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Celestron SkyProdigy 90 - 22091 Manual

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TELESCOPE BASICS
A telescope is an instrument that collects and focuses light. The
nature of the optical design determines how the light is focused.
Some telescopes, known as refractors, use lenses. Other telescopes,
known as reflectors, use mirrors. SkyProdigy 70 telescope is a
refractor telescope that uses an objective lens to collect its light.
SkyProdigy 90 and 130 are reecting telescopes with a primary
and secondary mirror to gather and focus light.
Focusing
Once you have found an object in the telescope, turn the focusing
knob until the image is sharp. To focus on an object that is nearer
than your current target, turn the focusing knob toward the
eyepiece (i.e., so that the focusing tube moves away from the
front of the telescope). For more distant objects, turn the
focusing knob in the opposite direction. To achieve a truly sharp
focus, never look through glass windows or across objects that
produce heat waves, such as asphalt parking lots.
Image Orientation
The image orientation of any telescope changes depending on
how the eyepiece is inserted into the telescope. When observing
through SkyProdigy 70 or 90 using the diagonal, the image will
be right side up, but reversed from left to right. When observing
straight through, with the eyepiece inserted directly into the
telescope, the image will be inverted.
When observing through SkyProdigy 130, a reecting telescope, the
image will be reversed (mirror image) when looking through the
eyepiece.
For astronomical viewing, out of focus star images are very diuse,
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.
Calculating Magnication
You can change the power of your telescope just by changing
the eyepiece (ocular). To determine the magnication 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)
Magnication = ___________________________
Focal Length of Eyepiece (mm)
Let’s say, for example, you are using the 25 mm eyepiece. To
determine the magnication you simply divide the focal length
of your telescope (for example, SkyProdigy 90 has a focal length
of 1250 mm) by the focal length of the eyepiece, 25 mm. Divid-
ing 1250 by 25 yields a magnication of 50 power.
Although the power is variable, each instrument under average
skies has a limit to the highest useful magnication. The general
rule is that 60 power can be used for every inch of aperture.
For example, SkyProdigy 90 is 3.5” (90 mm) in diameter.
Multiplying 3.5 by 60 gives a maximum useful magnication of
210 power. Although this is the maximum useful magnication,
most observing is done in the range of 20 to 35 power for every
inch of aperture which is 70 to 122 times for SkyProdigy 90.
Determining Field of View
Determining the eld 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 eld of view, divide the apparent eld of
the eyepiece (supplied by the eyepiece manufacturer) by the
magnication. In equation format, the formula looks like this:
Apparent Field of Eyepiece
True Field = ________________________________________
Magnication
As you can see, before determining the eld of view, you must
calculate the magnication. Using the example in the previous
section, we can determine the field of view using the same
25 mm eyepiece. The 25 mm eyepiece has an apparent eld of
view of 50°. Divide the 50° by the magnication, which is 50
power. This yields an actual eld of view of 1°.
To convert degrees to feet at 1,000 yards, which is more useful for
terrestrial observing, simply multiply by 52.5. Continuing with our
example, multiply the angular eld 1° by 52.5. This produces a linear
eld width of 52.5 feet at a distance of one thousand yards. The
apparent eld of each eyepiece that Celestron manufactures is found
in the Celestron Accessory Catalog (#93685-11).
General Observing Hints
When working with any optical instrument, there are a few
things to remember to ensure you get the best possible image:
• Never look through window glass. Glass found in household
windows is optically imperfect, and as a result, may vary in
thickness from one part of a window to the next. This
inconsistency can and will aect the ability to focus your
telescope. In most cases you will not be able to achieve a
truly sharp image, while in some cases, you may actually see
a double image.
• Never look across or over objects that are producing heat
waves. This includes asphalt parking lots on hot summer
days or building rooftops.
• Hazy skies, fog and mist can also make it dicult to focus
when viewing terrestrially. The amount of detail seen under
these conditions is greatly reduced. Also, when photographing
under these conditions, the processed lm may come out
a little grainier than normal with lower contrast and
underexposed.
• If you wear corrective lenses (specically glasses), you may
want to remove them when observing with an eyepiece
attached to the telescope. When using a camera, however,
you should always wear corrective lenses to ensure the
sharpest possible focus. If you have astigmatism, corrective
lenses must be worn at all times.
Reversedfromleftto
right,asviewedwitha
StarDiagonal
Invertedimage,as
viewedwiththeeyepiece
directlyintelescope
Inverted image, as viewed with
the eyepiece directly in telescope
Reversed from left to right, as
viewed with a Star Diagonal
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