Orion 9786 Users Manual
2015-02-05
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INSTRUCTION MANUAL
IN 319 Rev. A 09/07
Providing Exceptional Consumer Optical Products Since 1975
Customer Support (800)-676-1343
E-mail: support@telescope.com
Corporate Offices (831)-763-7000
89 Hangar Way, Watsonville, CA 95076
Orion® 6" Newtonian
Imaging Reflector
#9786
2
Figure 1. The 6" Newtonian Imaging Reflector.
Focuser
Focus
wheel
Primary mirror cell
Secondary
mirror holder
Fine focus
wheel
Dovetail holder
Focuser
thumbscrew
Drawtube
extension
thumbscrew
Focus
wheel
Focus lock
thumbscrew
3
Congratulations on your purchase of an Orion 6"
Newtonian Imaging Reflector.
Your 6" Newtonian Imaging Reflector is a Newtonian reflec-
tor telescope with high quality optics and excellent mechani-
cal construction. It has been specially optimized for use with
astronomical CCD imaging cameras. These instructions will
help you set up and use your telescope.
Getting Started
The 6" Newtonian Imaging Reflector comes nearly fully
assembled from the factory. The telescope’s optics have been
installed and collimated, so you should not have to make any
adjustments to them.
Please keep the original shipping box! In the unlikely event
you should need to ship the telescope back to Orion for war-
ranty repair service, you should use the original packaging.
The box also makes a very good container for storing the tele-
scope when it is not in use.
Attaching the 6" Newtonian Imaging Reflector to
a Mount
The 6" Newtonian Imaging Reflector can be attached to a
mount by the use of optional tube rings. Tube rings with an
inner diameter of 182mm (7.16"), such as Orion item #7375,
are needed. First attach the tube rings to your telescope
mount, then place the optical tube in the tube rings.
Use of Optional Finder Scope and Eyepieces
The 6" Newtonian Imaging Reflector OTA does not come with
a finder scope or eyepieces in order to grant the user the great-
est versatility in customizing the instrument to suit their tastes.
However, certain rules for using accessories still apply.
To connect a finder scope, simply unthread the thumbscrew
on the dovetail holder (Figure 1), and insert the base of the
finder scope bracket. Retighten the thumbscrew to secure the
finder scope and bracket in place. Finder scopes that do not
use a dovetail bracket will need to be attached by some other
means.
Almost any 1.25" or 2" eyepiece can be used with the 6" New-
tonian Imaging Reflector.
To use 2" eyepieces, you will need to remove the 1.25" eye-
piece adapter by loosening the drawtube thumbscrew by a
few turns and lifting the adapter out of the focuser. Place your
2" eyepiece in the focuser drawtube and secure it in place
with the thumbscrew.
In order to use a 1.25" eyepiece in the focuser, the 1.25" eye-
piece adapter is needed. Place this adapter into the drawtube
like a 2" eyepiece, and loosely secure it with the thumbscrew.
Insert a 1.25" eyepiece into the adapter, and secure the eye-
piece by further tightening the thumbscrew. Tightening the
thumbscrew compresses the 1.25" eyepiece adapter, which
in turn secures and precisely centers the 1.25" eyepiece.
The Dual-Speed Low-Profile Crayford Focuser
The 6" Newtonian Imaging Reflector comes equipped with a
high-quality dual-speed low-profile Crayford focuser. Crayford
focusers generally perform better than rack-and-pinion mod-
els because the design eliminates “focus shift.” Focus shift
occurs when an image changes position in the eyepiece dur-
ing focusing. The Crayford design provides constant tension
via four “roller bearings” and the focus shaft, so the drawtube
cannot move perpendicular to the desired motion.
The Crayford focuser provides a minimum focus height of
43mm, which is excellent for imaging applications that require
extra in-travel. The focuser also features a built-in extendable
drawtube which adds up to 44mm of travel yielding a total
focus range of 68mm. Extension of this drawtube is required
to achieve focus in an eyepiece with the telescope. To extend
the drawtube, loosen the drawtube extension thumbscrew
(Figure 1) and gently pull the drawtube upwards to the pre-
ferred position. Tighten the drawtube extension thumbscrew
to lock the extension in place. The extendable drawtube is a
welcome feature when switching between an eyepiece and
imager, as no external extension tubes are required.
Dual-Speed Focus Adjustments
The focuser features dual speed adjustment with the fine
focus wheel. This small black knob located on the side of the
right-hand focus wheel allows precise focus adjustment at a
ratio of 11:1, meaning eleven turns of the fine focus wheel
equals one turn of the focus wheel.
Use the focus wheels to achieve rough focus on your target
object, then use the fine focus knob to coax out even more
detail. You’ll be amazed at the amount of detail the fine focus
knob allows you to view on targets such as the lunar surface,
planets, double stars, as well as other celestial objects.
If you find that the focus wheels are too tight or too loose, you
can make adjustments to the drawtube tension by using the
drawtube tension adjustment set screw located on the bottom
of the focuser, between the focus wheels. Make adjustments
to this set screw with the provided 2.5mm hex key until the
focuser motion feels comfortable. Please note that you must
have at least some tension applied to the focuser drawtube or
else it will not move when you turn the focus wheels.
Once you have achieved focus, you can lock the focuser in
place by tightening the focus lock thumbscrew located between
on the bottom of the focuser between the focus wheels (Figure
1). Locking the focuser in place can be especially useful for
imaging applications. Be sure to loosen the focus lock thumb-
screw before making additional focus adjustments.
The focuser can be rotated, should the need arise. This
requires a 1.5mm hex key (not included). To reposition the
focuser, loosen the 4 small socket-head set-screws that are
located within the base. Rotate the focuser to the preferred
position and carefully tighten the four set screws with the
1.5mm hex key. Be sure to keep the focuser flat against the
base to ensure proper alignment.
Calculating Magnification (Power)
It is desirable to have a range of eyepieces of different focal
lengths to allow viewing over a range of magnifications. To
calculate the magnification, or power, of a telescope, simply
4
divide the focal length of the telescope by the focal length of
the eyepiece:
Telescope Focal Length (mm)
= Magnification
Eyepiece Focal Length (mm)
For example, the 6" Newtonian Imaging Reflector, which has
a focal length of 750mm, used in combination with a 25mm
eyepiece, yields a magnification of
750 mm
= 30x
25 mm
Every telescope has a useful limit of power of about 45x-60x
per inch of aperture. Claims of higher power by some tele-
scope manufacturers are a misleading advertising gimmick
and should be dismissed. Keep in mind that at higher pow-
ers, an image will always be dimmer and less sharp (this is
a fundamental law of optics). The steadiness of the air (the
“seeing”) will usually limit how much magnification an image
can tolerate.
Always start viewing with your lowest-power (longest focal
length) eyepiece in the telescope. After you have located and
observed the object with it, you can try switching to a higher-
power eyepiece to ferret out more detail, if atmospheric con-
ditions permit. If the image you see is not crisp and steady,
reduce the magnification by switching to a longer-focal-length
eyepiece. As a general rule, a small but well-resolved image
will show more detail and provide a more enjoyable view than
a dim and fuzzy, over-magnified image.
Astroimaging with the 6" Newtonian
Imaging Reflector
The 6" Newtonian Imaging Reflector has been specifically
designed for use with astronomical CCD imaging cameras
like the Orion StarShoot, but other imaging systems such as
digital SLR cameras will also work well with the telescope.
The secondary mirror of the 6" Newtonian Imaging Reflector
has been sized appropriately to provide a fully illuminated
field of view for Orion StarShoot cameras and most popular
digital SLR models.
Unlike most Newtonian reflector designs, the 6" Imaging
Reflector's secondary mirror has been recessed further into
the tube to prevent off-axis glare from being detected by imag-
ing devices. Glare can contaminate night-sky images by reduc-
ing image contrast and giving the object a “soft” appearance.
To use your CCD camera with the 6" Newtonian Imaging
Reflector, the camera must have a 1.25 inch “nosepiece”.
Otherwise an external camera adapter with T-threads is
required. All Orion StarShoot cameras feature this nosepiece
(Figure 2). Insert the nosepiece equipped camera into the
focuser just like an 1.25" eyepiece.
If your camera does not include a 1.25" nosepiece, you have
a digital SLR, or if you wish to utilize a secure T-thread con-
nection with a CCD camera like the Orion StarShoot, a zero-
profile camera adapter is required (available from Orion). The
zero-profile adapter is inserted into the focuser just like a 2"
eyepiece and provides T-threads for attachment of digital SLR
T-rings or T-threaded CCD cameras.
To attach a digital SLR to the telescope, remove any attached
lenses and connect a model-specific T-ring to the camera
body. Thread the T-ring onto the zero-profile adapter to com-
plete attachment. To securely attach a CCD imaging cam-
era like the Orion StarShoot via T-threads, remove the 1.25"
nosepiece and thread the CCD camera onto the zero-profile
camera adapter to complete attachment.
Due to its imaging-optimized design, no external extension
tubes are required to appropriately couple the telescope to an
imaging camera.
To record an image of a night-sky object, you will need to first
acquire and center the object with an eyepiece. You may need
to extend the focuser’s built-in extension tube to achieve focus
with an eyepiece. Once you have centered the target object
in the eyepiece field of view, remove the eyepiece and insert
your CCD camera into the telescope’s focuser (don’t forget
to retract the built-in extension tube if it has been extended).
Secure the camera with the thumbscrew on the focuser. Use
the focus and fine-focus wheels to bring the image into focus.
Collimating the Optics
Collimating is the process of adjusting the mirrors so they are
aligned with one another. Your telescope’s optics were aligned
at the factory, and should not need much adjustment unless
the telescope is handled roughly. Accurate mirror alignment is
important to ensure peak performance of your telescope, so it
should be checked regularly. Collimating is relatively easy to
do and can be done in daylight.
To check optical alignment, remove the eyepiece and look
down the focuser drawtube. You should see the secondary
mirror centered in the drawtube, as well as the reflection of
the primary mirror centered in the secondary mirror, and the
reflection of the secondary mirror (and your eye) centered in
the reflection of the primary mirror, as in Figure 3a. If anything
is off-center, proceed with the following collimating procedure.
The Collimating Cap and Primary Mirror Center Mark
Your 6" Newtonian Imaging Reflector comes with a collimat-
ing cap. This is a simple cap that fits on the focuser drawtube
like a dust cap, but has a hole in the center and a silver bot-
Figure 2. To use a CCD camera with the 6" Imaging OTA, the
camera must have a 1.25” nosepiece, like the Orion StarShoot
Imaging cameras, or else an external camera adapter with
T-threads is required.
1.25" nosepiece
5
tom. This helps center your eye so collimating is easy to per-
form. Figures 3b through 3e assume you have the collimating
cap in place.
In addition to the collimating cap, you’ll notice a small ring
label on the exact center of the primary mirror. This “center
mark” allows you to achieve a very precise alignment of the
primary mirror; you don’t have to guess where the center of
the mirror is. You simply adjust the primary mirror position
(described below) until the reflection of the hole in the col-
limating cap is centered inside the ring.
Note: The center ring sticker need not ever be removed from
the primary mirror. Because it lies directly in the shadow of
the secondary mirror, its presence in no way adversely affects
the optical performance of the telescope or the image quality.
That might seem counter-intuitive, but it’s true!
Aligning the Secondary Mirror
It helps to adjust the secondary mirror in a brightly lit room with
the telescope pointed toward a bright surface, such as white
paper or wall. Placing a piece of white paper in the telescope
tube opposite the focuser (i.e. behind the secondary mirror)
will also be helpful in collimating the secondary mirror.
With the collimating cap in place, look through the hole in the
cap at the secondary (diagonal) mirror. Ignore the reflections
for the time being. The secondary mirror itself should be cen-
tered in the focuser drawtube. If it isn’t, as in Figure 3b, it must
be adjusted. Typically, this adjustment will rarely, if ever, need
to be done.
Note: When make adjustments to the secondary mirror position,
be careful not to stress the spider vanes, or they may bend.
To adjust the secondary mirror left-to-right in the focuser
drawtube, use the included 2.5mm hex key to loosen the three
small alignment setscrews in the center hub of the 4-vaned
spider several turns. Now hold the mirror holder stationary
(be careful not to touch the surface of the mirror), while turn-
ing the center screw with a Phillips head screwdriver (Figure
4). Turning the screw clockwise will move the secondary mir-
ror toward the front opening of the optical tube, while turning
the screw counter-clockwise will move the secondary mirror
toward the primary mirror. When the secondary mirror is cen-
tered left-to-right in the focuser drawtube, rotate the second-
Figure 3. Collimating the optics. (a) When the mirrors are properly aligned, the view down the focuser drawtube should look
like this. (b) With the collimation cap in place, if the optics are out of alignment, the view might look something like this. (c)
Here, the secondary mirror is centered under the focuser, but it needs to be adjusted (tilted) so that the entire primary mirror
is visible. (d) The secondary mirror is correctly aligned, but the primary mirror still needs adjustment. When the primary mirror
is correctly aligned, the “dot” will be centered, as in (e).
drawtube
Reflection
of primary
mirror clip
a.
Primary mirror
center mark
Reflective surface
of collimation
cap
b. c.
d. e.
Figure 4. To center the secondary mirror under the focuser, hold
the secondary mirror holder in place with your fingers while adjusting
the center screw with the Phillips head screwdriver. Do not touch the
mirror’s surface.
Phillips head
screwdriver
6
ary mirror holder until the reflection of the primary mirror is as
centered in the secondary mirror as possible. It may not be
perfectly centered, but that is OK for now. Tighten the three
small alignment setscrews equally to secure the secondary
mirror in that position.
To adjust the secondary mirror up-and-down in the focuser
drawtube, adjust the length of the two spider vanes perpen-
dicular to the focuser. This is done by tightening the knurled
thumbnuts that secure the vanes to the tube (Figure 5).
Loosen one thumbnut, then tighten the other until the second-
ary mirror is centered in the drawtube.
The secondary mirror should now be centered in the focuser
drawtube. Now we will shift our attention to the reflections
within the secondary mirror.
If the entire primary mirror reflection is not visible in the sec-
ondary mirror, as in Figure 3c, you will need to adjust the tilt
of the secondary mirror. This is done by alternately loosen-
ing one of the three alignment setscrews while tightening the
other two, as depicted in Figure 6. You will need a 2mm hex
key to do this. The goal is to center the primary mirror reflec-
tion in the secondary mirror, as in Figure 3d. Don’t worry that
the reflection of the secondary mirror within the primary mirror
reflection (the smallest circle, with the collimation cap “dot” in
the center) is off-center. You will fix that in the next step.
Once the secondary mirror is centered in the focuser draw-
tube, and the primary mirror reflection is centered in the sec-
ondary mirror, the secondary mirror is properly aligned, and
no further adjustments to it should be needed.
Aligning the Primary Mirror
The final adjustment is made to the primary mirror. It will need
adjustment if, as in Figure 3d, the secondary mirror is cen-
tered in the focuser drawtube and the reflection of the pri-
mary mirror is centered in the secondary mirror, but the small
reflection of the secondary mirror (with the “dot” of the col-
limating cap) is off-center.
The tilt of the primary mirror is adjusted with the three large
knurled thumbscrews on the rear end of the optical tube (back
of the mirror cell) (Figure 7). The small thumbscrews (with
slots in them) serve to lock the mirror in place. Start by loos-
ening each of these smaller thumbscrews a few turns. Use a
screwdriver in the slots, if necessary. Now adjust the tilt of the
primary mirror by turning one of the large thumbscrews either
clockwise or counterclockwise. Look into the focuser and see
if the secondary mirror reflection has moved closer to the
center of the primary mirror reflection. You can determine this
easily with the collimating cap and primary mirror center mark
by simply watching to see if the “dot” of the collimating cap is
moving closer or farther away from the “ring” on the primary
mirror. If it isn’t getting closer, try turning the thumbscrew in
the opposite direction. Repeat this process for the other two
large thumbscrews, if necessary. It will take a little trial-and-
error to get the feel for how to adjust the primary mirror to
center the dot of the collimating cap in the ring of the primary
mirror center mark.
When you have the dot centered as much as possible in the
ring, your primary mirror is aligned. The view through the colli-
mating cap should resemble Figure 3e. Make sure the smaller
thumbscrews on the back of the mirror cell are tightened to
lock the primary mirror in position.
Figure 7. The tilt of the primary mirror is adjusted by turning the
three larger thumbscrews.
Figure 5. To center the secondary mirror up-and-down in the
focuser drawtube, make adjustments to the two knurled spider vane
thumbnuts that are perpendicular to the focuser.
Spider vane
thumbnuts
Figure 6. Adjust the tilt of the secondary mirror by loosening one
of the three alignment set screws then tightening the other two.
Alignment set
screws (3)
7
Figure 8. A star test will determine if the telescope's optics are
properly collimated. A defocused view of a bright star through the
eyepiece should appear as illustrated on the right if optics are per-
fectly collimated. If the circle is unsymmetrical, as illustrated on the
left, the scope needs alignment.
Out of collimation Collimated
A simple star test will tell you whether the optics are, in fact,
accurately aligned.
Star-Testing the Telescope
When it is dark, point the telescope at a bright star and accu-
rately center it in the eyepiece’s field of view. Slowly de-focus
the image with the focus knob. If the telescope’s optics are
correctly aligned, the expanding disk should be a perfect cir-
cle (Figure 8). If the image is unsymmetrical, the optics are
out of alignment. The dark shadow cast by the secondary mir-
ror should appear in the very center of the out-of-focus circle,
like the hole in a donut. If the “hole” appears off-center, the
optics are out of alignment.
If you try the star test and the bright star you have selected
is not accurately centered in the eyepiece, the telescope will
appear to need optical alignment, even though the optics may
be perfectly collimated. It is critical to keep the star centered,
so over time you will need to make slight corrections to the
telescope’s position in order to account for the sky’s apparent
motion.
Care & Maintenance
If you give your telescope reasonable care, it will last a life-
time. Store it in a clean, dry, dust-free place, safe from rapid
changes in temperature and humidity. Do not store the tele-
scope outdoors, although storage in a garage or shed is OK.
Small components like eyepieces and other accessories
should be kept in a protective box or storage case. Keep the
dust cover on the front of the telescope and the dust cap on
the focuser drawtube when it is not in use.
Your telescope requires very little mechanical maintenance.
The optical tube has a smooth painted finish that is fairly
scratch-resistant. If a scratch does appear on the tube, it will
not harm the telescope. If you wish, you may apply some auto
touch-up paint to the scratch. Smudges on the tube can be
wiped off with a soft cloth and household cleaning fluid.
Cleaning Mirrors
You should not have to clean the telescope’s mirrors very
often; normally once every year or so is fine. Covering the
front opening of the telescope with the dust cover when it is
not in use will prevent dust from accumulating on the mirrors.
Keeping the dust cap on the focuser’s 1.25" opening is also a
good idea. Improper cleaning can scratch the mirror coatings,
so the fewer times you have to clean the mirrors, the better.
Small specks of dust or flecks of paint have virtually no effect
on the visual performance of the telescope.
The large primary mirror and the elliptical secondary mirror of
your telescope are front-surface aluminized and over-coated
with hard silicon dioxide, which prevents the aluminum from
oxidizing. These coatings normally last through many years of
use before requiring re-coating.
To clean the secondary mirror, first remove it from the tele-
scope. Do this by keeping the secondary mirror holder sta-
tionary while completely unthreading the Phillips-head screw
in the center hub of the spider vane assembly (see Figure 4).
Do not touch the mirror surface when doing this. Be careful,
there is a spring between the secondary mirror holder and
the Phillips head screw; be sure it does not fall into the opti-
cal tube and onto the primary mirror. Once the Phillips-head
screw is unthreaded, the secondary mirror and its holder can
be removed from the telescope. Then follow the same pro-
cedure described below for cleaning the primary mirror. The
secondary mirror does not need to be removed from its holder
for cleaning.
To clean the primary mirror, first carefully remove the mirror
cell from the telescope. For the 6" Imaging Reflector, you must
completely unthread the four screws on the exterior perimeter
of the mirror cell (Figure 9). Then pull the cell away from the
tube. You will notice the primary mirror is held in the mirror cell
with three clips held by two screws each. Loosen the screws
and remove the clips.
You may now remove the primary mirror from its cell. Do not
touch the surface of the mirror with your fingers. Lift the mirror
carefully by the edges. Set the mirror on a clean soft towel. Fill
a clean sink free with room temperature water, a few drops
of liquid dishwashing detergent, and if possible, a capfull of
Figure 9. To remove the mirror cell from the telescope, the four
small Phillips-head screws on the perimeter of the mirror cell must
be completely unthreaded.
Small Phillips-head screws (4)
8
One-Year Limited Warranty
This Orion 6" Newtonian Imaging Reflector is warranted against defects in materials or workmanship for
a period of one year from the date of purchase. This warranty is for the benefit of the original retail pur-
chaser only. During this warranty period Orion Telescopes & Binoculars will repair or replace, at Orion’s
option, any warranted instrument that proves to be defective, provided it is returned postage paid to:
Orion Warranty Repair, 89 Hangar Way, Watsonville, CA 95076. If the product is not registered, proof of
purchase (such as a copy of the original invoice) is required.
This warranty does not apply if, in Orion’s judgment, the instrument has been abused, mishandled, or
modified, nor does it apply to normal wear and tear. This warranty gives you specific legal rights, and
you may also have other rights, which vary from state to state. For further warranty service information,
contact: Customer Service Department, Orion Telescopes & Binoculars, 89 Hangar Way, Watsonville, CA
95076; (800)-676-1343.
Orion Telescopes & Binoculars
89 Hangar Way, Watsonville, CA 95076
Customer Support Help Line (800)‑676‑1343 • Day or Evening
100% isopropyl alcohol. Submerge the mirror (aluminized
face up) in the water and let it soak for a few minutes (or hours
if it’s a very dirty mirror). Wipe the mirror under water with
clean cotton balls, using extremely light pressure and strok-
ing in straight lines across the mirror surface. Use one ball
for each wipe across the mirror. Then rinse the mirror under
a stream of lukewarm water. Any particles on the surface can
be swabbed gently with a series of cotton balls, each used
just one time. Dry the mirror surface with a stream of air (a
“blower bulb” works great). Cover the mirror surface with tis-
sue, and leave the mirror in a warm area until it is completely
dry before replacing it in the mirror cell and telescope.
Specifications
Optical tube: Steel
Primary mirror: Parabolic, center marked
Collimation adjustment: Three spring-loaded thumbnuts
to adjust mirror tilt, one thumbnut
in-line with focuser, three thumb-
screws to lock mirror position
Aperture: 6" (150mm)
Focal length: 750mm
Focal ratio: f/5.0
Minor axis of
secondary mirror: 2.28" (58.0mm)
Secondary mirror offset: 2.9mm away from focuser and
2.9mm towards primary mirror
Mirror coatings: Aluminum with silicon dioxide
(SiO2) overcoat
Focuser: Crayford, accepts 2" accessories,
dual-speed focus adjustment,
rotatable, focus-lock equipped
Minimum focus height: 43mm
Focus travel: 24mm, 68mm with 2" drawtube
extended
1.25" adapter: Included, compression-fit design
Weight: 10.5 lbs.
Length: 30.5"