Astronomy Picture of the Day

Explanation: Unspeakable beauty and unimaginable bedlam can be found together in the Trifid Nebula. Also known as M20, this photogenic nebula is visible with good binoculars towards the constellation of Sagittarius. The energetic processes of star formation create not only the colors but the chaos. The red-glowing gas results from high-energy starlight striking interstellar hydrogen gas. The dark dust filaments that lace M20 were created in the atmospheres of cool giant stars and in the debris from supernovae explosions. Which bright young stars light up the blue reflection nebula is still being investigated. The light from M20 we see today left perhaps 3000 years ago, although the exact distance remains unknown. Light takes about 50 years to cross M20.

January February March April May June July August September October November December

<  May 2005   > Mo Tu We Th Fr Sa Su 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 1995 1996 1997 1998 1999 2000 2001 2002 2003 2004 2005 2006 2007

Authors & editors: Robert Nemiroff (MTU) & Jerry Bonnell (USRA)
NASA Web Site Statements, Warnings, and Disclaimers
NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.

Publications with keywords: M20 - dust
Publications with words: M20 - dust
See also:

• Trifid Pillars & Jets
• Mountains of Creation
• Three Nebulae in Narrow Band
• The Trifid Nebula in Stars and Dust
• The Center of Centaurus A
• vdB 152: Reflection Nebula in Cepheus
• Dust Sculptures in the Rosette Nebula

All publications on this topic >>