| Where are Saturn's
Moons? |
Saturn taken from Conon Bridge on 21 April 2009 at
2300h
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Multiple
images were taken through a 2x Barlow on an 8" SCT
using a Canon 400D. The multipleimages were stacked
using
Registax4 and processed using Adobe Photoshop CS & NeatImage..
- Note
that the rings are totally "edge-on".
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- Saturn taken from Conon Bridge on 01 April 2007 at
2300h
-
Multiple
images were taken through a 2x Barlow on an 8" SCT
using a
Meade DSI Pro. The multiple FITS images were stacked
using
Registax4 and processed using Adobe Photoshop CS. Only the IR
and
Red filters were in focus so the resultant black & white image
is a
combination of only these two.
- Note
that the rings are even less "face-on" than the previous two years.
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Saturn taken from Conon
Bridge on 24 Feb 2006 at 2100h
-
Multiple images were taken afocally using a 15mm
Plossl + 2x Barlow eyepiece combination on an 8" SCT using a Nikon
Coolpix 5700 digital camera. Exposures varied from 0.25sec to
0.5 sec at ISO 200, 400, & 800, f/4.2. The multiple
images were stacked using Registax3 and processed using Adobe Photoshop
CS.
- Note that the rings are
less "face-on" than at this time last year (see below).
-
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Saturn taken from Conon
Bridge on 25 Feb 2005 at 2100h
-
Multiple images were taken afocally using a 32mm
Plossl + 2x Barlow eyepiece combination on an 8" SCT using a Nikon
Coolpix 5700 digital camera. Exposures varied from 0.125sec
to 0.5 sec at ISO 200, f/4.2. The multiple images were
stacked using Registax3 and processed using Adobe Photoshop CS.
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- Saturn
has been a great planet to view this winter. The angle it is currently
at maximises the view of its ring system we get on Earth.
-
- The
ring can be made out even with binoculars (13-36x with 70mm objective).
-
- The
image above was constructed by taking a CCD video image through a 114mm
reflector on 30 December 2003.
-
- The
video images were stacked and refined using Registax v.2.2.0.0. The
resultant image was then refined (unsharpen mask & despeckled)
using Adobe Photoshop.
-
- Even
this small image shows the ring system has a structure - a dense
(whiter) inner portion and a less dense (greyer) outer. The Cassini
division was visible through the telescope but it did not come out
clearly on the CCD image.
-
- The
shadow of the planet on the portion of the ring behind it is visible,
as is a stripe about half way down the planet which is part of a
weather system.
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