Orion 52986 Instruction Manual Download Page 13

13

Focusing the Telescope

To focus the telescope, turn the focus wheels (

Figures 14 

and 15

) forward or back until you see your target object (e.g., 

stars, the Moon, etc.) in the eyepiece. Then make finer adjust-
ments until the image is sharp. If you’re having trouble achiev-
ing initial focus, rack the focuser drawtube all the way in using 
the focus wheels, then while looking into the eyepiece slowly 
turn the focus wheels so that the drawtube extends outward. 
Keep going until you see your target object come into focus. 
Note that when you change eyepieces you may have to adjust 
the focus a bit to get a sharp image with the newly inserted 
eyepiece. 

What to Expect

So what will you see with your telescope? You should be able 
to see bands on Jupiter, the rings of Saturn, craters on the 
Moon, the waxing and waning of Venus, and many bright 
deep-sky objects. Do not expect to see color as you do in 
NASA photos, since those are taken with long-exposure cam-
eras and have “false color” added. Our eyes are not sensitive 
enough to see color in deep-sky objects except in a few of the 
brightest ones.

Objects to Observe

Now that you are all set up and ready to go, what is there to 
look at in the night sky?
A. The Moon
With its rocky surface, the Moon is one of the easiest and 
most interesting objects to view with your telescope. Lunar 
craters, maria, and even mountain ranges can all be clearly 
seen from a distance of 238,000 miles away! With its ever-
changing phases, you’ll get a new view of the Moon every 
night. The best time to observe our one and only natural satel-
lite is during a partial phase, that is, when the Moon is not full. 
During partial phases, shadows are cast on the surface, which 
reveal more detail, especially right along the border between 
the dark and light portions of the disk (called the “terminator”). 
A full Moon is too bright and devoid of surface shadows to 
yield a pleasing view. Make sure to observe the Moon when it 
is well above the horizon to get the sharpest images. 
Use an optional Moon filter to dim the Moon when it is very 
bright. It simply threads onto the bottom of the eyepieces (you 
must first remove the eyepiece from the focuser to attach a 
filter). You’ll find that the Moon filter improves viewing comfort, 
and helps to bring out subtle features on the lunar surface.
B. The Planets
The planets don’t stay put like the stars, so to find them you 
should refer to the monthly star charts at OrionTelescopes.
com, or to charts published monthly in Astronomy, Sky & 
Telescope, or other astronomy magazines. Venus, Mars, 
Jupiter, and Saturn are the brightest objects in the sky after 
the Sun and the Moon. Other planets may be visible but will 
likely appear star-like. Because planets are quite small in 
apparent size, optional higher-power eyepieces or a Barlow 
lens are recommended and often needed for detailed obser-
vations.
B. The Sun

You can change your nighttime telescope into a daytime Sun 
viewer by installing an optional full-aperture solar filter over 
the front opening of the telescope. The primary attraction is 
sunspots, which change shape, appearance, and location 
daily. Sunspots are directly related to magnetic activity in the 
Sun. Many observers like to make drawings of sunspots to 
monitor how the Sun is changing from day to day. 
Important Note: Do not look at the Sun with any optical instru-
ment without a professionally made solar filter placed over the 
front aperture of your telescope, or permanent eye damage 
could result.

Important Note: Do not look at the Sun with any opti-
cal instrument without a professionally made solar filter 
placed over the front aperture of your telescope, or per-
manent eye damage could result.

D. The Stars
Stars will appear like twinkling points of light. Even powerful 
telescopes cannot magnify stars to appear as more than a 
point of light. You can, however, enjoy the different colors of 
the stars and locate many pretty double and multiple stars. 
The famous “Double-Double” in the constellation Lyra and the 
gorgeous two-color double star Albireo in Cygnus are favor-
ites. Defocusing a star slightly can help bring out its color.
E. Deep-Sky Objects
Under dark skies, you can observe a wealth of fascinating 
deep-sky objects, including gaseous nebulas, open and 
globular star clusters, and different types of galaxies. Most 
deep-sky objects are very faint, so it is important you find an 
observing site well away from light pollution. 
To find deep-sky objects with your telescope, you first need 
to become reasonably familiar with the night sky. Unless you 
know how to recognize the constellation Orion, for instance, 
you won’t have much luck locating the Orion Nebula. A simple 
planisphere, or star wheel, can be a valuable tool for learning 
the constellations and seeing which ones are visible in the 
sky on a given night. Once you have identified a few constel-
lations, a good star chart, atlas, or astronomy app will come in 
handy for helping locate interesting deep-sky objects to view 
within the constellations. 
Do not expect these objects to appear like the photographs 
you see in books and on the internet; most will look like dim 
gray smudges. Our eyes are not sensitive enough to see color 
in deep-sky objects except in a few of the brightest ones. But 
as you become more experienced and your observing skills 
get sharper, you will be able to ferret out more and more sub-
tle details and structure.

VI. Collimation of Your 

Telescope’s Optics

Collimation is the process of adjusting the optics of a tele-
scope so they are precisely aligned with one another and 
with the telescope tube. Accurate collimation is important to 
ensure the peak performance of your telescope, so it should 

Summary of Contents for 52986

Page 1: ...ion or any of its contents may be reproduced copied modified or adapted without the prior written consent of Orion Telescopes Binoculars A N E M P L O Y E E O W N E D C O M P A N Y 52988 52986 52987 C...

Page 2: ...lternatively you could thread on the shaft first and then slide the counterweight onto it after removing the hex head bolt and washer from the bottom end of the shaft 5 Attach the slow motion cables J...

Page 3: ...3 Figure 1 A Parts included with the Orion Observer EQ telescopes B Optical tube assemblies of the Observer EQ telescopes H P I E F K L A B C G J M D Q O N O A B...

Page 4: ...he telescope For larger telescope move ment release the RA and Dec axis lock knobs Figure 16 and move the telescope tube by hand to the approximate location then retighten the lock knobs and make fine...

Page 5: ...adjustments to the alignment thumbscrews until the image in both the finder scope and the telescope s eye piece is exactly centered When it is no further adjustment of the finder scope will be needed...

Page 6: ...ng the shaft until it exactly counterbalances the telescope That s the point at which the shaft remains horizontal even when you let go of the telescope with both hands 3 Retighten the counterweight l...

Page 7: ...ccomplished by slowly rotating the telescope on its right ascension R A axis using only the R A slow motion cable But first the R A axis of the mount must be aligned with the Earth s rotational polar...

Page 8: ...ot make any further adjustments to the azimuth or the latitude of the mount nor should you move the tripod Doing so will ruin the polar alignment The telescope should be moved only about its R A and D...

Page 9: ...object through the telescope you ll see it drift slowly across the field of view To keep it in the field assuming the equatorial mount is polar aligned just turn the R A Figure 16 The R A and Dec loc...

Page 10: ...in the Northern Hemisphere The Dec setting circle is denoted in degrees with each main mark representing 10 increments 1 10 2 20 etc Values of Dec coordinates range from 90 to 90 The 0 mark indi cates...

Page 11: ...ng circles are not accurate enough to put an object dead center in the telescope s eyepiece but they should place the object somewhere within or near the field of view of the finder scope assuming the...

Page 12: ...r that mat ter Your eyes take about 30 minutes to reach perhaps 80 of their full dark adapted sensitivity As your eyes become dark adapted more stars will glimmer into view and you ll be able to see f...

Page 13: ...nt size optional higher power eyepieces or a Barlow lens are recommended and often needed for detailed obser vations B The Sun You can change your nighttime telescope into a daytime Sun viewer by inst...

Page 14: ...and error to determine which screws to loosen and tighten to move the reflection of the primary mirror to the center of the secondary mirror But be patient and you ll get it Aligning the Primary Mirr...

Page 15: ...me with your telescope Motor Drive A motor drive which attaches to the right ascension axis of an equatorial telescope mount enables your telescope to track the motion of stars and other celestial obj...

Page 16: ...German equatorial Tripod Aluminum Total instrument weight 16 lbs 1 5 oz Observer 134mm EQ Reflector Primary mirror diameter 134mm 5 3 Primary mirror coating Aluminum with silicon dioxide SiO2 overcoat...

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