Crab Nebula

By Jesse Russell

High Quality Content by WIKIPEDIA articles 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 observed by John Bevis in 1731; it corresponds to a bright supernova recorded by Arab, Chinese and Japanese 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 1012eV. 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. It is part of the Perseus Arm of the Milky Way Galaxy.

• Format: Paperback
• Language: English
• ISBN: 5510525282
• ISBN13: 9785510525281
• Release Date: January 1
• Publisher: Book on Demand Ltd.
• Length: 90 Pages
• Weight: 0.49 lbs.
• Dimensions: 0.2" x 8.3" x 11.0"