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Astronomy Picture of the Day
Astronomy Picture of the Day
@apod@reentry.codl.fr  ·  activity timestamp 3 days ago

M1: The Crab Nebula

Image Credit & Copyright: Alan Chen

Explanation: This is the mess that is left when a star explodes. The Crab Nebula, the result of a supernova seen in 1054 AD, is filled with mysterious filaments. The filaments are not only tremendously complex but appear to have less mass than expelled in the original supernova and a higher speed than expected from a free explosion. The featured image was taken by an amateur astronomer in Leesburg, Florida, USA over three nights last month. It was captured in three primary colors but with extra detail provided by specific emission by hydrogen gas. The Crab Nebula spans about 10 light years. In the Nebula's very center lies a pulsar: a neutron star as massive as the Sun but with only the size of a small town. The Crab Pulsar rotates about 30 times each second.

https://apod.nasa.gov/apod/ap251229.html #apod

APOD: 2025 December 29 – M1: The Crab Nebula

A different astronomy and space science related image is featured each day, along with a brief explanation.

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ADS

New Measurements of the Expansion of the Crab Nebula

Published images of the Crab Nebula have been scanned and measured to derive proper motions, the age of the nebula, and its point of origin. Astrometric reductions provided rms errors ranging from 0.14" to 0.31" in both axes for a given image. Proper motions of 50 optical filaments with a 53 yr baseline projected backward indicates the mean date of the supernova event as a.d. 1130 +/- 16 yr, in good agreement with previous investigations by Trimble and Wyckoff & Murray but 76 yr after the reported outburst recorded by the Chinese astronomers in a.d. 1054. This result confirms the well-known acceleration in the Crab's expansion. The image-scanning technique demonstrates that accurate astrometric reductions can be achieved on a personal computer.
ADS

Does the Crab Have a Shell?

We present deep images of a region around the Crab Nebula made with the VLA, utilizing new imaging and deconvolution algorithms in a search for a faint radio shell. The existence of a high-velocity, hydrogen-rich envelope has been predicted to account for the low total mass and kinetic energy of the observed nebula. No radio emission was detected from an extended source outside the Crab Nebula. Our limits on surface brightness are sufficiently low to rule out the existence of a shell around the Crab whose brightness is at least 2 orders of magnitude below that of SN 1006, the faintest historical shell-type supernova remnant. We consider models for the progenitor star and the presupernova environment and conclude that if a fast, outer shock exists, then it has a sharply reduced efficiency at accelerating relativistic particles from the kinetic energy of the blast wave. We also looked for a steepening of the spectral index along the boundary of the Crab Nebula itself, the signature of an outer shock. However, contrary to previous claims, no such steepening was found. The absence of any evidence at radio wavelengths that either the Crab Nebula or a hypothetical shell is interacting with the ambient medium leads to an interpretation that the supernova of A.D. 1054 was a peculiar low-energy event.

APOD: February 8, 1998 - M1: Filaments of the Crab Nebula

Supernova 1054 - Creation of the Crab Nebula

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Messier 1 (The Crab Nebula)

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A dark starfield surrounds a colorful nebula filled with tangled filaments.
A dark starfield surrounds a colorful nebula filled with tangled filaments.
A dark starfield surrounds a colorful nebula filled with tangled filaments.
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