|
|
The
Crab Nebula is the remains of a star that became a super novae in 1054
AD. At that time it was bright enough to be seen in daylight.
Today it is only a dim patch of light in amateur scopes. To
see it visually you really need dark skies, and a 6-8 inch scope.
It is not an easy object to see visually because the surface brightness
is very low, and if you have any light pollution it gets lost in the background.
I have tried unsuccessfully on more than one occasion to see it with a
10" reflector from light polluted skies. Capturing a CCD image is
much easier. Even with my 90 mm guide scope, I could see the outline
of the image after only a two minute exposure.
|
|
|
Size: 6 x 4 arcmin RA: 05h 34m 30.0s Dec: 22 d 01m 00s |
|
Scope: Orion MAK 500 | |
M-5C CCD Camera | ||
Focal Ratio: f5.5 | ||
Exposure: 20 min | ||
|
Scope: 8" LX 200 SCT | |
MX-5C CCD Camera & STAR 2000 | ||
Focal Ratio: f3.3 | ||
Exposure: 20 min | ||
|
Scope: 8" LX 200 SCT | |
MX-5C CCD Camera using the Pixcolm track and accumulate feature | ||
Focal Ratio: f4.6 | ||
Exposure: 30 min | ||
This image shows the advantage of a longer exposure and the light pollution filter as much more of the fainter areas are captures. |
Scope: 8" LX 200 SCT | |
MX-5C CCD, STAR 2000 and IDAS LPR | ||
Focal Ratio: f4.8 | ||
Exposure: 50 min | ||
|
Scope: 8" LX 200 SCT | |
MX-5C CCD Camera & STAR 2000 | ||
Focal Ratio: f10 | ||
Exposure: 45 min | ||
Click Here for a Larger Image |
|
Link
to Univ of Tenn Pulsar Page
Multiwavelength Messier Museum Bill Blair's Crab Nebula Photo File National Optical Astronomy Observatory High Energy Astrophysics Science Archive Research Center (HEASARC) Click here to link to Images taken by the Chandra X-Ray Observatory Click here to link to an image by the HST |
|
|