Low in the southern sky, this is my first run at imaging the popular Trifid Nebula. Almost two hours of 400 second subs brought this image to life. The seeing so low in the sky is generally not so good, but last night the sky was rather clear. This has been cropped by about half of my full imaging scale. 

From http://www.messier-objects.com/messier-20-trifid-nebula/   :

The name Trifid refers to its three-lobed appearance. Messier 20 consists of several different objects: an emission nebula, a reflection nebula, a dark nebula and an open star cluster.

The dark nebula, catalogued as Barnard 85, consists of dust clouds that absorb and block light from the bright objects behind them. It is responsible for the apparent gaps in the larger emission nebula that give M20 its trifurcated look.

The other two types of nebulae – emission and reflection – make M20 glow in different colours in images.

Emission nebulae are energised by the ultraviolet light of nearby stars and usually appear red in photographs. These nebulae are clouds of extremely hot hydrogen gas and usually regions where new stars are being formed. The light of the stars illuminates the surrounding clouds, ionizing photons in large portions of the clouds.

Messier 20 is a popular target for amateur astronomers as it is quite bright, even when seen through a small telescope. It has an apparent magnitude of 6.3 and lies at an approximate distance of 5,200 light years, or 1,600 parsecs, from Earth. M20 has a linear diameter of over 40 light years and is only 300,000 years old.

Trifid Nebula

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