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covered until the Sun sets so the tube does not heat greatly
above the temperature of the outside air.

The SkyQuest XT10 has the ability to mount a small fan to
make cooling the tube faster. On the bottom of the mirror cell
there are four threaded holes (M4-.7) where a fan can be
attached. Orion sells a fan  for the SkyQuest XT10; consult
the catalog or website for details.

D. Let Your Eyes Dark-Adapt

Do not expect to go from a lighted house into the darkness of
the outdoors at night and immediately see faint nebulas,
galaxies, and star clusters - or even very many stars, for that
matter. Your eyes take about 30 minutes to reach perhaps
80% of their full dark-adapted sensitivity. Many observers
notice improvements after several hours of total darkness. As
your eyes become dark-adapted, more stars will glimmer into
view and you will be able to see fainter details in objects you
view in your telescope. Exposing your eyes to very bright day-
light for extended periods of time can adversely affect your
night vision for days. So give yourself at least a little while to
get used to the dark before you begin observing.

To see what you are doing in the darkness, use a red-filtered
flashlight rather than a white light. Red light does not spoil
your eyes’ dark adaptation like white light does. A flashlight
with a red LED light is ideal, or you can cover the front of a
regular incandescent flashlight with red cellophane or paper.
Beware, too, that nearby porch and streetlights and automo-
bile headlights will spoil your night vision.

Tracking Celestial Objects

The Earth is constantly rotating about its polar axis, complet-
ing one full rotation every 24 hours; this is what defines a
“day”. We do not feel the Earth rotating, but we can tell that it
is at night by seeing the apparent movement of stars from
east to west. This movement translates into a rate of approxi-
mately .25° per minute, or 15 arc-seconds per second. (There
are 60 arc-minutes in 1°, and 60 arc-seconds in one arc-
minute.) This is called the sidereal rate.

When you observe any astronomical object, you are watching
a moving target. This means the telescope’s position must be
slowly updated over time to keep an object in the field of view.
To keep the object in the telescope’s field of view (to “track”
it), the telescope must be moved by small increments every
now and then, in the direction the object is moving. This is
easy to do with a SkyQuest XT10 Dobsonian because of its
buttery smooth motion on both axes. As the object moves off
toward the edge of the field of view, you just lightly nudge the
telescope to bring it back to the center.

You will notice that it is more difficult to track objects when the
telescope tube is aimed nearly straight up. This is inherent to
the basic design of the Dobsonian, and stems from the fact
that there is very little leverage to move in azimuth when the
tube is in a near-vertical position. To gain more leverage, try
grasping the tube close to the altitude side bearings with both
hands. Also, when looking overhead, if the telescope cannot
be moved any more in altitude, rotate the telescope 180° in
azimuth to continue motion.

Remember that objects appear to move across the field of
view faster at higher magnifications. This is because the field
of view becomes narrower.

Eyepiece Selection

By using eyepieces of varying focal lengths, it is possible to
attain many magnifications with the SkyQuest XT10
Dobsonian. The telescopes come with two high-quality
SiriusPlössl eyepieces: a 25mm, which gives a magnification
of 48x, and a 10mm, which gives a magnification of 120x.
Other eyepieces can be used to achieve higher or lower pow-
ers. It is quite common for an observer to own five or more
eyepieces to access a wide range of magnifications. This
allows the observer to choose the best eyepiece to use
depending on the object being viewed. At least to begin with,
the two supplied eyepieces will suffice nicely.

Whatever you choose to view, always start by inserting your
lowest power (longest focal length) eyepiece to locate and
center the object. Low magnification yields a wide field of
view, which shows a larger area of sky in the eyepiece. This
makes acquiring and centering an object much easier. If you
try to find and center objects with high power (narrow field of
view), it’s like trying to find a needle in a haystack!

Once you’ve centered the object in the eyepiece, you can
switch to higher magnification (shorter focal length eyepiece),
if you wish. This is especially recommended for small and
bright objects, like planets and double stars. The Moon also
takes higher magnifications well.

Deep-sky objects, however, typically look better at medium or
low magnifications. This is because many of them are quite
faint, yet have some extent (apparent width). Deep-sky
objects will often disappear at higher magnifications, since
greater magnification inherently yields dimmer images. This
is not the case for all deep-sky objects, however. Many galax-
ies are quite small, yet are somewhat bright, so higher power
may show more detail.

The best rule of thumb with eyepiece selection is to start with
a low power, wide field, and then work your way up in magni-
fication. If the object looks better, try an even higher
magnification. If the object looks worse, then back off the
magnification a little by using a lower power eyepiece.

Use of 2" Eyepieces

The SkyQuest XT10 comes with a large format focuser
(Figure 9) as standard equipment. Because of its large size, it
is able to accept eyepieces that have a 2" barrel diameter. 2"
eyepieces are desirable because they allow for a wider field
of view than 1.25" eyepieces. Many observers own at least
one 2" eyepiece to yield the largest field of view possible for
looking at wide deep sky objects, such as open star clusters
and gaseous nebulae. 2" eyepieces can also give nice views
of the Moon.

To use a 2" eyepiece, simply remove the 1.25" eyepiece
adapter from the end of the focuser drawtube. You must first
loosen the two thumb screws on the 2" eyepiece adapter to
do this. Now, insert a 2" eyepiece into the focuser, and secure
it with the two thumb screws. Focus the eyepiece as
described previously.

Summary of Contents for SkyQuest XT10 9810

Page 1: ...nal Consumer Optical Products Since 1975 Customer Support 800 676 1343 E mail support telescope com Corporate Offices 831 763 7000 P O Box 1815 Santa Cruz CA 95061 INSTRUCTION MANUAL Orion SkyQuest XT10 9810 Dobsonian Reflecting Telescope ...

Page 2: ... side panel Front brace Handle Top baseplate Ground baseplate Finder scope Finder scope bracket Eyepiece Focus knob Optical tube Altitude side bearing CorrecTension XT Friction Optimization system Eyepiece rack Primary mirror cell Left side panel Figure 1 The SkyQuest XT10 Foot 3 ...

Page 3: ...s in the Parts List below are present Be sure to check boxes carefully as some parts are small If any thing appears to be missing or broken immediately call Orion Customer Support 800 676 1343 or email sales tele scope com for assistance Parts List Box 1 Optical Tube Assembly and Accessories Qty Description 1 Optical tube assembly 1 Dust cover 1 25mm Sirius Plössl eyepiece 1 10mm Sirius Plössl eye...

Page 4: ...ace of the top baseplate 6 Insert the T nut K into the center hole of the ground baseplate A so the nut s flanged top is on the same side of the baseplate as the Teflon pads Thread the large hex head screw G with a 3 8 washer F attached up through the ground baseplate and through the T nut until it is tight Now position the top baseplate D with side pan els attached over the ground baseplate and l...

Page 5: ...ng new feature of the SkyQuest XT10 Dobsonian is the CorrecTension Friction Optimization system Because of their relatively light weight 10 and smaller Dobsonians have always been plagued by insufficient friction on the altitude bearing surfaces As a result such telescopes move up and down much too freely This causes problems when the observer tries to accurately center and track an object for vie...

Page 6: ...cope from the base you will first need to disconnect the springs from the posts on the Dobsonian base The springs will remain captive on the alti tude side bearings so they will not get lost Installing the Finder Scope SkyQuest XT10 Dobsonians come with a high quality large aperture 9x50 achromatic crosshair finder scope Figure 8a as standard equipment This greatly aids in finding objects to view ...

Page 7: ...t using a proper solar filter over the front aperture Altitude and Azimuth The Dobsonian base of the SkyQuest XT10 permits motion of the telescope along two axes altitude up down and azimuth left right see Figure 10 This is very convenient since up down and left right are the most natural ways that people aim As a result pointing the telescope is exceptionally easy Simply take hold of the navigati...

Page 8: ... located behind the objective lens cell on the body of the finder scope see Figure 8a Back the lock ring off by a few turns for now Refocus the finder scope on a distant object by threading the objective lens cell in or out on the finder scope body Precise focusing will be achieved by focusing the finder scope on a bright star Once the image appears sharp retighten the lock ring behind the objecti...

Page 9: ...ystems can be expensive and unwieldy The CorrecTension Friction Optimization system of the SkyQuest XT10 Dobsonian however solves the finicky bal ance problem The spring coils pull the tube down onto the base thereby increasing the friction on the altitude bearing pads With CorrecTension the added weight of small front end loads will not adversely affect the balance of the telescope If you install...

Page 10: ...rk it yourself 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 tele scope or the image quality That might seem counterintuitive but its true Aligning the Secondary Mirror With the collimation cap in place look through the hole in the c...

Page 11: ...n tered under the focuser and the reflection of the primary mirror is centered in the secondary mirror but the small reflection of the secondary mirror with the dot of the colli mation cap is off center The tilt of the primary mirror is adjusted with three spring loaded collimation thumbscrews on the back end of the optical tube bottom of the primary mirror cell these are the larger thumbscrews Th...

Page 12: ...uld not observe through an open window from indoors Better yet choose a site out of town away from any light pollution You ll be stunned at how many more stars you ll see Most importantly make sure that any chosen site has a clear view of a large portion of the sky B Seeing and Transparency Atmospheric conditions play a huge part in quality of viewing In conditions of good seeing star twinkling is...

Page 13: ...ide bearings with both hands Also when looking overhead if the telescope cannot be moved any more in altitude rotate the telescope 180 in azimuth to continue motion Remember that objects appear to move across the field of view faster at higher magnifications This is because the field of view becomes narrower Eyepiece Selection By using eyepieces of varying focal lengths it is possible to attain ma...

Page 14: ...faint stars The brightest is the moon Titan VENUS At its brightest Venus is the most luminous object in the sky excluding the Sun and the Moon It is so bright that sometimes it is visible to the naked eye during full daylight Ironically Venus appears as a thin crescent not a full disk when at its peak brightness Because it is so close to the Sun it never wanders too far from the morning or evening...

Page 15: ...hy SkyQuests have also been optically opti mized for visual use since photographic optimization degrades visual performance With that in mind however it is possible to do some simple astrophotography with a SkyQuest With the use of afocal photography techniques where the camera is simply placed to the eyepiece to take a picture and digital cameras it is possible to take pictures of bright objects ...

Page 16: ...nthread the mirror clip anchor screws Next hold the mirror by its edge and remove it from the mir ror cell Be careful not to touch the aluminized surface of the mirror with your fingers Set the mirror on a clean soft towel Fill a clean sink free of abrasive cleanser with room temper ature water a few drops of liquid dishwashing detergent and if possible a cap full of rubbing alcohol Submerge the m...

Page 17: ...17 ...

Page 18: ...r 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 F...

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