Celestron NexStar 5, Инструкция по эксплуатации

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Figure 9-3
A collimated telescope
should appear
symmetrical with the
central obstruction
centered in the star's
diffraction pattern.
To verify collimation, view a star near the zenith. Use a medium to high power ocular — 12mm to 6mm focal length. It is
important to center a star in the center of the field to judge collimation. Slowly cross in and out of focus and judge the
symmetry of the star. If you see a systematic skewing of the star to one side, then recollimation is needed.
To accomplish this, you need to tighten the secondary collimation screw(s) that move the star across the field toward the
direction of the skewed light. These screws are located in the secondary mirror holder (see figure 9-1). Make only a small 1/6 to
1/8 field correction and re-center the star by moving the scope before making any improvements or before making further
adjustments.
To make collimation a simple procedure, follow these easy steps
1. While looking through a medium to high power eyepiece, de-focus a bright star until a ring pattern with a dark shadow
appears (see figure 9-2). Center the de-focused star and notice in which direction the central shadow is skewed.
2. Place your finger along the edge of the front cell of the telescope (be careful not to touch the corrector plate), pointing
towards the collimation screws. The shadow of your finger should be visible when looking into the eyepiece. Rotate your
finger around the tube edge until its shadow is seen closest to the narrowest portion of the rings (i.e. the same direction in
which the central shadow is skewed).
3. Locate the collimation screw closest to where your finger is positioned. This will be the collimation screw you will need to
adjust first. (If your finger is positioned exactly between two of the collimation screws, then you will need to adjust the
screw opposite where your finger is located).
4.
Use the hand control buttons to move the de-focused star image to the edge of the field of view, in the same direction that
the central obstruction of the star image is skewed.
5. While looking through the eyepiece, use an Allen wrench to turn the collimation screw you located in step 2 and 3. Usuall
a tenth of a turn is enough to notice a change in collimation. If the star image moves out of the field of view in the direction
that the central shadow is skewed, than you are turning the collimation screw the wrong way. Turn
the screw in the opposite direction, so that the star image is moving towards the center of the field
of view.
6. If while turning you notice that the screws get very loose, then simply tighten the other two
screws by the same amount. Conversely, if the collimation screw gets too tight, then loosen the
other two screws by the same amount.
7. Once the star image is in the center of the field of view, check to see if the rings are
concentric. If the central obstruction is still skewed in the same direction, then continue turning the
screw(s) in the same direction. If you find that the ring pattern is skewed in a different direction,
than simply repeat steps 2 through 6 as described above for the new direction.
Perfect collimation will yield a star image very symmetrical just inside and outside of focus. In
addition, perfect collimation delivers the optimal optical performance specifications that your
telescope is built to achieve.
If seeing (i.e., air steadiness) is turbulent, collimation is difficult to judge. Wait until a better night if
it is turbulent or aim to a steadier part of the sky. A steadier part of the sky is judged by steady versus twinkling stars.
Figure 9-2 -- Even though the star pattern appears the same on both sides of focus, they are asymmetric. The
dark obstruction is skewed off to the left side of the diffraction pattern indicating poor collimation.