Even though the moon was full on Tuesday, I bugged out of work an hour early
Wednesday afternoon and drove out into the Everglades to capture the comet as
it made its closest approach to the Double Cluster in Perseus. The sky wasn't
dark enough for imaging till 7:05 PM, and the moon poked its nose above the
horizon at 7:16 PM. Within that somewhat narrow time window, I captured
12 minutes worth of photons, which is just about right for this comet at
the magnification factor needed for this picture. The field of view is
7¼° wide by 5½° high, with North up and East to the
left. Both the comet's tail (heading SouthSouthEast) and its ion stream
(heading East by North) are just barely visible. The double cluster can
be found on the opposite side of the photo, with NGC884 immediately to the
left of NGC869.
Even though the full moon was now high in the sky, I could not resist the urge
to capture a wide-field shot of the Orion Nebula. The sky was getting quite
bright, so the picture is a bit washed out with poor detail in the dimmer
areas. I wanted to show the Running Man Nebula in perspective with M43 and
M42, although next time I will center things a bit better. The FOV is
1¾° wide by 1¼° high. This is the result of only
twelve minutes of exposure, so in addition to being washed out from the
moon, the picture is a bit grainy. I am a bit puzzled by the bright stars
that appear to have five points on them as if they were drawn by some young
child with a dull marker. Still, any picture of the sky is better than no
picture at all.
I don't think there has ever been a time before this when I have set up all
my equipment, only to tear it all back down again after only a half hour of
imaging. The worst part is that the sky was perfectly clear, with no haze
and no clouds at all. The stability was quite good as well. I wish these
conditions would occur when the moon wasn't full. It feels very strange
to be home by 9 PM.
Fred Lehman, January 26, 2005
C/2004 Q2 (Machholz) with the Double CLuster
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The Great Orion Nebula and surrounding clusters
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