Bresser National Geographic EQ3 Mode D'emploi page 17

6. Finder scope
Your telescope is now roughly aligned and set.
To arrive at a comfortable observation position, carefully undo the
main tube mounting screws (No. 9, X) until you can rotate the tel-
escope's main tube. Move the eyepiece and finder scope/LED finder
scope until the position is comfortable for you.
Fine adjustment is done with the aid of the finder scope. Look
through the finder scope and try to align it with the North Star (No.
27) in the centre of the crosshairs (No. 31). In precisely adjusting your
telescope, you will find the shaft (No. 16, K) of the right ascension
axis (No. 16, b) and that (No. 16, E) of the declination axis (No. 16, a)
helpful.
7. Observation
Once you have found the North Star with your finder scope/LED finder
scope, you will be able to view it through your telescope eyepiece.
If necessary, you can, with help of the flexible handles, align the star
more exactly, just as you can adjust the definition by using the focus-
ing wheel (No. 16, B).
Furthermore, you can now, by changing the eyepiece, increase the
magnification. Note that the magnification of the stars can hardly be
seen.
i
NOTE
Eyepieces enlarge the picture of the telescope's
prime focus. The less the eyepiece's focal lengths
is, the stronger the magnification is.
Various eyepieces are needed to reach different
magnifications. Begin every observation with a
low-powered magnification (20 mm eyepiece).
8. Find a Star:
Initially, it may be difficult for you to find your bearings in the sky,
since the stars and constellations are constantly moving, and accord-
ing to season, date and time, their positions in the sky will change.
The North Star is the exception. It is a fixed star and the starting point
for all star maps.
When you first begin to observe the night sky, look at some well-
known constellations and star groups that are visible year-round.
This will help you to orient yourself and learn the functions of your
telescope.
If you have aligned your telescope accurately on one of these stars,
you will find that it vanishes from your visual field after a few minutes
due to the Earth's rotation. To even out this effect, you must turn the
flexible handle (No. 16, K) of the right ascension axis, and your tel-
escope will follow the trajectory of this star.
9. Part circles:
Stars and other celestial bodies are positioned in the sky by coordi-
nates. The place of a star is fixed in the universe by its right ascen-
sion and declination coordinates, similar to latitude and longitude on
Earth.
Declintion (No. 16, C) is the spacing of a celestial body from the sky's
equator, in angle degrees. To the north of the equator, the degree
number is positive. To the south of the equator, the degree number is
negative.
Right ascension (No. 16, M) is the measured distance of a star from
the sky's equator in sidereal (star) time. The vernal equinox is the
point where the ecliptic meets the equator (No. 26, e) at the begin-
ning of spring. The value of the daily celestial revolutions is counted
in the tempo of a 24-hour clock.
For more accurate information about this topic, consult star maps
and other literature, or the Internet.
10. Accessories
Your telescope is supplied with a number of accessories (No. 2).
Depending on your telescope's model, these accessories may include
the following:
10.1. Eyepieces
Change eyepieces to change your telescope's magnification.
Formula for calculating magnification:
Focal length (Telescope) ÷ Focal length (Eyepiece) = Magnification
Examples:
700 mm ÷ 20 mm
700 mm ÷ 12.5 mm
700 mm ÷ 4 mm
10.2. Zenith mirror (refraction telescope only)
The zenith mirror (No. 2, 19) reverses the image you see, and is there-
fore used only for celestial observation.
10.3. Inversion lens
To see a vertical image the right way up, an inversion lens may be
used.
Loosen the clamping screws (No. 25, X) and remove all accessories
from the eyepiece supports (No. 1, 6). Insert the inversion lens (No. 2,
20) straight into the eyepiece supports and hand tighten the clamping
screws. Then insert the eyepiece (e.g. f=20 mm) into the inversion
lens opening and tighten the clamping screws (No. 25, Y).
10.4. Barlow lens
A Barlow lens increases magnification by a factor of three.
10.4.1 Assembling and using with refracting telescopes
If you use a refracting telescope, the Barlow lens should only be
inserted into the zenith mirror (No. 13a, X). Remove the eyepiece from
the zenith mirror and replace it with the Barlow lens. Then insert the
eyepiece with the greatest focal length and hand tighten the clamping
screws to affix it in place (No. 24).
10.4.2 Assembling and using with reflecting telescopes
If you use a reflecting telescope, loosen the clamping screws on the
eyepiece supports (No. 13b, X), and remove the eyepiece from those
supports. Then insert the Barlow lens straight into the supports and
hand tighten the clamping screws. Finally, insert the eyepiece with the
greatest focal length into the Barlow lens, and then fasten it in place
with the clamping screws (No. 24).
10.5.1 Smartphone holder (32a) (Optional)
Insert the eyepiece (1) into the smartphone holder and tighten the screw
(X) to the bracket firmly. Then set the smartphone holder with the eye-
piece into the eyepiece connection (2) and tighten the clamping screws
(Y) by hand firmly. Now start your smartphone camera app and press
your smartphone on the plate. Make sure that it is properly secured.
The camera should rest just above the eyepiece. Place the smartphone
exactly over the eyepiece, so that the image is exactly centered on your
display. It may be necessary to use the zoom function to fill out the
whole screen of your smartphone. The suction cups must be dry, clean
and free from all kinds of dust and dirt. We assume no responsibility for
dropped and broken smartphones due to incorrect handling.
10.5.2 Smartphone-Adapter (32b) (Optional)
Open the flexible holder and put your smartphone in it. Close the
holder and make sure your phone is properly secured. The camera
must be positioned exactly above the eyepiece. Open the locking
clip on the back of the holder and fit the eyepiece exactly onto your
smartphone camera. Now retighten the locking clip and attach the
smartphone adaptor to the eyepiece of your telescope. Now start the
camera app. If the image is not yet centered on your display, loosen
the locking clip slightly and readjust. It may be necessary to use the
zoom function to fill the image on the display. A slight shading at the
edges is possible. Remove the smartphone from the holder after use!
WARNING
Make sure that the smartphone can not slip out of the holder. Bresser
GmbH assumes no liability for any damages caused by a dropped
smartphone.
= 35X
= 56X
= 175X
17
EN