The Grus Quartet, NGC 7552, 7582, 7590, 7599 Here we are looking well away from the plane of our Milky Way Galaxy into a realm many, many millions of light years away. In the midst of a field containing thinly dispersed stars of our own Galaxy are countless galaxies, the four of the Quartet appear the largest and are closest to us at distances estimated at 55-70 Mly. They are beautiful spiral galaxies presented to us in a range of orientations: NGC 7552, at the top right, is a lovely face-on barred spiral; NGC 7582, in the middle, is a loosely wound spiral, whilst the pair at the bottom, NGC 7590 and NGC 7599, are more tightly wound. Note the compact cores, red star-forming regions and dusty structures visible. Close inspection of this deep exposure reveals that there are many hundreds of deep yellow and red objects with fuzzy outlines; these are in fact distant galaxies hundreds of millions of light years away! To the left of NGC 7590 and NGC 7599 is what appears to be a substantial galaxy cluster dominated by two giant elliptical galaxies. There are several such collections in the field in addition to several very distant edge-on spirals.
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Camera: | SBIG STL11000M, Astrodon filters | Scope: | Takahashi TOA-130, f=1000mm, f7.7+flattner (fov ~2.1° x 1.4°) |
Mount: | Takahashi EM-200 Temma2 | Guiding: | external, E-finder |
Filters/Exposures: | L:R:G:B = 180:100:90:90min ≡ 7h40m | Location: | Heathcote, Victoria, Australia |
Dates: | August 2014 | Processing: | CCDStack2, RegiStar and Photoshop CS5 |