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M20, Trifid Nebula

M20, known as the Trifid Nebula, is an active emission region where gas and dust form a complex structure. It consists mainly of ionised gas: chiefly hydrogen, which emits a characteristic red glow, and doubly ionised oxygen, responsible for the bluish tones. It has a combined morphology comprising an emission region, a bluish reflection area and dark dust lanes that visually divide it into three lobes. It lies approximately 5,200 light-years from Earth, has an apparent size of 29.0 × 27.0 arcminutes and a visual magnitude of +6.3.

General information

Constellation
Sagittarius
Category
Nebulae
Date
25 June 2025

Capture

Total time
6h 50min
Subframes
300s (Ha: 42x + OIII: 40x) bin1
Gain / Offset
125 / 30
Calibration
N/A

Equipment

Telescope
TS102 f/5.6
Camera
ASI294MM at -10ºC
Filters
Ha and OIII, 6 nm Astronomik
Mount
Sky Watcher Wave 150i
Guiding
Guide scope 60mm f/4 + ASI220MM with PHD2
Focuser
PegasusAstro PPBMicro
Filter wheel
ZWO EFW 7pos

Processing and environment

Processing
PixInsight 1.9-3
Acquisition
NINA
Location
l'Ampolla
Sky
Bortle 4

Additional versions

Wide field of view
Identified objects
Post-processing workflowDiagram of the PixInsight workflow used to produce the final image.