Celestial hemisphere:  Northern  ·  Constellation: Cepheus (Cep)  ·  Contains:  HD208020  ·  HD209111  ·  LBN 569
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LBN 569, Reg Pratt
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LBN 569

Getting plate-solving status, please wait...
LBN 569, Reg Pratt
Powered byPixInsight

LBN 569

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Description

LBN 569 sits 9° from Polaris near the point of Cepheus. Its a small part of a very large structure of Integrated Flux Nebula that blankets the entire northern celestial pole. This is same extra-galactic dust present in my image of open cluster NGC 188 (7° away). When looking at the 2 fields one thing jumps out at me immediately. The IFN found around NGC 188 is basically void of color while LBN 569 glows golden and there are even hints of red present in a few parts of the frame. My guess is that the golden hue is largely, if not mostly, due to the dust being illuminated by the class M3 variable star V438 Cephei. Don't quote me on that though. I'm just a bro with a telescope, not an Astronomer.

I also collected 25 hours of hydrogen-alpha data which revealed that the entire dust structure contains a weak but detectable amount of HA. Unfortunately the signal was too weak to be of any use though. This HA could also be contributing to the overall color of the dust especially since patches of it are visible even in the RGB data.

For me the cool thing about this field is how the golden glow of V438 Cep contrasts against the cold blue glow coming from nearby pair of blue stars above it. I tired to get some info on those stars but after 10 minutes in search engines and sky surveys all I was able to find out was that the blue star on the right is HD 208020 and it is apparently also a variable star.

This was an extremely difficult target to process. I didn't get anywhere near the vision I had in my head but when I look at other imagers attempts its very clear that this region of space is not for casuals and the result I got is pretty good so I'm trying to shake the bummer of a feeling one gets when they feel they've miss the mark on an image.

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