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PIA10392: NGC 6090—a Pair of Spiral Galaxies
Mission: Hubble Space Telescope
Spacecraft: Hubble Space Telescope
Instrument: Wide Field Planetary Camera 2
Product Size: 3481 samples x 3481 lines
Produced By: Space Telescope Science Institute
Full-Res TIFF: PIA10392.tif (36.35 MB)
Full-Res JPEG: PIA10392.jpg (1.478 MB)

Click on the image to download a moderately sized image in JPEG format (possibly reduced in size from original).

Original Caption Released with Image:

Click here for Poster Version of Galaxies Gone Wild PIA10385 Click here for Hubble Interacting Galaxies Poster PIA10385
Galaxies Gone Wild!
Poster Version

Unannotated Poster Version
Hubble Interacting Galaxies Poster

NGC 6090 is a beautiful pair of spiral galaxies with an overlapping central region and two long tidal tails formed from material ripped out of the galaxies by gravitational interaction. The two visible cores are approximately 10,000 light-years apart, suggesting that the two galaxies are at an intermediate stage in the merging process. The Hubble image reveals bright knots of newborn stars in the region where the two galaxies overlap. The right hand component has a clear spiral structure if viewed face-on, while the other is seen edge-on with no spiral arms visible. NGC 6090 is located in the constellation of Draco, the Dragon, about 400 million light-years away from Earth. A number of fainter, and more distant, background galaxies is seen in the image. This system has much in common with the famous Antennae galaxies both in terms of how far the merger has progressed and in our viewing angle.

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. It was taken by the telescope's Wide Field and Planetary Camera 2, which was designed and built by JPL.

Image Credit:
NASA, ESA, the Hubble Heritage Team (STScI/AURA)-ESA/Hubble Collaboration, A. Evans (University of Virginia, Charlottesville/NRAO/Stony Brook University), and G. Ostlin (Stockholm University)


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