Celestial hemisphere:  Southern  ·  Constellation: Fornax (For)  ·  Contains:  NGC 1360
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NGC 1360, Jochen Maes
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NGC 1360, Jochen Maes

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Description

NGC 1360 is a planetary nebula in the Fornax constellation, around 1500 light years from earth.

You're essentially looking at the remnants of a "dead" star that has ejected its shell (the gas cloud you see was once the star's outer layer). Interestingly, this specific planetary nebula looks quite different from what we would expect. Typically, we only see oxygen emissions (the green/blue'ish colour) close to the remnants of our "dead" star because the energy emitted by it is still potent enough to ionize the oxygen (for the sake of simplicity, think of it as the material getting energized and emitting light in the process). As we move further and further away from the remnants of the star, energy emissions become less potent up to the point where there's not enough to ionize the oxygen and we should instead see emissions of less energy demanding elements being dominant (hydrogen for example, resulting in a red'ish colour). That's clearly not the case here. So why is that?

The answer lies with the big bright object you see right at the center of the nebula. This is not a foreground star, but one that's actually in the nebula itself. On top of that, it's a quite massive and very energetic star. Its energy emissions alone basically overrule everything I just explained and causes oxygen to be ionized all throughout the structure, resulting in the somewhat different aesthetics.

Image acquisition details:

19x1800" OIII
21x1200" Luminance
20x900" Red
20x900" Green
20x900" Blue

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NGC 1360, Jochen Maes