Vixen VC200L User manual

Daniel Evaluates the VC200L’s
Visual Capabilities
I was pleased to have the opportunity
to report my visual experiences with the
Vixen -inch VC200L Sixth-Order
Aspherical Cassegrain (“VISAC” for short).
The VISAC optical system differs signifi-
cantly from that of the more common
Schmidt-Cassegrain Telescope, because it
does not rely on a frontal corrector plate.
Instead, the VISAC houses a four vane spi-
der supported mount that holds the sec-
ondary mirror, while a three element cor-
rector lens resides at the back of the OTA,
in front of the focuser.
I personally find this optical design to
be an advantage because dew formation on
the frontal corrector plate of a typical
Schmidt-Cassegrain is a recurring problem.
In a way, the VISAC optical tube behaves
like a dew shield in itself with its primary
mirror safely tucked at the bottom of the
open optical tube. This design also speeds
up the cooling process compared to stan-
dard Schmidt-Cassegrain designs.
With a focal length of 1 00 mm, at
F/9 the focal ratio is also a
bit faster than that of the
typical Schmidt-Cassegrain,
and its central obstruction,
at 40%, is a little larger.
Keep in mind though that
the VISAC is designed pri-
marily to serve as an astro
imaging system, but many
observers have been curious
to learn more about its visu-
al performance and that is
the focus of my report.
The focuser with which
the VISAC is fitted is sim-
ply wonderful. It is an independent rack &
pinion model mounted behind the pri-
mary, which remains stationary. Most
Schmidt-Cassegrains suffer from mirror
shift, to one degree or another. Companies
have done their best to minimize this com-
mon issue, but it is still present in the many
models I’ve tested. The typical Schmidt-
Cassegrain is focused by moving the pri-
By Daniel Mounsey and Shawn Hendrix
Astronomy TECHNOLOGY TODAY 41
VIXEN
VC 200L
One As ronomer Takes
a Visual Tour While Ano her
Enjoys he Imaging
Experience.
T o Looks at the Visual
and Imaging Perfomance
of the VISAC
Optica Design Catadioptric
Aperture 8" (200mm)
Limiting Visua Magnitude 13.3 Mag
Foca Ratio f/9
Foca Length 70.9" (1800mm)
Focuser Design* 2" Rack-and-Pinion
Weight – OTA 13.2 bs (6 kg)
Tube Length 24.4" (486mm)
Diameter 9.13" (232mm)
*(1.25" or T2 adaptations are optiona )
Vixen VC200L - 8" f/9 Modified Cassegrain OTA
Specifications

42 Astronomy TECHNOLOGY TODAY
VIXEN VC 200L
mary optic back and forth, in effect chang-
ing the focal length of the optical train to
match the location of the imaging sensor or
eyepiece focal point, rather than moving
those elements to a fixed focal point. This
mirror shift can sometimes cause target
objects to shift on the focus plane during
focus and can be quite troublesome while
imaging deep sky objects. Because the
VISAC primary stays stationary, mirror shift
induced image shift is essentially eliminated.
Another interesting feature is the
VISAC’s metal side plate which runs along
one side of the dovetail plate. This brilliant
idea prevents the clamp screws of the saddle
plate from marring the dovetail plate and
should be incorporated on other designs.
Another nice feature is a carrying handle
located on top of the OTA. This proved to
be very useful when lifting the optical tube
on and off the mount. The VISAC is sur-
prisingly light at about 16 pounds including
the supplied 7x50mm finder and 1.25-inch
star diagonal. Vixen also offers an optional
carrying case, and an f/6.4 focal reducer
which is highly recommended for imaging.
The focuser does accommodate a larger
2-inch star diagonal if desired. I would have
preferred that the 2-inch visual back be
equipped with a compression ring instead of
the older school thumb screws as this would
further help prevent possible oscillation of
the diagonal. Compression rings tend to
secure diagonals a bit more solidly than set
screws alone and also help prevent set screw
marring of the diagonal barrel.
These observations took place on June
19, 2007, from Pasadena, California. Seeing
conditions on this evening were about 7 out
of 10 and nice enough to conduct some
good observations of deep sky objects as well
as planets. I started my first observations on
Vega in order to check collimation and star
test the instrument. The collimation was
dead perfect, while the optics exhibited just
a bit of under-correction.
My first observations started with a
Televue 22-mm Panoptic eyepiece. This pro-
duced a magnification of 2x, and framed
M , the Lagoon nebula, very nicely. The
emission nebula exhibits an ample number
of stars for demonstrating the full field per-
formance of the VICAC, and, to my sur-
prise, these were pinpoint from nearly edge
to edge and proved to be much tighter than
those produced by the Schmidt-Cassegrains
I’ve tested in the past. I then slipped in a 2-
inch star diagonal and my 35-mm Televue
Panoptic eyepiece for a magnification of 51x,
and, once again, the stars were pin point
from nearly edge to edge.
One thing that really stood out while
focusing the image was the actual focuser
itself. The VISAC’s stock focuser is one of
the smoothest I’ve ever tested and I really
liked it; in fact it felt even nicer than the
focuser on my 6-inch Takahashi refractor.
Two other observers who were present dur-
ing this observation agreed that the rack and
pinion focuser was exceptional.
Jupiter was pretty well placed at this
point, so I decided to put in some higher
magnification using a Pentax 10-mm XW
eyepiece to yield 1 0x. Although the deep
sky images were quite wonderful, the size of
the central obstruction was a bit less favor-
able for teasing out optimum contrast of the
features of Jupiter. Jupiter however still
revealed a number of colored belts and
enough detail for an interesting and enjoy-
able view. Although there may be more
appropriate choices for planetary observa-
tions, it is important to remember that the
VISAC was not really designed with plane-
tary work in mind.
Next, I decided to have a look at
Alberio, the famous colored double in
Cygnus. High magnifications with a Pentax
7-mm XW at 257x, revealed two very nice
Airy discs surrounded by a few very faint dif-
fraction rings. The red and blue colors of the
pair also stood out quite well.
Overall, the visual image quality of the
VISAC was quite impressive, particularly
considering how portable and light weight it
is. It is a step up in image quality from the
typical Schmidt-Cassegrain in my opinion,
particularly with regard to edge sharpness.
Although the VISAC costs nearly double
what an -inch Schmidt-Cassegrain optical
tube does, I think it’s worth it! The build
quality is very high and collimation options
are almost limitless. There are a series of
adjustment screws at the back of the optical
tube for collimation by adjustment of the
primary and focuser orientation can even be
adjusted as well.

Astronomy TECHNOLOGY TODAY 43
VIXEN VC 200L
Shawn Tries His Hand at
Imaging with the VISAC
I would like to thank Woodland Hills
Telescope for allowing me to test the Vixen
VC200L. I was given the telescope with the
claim that the Vixen VC200L was designed
to produce one of the best astro-imaging
instruments available and I set out to prove
them right, wrong, or somewhere in
between.
It would not be fair to test the scope on
an inferior mount, so the scope was
equipped with a Vixen Sphinx Mount, the
same that is paired with the VC200L when
purchased as a package. I can sum up my
impressions of the mount this way: smooth,
solid, and Xbox meets astronomy. The Star
Book is a fantastic product and the
mount/tripod combination a very well engi-
neered machine. But, that is another review
for another time.
The VC200L is an excellent visual
scope as well as imaging platform. Once
cooled and set up properly, the scope deliv-
ers sharp, low power images, bright objects
with crisp stars, and very good high power
images of double stars, carbon stars, and
most every other deep sky object I pointed
it at. Views of Jupiter were pleasing, but not
optimum, due to loss of contrast caused pri-
marily by the effects of the secondary mirror
assembly central obstruction. That is the
downside of the relatively large 40 per cent
obstruction of that assembly.
This however is very important to the
photographic side. The large secondary
allows the Telescope to fully illuminate a
35mm film frame. This is one of the very
nice features of its unique catadioptric
design. The VC200L is not a Schmidt-
Cassegrain as it may appear upon first
inspection. You will quickly notice the lack
of a corrector lens on the front of the tube
assembly. This is because it uses a sixth order
aspherical primary mirror, a convex second-
ary mirror, and finally a triplet corrector
lens. Vixen has assigned the abbreviation
VISAC (Vixen Sixth Order Aspherical
Cassegrain). I simply call it stunning.
The optical train contains a 3-element
corrector which corrects for field curvature
and coma much better than a Schmidt cor-
rector. This lends to stars as sharp on the
edge as they are in the center of the film or
CCD. A nice secondary benefit of the
design is that it does not dew up as easily,
but you still may want to use a dew shield to
protect the secondary from dew. The open
tube also cools much faster and cool down is
an absolute necessity to image quality.
Indeed, the VC200L showed large thermal
currents that were very visible in the image
until it has fully cooled. Fortunately, this did
not take long.
Along with proper cool down, perfect
collimation is key to obtaining a good star
test. Collimation is accomplished by a pro-
cedure similar to that used for Newtonians;
tilt of the secondary mirror is first adjusted
and then that of the primary mirror.
Collimation held much better than with
Newtonians I've experienced, but not as
well as with a standard Schmidt-Cassegrain.
That said, if you are going to use the scope
for imaging, take the time to tune it and it
will exceed your expectations.
Another benefit of the design is that the
fixed primary mirror eliminates the mirror
shift that plagues Cassengrains that accom-
plish focus by moving the primary. While
the rack and pinion focuser with which the
scope was equipped was a pleasure to use, I
recommend adding a JMI “Motofocus” to
that focuser for convenient, hands-off focus-
ing. This makes achieving optimum image
focus a much faster, less frustrating process.
There are a ton of little things that add
up to make this telescope a joy to work with:
simple things like a built in camera bracket
to more advanced features like a 60mm
visual back that illuminates 2-inch eyepieces
without vignetteing.
After adding a few accessories such as
anti-vibration pads, Vixen's optional f/6.4
focal reducer, and the JMI Motofocus unit,
I would agree with Vixen Optics that this is
one of the best telescopes available for astro-
imaging. This telescope is a good value for
the astronomer that is ready to get serious
about astrophotography. I rate this telescope
a 9/10 for the imager, but would recom-
mend a more traditional Schmidt-
Cassegrain for the visual only astronomer, as
they would find more aperture and contrast
for the same cost.
As you can tell, I was really impressed
with this scope and couldn’t wait to take it
out to clear, dark skies.

Finally the new moon arrived and I joined an
informal gathering of astronomy enthusiasts at
Mount Pinos Recreation Area. Operated by the U. S.
Forestry Service, the observing site is a large paved
parking area at the very end of a paved road (no lights
in the parking lot).
A summer evening at the Pinos observing
site, which sits at an elevation about of about ,300
feet, can get pretty chilly after sunset requiring a light
jacket. In winter months it is much colder, which
means there are sometimes only a handful of people
viewing.
However, in the summer there can be more than
150 people enjoying the dark skies, which was the
case when I took the VC200L out for its paces. And
the skies were dark this night, offering excellent view-
ing conditions. It took me a couple of hours to get set
up, and then for the next six hours I was entranced
with using the scope. I have to say, having the com-
plete package with the Sphinx Mount and STAR-
BOOK S, which incorporates Vixen’s GOTO con-
troller with a built in star chart that shows you exact-
ly where the telescope is pointing and displays “what’s
up” right now, just makes constellation surfing so
easy and I was able to explore so much more of the
sky than I was used to!
That night I shot over 200 short exposures until
finally knocking off. I broke everything down and
headed home to process the images using the Maxim
DL imaging processing software.
I have to say I love my Meade DSI Pro camera
and LX75SN , but the Vixen package was definitely
a joy to use and I would not mind seeing one appear
in my stocking on Christmas day!
VIXEN VC 200L
44 Astronomy TECHNOLOGY TODAY
M3
The images of M3, M13 and M27 were
taken using the VC200L, Sphinx Mount
and a Canon 350D DSLR. Each of the 180
second exposures were unguided,
re ying so e y on accuracy of my initia
a ignment and the subsequent tracking of
the Sphinx Mount.
M27
M13