M20

The Trifid Nebula

 

Object M20 -- Emision Nebula
Constellation Sagittarius
Date Aquired 08/01/2002
Camera ST-7E with CFW-8
Exposure 6X5Min L, 5X5Min R (2x2), 5X5Min G (2x2), 5X8Min B (2x2)
Telescope Takahashi FS-102 @f/8
Mount Losmandy G11

 

This is a picture of M20, the Trifid Nebula.  Actually, this is a picture of 3 of the 4 types of Nebula.  The bright red nebula on the left is an emission nebula, where the gas in the cloud is heated so highly by the star in the center (actually its 3 stars close together), that the gas glows red. If your monitor and video card are good enough, you should be able to see a blue nebula surrounding the bright star on the right.  In this area, the gases that make up the nebula have become so thin that it can no longer produce it own light.  This is called a reflection nebula, because the glow of this nebula is caused simply by the reflected light from the large star in the center.  The dark lanes in the emission nebula divide the red nebula into 3 parts (hence the name Trifid), is a dark nebula, which is simply a cloud of dust that isn't producing or reflecting light. 

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