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CRAB NEBULA 

 

The Crab Nebula is the remnant of a supernova explosion that was seen on Earth in 1054 AD. It is 6000 light years from Earth. At the center of the bright nebula is a rapidly spinning neutron star, or pulsar that emits pulses of radiation 30 times a second.

The nebula was first observed in 1731 by John Bevis, and corresponds to a bright supernova that was recorded by Chinese and Arab astronomers in 1054. Located at a distance of about 6,300 light years (2 kpc) from Earth, the nebula has a diameter of 11 ly (3.4 pc) and is expanding at a rate of about 1,500 kilometres per second.

The nebula was the first astronomical object identified with a historical supernova explosion. The nebula acts as a source of radiation for studying celestial bodies that occult it. In the 1950s and 1960s, the Sun's corona was mapped from observations of the Crab's radio waves passing through it, and more recently, the thickness of the atmosphere of Saturn's moon Titan was measured as it blocked out X-rays from the nebula.

 

 

 

http://www.mpa-garching.mpg.de/~thj/popular/Crab_Nebula.jpg
http://chandra.harvard.edu/photo/2002/0052/0052_xray_opt.jpg
http://chandra.harvard.edu/photo/0052/0052_xray_lg.jpg
http://www.physics.hku.hk/admission/why_phy/image005.jpg
http://nssdc.gsfc.nasa.gov/image/astro/hst_southern_crab_9932.jpg
http://eagle.la.asu.edu/hester/crab_prettypics/crab_composite.jpg
http://www.inkycircus.com/jargon/images/crab_nebula.jpg