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Supernova remnant · evidence and sources

Crab Nebula

The expanding debris of the supernova seen in 1054, energised from within by a 33-millisecond pulsar.

Also known as M1, NGC 1952, Tau A.

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, distance and size

Crab Nebula is placed at J2000 RA 5.6 h, Dec 22° at 6,500 light-years, with a bright-shell diameter of 11 light-years.

EpochJ2000
Physical data Catalog

Adopted distance and size

The model is scaled to a bright-shell diameter of 11 light-years at 6,500 light-years, the values published with the source model.

LimitDistance estimates for remnants differ between methods; the page uses the value adopted by the model's authors.
Appearance Reconstructed

Published 3D reconstruction

The fly-in shows the published NASA multi-observatory 3D reconstruction mesh, placed at the remnant's sky position and scaled to the listed diameter. It is an authored scientific visualisation built from observations, not a tomographic map of the gas.

LimitThe single-colour source mesh is tinted for legibility; brightness and colour are not calibrated.

What is not measured

  • Appearance: a reconstruction from measurements, not a direct observation. Published 3D reconstruction. The single-colour source mesh is tinted for legibility; brightness and colour are not calibrated.

Sources cited

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