
Never look at or near the sun with the telescope: THERE IS A RISK OF BLINDNESS! 13
OBSERVATION
Observation
Observation with manual operation
After the telescope is assembled and balanced as described, you are
ready for manual observation. Pick an easy-to-observe object on Earth
such as a street sign or traffic light and familiarize yourself with the tele-
scope's functions. To achieve the best possible result, please observe the
following instructions:
•
To locate an object, first loosen the RA clamp (33, Fig. 1d) and the DEC
clamp (17, Fig.1d). The telescope can now move freely around its axes.
First loosen the clamps individually and familiarise yourself with the
individual movements. Then loosen both clamps at the same time. It is
important that you familiarise yourself with all the movements of your tel-
escope, as handling a parallactic mount can take some getting used to,
especially at night in complete darkness.
• Now use the finder scope to locate the object of your choice. When you
have the desired object in your sights, close the RA and DEC clamps
again.
• The eyepiece of a telescope magnifies the image captured by the tele-
scope's primary mirror. Each eyepiece has a focal length, expressed in
millimeters (mm). The smaller the focal length, the higher the magnifica-
tion. For example: an eyepiece with a focal length of 9mm has a higher
magnification than an eyepiece with a focal length of 26mm.
Eyepieces with a lower magnification offer a larger field of view, provide
brighter and higher contrast images and are more comfortable for the
eye during longer observations. At the beginning of an observation, you
should always start with a weaker eyepiece, such as the supplied Plössl
25 mm. When the desired object is centred and focused, you can switch
to a larger eyepiece to magnify the object as much as the observing con-
ditions will allow.
• Once centered, an object can be brought into focus using the focusing
knobs on the focusing unit (8 Fig. 1b). However, keep in mind that the
desired object will slowly move out of field of view due to the rotation of
the earth on its own axis. This impression is even reinforced at high mag-
nification.
Moon Observations
Point the telescope (picture: (Keep in mind, however, that the moon is not
visible every night) Now practice using the different eyepieces to observe
different details on the moon. There are many different details to look at on
the moon, such as craters, mountain ranges, and grooves. The best time
to observe the moon is during its crescent or sickle phase. At this time,
the sunlight hits the moon at a very shallow angle, giving its appearance
a vivid depth. At full moon there are no shadows to be seen at all, which
makes the surface of the moon look very bright, flat and uninteresting.
Therefore, when viewing the moon, you may want to consider using a
neutral density moon filter. Among other things, this not only dampens the
glaring light of the moon, but also increases the contrast at the same time.
Tracking of an object
While the earth turns under the night sky, the stars seem to wander from
east to west. The speed with which the stars perform this movement is
called "sidereal velocity".
WARNING!
Never use a tele-scope for an
unprotected view of the sun! As
soon as you look directly at the
sun, or even at its immediate
surroundings, you risk immediate
and irreparable damage to your
eye. This damage to the eye usu-
ally occurs painlessly and there-
fore without any warning to the
observer that perhaps everything
is already too late and that eye
damage has occurred. Therefore,
never point the telescope or its
viewfinder at or near the sun.
Never look through the tele-
scope or its viewfinder when it is
moving. During an observation,
children must remain under adult
supervision at all times.
IMPORTANT NOTE:
Objects viewed through the view-
finder appear upside down and
upside down.
Objects observed through the
eyepiece of the main tube, which
sits on the telescope via a zenith
prism, appear upright but also
laterally inverted.
This effect does not interfere with
the observation of astronomical
objects. Incidentally, these effects
occur with all astronomical tele-
scopes.