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Sh 2-119 – Clamshell Nebula

Sh 2-119 is an extensive, faint emission nebula in the constellation Cygnus, approximately three degrees east of the North America Nebula and about 2,200 light-years away. Popularly known as the Clamshell Nebula, it appears to surround the bright star 68 Cygni, a massive, extremely hot O-type star whose intense ultraviolet radiation ionises the surrounding gas. The nebula displays a complex structure formed by two large shells on either side of 68 Cygni, with emission arcs, delicate filaments, cavities and dark clouds silhouetted against Cygnus’s dense star field. In the image, the golden hydrogen structures contrast with the bluish oxygen emissions surrounding 68 Cygni, highlighting the effect of its radiation and stellar winds on the interstellar gas. The image was processed in narrowband using an HOO combination and treated with PixInsight’s NarrowbandNormalization script to balance and enhance the different emissions.

General information

Constellation
Cygnus
Category
Nebulae
Date
28 July 2026

Capture

Total time
6h 00min
Subframes
300s (Ha: 36x, OIII: 36x) bin1
Gain / Offset
125 / 30
Calibration
30 flat frames, 30 dark-flat frames and 40 library dark frames, without bias frames

Equipment

Telescope
TS102ED f/5.6
Camera
ASI294MM at -10ºC
Filters
Ha and OIII Astronomik, 6 nm
Mount
Sky Watcher Wave 150i
Guiding
PHD2, Guide scope 60mm/f4 + ASI220MM + PegasusAstro UCH + PPBMicro
Focuser
ZWO EAF
Filter wheel
ZWO EFW 7pos

Processing and environment

Processing
Stacked and post-processed with PixInsight 1.9.4
Acquisition
NINA
Location
l'Ampolla
Sky
Bortle 4

Additional versions

Starless versionStarless version that reveals more clearly the shells, filaments, and hydrogen and oxygen emissions of Sh 2-119.
Identified objectsIdentification of Sh 2-119, 68 Cygni, the planetary nebula PK 087-03.1, and several LBN regions and PGC galaxies in the photographed field.
Post-processing workflowPost-processing workflow for the HOO composition of Sh 2-119 in PixInsight.