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Star-forming emission nebula · evidence and sources

Rosette Nebula

Also known as NGC 2237, NGC 2238, NGC 2239, NGC 2246, Caldwell 49, Rosette.

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

Image-field position and adopted distance

Rosette Nebula image-field center is placed at J2000 RA 6.5 h, Dec 4.9° in Monoceros, at an adopted distance of 5,000 light-years.

EpochJ2000
LimitImage north is 0 degrees right of vertical. Line-of-sight thickness is illustrative.
Physical data Catalog

Image field at the adopted distance

Rosette Nebula (star-forming emission nebula; central source Rosette Nebula, embedded stellar population): projected footprint at the adopted distance 137.8 × 117.3 light-years; outer radius used for arrival 68.9 light-years.

Methodmeasured sky-plane structure with constrained display depth
Appearance Reconstructed

Sky-plane structure with a display depth

DECam emission-line colors are assigned to sulfur, hydrogen and oxygen filters. Embedded and foreground stars remain in the observation. Projected structure follows the credited observation at its published angular scale and an approximate adopted distance. Shallow depth is illustrative, not measured tomography. The source palette is preserved; brightness is adjusted for the navigable view.

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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