M8 + M20 (Lagoon and Trifid Nebulae)

 Posted: May 6th, 2026
Technical Info
Telescope/Lens: Askar SQA 85 мм f/4.8
Camera: ZWO ASI2600MC Pro
Mount: MT-20-100LHN
Guide Scope: ZWO OAG-L
Guide Camera: ZWO ASI174MM Mini
Software: Pixinsight
Exposure:
22 x 300" ISO/Gain: 100 - Antlia Quadband
 Maldives
 Apr 23rd, 2026
1 h 50 m
7
Resolution: 6140x4096 px
Scale: 5488 KB

M8 Lagoon is one of only two star-forming nebulae visible without a telescope from mid-northern latitudes (the other is the famous M42 in Orion). All other stellar "maternity wards" are only accessible through optics.
Estimates suggest the star formation rate in M8 is about 10 times higher than the rate of the same process in the Orion Nebula.
M20 — three types of nebula in a single object — a unique "museum." It is simultaneously an emission nebula (red hydrogen zone), a reflection nebula (blue dust zone to the north), and a dark nebula (black "veins" of Barnard 85), plus an open star cluster. There are truly few such cosmic "combos."
It is only about 300,000 years old — almost newborn. M20 is one of the youngest nebulae in the sky. The star cluster at its center may be the youngest in the entire Milky Way.

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