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. |