The Clamshell Nebula | Sh2-119

The Clamshell Nebula Sh2-119 in Cygnus, imaged from a light polluted urban sky

THE CLAMSHELL NEBULA

Sharpless 2-119 • Emission nebula • Cygnus • 2200 light-years from Earth


🗓️
Sep – Oct 2024

Overview

The Clamshell Nebula, also known as Sh2 119, is an emission nebula located around 2200 light years away in the constellation Cygnus. This image focuses on the central region of the nebula, where complex clouds of gas and dust are being shaped by intense stellar winds and ultraviolet radiation from nearby hot, massive stars. Much of this structure is driven by the supergiant star 68 Cygni, visible here as the bright point toward the lower right of the frame.

Background

I’ve wanted to image the Clamshell Nebula for quite a while. For some reason I’d always assumed it was quite small, so I was surprised to find that it’s actually more of a wide-field target. Still, I wanted to give it a crack, so decided to leverage my Askar 130PHQ‘s 1000mm focal length to zero in on a composition around the centre of the nebula.

The Clamshell Nebula Sh2-119 in Cygnus, imaged from a light polluted urban sky
Framed astrophoto taken from a light-polluted city, available to buy as a fine art print

Close-ups

  • Close-up view showing dense nebulosity
  • Close-up view showing darker areas
  • Close-up view showing structure in the nebulosity
  • Close-up view showing a brighter region
  • Close-up view featuring a bright star

Imaging details

Date

27 September – 26 October 2024

Location

Bristol, UK (Bortle 8)

Telescope

Askar 130PHQ Flatfield Astrograph

Camera

ZWO ASI 2600MC Pro

Mount

Sky-Watcher EQ6-R Pro

Guiding

WO 50mm + ZWO ASI 120MM Mini

Control

ASIAIR Plus

Software

PixInsight, Lightroom

Image by

Lee Pullen

Filter

Channels

Exposure

No filter

RGB (stars)

30 × 2-minutes (1 hour)

Optolong L-Ultimate

Hα / OIII

144 × 5-minutes (12 hours)

Askar Colour Magic D2

SII / OIII

288 × 5-minutes (24 hours)

37 hours

Imaging details

Date
27 September – 26 October 2024

Location
Bristol, UK (Bortle 8)

Telescope
Askar 130PHQ Flatfield Astrograph

Camera
ZWO ASI 2600MC Pro

Mount
Sky-Watcher EQ6-R Pro

Guiding
WO 50mm + ZWO ASI 120MM Mini

Control
ASIAIR Plus

Software
PixInsight, Lightroom

Image by
Lee Pullen

Filters

No filter
RGB (stars)
30 × 2-minutes (1 hour)

Optolong L-Ultimate
Hα / OIII
144 × 5-minutes (12 hours)

Askar Colour Magic E2
SII / OIII
288 × 5-minutes (24 hours)

Total exposure: 37 hours

Kit list

This is the equipment I used to capture the image.
Affiliate links help support the site at no extra cost to you.

William Optics 50mm with ROTO Lock guidescope

Guidescope: William Optics 50mm with ROTO Lock
Read my review

Buy from Astroshop.eu
Buy from High Point Scientific

Processing

As usual for these types of nebulae, I used an Optolong L-Ultimate for /OIII data, and an Askar D2 for SII/OIII. I normally use an Optolong L-Quad Enhance for RGB data — in this case just the stars — but I actually forgot to use it this time! It doesn’t really make much difference for the stars though, as they’re bright and use just an hour of integration time.

As for the L-Ultimate, that’s 12 hours of data. I knew the SII/OIII component would be fainter, so I doubled that and collected 24 hours. Unfortunately, the SII/OIII was even weaker than I expected. This caused some issues during processing (outlined below) so I needed to take a slightly different approach.

If I were to tackle this target again, I’d be tempted to forego the SII/OIII aspect, and just aim to get a very high signal-to-noise ratio with the channel. As it stands, it’s a really tricky target with an OSC set-up from a city centre. It may be a more realistic approach with full Mono, and definitely with darker skies!

I don’t have time for a full processing walkthrough this time, but the first steps are the same as I followed for the Wizard Nebula. The main difference came after running DBXtract to make an SHO image from the /OIII and SII/OIII data. The SII/OIII channel was so weak / noisy in comparison to the Ha/OIII, I just couldn’t get a high quality result. So, I decided to try something new. I used NarrowbandHueCombination to mix together the , SII, and OIII channels produced by DBXtract.

Check the image below to see the settings I used. I used red at Contribution 100 for the channel; but Contribution 0.5 for both OIII (blue) and SII (green). This made the stronger channel much more dominant. The end result isn’t as colourful as I’d initially planned, but the actual image quality was higher, in that it wasn’t ridiculously noisy.

After that, I used SelectiveColorCorrection to make the red, orange, and yellow colours a bit more distinct. Then it was a case of my usual processes, including UnsharpMark, NosieXTerminator, and DarkStructureEnhance.

Here are two images I initially made using my regular method. The don’t look so bad when viewed small, but when viewed original size on my screen I just wasn’t happy with the image quality.

Example astrophotography image promoting one-to-one online astrophotography masterclasses

Example source data

Here are example single subframes and freshly integrated stacks, just with simple stretches applied.

No filter single subframe
No filter single subframe.
No filter integrated stack
No filter integrated stack.
Optolong L-Ultimate single subframe
Optolong L-Ultimate single subframe.
Optolong L-Ultimate integrated stack
Optolong L-Ultimate integrated stack.
Askar D2 single subframe
Askar D2 single subframe.
Askar D2 integrated stack
Askar D2 integrated stack.

Seestar S50 image

This photo of the Clamshell Nebula was taken using my Seestar S50 telescope. It’s hard to make out much nebulosity, but the bright star 68 Cygni shows up well.






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