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Crab Nebula Supernova Remnant
(Spitzer/IRAC-MIPS Image)
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Name: Crab Nebula, Messier 1, M1, NGC 1952
Description: Supernova Remnant
Position (J2000): RA 5h 34m 31.0s Dec 22° 1' 4.6"
Constellation: Taurus
Distance: 6,300 Light Years
Orientation: North is 1.0° left of vertical
Image Credit: NASA/JPL-Caltech/R. Gehrz (U of Minnesota)
Release date: June 11, 2005

Other images:  S9948eo  S0504sp  S0537a  S0537b  S0909sp
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The Crab Nebula is the shattered remnant of a massive star that ended its life in a massive supernova explosion. Nearly a thousand years old, the supernova was noted in the constellation of Taurus by Chinese astronomers in the year 1054 AD.

This view of the supernova remnant obtained by the Spitzer Space Telescope shows the infrared view of this complex object. The blue region traces the cloud of energetic electrons trapped within the star's magnetic field, emitting so-called "synchrotron" radiation. The yellow-red features follow the well-known filamentary structures that permeate this nebula. Though they are known to contain hot gasses, their exact nature is still a mystery that astronomers are examining.

The energetic cloud of electrons are driven by a rapidly rotating neutron star, or pulsar, at its core. The nebula is about 6,500 light-years away from the Earth, and is 5 light-years across.

This false-color image presents images from Spitzer's Infrared Array Camera (IRAC) and Multiband Imaging Photometer (MIPS) at 3.6 (blue), 8.0 (green), 24 (red) microns.