NGC 6090

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 upper component has a clear spiral structure viewed face-on while the component just below 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.

Credit:

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

About the Image

Id:heic0810ay
Type:Observation
Release date:24 April 2008, 15:00
Related releases:heic0810
Size:3481 x 3481 px

About the Object

Name:NGC 6090
Type:Local Universe : Galaxy : Type : Interacting
Distance:400 million light years
Constellation:Draco
Category:Anniversary
Galaxies

Image Formats

r.titleLarge JPEG
4.4 MB
r.titleScreensize JPEG
231.0 KB

Zoomable


Coordinates

Position (RA):16 11 40.12
Position (Dec):52° 27' 19.07"
Field of view:2.91 x 2.91 arcminutes
Orientation:North is 72.7° right of vertical


Colours & filters

BandWavelengthTelescope
Optical
B
435 nm Hubble Space Telescope
ACS
Optical
H-alpha
656 nm Hubble Space Telescope
ACS
Infrared
I
814 nm Hubble Space Telescope
ACS

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