Starless view
Original view
The Trifid Nebula (catalogued as Messier 20 or M20 and as NGC 6514) is an H II region in the north-west of Sagittarius in a star-forming region in the Milky Way's Scutum–Centaurus Arm. It was discovered by Charles Messier on June 5, 1764. Its name means 'three-lobe'. The object is an unusual combination of an open cluster of stars, an emission nebula (the relatively dense, reddish-pink portion), a reflection nebula (the mainly NNE blue portion), and a dark nebula (the apparent 'gaps' in the former that cause the trifurcated appearance, also designated Barnard 85). Viewed through a small telescope, the Trifid Nebula is a bright and peculiar object, and is thus a perennial favorite of amateur astronomers.
Luminance data: Kostas TsekasAvalon linear fast reverse
Askar 107 PHQ Flatfield Astrograph
Asi 533 MΜ Pro
ZWO ASI290MM Mini + WO UniGuide 50mm Scope
Pegasus Astro Pocket Powerbox Advance Gen2
Luminance Baader Ir/cut
Exposure: 190*180sec
Location: Stinger of Scorpius Observatory, Filiates, Thesprotia, Greece.
Color data: Aras Teo
W.O FLT110 with dedicated TMB field flattener
Sky-Watcher EQ6 Pro Belt Drive Mod
Asi 533 MC Pro
W.O ZS 80 ED
P1 Mars-C IMX 462
FeatherTouch 3'' focuser
Starizona MicroTouch autofocuser
Exposure: 103*180sec
Location: Via Lactea Observatory, Kristallopigi Paramithia, Greece
Total Integration:14h 39min