Spaghetti Nebula, two-panel SHO mosaic with RGB stars
This is a two-panel mosaic of Siemeis 147, AKA Sharpless 2-240, affectionately known as the “Spaghetti Nebula”. The Spaghetti Nebula is a striking astronomical object located in the constellation of Taurus. This ethereal cloud of gas and dust appears as a delicate, curved nebula with intricate filaments that evoke the image of twisted pasta.
When viewed through a telescope or binoculars, the Spaghetti Nebula measures approximately 4’ x 1’, making it a relatively compact object in the night sky. Its distance from Earth is estimated to be around 3,000 light-years away, providing astronomers with a unique opportunity to study its composition and evolution. One of the most intriguing aspects of this nebula is its complex structure, which suggests that it may have originated as a supernova remnant (SNR), resulting from the collapse of a massive star or the interaction between multiple stars. The Spaghetti Nebula’s delicate filaments appear to be in the process of dissolving, a phenomenon known as “dissipation,” where the gas and dust are being eroded away by the intense radiation and strong stellar winds emanating from nearby stars.

Acquisition Details
- Mount: Astro-Physics Mach2GTO
- Telescope: Takahashi FSQ-106EDXv4
- Camera: ZWO ASI6200MM
The data for this was captured over eleven different nights in January, February, and March, 2025, for a total of 42 hours of data for both panels.
Per-filter totals:
- Panel 1, the lower half
- Red: 2.42 hours (29 subs)
- Green: 2.42 hours (29 subs)
- Blue: 2.42 hours (29 subs)
- Sii: 3.67 hours (22 subs)
- Ha: 4.00 hours (24 subs)
- Oiii: 4.17 hours (25 subs)
- subtotal: 19.08 hours (158 subs)
- Panel 2, the upper half
- Red: 3.08 hours (37 subs)
- Green: 3.08 hours (37 subs)
- Blue: 3.08 hours (37 subs)
- Sii: 4.67 hours (28 subs)
- Ha: 4.50 hours (27 subs)
- Oiii: 4.50 hours (27 subs)
- subtotal: 22.92 hours (193 subs)
- total: 40 hours (451 subs)
Processing Overview
All processing was done in PixInsight, using several plugins and scripts.
RGB filters
The processing included (see the updated processing icons here): (this process was repeated for each panel)
- For each of the RGB channels:
- Dynamic Crop
- GradientCorrecton
- BlurXTerminator (correct only)
- RGB combination via PixelMath
- Auto Linear Fit
- ImageSolver
- SpectrophotometricColorCalibration (PhotonFlux)
- BlurXTerminator (full)
- NoiseXTerminator
Narrowband Filters
(this process was also repeated for each panel)
- For each of the individual Ha, Oiii, and Sii master images:
- BlurXTerminator (full)
- GradientCorrection
- NoiseXTerminator
Combination
At this point I had two different sets of four linear images to combine (one set for each panel):
- RGB
- Sii
- Ha
- Oiii
Building the mosaics
To build the mosaics, I needed to use the MosaicByCoordinates
script. First,
however, I had to plate solve the images. Because I was careful, each set of
frames for the respective panel were the same, so I just plate solved the RGB
image then applied the astrometric solution to the corresponding narrowband
frames by entering this in the process console’s command bar:
cpast -s=RGB Sii Ha Oiii
I performed the MosaicByCoordinates
against each panel’s frames (RGB 1 & 2, etc), and ended up with:
- RGB_panel_1_ra.xisf
- RGB_panel_2_ra.xisf
- Sii_panel_1_ra.xisf
- Sii_panel_2_ra.xisf
- Ha_panel_1_ra.xisf
- Ha_panel_2_ra.xisf
- Oiii_panel_1_ra.xisf
- Oiii_panel_2_ra.xisf
These aligned frames themselves were about 4GB of data.
Once that was done I used GradientMergeMosaic
for each pair, then continued on with post processing.
Post Processing
- StarXTerminator on each of the four frames, needing only the narrowband starless frames and the RGB stars
- Manually used GHS to stretch the individual narrowband frames
- SHO combination with PixelMath
- AutoLinearFit on the SHO
- Several hours of masks, GHS, curves, and HistogramTransformation to get something I liked
- Stretched the RGB stars via SetiAstro’s “Star Stretch” (stretch: 6, color boost: 0)
- SetiAstro’s Stretched
- PixelMath to screen the RGB stars back on the SHO
- A couple iterations of
DarkStructureEnhance
to get it to pop - And, of course, more time with GHS, Curves, and friends
In the end this was a 9131x8615 image (downsized here), and the processing really taxed my machine. The final XISF itself was almost 1gb.


Image details on Astrobin
