background image

the center screw with a larger 
Phillips head screwdriver (see 
Figure  9). Turning  the  screw 
clockwise will move the sec-
ondary mirror toward the front 
opening  of  the  optical  tube, 
while turning the screw coun-
ter-clockwise  will  move  the 
secondary mirror toward the 
primary mirror.
When the secondary mirror is 
centered in the focuser draw-
tube,  rotate  the  secondary 
mirror holder until the reflec-
tion  of  the  primary  mirror  is 
as  centered  in  the  second-
ary mirror as possible. It may 
not be perfectly centered, but 
that  is  OK.  Now  tighten  the 
three small alignment screws 
equally to secure the second-
ary mirror in that position.
If  the  entire  primary  mirror 
reflection is not visible in the 
secondary mirror, as in Figure 
8c,  you  will  need  to  adjust 
the tilt of the secondary mir-
ror. This is done by alternately 
loosening  one  of  the  three 
alignment screws while tight-
ening the other two, as depict-
ed  in  Figure  10. The  goal  is 
to  center  the  primary  mirror 
reflection  in  the  secondary 
mirror, as in Figure 8d. Don’t 
worry that the reflection of the 
secondary mirror (the small-
est circle, with the collimation 
cap “dot” in the center) is off-
center. You will fix that in the 
next step.

adjusting the Primary 

Mirror

The final adjustment is made 
to  the  primary  mirror.  It  will 
need  adjustment  if,  as  in 
Figure  8d,  the  secondary 
mirror  is  centered  under  the 
focuser and the reflection of the primary mirror is centered in 
the secondary mirror, but the small reflection of the secondary 
mirror (with the “dot” of the collimation cap) is off-center.
The tilt of the primary mirror is adjusted using the three sets 
of two collimation screws on the back end of the optical tube. 
Adjusting the tilt of the mirror requires a “push-pull” technique 
involving adjustment of each set of collimation screws. Loosen 

the flush screw one full turn, 
and then tighten the adjacent 
raised  screw  until  it  is  tight 
as in Figure 11 (do not over-
tighten). Look into the focuser 
and  see  if  the  secondary 
mirror  reflection  has  moved 
closer to the center of the pri-
mary. You can tell this easily 
with the collimation cap and 
mirror center mark by simply 
watching to see if the “dot” of 
the collimation cap is moving 
closer  or  farther  away  from 
the ring on the center of the 
primary  mirror.  Repeat  this 
process  on  the  other  two 
sets of collimation screws, if 
necessary. It will take a little 
trial and error to get a feel for 
how  to  tilt  the  mirror  in  this 
way. When you have the dot 
centered  as  much  as  pos-
sible in the ring, your primary 
mirror is collimated. The view 
through  the  collimation  cap 
should  resemble  Figure  8e. 
Make sure all the collimation 
screws are tight (but do not 
overtighten),  to  secure  the 
mirror tilt.
A simple star test will tell you 
whether the optics are accu-
rately collimated.

star‑testing the 

telescope

When  it  is  dark,  point  the 
telescope at a bright star and 
accurately center it in the eye-
piece’s  field  of  view.  Slowly 
de-focus the image with the 
focusing  knob.  If  the  tele-
scope is correctly collimated, 
the expanding disk should be 
a perfect circle (Figure 12). If 
the image is unsymmetrical, 
the  scope  is  out  of  collima-
tion. The  dark  shadow  cast 

by the secondary mirror should appear in the very center of 
the out-of-focus circle, like the hole in a donut. If the “hole” 
appears off-center, the telescope is out of collimation.
If you try the star test and the bright star you have selected is 
not accurately centered in the eyepiece, the optics will always 
appear out of collimation, even though they may be perfectly 
aligned. It is critical to keep the star centered, so over time you 

12

Figure 8. 

Collimating the optics. (a) When the mirrors are 

properly aligned, the view down the focuser drawtube should look 
like this. (b) With the collimation cap in place, if the optics are out 
of alignment, the view might look something like this. (c) Here, the 
secondary mirror is centered under the focuser, but it needs to be 
adjusted (tilted) so that the entire primary mirror is visible. (d) The 
secondary mirror is correctly aligned, but the primary mirror still 
needs adjustment. When the primary mirror is correctly aligned, the 
“dot” will be centered, as in (e).

drawtube

Reflection
of primary
mirror clip

a.

b.

c.

d.

e.

Содержание SpaceProbe 3 EQ

Страница 1: ...oviding Exceptional Consumer Optical Products Since 1975 Customer Support 800 676 1343 E mail support telescope com Corporate Offices 831 763 7000 89 Hangar Way Watsonville CA 95076 Orion SpaceProbe 3...

Страница 2: ...Declination setting circle Counterweight shaft Counterweight Counterweight lock knob Right Ascension lock knob not shown Leg lock knob Eyepiece Focuser Optical tube assembly Right Ascension setting c...

Страница 3: ...should be tightened securely to eliminate flexing and wobbling but be careful not to over tighten or the threads may strip Refer to Figure 1 dur ing the assembly process During assembly and anytime f...

Страница 4: ...the counterweight shaft to pass through the hole Position the counterweight about halfway up the shaft and tighten the lock knob Replace the screw and washer on the end of the shaft 8 Remove the two w...

Страница 5: ...ew to only a portion of the full field If the glasses do restrict the field of view you may be able to observe with your glasses off by just refocusing the telescope the needed amount If your eyes are...

Страница 6: ...bserving This is accomplished 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...

Страница 7: ...s The setting circles on an equatorial mount enable you to locate celestial objects by their celestial coordinates Every object resides in a specific location on the celestial sphere That location is...

Страница 8: ...ons you rotate the telescope on its R A and Dec axes Depending on the altitude of the object you want to observe the counterweight shaft will be oriented somewhere between vertical and horizontal Figu...

Страница 9: ...ect being viewed To calculate the magnification or power of a telescope and eyepiece combination simply divide the focal length of the telescope by the focal length of the eyepiece Telescope Focal Len...

Страница 10: ...nt ears on each side of Saturn s disk A steady atmosphere good see ing is necessary for a good view You will probably see a bright star close by which is Saturn s brightest moon Titan VENUS At its bri...

Страница 11: ...ddition to providing the collimation cap you ll notice a tiny ring sticker in the exact center of the primary mirror This center mark allows you to achieve a very precise collima tion of the primary m...

Страница 12: ...ved closer to the center of the pri mary You can tell this easily with the collimation cap and mirror center mark by simply watching to see if the dot of the collimation cap is moving closer or farthe...

Страница 13: ...or flecks of paint have virtually no effect on the visual performance of the telescope The large primary mirror and the elliptical secondary mirror of your telescope are front surface aluminized and...

Страница 14: ...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 pressure and stroking in straight lines across the surface U...

Страница 15: ...Way Watsonville CA 95076 If the product is not registered proof of purchase such as a copy of the original invoice is required This warranty does not apply if in Orion s judgment the instrument has be...

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