Citiwell OR2010 Quick start guide

60mm AZ
Telescope
Instructions
and
Owner’s Manual
Part # 260029

2
Some models can accept an optional vertical fine adjustment rod. This part has no effect on the
mechanical or optical performance of your telescope.
Components and colors may vary from those shown in the illustrations.
WARNING!
NEVER aim your telescope at the sun or even close to the sun!
Instant and irreversible damage can occur,
including blindness!
Do not let children use any telescope without adult supervision.
A. Accessory tray
B. Finder scope
C. Finder scope bracket
D. Diagonal mirror
E. 3X Barlow lens
F. Image erector
G. Eyepieces
H. Eyepiece cases
I. Yoke
J. Tripod support bracket
L. Screwdriver
M. Altitude control locking
knobs (2)
N. Tripod leg attachment bolts and
wing nuts (3)
O. Tripod leg adjustment knobs (3)
P. Optical tube assembly
Q. Dew shield
R. Tripod leg (3)
Parts of your 60mm AZ Telescope:

3
Introduction
Congratulations on your purchase of a new precision-crafted telescope. With proper
care and handling of your telescope, you will enjoy the pleasure of looking at nature’s
wondrous sights through the eye of this instrument for many years.
This telescope has been designed to provide views of the moon’s craters, Jupiter’s
major moons, and Saturn’s rings, in addition to dozens of galaxies, star clusters, and
nebulae.
As a terrestrial (land) telescope, your telescope delivers great views of mountains,
valleys, and many other features of the world around us. You can also use it to study
animals and landscapes at a distance. To obtain the best performance from your
telescope, please read this manual carefully and completely.
TO SEE ANY NEW REVISIONS TO THIS MANUAL, OR FOR
ANSWERS TO COMMON QUESTIONS, PLEASE VISIT OUR WEBSITE
AT:
www.citiwellint.com.

4
ASSEMBLY
1) Carefully remove all parts from the cardboard cartons and lay them on a table or
floor in order to take an inventory of all the pieces. Keep your box for storage or in
case you ever need to ship your telescope.
2) Extend the legs, and lock each one at the desired height with the supplied tripod
adjustment knob (See Fig. 1).
(Fig. 1)
3) Connect all three tripod legs to the yoke with the supplied tripod leg attachment
bolts, washers and wing nuts (See Fig. 2).
(Fig. 2)
Azimuth Locking Knob

5
4) Fasten the tripod support bracket to each leg using the included bolts and nuts that
come attached to the end of each arm of the tripod support bracket. Remove each
bolt and nut. (See Fig. 3). Then position one arm of the tripod support bracket so that
the holes at the end of the arm line up with the hole through the attachment point on
the tripod leg (See Fig. 4). Insert the bolt to attach the tripod support bracket to the
tripod leg and tighten the nut. Repeat this procedure with the other two legs.
(Fig. 3) (Fig. 4)
5) Fasten the accessory tray to the tripod support bracket by placing the tray’s bolt
into the threaded hole and turning the tray clockwise until tight (See Fig. 5).
(Fig. 5)

6
6) After all nuts and bolts have been firmly tightened the telescope optical tube
assembly can be attached to the yoke. Mount the optical tube assembly in the yoke as
shown in Fig. 6 and tighten the two altitude control locking knobs.
(Fig. 6)
7) Remove the finder scope (with attached bracket) from the box. Remove the two
knurled thumbscrews from the telescope main tube (See Fig. 7). Position the finder
scope bracket onto the telescope tube so that the holes in the base of the bracket
line up with the exposed holes in the telescope tube. Replace the two knurled
thumbscrews and tighten securely (See Fig. 8).
(Fig. 7) (Fig. 8)

7
8) Insert the diagonal mirror into the focusing tube (See Fig. 9). Secure by tightening
the small chrome set screw located on the focusing tube (See Fig. 10).
(Fig. 9) (Fig. 10)
9) Insert the 25 mm eyepiece into the diagonal mirror (See Fig. 11). Tighten the
small chrome set screw to hold the eyepiece securely in place (See Fig. 12).
(Fig. 11) (Fig. 12)

8
10) A 3x Barlow lens is supplied to triple the basic magnifying power provided by an
eyepiece. In viewing situations where very high magnifying powers are desired, insert
the 3x Barlow lens between the eyepiece and the focusing tube (See Fig. 13).
(Fig. 13)
FINDER SCOPE ALIGNMENT
Since a telescope has a narrow field of view by design, it can be challenging to locate a
particular star or planet. For this reason the telescope is fitted with a low-power, wide-
field miniature telescope called a finder scope. Always use your finder scope to locate
the object you want to view FIRST. The finder scope should be aligned with the
main telescope tube before you begin using the telescope, in order that both
scopes are positioned to always provide exactly the same angle and view.
Note: Objects in the finder scope are upside down. This is normal and is common to all
astronomical telescopes.
Complete the following settings in daylight:
1) Insert the 25 mm eyepiece into the diagonal mirror. Look at an easily recognizable,
stationary object that is at least 300 feet away. Slightly loosen the two altitude control
locking knobs and the azimuth locking knob (See Fig. 2 - Page 4). Turn the telescope
on both its horizontal and vertical axis until the object is in the center of the field of
view. Then bring the image into focus.
2) Firmly re-tighten the adjusting knobs so that the telescope is locked in position.
3) Look through the finder scope. If the object is not visible or centered in the finder
scope, simply release one of the three small adjusting screws holding the finder scope
and reposition the finder scope until the object is centered within the “X” cross hairs.
4) All screws should be completely tightened as soon as the view through the finder
scope coincides with the view of the main telescope.
5) You may need to repeat this procedure to ensure a perfect alignment.
THE ALTAZIMUTH MOUNT

9
This telescope is fitted with an Altazimuth mount. “Alt” refers “Altitude”, the vertical
movement of the telescope, while “Azimuth” refers to the horizontal movement.
ABOUT MAGNIFICATION
The magnification power of a telescope indicates how much an image is enlarged or
how big and close it appears to the viewer. The focal length of the eyepiece, combined
with the focal length of the telescope, determines the magnification power. To calculate
the power of your telescope with any particular eyepiece, simply divide the focal length
of the telescope (700 mm) by the focal length of the eyepiece (indicated in “mm” on the
eyepiece collar).
Example: 700 mm focal length (tube) = 56X magnification power
12.5 mm focal length (eyepiece)
The 3X Barlow lens and interchangeable eyepieces provide the following magnification
values:
Eyepiece Power Power with 3X Barlow Lens
25 mm 28X 84X
12.5 mm 56X 168X
4 mm 175X 525X
The level of magnification required depends on the object being observed. Optimal
performance is obtained if the magnification is typically not more than appromiately 30X
for every 10 mm of objective lens diameter. Magnification of around 175X or less is
ideal for a telescope with a 60 mm diameter objective lens and is best for observing
most celestial objects. A lower magnification power and a wider field of view are
advisable for observing galaxies and nebulae. The highest magnification power should
be used for highly detailed observations of the moon, Jupiter and Saturn or any object
that is quite bright.
The highest magnification power of the Barlow lens / 4mm eyepiece combination should
only be used for large or bright objects such as the moon and the brightest planets.
USING YOUR TELESCOPE FOR ASTRONOMICAL VIEWING
1) Take your telescope outside. Viewing objects through closed or open windows is not
recommended. Your view can be distorted by reflections in the glass of a closed
window or by air currents of differing temperatures passing through an open window.
2) Let your telescope adjust to the outside temperature. Your telescope will perform
much better if the lenses and the air inside the tube are the same temperature as
outside. It may take up to 30 minutes to equalize the temperatures when the
difference in temperatures is extreme.

10
3) Find a location far from glaring light. If you live in an urban area, your viewing will
probably improve the farther you move away from the city lights. The sky glow of a
town or city can dramatically reduce the telescope’s performance and viewing
capabilities.
4) Remove the large, round plastic dust cover from the front of your telescope.
5) We recommend starting your viewing with the 25 mm eyepiece because it gives you
the widest angle and brightest, sharpest views. To adjust the angle of the telescope,
loosen the azimuth lock knob by turning it counterclockwise (See Fig. 2 - Page 4).
You can then aim the telescope in the desired direction. Then tighten the tripod
locking knob.
When possible, avoid sudden temperature changes, as the moisture in the air will
condense on the objective lens. Should this occur after bringing your telescope inside,
leave the lens cap off the objective lens, tilt the objective (front) lens face down, and
allow the telescope to reach room temperature.
NOTE: When using the diagonal mirror, objects will appear right side up in your
telescope, but reversed, like a reflection in a mirror. This is normal, and does not
indicate a defect.
USING YOUR TELESCOPE FOR TERRESTRIAL VIEWING
You may notice that when you observe a terrestrial subject on land or water it appears
right side up, but is reversed — like looking in a mirror.
Use the 1.5X image erector, included with your telescope, to reorient the object. This
accessory is inserted in the eyepiece holder of the telescope between the eyepiece and
the telescope, in the same manner as the 3X Barlow lens (See Fig. 16).
(Fig. 16)
The image erector provides 1.5X magnification, which means that the 25 mm eyepiece
will magnify objects from 28X to 42X when used in conjunction with the image erector.
NOTE: Do not use the diagonal mirror or the 3X Barlow lens with this accessory.

11
CARE AND CLEANING OF OPTICS
Optical components of a telescope get dirty over time. Dirt or dust on a lens should be
removed with the utmost care. A considerable amount of dirt or dust would have to
accumulate on the optical surface before your view would be compromised.
1) Keeping dust caps on during storage and transport will reduce dust collection.
2) Condensation may collect on the optical surfaces when the telescope is not in use.
Remove the dust caps and allow the moisture to evaporate naturally. Point the
telescope downward to minimize the accumulation of airborne dust.
3) Once all moisture has evaporated, replace the dust caps.
4) Filtered, compressed air may be used to remove surface dust from lenses and
mirrors. Remove the dust cap and the dew shield. Once removed, point the can away
from the lens and gently expel some air and any condensation or dust that has
accumulated on the discharge tube. Spray the lens or mirror with short bursts of air to
carefully remove the dust particles. DO NOT HOLD THE TRIGGER OF THE
COMPRESSED AIR CAN FOR EXTENDED PERIODS BECAUSE PROPELLANT
FROM THE CAN MIGHT ESCAPE AND DAMAGE THE OPTICAL SURFACE.
If, after several attempts, you cannot remove the particles, take the telescope to an
optical professional for cleaning.
If you keep the dust caps on your telescope when it is not in use and avoid handling the
lenses or mirrors, only minimal optical maintenance of your telescope should be
required. Extensive cleaning is usually only necessary every few years.
WHAT TO LOOK FOR IN THE NIGHT SKY
There is a whole universe of objects you could view at night, so where do you start?
We recommend starting with the most prominent objects first.
The moon
The moon is the easiest target to find at night. When the moon is in full position, it
bathes the night with a silvery light that washes the sky of all but the brightest objects.
The best time to view the moon is not when it is full, but rather when it is less than half
full. The dividing line between dark and light on the moon, called the terminator, shows
the best detail in the craters and mountains.
The planets
The planets, our solar system companions, range in size from moon-size rocky bodies
to giant gas balls, which could hold Earth 1000 times over. To find the planets, you will
need information about their times of visibility. An astronomy magazine will give you the
locations of the planets as they change position from month to month. The Internet is
also an excellent source of information, offering starcharts, maps, and more!

12
The popular and more familiar constellations often provide the easiest landmarks to
help find the planet’s locations and paths of orbit. Most people have looked up at night
and seen some of the planets without even realizing it. A planet looks like a bright star
but does not twinkle like a star does; it looks like a tiny ball. Venus, Mars, Jupiter, and
Saturn are the easiest planets to view. Mercury is dimmer, usually below the horizon,
and more challenging to find.
Each of the planets provides interesting views. Venus is covered with clouds so all that
is visible is an extremely bright light, the brightest next to the moon. However, Venus,
like the moon, goes through phases. As it travels around the sun, different areas of its
surface are illuminated, producing crescent shapes of varying size. Mars is the red
planet. When it is above the horizon, it is noticeably red and stands out like a beacon in
the night sky. The apparent brightness of Mars varies as the planet orbits around the
sun and throughout its period of visiblity, it will brighten and dim depending on its
distance from Earth.
Jupiter is the largest planet in our solar system and the second brightest next to Venus.
Jupiter has many moons, four of which are often visible through your telescope when
viewing conditions permit. As you watch them throughout the evening, you will see that
they change position relative to each other and to Jupiter. It is possible with careful
planning to actually see one of the moons disappear either in front of or behind Jupiter
as it orbits around the planet. Another great feature of Jupiter is the cloud belt pattern.
Jupiter is alive with weather activity and its clouds have formed over time into belts
visible through telescopes in the right atmospheric conditions.
Saturn, the second largest planet, is not as bright as Jupiter and so its moons are not as
visible through small telescopes. The large rings that encircle Saturn are spectacular to
observe, however. The planet and its rings appear pale yellow. The major division in the
rings, the Cassini division, is possible to see if you keep the telescope firmly in position.
Uranus and Neptune are the last of the solar system gas giants. They do not provide as
spectacular a sight as Jupiter or Saturn, but are nonetheless rewarding to see.
Beyond our solar system, there are many more objects to be found. Galaxies, nebulae,
and star clusters abound!

13
FREQUENTLY ASKED QUESTIONS
1) How far can I see?
If you stand outside and look up at the night sky on a clear evening, you can see
hundreds of stars without the aid of your telescope. The telescope is a light-gathering
instrument that magnifies the view — providing significantly more detail and unveiling
more stars, nebulae, and celestial objects. With the aid of a telescope, you will be able
to enjoy exciting views of Saturn’s rings, Jupiter’s major moons, the Orion Nebula, and
much more.
2) Why can’t I see anything through my telescope?
If you see only gray or black when looking through your telescope, even after searching
for an object to view, it is very likely that you are using an eyepiece that is too powerful.
To solve this problem always start with the lowest power eyepiece first, and only insert
the higher power eyepiece after you have located an object.
3) When I use my high power eyepiece, everything looks much darker. Why?
As magnification in a telescope increases, brightness diminishes. Conversely,
brightness increases when magnification is reduced. If an image appears too dark or
unclear, use a lower-powered eyepiece. Views of small, bright objects are superior to
those of large, dark, or blurry ones! Atmospheric conditions, air currents, as well as light
and air pollution also affect viewing quality.
4) As I look through my telescope, objects in the sky appear to move. Why is
that?
The constant rotation of the earth makes things appear to move. Lower-power
eyepieces will reduce this effect of movement considerably and allow you to observe an
object for a longer duration before you have to readjust your telescope.
!
Made in China
Part # 260029
WARNING! CHOKING HAZARD –
Small parts. Not suitable for children
under 3 years.