Celestial hemisphere:  Southern  ·  Constellation: Centaurus (Cen)  ·  Contains:  NGC 5139  ·  Omega Centauri
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Omega Centauri, Jochen Maes
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Omega Centauri, Jochen Maes

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Description

Omega Centauri is a globular cluster in the Centaurus constellation, around 17000 light years from earth.

Containing an estimated 10 million individual stars, Omega Centauri is quite sizeable to say the least (and in fact the largest globular cluster in our Milky Way galaxy as far as our observations have been able to show). What's perhaps even more interesting is the properties of some of those individual stars. Generally speaking, globular clusters formed in the early universe out of a single large cloud of gas. As such, you expect the majority of its stars to have certain things in common (age, composition,...). In the case of Omega Centauri, that's not the case.

The most commonly accepted explanation for this is that Omega Centauri is actually not a globular cluster but the remnant of a dwarf galaxy that collided with and got "absorbed" by the Milky Way. As a result, the core of said galaxy was able to gravitationally stick together while the outer layers got flung out and scattered all over the place. That core is what we now see as Omega Centauri.

Image acquisition details:

8x600" Luminance
10x300" Luminance
8x600" Red
10x300" Red
8x600" Green
10x300" Green
8x600" Blue
10x300" Blue

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Omega Centauri, Jochen Maes