STScI)Image Details
| About The Object | |
|---|---|
| Object Name | NGC 520, Arp 157, VV 231, KPG 031 |
| Object Description | Interacting Galaxies |
| R.A. Position | 01h 24m 35.41s |
| Dec. Position | 03° 47' 54.99" |
| Constellation | Pisces |
| Distance | 100 million light-years (50 million parsecs) |
| About The Data | |
| Data Description | HST Proposal: B. Whitmore (STScI) |
| Instrument | HST>ACS/WFC |
| Exposure Dates | October 22, 2004, Exposure Time: 77 minutes |
| Filters | F435W (B) and F814W (I) |
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Image and source material are credited to the official mission archive linked below.
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