Crab Nebula NGC1952 (M1)



Object Data
Description The Crab Nebula is a supernova remnant from a giant star that suffered a catastrophic core collapse on July 4, 1054, almost a millennium ago. The enormous amount of electrical power needed to light up this structure comes from the rotational energy of a tiny stellar cinder called a neutron star, which is located near the center of the nebula and is spinning at thirty times per second. With its trillion gauss magnetic field, this rapidly spinning neutron star effectively becomes a 30Hz electric generator, inducing a tremendous current into the highly conductive surrounding plasma. The ionized gas is heated to millions of degrees, where it radiates prodigiously in the X-ray and extreme ultra-violet portions of the spectrum. The outer reaches of the nebula, which are bathed in the ultra-violet from the core, re-radiate in the visible spectrum much like a conventional household florescent lamp. Although it is quite beautiful in photographs, it is difficult to discern any detail in this object with a small telescope.
Constellation Taurus the Bull
Right Ascension 5h 35m 12s
Declination +22° 2' 7"
Magnitude 8.4
Angular size 8.0 arcminutes
Distance 1.8 kiloparsecs (5,800 light years)
Radial Velocity ?? kilometers per second
Image Data
Photographer Charlie Warren
Main Scope Meade 10" LX200 GPS @ f/7
Guide Scope None
Guide Camera None
Imaging Camera Starlight Xpress MX7C
Resolution 720 x 537 @ 1.0 arcseconds per pixel
Exposure Forty exposures of one minute each. Aligned, stacked, and processed with AstroArt.
Date February 28, 2003
Location Mid Florida StarGaze at Fish Eating Creek Campground in Glades County, Florida


StarFred Home Page