Celestial hemisphere:  Southern  ·  Constellation: Fornax (For)  ·  Contains:  Fornax A  ·  Fornax B  ·  NGC 1310  ·  NGC 1316  ·  NGC 1317
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NGC 1316, Jochen Maes
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NGC 1316, Jochen Maes

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Description

NGC 1316 is a lenticular/elliptical galaxy in the Fornax constellation, around 60 million light years from earth.

What you're looking at here is very likely the result of a past merger/collision of multiple smaller galaxies roughly 3 billion years ago. So how do we know that? There's a few telltale signs:

- First of all, lets establish that lenticular/elliptical galaxies tend to be very "quiet". They've used up most of their material in past star formation, so very little new star formation is happening. Their core regions tend to be relatively uneventful compared to other galaxies as well.

- In the case of NGC 1316, it's anything but "quiet". When observing it in in the radiowave end of the spectrum, it's in fact one of the most powerful emission sources in the entire night sky. These emissions are triggered by large amounts of material falling into the galaxy's central supermassive black hole. The fact that this material is even there to begin with is a good indication that it had to come from elsewhere (galactic merger).

- Visually, the above can be seen to an extent by the dark dust lanes near the galactic core as well (the dark orange/brown structures in the center).

- The halo around the galaxy (the thin glow-like structure far around it) is quite a bit larger than one would expect, hinting at past gravitational interactions that flung out large amounts of stars/gas.

Image acquisition details:

21x1200" Luminance
15x1200" Red
15x1200" Green
15x1200" Blue
6x1800" HA

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NGC 1316, Jochen Maes