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Trifid Nebula

Trifid Nebula

In the Center of the Trifid Nebula Image Credit: Subaru Telescope (NAOJ), Hubble Space Telescope, Martin Pugh; Processing: Robert Gendler

What’s happening at the center of the Trifid Nebula? Three prominent dust lanes that give the Trifid its name all come together. Mountains of opaque dust appear near the bottom, while other dark filaments of dust are visible threaded throughout the nebula. A single massive star visible near the center causes much of the Trifid’s glow. The Trifid, cataloged as M20, is only about 300,000 years old, making it among the youngest emission nebulas known. The star forming nebula lies about 9,000 light years away toward the constellation of the Archer (Sagittarius). The region pictured here spans about 10 light years. The featured image is a composite with luminance taken from an image by the 8.2-m ground-based Subaru Telescope, detail provided by the 2.4-m orbiting Hubble Space Telescope, color data provided by Martin Pugh and image

Trifid Nebula
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Trifid Nebula

Trifid Nebula

Trifid Nebula
Unidentified photographer
Medium unknown
Date unknown
National Air and Space Museum,
Center for Earth and Planetary Studies
Accession no. ASU-IPF-181
Located in the constellation Sagittarius, this beautiful, often-photographed nebula is a dynamic cloud of gas and dust where many stars are born. One of the massive stars at the nebula’s center was born approximately 100,000 years ago. Scientists dispute the nebula’s distance from our solar system but generally agree it is somewhere between 2,200 and 9,000 light years away.