38
generate. All these problems result in guiding errors. The goal of rebalancing the telescope is to
put the telescope‟s center of gravity back at that intersection, to restore optimal function of the
system.
By first balancing the telescope vertically, you ensure that the telescope‟s center of gravity lies
somewhere along the longitudinal axis. If the telescope swings north, that means the center of
gravity is actually somewhere above the longitudinal axis. If the telescope swings south, then it
is somewhere below the longitudinal axis. This is why you must add weight to the opposite side
until the movement stops, which indicates that the center of gravity has been put back
somewhere along the longitudinal axis. At this point, where the weight is added along the
longitudinal axis is totally irrelevant. That will be dealt with during the horizontal balancing.
However, if the center of gravity is not somewhere along the longitudinal axis, then sliding
weights either forward or backward during the horizontal phase of balancing has no hope of
putting the center of gravity back on the intersection point of the three axes. It will always be
somewhere above or below that intersection point.
You will learn whether the added weight has put the center of gravity in front of or behind the
triple intersection point when you start the horizontal phase of balancing. If the front end drops
down, then you have put the center of gravity somewhere along the longitudinal axis in front of
the triple intersection. If the front end swings up, then you have put the center of gravity
somewhere along the longitudinal axis toward the rear of the triple intersection point. When you
have counteracted any movement, then you have achieved putting the center of gravity on the
triple intersection point and the telescope is dynamically balanced. This is also why just sliding
counterweights forward or backward along the counterweight bar until the telescope seems
balanced when aimed at the its imaging target, which is what most people do, doesn‟t properly
do the job of balancing the telescope.
There are some practical pointers. If most of the weight you add to your Compustar is camera
equipment at the rear cell, then the additional weight will be centered along the longitudinal axis
and the telescope will likely remain in vertical balance. Therefore, you will not need to add any
weight on either the top or bottom counterweight bar assemblies. Unfortunately, this will leave
you lacking any ballast that you can slide forward or backward to achieve horizontal balance.
The solution is to add an equal amount of weight to both counterweight bar assemblies anyway.
This will maintain the telescope in vertical balance and still provide you with the ballast you
need to ultimately balance the telescope horizontally.
If you are really smart, you are wondering about balancing the telescope in the third direction,
along the axis between the two fork arm swivels. Measures have already been taken to balance
the unique configurations of the Compustars in that third dimension. For example, the 8x50
finderscope on the Compustar C8 has been shifted from the left rear side of the optical tube to
the lateral side of the left fork arm to counterbalance the weight of the declination drive box on
the right fork arm. The Compustar C11 and C14 have finderscopes in their usual positions, but
Komentáře k této Příručce