With such a camera you can capture stunning
photographs of deep sky objects which otherwise look like fuzz balls of
light. The
picture to the right is of the modified webcam I use for this purpose.
The webcam is a Logitech QC Pro 3000. There are better options out there
for deep sky work, but at this time this is what my budget will allow.
Nevertheless, I am very satisfied with how this webcam has performed so
far. I am now able to take deep sky photographs successfully. This has
been a dream for me since I was a youngster, and I never would have
imagined that I would be doing it with an inexpensive web camera. Boy,
how times have changed.
I have purchased a few
filters that I feel are very important for astrophotography. Because
webcams are sensitive in the IR range as well as the visible range, if
not filtered, the images captured tend to not be of very good quality.
After all, you normally just want to capture the visible light not
the IR light. This is not always the case, but
normally you want to cut out the IR range and UV range, and just leave
the visible light range. The filter in the bottom right of the picture
is my Baader Planetarium UV/IR-Cut-Filter. I can screw this filter
directly onto the webcam adaptor.
Another very important yet rather
expensive filter is the H-alpha filter. This filter, top center, blocks all light
wavelength except for the 656nm H-alpha emission line. In other words
this filter effectively filters out all light pollution found around
most backyard observatories. This filter is mostly used for H-alpha
emitting nebulae and tends to lower the amount of light which reaches
the CCD. This is not always a bad thing as it allows for longer exposure
times without over exposure problems. A good focal length reducer
(FLR) is a great addition to any telescope setup, and a must for
astrophotography in my opinion. An FLR screwed onto an eyepiece or CCD
camera effectively increases your field of view and amount of light
reaching your eye or CCD chip. The trade off is less
magnification. I use an Atik x.5 FLR pictured bottom left.
My Meade DS114 came equipped with an Altazimuth
GOTO mount as already mentioned previously. This mount is not adequate
for exposure times of much more than thirty seconds due to motor drift
and field rotation. I have learned this fact from experience. Trying to
take long exposure photographs with this mount is a frustrating
task to say the very least. Due to this I decided to purchase an
Orion EQ1 equatorial mount, and an
Orion EQ1M electronic drive system. With this mount system I am now
able to polar align my telescope, which in all reality is the setup of
choice when it comes to astrophotography. By using an equatorial mount
as opposed to an Altazimuth mount you solve the problem of field
rotation, so long as the mount is accurately aligned with the celestial
pole.
Focusing of the telescope can pose problems as well. I have had
many instances were the object I am trying to focus gets bumped out of
the eyepiece or webcam field of view due to trying to focus the object
by hand. To solve this problem I purchased a
Mead #1240 Electronic focuser. My electronic focuser can be seen in
the picture to the right. This device is indispensable when it comes to
astrophotography, and should be near the top of your "need to get list."
Update:
I recently purchased a used Meade DSI Pro from eBay as I was noticing
that I was reaching the limits of what my Logitech QC Pro 3000 modified
webcam was capable of achieving. The biggest problem with the Logitech
is the sensitivity of its ccd chip. I was having to take longer and
longer exposure times in attempts to image dimmer DSOs. A perfect
example of one of these dim DSOs is the Horsehead nebula, B33/IC434. With the Logitech I
was taking two minute exposures through a 135mm SLR lens, and even at
these exposure times I was only getting hints of the Hoursehead nebula.
You can see these attempts on my astrophotography gallery under IC434. This was
becoming very frustrating for me, and really the only solution was to
acquire a more sensitive camera.