43
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 direction 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 shad-
ow is offset in the ring of light or notice which part of the ring is the thinnest (1,
Fig. 33a). 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 sup-
port until you see the shadow of the finger 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 sup-
port. This is the set screw that you will adjust.
c.
Using the Autostar's Arrow keys at the slowest slew speed, move the defocused
image to the edge of the eyepiece field of view (2, Fig. 33a), in the same direc-
tion 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 turn-
ing 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. 33a), 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 direc-
tion (e.g., instead of being off side-to-side it is now off in an up-and-down direc-
tion). 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 of alignment, examine the star image in focus with the higher
power eyepiece as suggested (j), 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 pos-
sible with this telescope.
Fig. 33a: Defocused star images. Misaligned (1, 2), Aligned
1
2
3
Fig. 33b: Collimation screws.
Summary of Contents for LXD55 Series
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