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6

Telescope Maintenance

While your StarBlast telescope requires little maintenance, 
there are a few things to remember that will ensure your tele-
scope performs at its best.

care and cleaning of the Optics

In general, your telescope’s mirrors will only need to be cleaned 
very infrequently, if ever. Covering the front opening of the tele-
scope with the dust cover when it is not in use will prevent dust 
from accumulating on the mirrors. Keeping the dust cap on the 
focuser’s 1.25" opening is also a good idea. Improper cleaning 
can scratch the mirror coatings, so the fewer times you have 
to clean the mirrors, the better. A little dust or small specks of 
paint from the scope’s interior have virtually no effect on the 
visual or imaging performance of the telescope. So avoid the 
urge to clean the optics unless it is absolutely necessary!
To clean the primary mirror, carefully remove the mirror cell 
from the telescope. To do this, you must remove the screws that 
attach the mirror cell to the steel tube. These screws are located 
on the outer edge of the mirror cell. Then pull the cell away from 
the tube. Be careful not to touch the aluminized surface of the 
mirror with your fingers. Set the mirror on a clean, soft towel.
Fill a clean sink, free of abrasive cleanser, with room-temper-
ature water, a few drops of liquid dishwashing detergent, and 
if possible, a cap-full of rubbing alcohol. Submerge the mirror 
(aluminized face up) in the water and let it soak for several 
minutes (or hours if it is a very dirty mirror). Wipe the mirror 
underwater with clean cotton balls, using extremely light pres-
sure and stroking in straight lines across the surface. Use one 
ball for each wipe across the mirror. Then rinse the mirror 
under a stream of lukewarm water. Any particles on the sur-
face can be swabbed gently with a series of clean cotton balls, 
each used just one time.
Dry the mirror in a stream of air (a “blower bulb” works great), 
or remove any stray drops of water with the corner of a paper 
towel. Dry the bottom and the edges with a towel (not the mir-
ror surface!). Leave the entire assembly in a warm area until it 
is completely dry. Then reinstall the mirror cell in the telescope 
optical tube with the screws.
To minimize the need to clean your telescope, replace all lens 
covers once you have finished using it. This will prevent con-
taminants from entering the optical tube.

collimation

Collimation is the process of adjusting the telescope’s mir-
rors so they are aligned with one another. Your telescope’s 
optics were aligned at the factory, and should not need much 
adjustment unless the telescope was jarred while in transit. 
Accurate mirror alignment is important to ensure the peak per-
formance of your telescope, so it should be checked regularly. 
Collimation is a relatively easy process and can be done in 
daylight or darkness.
To check collimation, remove the eyepiece and look down the 
focuser drawtube. You should see the secondary mirror cen-
tered in the drawtube, as well as the reflection of the primary 
mirror centered in the secondary mirror, and the reflection of 
the secondary mirror (and your eye) centered in the reflection 

of the primary mirror, as in 

Figure 5a. If anything is off-center, 

proceed with the following collimating procedure.

The collimation cap

Your StarBlast comes with a “quick collimation cap”. This is a 
simple cap that fits on the focuser drawtube like a dust cap, 
but has a tiny hole in the center and a reflective inner surface. 
The collimation cap helps center your eye over the focuser 
drawtube so that aligning the optical components is easier to 
achieve. The reflective surface provides a distinct visual refer-
ence that is helpful in centering the mirror reflections

. Figures 

5b through 5c assume that you have the collimation cap in 
place.

The Primary Mirror center Mark

You’ll notice that the primary mirror of the StarBlast has a tiny 
ring (sticker) marking its center. This “center mark” allows you 
to achieve a very precise collimation; you don’t have to guess 
where the exact center of the mirror is.

Figure 5. 

Collimating the optics. 

(a) 

When the mirrors are 

properly aligned, the view down the focuser drawtube should 

look like this. 

(b) 

Here, the secondary mirror is centered 

under the focuser, but it needs to be adjusted (tilted) so that 

the entire primary mirror is visible. 

(c) 

When the mirror is 

correctly aligned, the center “dot” of the collimation cap will 

be centered.

a.

b.

c.

Summary of Contents for StarBlast AutoTracker 10140

Page 1: ...676 1343 E mail support telescope com Corporate Offices 831 763 7000 89 Hangar Way Watsonville CA 95076 Providing Exceptional Consumer Optical Products Since 1975 Orion StarBlast 114mm AutoTracker 101...

Page 2: ...ameter eyepieces a 25mm and a 10mm The longer the focal length i e the larger the number the lower the eyepiece power or magnification and the shorter the focal length i e the smaller the number the h...

Page 3: ...e or roof chimney and center it in the telescope s eyepiece The object should be at least 1 4 mile away Now turn on the EZ Finder II and look through it Without moving the main telescope use the EZ Fi...

Page 4: ...can see before determining the field of view you must calculate the magnification Using the example in the previous section we can determine the field of view using the same 25mm eyepiece The 25mm eye...

Page 5: ...e power is all you need to see them Visually they are too faint to reveal any of the color seen in long exposure photographs Instead they appear grayish And because of their low surface brightness the...

Page 6: ...til it is completely dry Then reinstall the mirror cell in the telescope optical tube with the screws To minimize the need to clean your telescope replace all lens covers once you have finished using...

Page 7: ...e optics are collimated Another even easier and more precise way to collimate your reflector is to use a laser collimator such as the Orion LaserMate II Deluxe collimator sold separately It comes with...

Page 8: ...ass If a group of three or more stars revolve around one another it is called a mul tiple system It is believed that approximately 50 percent of all stars belong to binary or multiple systems Systems...

Page 9: ...om the focal plane of the telescope to be in focus This means when you focus one parfocal eye piece all the other parfocal eyepieces in a particular line of eyepieces will be in focus Parsec The dista...

Page 10: ...10 Time Zones...

Page 11: ...11...

Page 12: ...12 Sky Maps...

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Page 18: ...rranted instrument that proves to be defective provided it is returned postage paid Proof of purchase such as a copy of the original receipt is required This warranty is only valid in the country of p...

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