Messier 33, the Triangulum Galaxy, is a face-on spiral galaxy in the constellation Triangulum and the third-largest member of the Local Group after the Milky Way and Andromeda.

Click the image to zoom in (4 steps), then again for full view · hover to see it annotated · open full resolutionAnnotated image · click to zoom in (4 steps), then again for full view · open full resolutionSky location chart · click to zoom in (4 steps), then again for full view · open full resolution

Messier 33, the Triangulum Galaxy, is a face-on spiral galaxy in the constellation Triangulum and the third-largest member of the Local Group after the Milky Way and Andromeda. It lies approximately 2.7 million light-years away, with a true diameter of roughly 60,000 light-years. Unlike the more dramatic M31, M33 has a comparatively low surface brightness, making it more challenging to image well from light-polluted skies despite its relatively large apparent size. Its loosely wound spiral arms host numerous star-forming HII regions, most notably NGC 604, one of the largest known star-forming regions in the Local Group. M33 rewards long, dark-sky exposures that bring out its faint spiral structure and pink-tinged nebular knots.

[Source: Wikipedia, en.wikipedia.org/wiki/Triangulum_Galaxy]

Annotated Image

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Sky Location

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Image Details

Moon Phase:New Moon
Camera:Seestar S30
Optics:150 mm focal length, f/5, 30 mm aperture (APO triplet)
Date:2025-12-18
Number of images:567
Exposure per image:30 s
Total imaging time:4 h 44 min

PixInsight Processing

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  6. StarXTerminator (star removal) (x2)
  7. Generalized Hyperbolic Stretch (x9)
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  10. Drizzle Integration
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