Atoms for Peace Galaxy (NGC 7252 / Arp 226)
This peculiar galaxy is the result of a merger between two separate disc galaxies which has now just entered the phase of settling down. The two original galaxy cores have recently merged leaving giant arcs and swirls of the collision still remaining in orbit around the now combined centre.
The resulting structure is known as the Atoms for Peace Galaxy, named for its resemblance to the traditional depiction of an atom, with electrons orbiting the central nucleus. The name was directly inspired by the famous Atoms for Peace speech given by U.S. President Dwight D. Eisenhower before the United Nations in 1953.
This intriguing galaxy is located in Aquarius at a distance of 220 million light years. The outer loops and especially the long ejecta streams are very faint, but the core shines relatively brightly as a stellar point. The combined magnitude of the system is 12.7 within an area of approximately 1.9 x 1.6 arc minutes.
The galaxy is also known as Arp 226, the 226th entry in Arp’s list of peculiar galaxies.
Also visible in the background are numerous distant background galaxies.
Within the swirls of the collision are numerous bright knots some of which are young ultra-luminous globular clusters containing up to a million hot blue stars each. Several hundreds of these exist near the core of the galaxy.
It is known that giant elliptical galaxies often contain a vast amount of globular clusters, for example the galaxy M87 in Virgo contains over 12,000 globulars. These are thought to have been acquired during past mergers with other galaxies which ultimately formed the elliptical galaxy itself. Still, the number of globulars around giant elliptical galaxies far exceeds the expected number that could be acquired from mergers alone. In this context it is therefore interesting that the collision currently happening in the Atoms for Peace galaxy seems to have triggered the creation of fresh young globular clusters, in addition to any ordinary globulars that would already have been orbiting the merging galaxies. The creation of new globulars during collisions could explain how giant ellipticals amass such a massive number of globulars over time.
This image likely represents the most distant globular clusters imaged with amateur equipment, being 220 million light years away. This is only possible due to the extremely high luminousity of these young globulars. To illustrate the luminousity of these clusters one can compare with globulars in our own Milky Way. The absolute magnitude M of an object can be calculated as follows, given its apparent magnitude m and luminosity distance DL in parsecs:
M = m - 5(log10(DL) - 1)
For very large distances, the cosmological redshift complicates the relation between absolute and apparent magnitude, but for the Atoms for Peace galaxy it is probably safe to ignore this given that 220 million light years is not a very large distance in cosmological terms.
The brightest of the globulars in this image is [WSL93]3, the bright knot immediately to the left of the galaxy core, with a magnitude of 17.86. This translates to an absolute magnitude of -16.28 as per the equation above. Omega Centauri, the largest known globular cluster of the Milky Way, has an absolute magnitude of -10.26 and from the logarithmic nature of the magnitude scale it thus follows that [WSL93]3 is therefore 256 times more luminous than our own Omega Centauri - a truly impressive sight if it was placed in our own galaxy.
Date: 30th June, 19th/20th/27th July, 18th August, 12th/14th/18th September 2012
Exposure: LRGB: 635:91:103:91m, total 15hrs 20mins @ -30C
Telescope: 10" Serrurier Truss Newtonian f/5
Camera: QSI 683wsg with Lodestar guider
Filters: Astrodon LRGB E-Series Gen 2
Taken from my observatory in Auckland, New Zealand
Click here to see an inverted image.
Click here to see a larger crop of the galaxy itself.