What we found on the web about Crab Nebula
The Crab Nebula (catalogue designations M 1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The nebula was first observed by John ...
The Crab Pulsar (PSR B0531+21) is a relatively young neutron star. The star is the central star in the Crab Nebula, a remnant of the supernova SN 1054, which was widely observed on ...
Crab Nebula ( ′krab ′nebyələ ) ( astronomy ) A gaseous nebula in the constellation Taurus; an amorphous mass which radiates a continuous spectrum
Astronomy Picture of the Day . Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a ...
About This Image. The Crab Nebula is a supernova remnant, all that remains of a tremendous stellar explosion. Observers in China and Japan recorded the supernova nearly 1,000 years ...
updated: 03/09/2003. The Crab Nebula Before you come to lab. Print out the following images: Crab Nebula in 1973 Crab Nebula in 2000 Spectra of the Crab Nebula
A collection of images taken by the Chandra X-ray Observatory, including image descriptions, constellations, an X-ray sky map and comparisons with images in other wavelengths such ...
John Hester, Allison Loll, Davide De Martin, ESA, NASA Larger and jumbo mosaic images. Roughly a thousand years old, the Crab Nebula shines brightly from
This new Hubble image - One among the largest ever produced with the Earth-orbiting observatory - shows gives the most detailed view so far of the entire Crab Nebula ever made.
The Crab Nebula Filaments The photo shows an image of filaments of material blasted into space by the tremendous stellar explosion which was the supernova that was witnessed by ...
This article from Sol Station discusses the Crab Nebula and pulsar in detail, including historical and scientific aspects of the objects. Using the Crab Nebula and pulsar as ...
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The Crab Nebula (catalogue designations M1, NGC 1952, Taurus A) is a supernova remnant and pulsar wind nebula in the constellation of Taurus. The nebula was first observed by John Bevis in 1731, and corresponds to a bright supernova recorded by Chinese and Arab astronomers in 1054. At X-ray and gamma-ray energies above 30 KeV, the Crab is generally the strongest persistent source in the sky, with measured flux extending to above 1012 eV. Located at a distance of about 6,500 light-years (2 kpc) from Earth, the nebula has a diameter of 11 ly (3.4 pc) and expands at a rate of about 1,500 kilometers per second.

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