In 1054 there suddenly appeared an new star in the sky. This was recorded by Chinese astronomers, amongst others, and was so bright that it was visable in daylight. This was the light from a star which had exploded into a supernova.The residue from this explosion is the Crab Nebula which is still expanding as it blasts into space today.
Currently M1 is around 10 light years in diameter and expanding at 1800 km/s. At the scale of the image above it is growing by 1 pixel every 4 years.
The original star was not compleatly destroyed and remains as a Pulser rotating about 30 times a second. It can be seen in the image as the lower of the pair of stars just left of center.
M1 was originally discovered by John Beavis in 1731
References;
http://www.seds.org/messier/M/m001.html
Capture Device
Starlight-Xpress SXV-H9 Sony ICX285AL Exview HAD Cooled CCD Array 1392 x 1040 @ 6.45uM / Pixel
Filter Type
Astronomik Type IIc RGB
Colour Technique
L(Ha) R(Ha)GB
FOV
≈16.38 x 12.24 arc mins (0.706 arcsec/pixel) before cropping
Exposure
426 m (7.1 hours) Total
Integration
Ha 12nm (21x 800 sec bin 1x1)
R = 100% Ha
G (12 x 300 sec bin 2x2)
B (12 x 430 sec bin 2x2)
Notes
This image uses Hydrogen Alpha light to provide the luminance and for the Red colour channel. This was found to give the most detail to the fine filamentary structures in the Crab Nebula. Conventional clear filtered luminance data was gathered along with red information but this was not used in the final image.
Frames were Bias calibrated only and RGB combined in Maxim. Post processing with levels and sharpening and the addition of luminace (Ha) in Photoshop.