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>>ĎėėĔėĚĕĕĔėęđĚęĈčĊĘ
help support and minimize lateral movement of the primary mirror
during astrophotography.
To use the mirror clutches:
͙Ǥ Ǥ
͚Ǥ ǡ
very tight and can be turned no further.
Warning! Once the mirror is locked down, do not turn the focuser
ƤǤ
the focus knob should not damage the telescope, undue stress can
be placed on the focus mechanisms causing excessive image shift
while focusing.
>>ĆđĈĚđĆęĎēČĆČēĎċĎĈĆęĎĔē
ȋȌǤƤǡ
simply divide the focal length of the telescope by the focal length of the
Ǥǡǣ
Let’s say, for example, you are using the 40 mm Plössl eyepiece. To
Ƥ
telescope (the CPC 800, for example, has a focal length of 2032 mm) by
the focal length of the eyepiece, 40 mm. Dividing 2032 by 40 yields a
Ƥ͙͝Ǥ
Although the power is variable, each instrument under average skies
ƤǤ
͘͞Ǥǡ
͘͘͠͠Ǥ͘͠͞
Ƥ͘͜͠Ǥ
Ƥǡ͚͛͘͝
͙͚͘͘͘͘͞͠͠Ǥ
ĆČēĎċĎĈĆęĎĔēȂ
ȋȌ
ȋȌ
>>ĊęĊėĒĎēĎēČĎĊđĉĔċĎĊĜ
Ƥ
Ǥ
ƤǡƤȋ
ȌƤǤǡ
formula looks like this:
ǡƤǡ
ƤǤǡ
Ƥ͘͜Ǥ͘͜
ÚƤ͜͞λǤ͜͞λ
Ƥǡ͙͝ǤƤǤ͡λǡ
almost a full degree.
To convert degrees to feet at 1,000 yards, which is more useful for
terrestrial observing, simply multiply by 52.5. Continuing with our
ǡƤǤ͡λ͚͝Ǥ͝Ǥ
Ƥ͜͟Ǥ
Ƥ
ȋ͗͛͡͞͠͝ȌǤ
ėĚĊĎĊđĉȂ
Ƥ
>>ĊēĊėĆđćĘĊėěĎēČĎēęĘ
When working with any optical instrument, there are a few things to
remember to ensure you get the best possible image.
Ȉ Ǥ
is optically imperfect, and as a result, may vary in thickness from one
Ǥơ
Ǥ
achieve a truly sharp image, while in some cases, you may actually see
a double image.
Ȉ Ǥ
includes asphalt parking lots on hot summer days or building rooftops.
Ȉ ǡƥ
viewing terrestrially. The amount of detail seen under these conditions
is greatly reduced. Also, when photographing under these conditions,
Ƥ
lower contrast and underexposed.
Ȉ ȋƤȌǡ
to remove them when observing with an eyepiece attached to the
telescope. When using a camera, however, you should always wear
Ǥ
stigmatism, corrective lenses must be worn at all times.
͝ǧ͜
Mirror
Clutch
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