Celestron CGE800 User Manual
32
Figure 4-3
The emblem on the end of
the focus knob shows the
correct rotational direction
for focusing the CGE
.
Focusing
The CGE's focusing mechanism controls the primary mirror which is mounted on a ring that
slides back and forth on the primary baffle tube. The focusing knob, which moves the
primary mirror, is on the rear cell of the telescope just below the star diagonal and eyepiece.
Turn the focusing knob until the image is sharp. If the knob will not turn, it has reached the
end of its travel on the focusing mechanism. Turn the knob in the opposite direction until
the image is sharp. Once an image is in focus, turn the knob clockwise to focus on a closer
object and counterclockwise for a more distant object. A single turn of the focusing knob
moves the primary mirror only slightly. Therefore, it will take many turns (about 30) to go
from close focus (approximately 60 feet) to infinity.
slides back and forth on the primary baffle tube. The focusing knob, which moves the
primary mirror, is on the rear cell of the telescope just below the star diagonal and eyepiece.
Turn the focusing knob until the image is sharp. If the knob will not turn, it has reached the
end of its travel on the focusing mechanism. Turn the knob in the opposite direction until
the image is sharp. Once an image is in focus, turn the knob clockwise to focus on a closer
object and counterclockwise for a more distant object. A single turn of the focusing knob
moves the primary mirror only slightly. Therefore, it will take many turns (about 30) to go
from close focus (approximately 60 feet) to infinity.
For astronomical viewing, out of focus star images are very diffuse, making them difficult to
see. If you turn the focus knob too quickly, you can go right through focus without seeing
the image. To avoid this problem, your first astronomical target should be a bright object
(like the Moon or a planet) so that the image is visible even when out of focus. Critical
focusing is best accomplished when the focusing knob is turned in such a manner that the
mirror moves against the pull of gravity. In doing so, any mirror shift is minimized. For
astronomical observing, both visually and photographically, this is done by turning the focus
knob counterclockwise.
see. If you turn the focus knob too quickly, you can go right through focus without seeing
the image. To avoid this problem, your first astronomical target should be a bright object
(like the Moon or a planet) so that the image is visible even when out of focus. Critical
focusing is best accomplished when the focusing knob is turned in such a manner that the
mirror moves against the pull of gravity. In doing so, any mirror shift is minimized. For
astronomical observing, both visually and photographically, this is done by turning the focus
knob counterclockwise.
NOTE: Before turning the focus knob, remember to lossen to two mirror locking knobs located on the rear cell of the
telescope. These knobs connect a screw to the primary mirror mounting plate and prevent the mirror from moving when
locked down. These screws should be locked down when transporting the telescope.
telescope. These knobs connect a screw to the primary mirror mounting plate and prevent the mirror from moving when
locked down. These screws should be locked down when transporting the telescope.
Calculating Magnification
You can change the power of your telescope just by changing the eyepiece (ocular). To determine the magnification of your
telescope, simply divide the focal length of the telescope by the focal length of the eyepiece used. In equation format, the
formula looks like this:
Focal Length of Telescope
(mm)
Magnification
=
Focal Length of Eyepiece
(mm)
Let’s say, for example, you are using the 40mm Plossl eyepiece. To determine the magnification you simply divide the focal
length of your telescope (the CGE1100 for example has a focal length of 2800mm) by the focal length of the eyepiece, 40mm.
Dividing 2800 by 40 yields a magnification of 70 power.
Although the power is variable, each instrument under average skies has a limit to the highest useful magnification. The general
rule is that 60 power can be used for every inch of aperture. For example, the CGE1100 is 11 inches in diameter. Multiplying 11
by 60 gives a maximum useful magnification of 660 power. Although this is the maximum useful magnification, most observing
is done in the range of 20 to 35 power for every inch of aperture which is 220 to 385 times for the CGE1100 telescope.
rule is that 60 power can be used for every inch of aperture. For example, the CGE1100 is 11 inches in diameter. Multiplying 11
by 60 gives a maximum useful magnification of 660 power. Although this is the maximum useful magnification, most observing
is done in the range of 20 to 35 power for every inch of aperture which is 220 to 385 times for the CGE1100 telescope.
Determining Field of View
Determining the field of view is important if you want to get an idea of the angular size of the object you are observing. To
calculate the actual field of view, divide the apparent field of the eyepiece (supplied by the eyepiece manufacturer) by the
magnification. In equation format, the formula looks like this:
Apparent Field of Eyepiece
True Field =
Magnification
As you can see, before determining the field of view, you must calculate the magnification. Using the example in the previous
section, we can determine the field of view using the same 40mm eyepiece. The 40mm Plossl eyepiece has an apparent field of
view of 46°. Divide the 46° by the magnification, which is 70 power. This yields an actual field of .66°, or two-thirds of a full
degree.