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Star-forming emission nebula · evidence and sources

Trifid Nebula

Also known as M20, Messier 20, NGC 6514.

Catalog Position basis, the same label the app shows on the selection card.

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Every aspect, with its origin

One record per aspect. The origin says what kind of thing each value is; the source says where it came from; the limit says what it cannot tell you.

ObservedCatalogComputedReconstructedIllustrativeUndocumented
Position Catalog

Sky position and adopted distance

Trifid Nebula is placed at J2000 RA 18 h, Dec -23° in Sagittarius, at an adopted distance of 5,200 light-years.

EpochJ2000
LimitThe three dust lanes and emission/reflection regions are constrained in projection; their depth is not inferred.
Physical data Catalog

Measured dimensions

Trifid Nebula (star-forming emission nebula; central source HD 164492A, O-type ionizing star): measured footprint 32 × 24 light-years; display depth 7 light-years (not measured); outer radius used for arrival 16 light-years.

Methodmeasured sky-plane structure with constrained display depth
Appearance Reconstructed

Sky-plane structure with a display depth

The observed three-lane silhouette, ionized cavity, blue reflection region, and HD 164492A anchor the model in the sky plane. Their line-of-sight placement is not measured, so the shallow physical depth is a disclosed presentation volume rather than claimed tomography.

Methodmeasured sky-plane structure with constrained display depth
LimitEmission points and knots are deterministic presentation samples, not individually catalogued gas parcels.

What is not measured

  • Appearance: a reconstruction from measurements, not a direct observation. Sky-plane structure with a display depth. Emission points and knots are deterministic presentation samples, not individually catalogued gas parcels.

Sources cited

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