

As you begin to enter the Pacman Nebula, you'll reach what I call the "sulfur shores." These are pillars of dust with ionized sulfur caps that project towards the central core, shaped by stellar forces from the central cluster IC

This region of the Pacman Nebula leads up to the central cluster. It contains many Bok globules (isolated dusty nebulae-you can see a prominent one at the far right of this frame), intricate filaments, and prominent dust pillars. Its brightness increases from left to right as you approach the central cluster.

Here, we reach the central core of the Pacman Nebula, open cluster IC 1590. Its stars power the bright nebulosity of the region and shape the pillars of dust, and have managed to carve out one massive region you'll see below.

This region of the Pacman is a huge dust rift carved out by the central cluster. It is clearly visible in my full image and is one of the most prominent features in the nebula. An interesting aspect is this feature makes it very apparent which stars are in front of, and behind it. Look for stars that have a dim, reddish tone-those are likely behind the dust. Bright stars with blues and yellows are likely in front of the dust.
Firstly, I captured many images of this subject, with a monochrome astronomy camera. To create a color image, I use many different filters and then map the images through each filter to red, green, and blue. For this image, I captured broadband 60-second exposures of red (20), green(20), and blue(20), and narrowband 300-second exposures of Hydrogen-alpha(17), Sulfur-II(23), and Oxygen-III(15). This gives a total of 5 hours, 35 minutes for all filters.
I processed this image in the program PixInsight. I extracted sky backgrounds for every image. Then, I combined each filter's data to create a color image. Afterwards, I did several adjustments including a "histogram stretch" to massively brighten the nebula. Other adjustments include contrast, saturation, and adjusting various blending of the images. This image is a blend of narrowband data to extract the nebula and broadband data to capture the vibrant star colors of the dense starfield throughout the region.
This image was taken over one night. By far the biggest challenge was the moon. Moonlight does not affect Hydrogen-alpha and Sulfur-II data, however Oxygen-III data is a different story. Oxygen-III's emission wavelength is right where the moon glows brightest, so extracting the blue oxygen components you see in my image was a challenge in terms of noise reduction and background gradient removal. Additionally, I only had one clear night to do this, so filter time management was critical.