15
Note About the Collimatable 2" Focuser
(XT8, XT10 only)
The 2" focuser of the SkyQuest XT8 and XT10 can be colli-
mated using three pairs of push-pull screws located at the
base of the focuser (Figure 13). The focuser was collimated
at the factory however, and should never need to be adjusted.
Focuser collimation is only required under very rare circum-
stances but has been made available for this telescope
should such a need arise.
5. Astronomical Observing
SkyQuest IntelliScope Dobsonians provide prodigious capa-
bility for observing the many wonders of the heavens, from
the major planets to deep-space nebulas and galaxies. In this
section we give you some observing tips and briefly summa-
rize what you can expect to see.
A. Selecting an Observing Site
Since most astronomical objects are faint, observing them
from dark skies will give you the best views. While some
objects, such as the planets and Moon, are bright enough to
see clearly even from light-polluted city skies, for nebulas,
galaxies, and most star clusters, the less ambient light there
is to reduce contrast, the better.
When it isn’t possible or convenient to get out of town to a
pitch-dark observing location, try to set up in a spot that is
removed from street and building lights and that has a clear
view of a large portion of the sky. For observing faint deep-sky
objects, choose a Moonless night. Use of a light-pollution fil-
ter can mitigate the effects of background sky brightness,
enhancing the view of faint objects.
B. Seeing and Transparency
Atmospheric conditions play a huge part in quality of viewing.
Light from stars and other celestial objects must travel
through miles of Earth’s atmosphere to reach our eyes. The
air in the atmosphere will refract and bend the light.
Atmospheric turbulence will worsen the effects of refraction,
which can cause the image you see in your telescope to be
unstable. The steadiness of the atmosphere is called “seeing.”
In conditions of good “seeing,” star twinkling is minimal and
objects appear steady in the eyepiece. Seeing is best over-
head, worst at the horizon. Also, seeing generally gets better
later in the evening as much of the heat absorbed by the
Earth during the day has radiated off into space. In conditions
of bad seeing, stars will twinkle and objects will appear
unsteady and blurry in the telescope.
“Transparency” is the clarity of the atmosphere, which can be
adversely affected by the presence of moisture, smoke, and
dust. All tend to scatter light, which reduces an object’s bright-
ness. Good transparency is desirable for astronomical
observing, especially for viewing faint objects.
One good measure of transparency is by how many stars you
can see with your unaided eyes. If you cannot see stars of
magnitude 3.5 or dimmer then transparency is poor.
Magnitude is a measure of how bright a star is. The brighter a
star, the lower its magnitude. A good star to remember for this
is Megrez (magnitude 3.4), which is the star in the Big Dipper
that connects the handle to the “dipper.” If you cannot see
Megrez, then you have fog, haze, clouds, smog, light pollution
or other conditions that are hindering your viewing (see
Figure 25).
C. Cooling the Telescope
All optical instruments need time to reach “thermal equilibri-
um” to achieve maximum stability of the lenses and mirrors,
which is essential for peak performance. Images will be
unstable if the optics are not in equilibrium with the outdoor
temperature. When moved from a warm indoor location out-
side to cooler air (or vice-versa), a telescope needs time to
cool to the outdoor temperature. The bigger the instrument
and the larger the temperature change, the more time will be
needed.
Allow at least 30 minutes for your SkyQuest IntelliScope to
equilibrate. If the temperature difference between indoors and
outdoors is more than 40°, allow an hour or more. In the win-
ter, storing the telescope outdoors in a shed or garage greatly
reduces the amount of time needed for the optics to stabilize.
It also is a good idea to keep the scope covered until the Sun
sets so the tube does not heat greatly above the temperature
of the outside air.
SkyQuest XT8 and XT10 models are designed to accept an
optional Orion Cooling Accelerator Fan (#7814). When
attached to the rear cell of the telescope, the fan hastens the
equilibration of the primary mirror to ambient temperature.
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
2.4
1.7
3.4
2.4
4.9
1.9
1.9
2.5
Figure 25.
Megrez connects the Big Dipper’s handle to it's “pan”.
It is a good guide to judging the “seeing” conditions. If you cannot
see Megrez (a 3.4-magnitude star) then seeing is poor.
