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ring of light fills about 10% of the eyepiece field-diameter. If the dark central spot is offset in
(i.e., not concentric with) the ring of light, your telescope's optical system is misaligned and
requires collimation.
Follow these steps for collimation of the optical system:
a.
The only adjustments possible, or necessary, on the LX90 are from the three screws (Fig.
25) located at the edge of the outer surface of the secondary mirror housing.
CAUTION: Do not force the three collimation screws past their normal travel
and do not loosen them more than two full turns in a counterclockwise direc-
tion or the secondary mirror may come loose from its support. You will find
that the adjustments are very sensitive, usually requiring only one-half turn
or less to produce the desired result.
b.
While looking at the defocused star image, notice which direction the darker shadow is
offset in the ring of light or notice which part of the ring is the thinnest (1, Fig. 25). Place
your index finger in front of the telescope so that it touches one of the collimation set
screws. You will see the shadow of your finger in the ring of light. Move your finger around
the edge of the black plastic secondary mirror support until you see the shadow of the fin-
ger crossing the thinnest part of the ring of light. At this point, look at the front of the
telescope where your finger is aiming. It will either be pointing directly at a set screw, or it
will be between two set screws aiming at the set screw on the far side of the black plastic
secondary mirror support. This is the set screw that you will adjust.
c.
Using the Arrow keys at the slowest slew speed, move the defocused image to the edge
of the eyepiece field of view (2, Fig. 25), in the same direction as the darker shadow is
offset in the ring of light.
d.
Turn the set screw that you found with the pointing exercise while looking in the eyepiece.
You will notice that the star image will move across the field. If while turning the defocused
star image flies out of the eyepiece field, then you are turning the screw the wrong way.
Turn the opposite direction and bring the image back to the center of the field.
e.
If the screw you are turning becomes very loose, tighten the other two screws by even
amounts. If the screw you are turning gets too tight, unthread the other two by even
amounts.
f.
When you bring the image to center (3, Fig. 25), carefully examine the evenness of the
ring of light (concentricity). If you find that the dark center is still off in the same direction,
continue to make the adjustment in the original turning direction. If it is now off in the
opposite direction, you have turned too far and you need to turn in the opposite direction.
Always double check the image in the center of the field of the eyepiece.
g.
You may find after your initial adjustment that the dark center is off in a new direction (e.g.,
instead of being off side-to-side it is now off in an up-and-down direction). In this case
repeat steps b through f to find the new adjustment screw.
h.
Now try a higher power eyepiece (e.g., 9mm or less) and repeat the above tests. Any lack
of collimation at this point will require only very slight adjustments of the three set screws.
You now have good collimation of the optics.
i.
As a final check on alignment, examine the star image in focus with the higher power eye-
piece as suggested above, under good viewing conditions. The star point should appear
as a small central dot (commonly referred to as an "Airy disc") with a diffraction ring
surrounding it. To give a final precision collimation, make extremely slight adjustments of
the three set screws, if necessary, to center the Airy disc in the diffraction ring. You now
have the best alignment of the optics possible with this telescope.
Looking at or near the Sun will cause irreversable damage to your eye. Do not point this telescope at or near the
Sun. Do not look through the telescope as it is moving.
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