The Trifid Nebula

M20 / NGC 6514 • Sagittarius

The Trifid Nebula
1. The dark dust 'lanes' of the core
The Trifid Nebula
2. The blue reflection wing
The Trifid Nebula
3. The Trifid and Lagoon in one field

A Three-Fold Masterpiece

The name 'Trifid' means 'divided into three lobes,' referring to the prominent dark dust lanes that split the glowing red emission nebula into sections. M20 is a rare combination of an emission nebula (red, powered by the central star HD 164492A), a reflection nebula (the blue 'top' portion), and a dark nebula (the 'gaps' between the red lobes). It is a star-forming factory located in the star-rich fields of the Sagittarius arm of our galaxy, providing a vivid example of the life cycle of stars and the diversity of cosmic dust.

Imaging Challenges

  • • Low Altitude: Like Thor's Helmet, the Trifid sits low in the southern sky for northern observers, meaning you are fighting atmospheric dispersion and 'boiling' air.
  • • Color Separation: It is easy to accidentally bleed the red Ha signal into the blue reflection area during processing. Keeping these colors distinct is the sign of a pro-level edit.
  • • Dynamic Range: The central star system is quite bright, and the fine dark filaments within the red lobes require careful HDR processing.
M20 is home to 'stellar jets'—long, finger-like stalks of gas and dust that contain embryonic stars, visible as tiny 'spikes' in high-resolution images.

Astro Data

Distance 5,200 Light Years
Object Type Emission, Reflection & Dark Nebula
Constellation Sagittarius

Acquisition

Telescope Sharpstar 130HNT
Camera Player One Uranus-C Pro
Integration 4-6 hours Hours
Integration Broadband (UV/IR Cut) or Ha-RGB blend Hours
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Bring the Cosmos Home

The The Trifid Nebula offers a unique and complex aesthetic for any modern collection.

All images are available as limited edition, museum-quality fine art prints...

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