INSTRUCTION MANUAL
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TELESCOPE BASICS .................................................................................................................................................27
Image Orientation ...................................................................................................................................................27
Focusing..................................................................................................................................................................27
Calculating Magnification ......................................................................................................................................28
Determining Field of View ......................................................................................................................................28
General Observing Hints.........................................................................................................................................28
ASTRONOMY BASICS...............................................................................................................................................30
The Celestial Coordinate System.............................................................................................................................30
Motion of the Stars..................................................................................................................................................31
Polar Alignment (with optional Wedge)..................................................................................................................32
Wedge Align .......................................................................................................................................................32
Finding the North Celestial Pole.............................................................................................................................32
Declination Drift Method of Polar Alignment.....................................................................................................33
CELESTIAL OBSERVING.........................................................................................................................................35
Observing the Moon................................................................................................................................................35
Lunar Observing Hints........................................................................................................................................35
Observing the Planets .............................................................................................................................................35
Planetary Observing Hints...................................................................................................................................35
Observing the Sun ...................................................................................................................................................36
Solar Observing Hints .........................................................................................................................................36
Observing Deep Sky Objects ...................................................................................................................................36
Seeing Conditions....................................................................................................................................................36
Transparency...........................................................................................................................................................36
Sky Illumination ......................................................................................................................................................36
Seeing......................................................................................................................................................................37
CELESTIAL PHOTOGRAPHY .................................................................................................................................38
Short Exposure Prime Focus Photography.............................................................................................................38
Eyepiece Projection.................................................................................................................................................39
Long Exposure Prime Focus Photography..............................................................................................................40
Periodic Error Correction (PEC) ...........................................................................................................................41
Using Periodic Error Correction..........................................................................................................................41
Terrestrial Photography..........................................................................................................................................42
Metering..............................................................................................................................................................42
Reducing Vibration .............................................................................................................................................42
F/6.3 with Reducer/Corrector..............................................................................................................................42
Auto Guiding.......................................................................................................................................................43
TELESCOPE MAINTENANCE .................................................................................................................................44
Care and Cleaning of the Optics.............................................................................................................................44
Collimation..............................................................................................................................................................44
OPTIONAL ACCESSORIES.....................................................................................................................................46
APPENDIX A - TECHNICAL SPECIFICATIONS ..................................................................................................48
APPENDIX B - GLOSSARY OF TERMS..................................................................................................................49
APPENDIX C – LONGITUDES AND LATITUDES.................................................................................................52
APPENDIX D – RS-232 CONNECTION....................................................................................................................57
APPENDIX E – TIME ZONE MAP............................................................................................................................58
SKY MAPS....................................................................................................................................................................60
OBSERVATIONAL DATA SHEET ...........................................................................................................................66
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Congratulations on your purchase of the Celestron CPC telescope! The CPC GPS ushers in the next generation of computer
automated telescopes. The CPC series uses GPS (Global Positioning System) technology to take the guesswork and effort out of
aligning and finding celestial objects in the sky. Simple and easy to use, the CPC with its on-board GPS, is up and running after
locating just three celestial objects. It’s so advanced that once you turn it on, the integrated GPS automatically pinpoints your
exact coordinates. No need to enter the date, time, longitude and latitude or even know the name of a single star in the sky.
If you are new to astronomy, you may wish to start off by using the CPC's built-in Sky Tour feature, which commands the CPC
to find the most interesting objects in the sky and automatically slews to each one. Or if you are more experienced, you will
appreciate the comprehensive database of over 40,000 objects, including customized lists of all the best deep-sky objects, planets
and bright double stars. No matter at what level you are starting out, the CPC will unfold for you and your friends all the
wonders of the Universe.
Some of the many standard features of the CPC include:
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Integrated Global Positioning System for easy alignment.
Fully enclosed optical encoders for position location.
Ergonomically designed hand controller – built into the side of the fork arm.
Database filter limits for creating custom object lists.
Storage for programmable user defined objects; and
Many other high performance features!
The CPC’s deluxe features combined with Celestron’s legendary Schmidt-Cassegrain optical systems give amateur astronomers
the most sophisticated and easy to use telescopes available on the market today.
Take time to read through this manual before embarking on your journey through the Universe. It may take a few observing
sessions to become familiar with your CPC, so you should keep this manual handy until you have fully mastered your telescope’s
operation. The CPC hand control has built-in instructions to guide you through all the alignment procedures needed to have the
telescope up and running in minutes. Use this manual in conjunction with the on-screen instructions provided by the hand
control. The manual gives detailed information regarding each step as well as needed reference material and helpful hints
guaranteed to make your observing experience as simple and pleasurable as possible.
Your CPC telescope is designed to give you years of fun and rewarding observations. However, there are a few things to
consider before using your telescope that will ensure your safety and protect your equipment.
Warning
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Never look directly at the sun with the naked eye or with a telescope (unless you have the proper solar filter).
Permanent and irreversible eye damage may result.
Never use your telescope to project an image of the sun onto any surface. Internal heat build-up can damage the telescope
and any accessories attached to it.
Never use an eyepiece solar filter or a Herschel wedge. Internal heat build-up inside the telescope can cause these devices to
crack or break, allowing unfiltered sunlight to pass through to the eye.
Never leave the telescope unsupervised, either when children are present or adults who may not be familiar with the correct
operating procedures of your telescope.
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–
A
B
C
D
E
F
Figure2–TheCPCSeries
1
2
3
4
5
6
7
Control Panel (see below)
Focus Knob
8
9
Optical Tube
Schmidt Corrector Lens
Star Diagonal
10 Fork Arm
Hand Control
11 Carrying Handle
Eyepiece
12 Right Ascension Locking Knob
13 Tripod
Finderscope
Finderscope Quick Release Bracket
14 Accessory Tray / Center Support Bracket
A
B
C
Hand Control Port
Auxiliary Port s
D
E
F
Auto Guider Port
On/Off Switch
PC Interface Port
12v Input Jack
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The CPC telescope comes completely pre-assembled and can be operational in a matter of minutes. The CPC and its
accessories are conveniently packaged in one reusable shipping carton while the tripod comes in its own box. Included with
your telescope are the following:
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40mm Eyepiece – 1¼"
1¼" Star Diagonal
8x50 Finderscope and Quick Release Mounting Bracket
1¼" Visual Back
Car Battery Adapter
Heavy Duty Tripod
NexRemote Telescope Control Software w/ RS-232 cable
Assembling the CPC
Start by removing the telescope and tripod from their shipping cartons and set the telescopes round base on a sturdy flat
surface. Always carry the telescope by holding it from the lower portion of the fork arm on the hand control side and from
the handle on the opposite side. Remove all of the accessories from their individual boxes. Remember to save all of the
containers so that they can be used to transport the telescope. Before attaching the visual accessories, the telescope should be
mounted on the tripod and the tube should be positioned horizontal to the ground.
Setting up the Tripod
For maximum rigidity, the Celestron heavy duty tripod has a leg support bracket/accessory tray. This bracket fits snugly
against the tripod legs, increasing stability while reducing vibration and flexure. However, the tripod must be shipped with
the leg support bracket detached so the tripod legs can collapse. To set up the tripod:
1. Hold the tripod with the head up and the legs pointed toward the ground.
2. Pull the legs away from the central column until they will not separate any further. The top of each tripod leg presses
against the tripod head to indicate maximum separation.
3. Remove the tension knob, located on the central column. See figure 3-1.
4. Place the leg support bracket over the central rod so that the cups on the end of each bracket are directly underneath
each leg.
5. Rotate the tension knob until the bracket is secure against the tripod legs. Do not over tighten.
The tripod will now stand by itself. Once the telescope is attached to the tripod, readjust the tension knob to ensure that the
leg support bracket is snug. Once again, do not over tighten!
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Adjusting the Tripod Height
The tripod that comes with your CPC telescope is adjustable. There is a bubble level located on the top of the tripod head to assist you
in leveling the tripod. To adjust the height at which the tripod stands:
Tripod Head
Center Support
Bracket /
Central Column
Accessory tray
Tension Knob
Extension Leg
Clamp
Figure 3-1
1. Loosen the extension clamp on one of the tripod legs (see figure 3-1).
2. Extend the leg to the desired height.
3. Tighten the extension clamp to hold the leg in place.
4. Repeat this process for each of the remaining legs making sure that the tripod is level when complete.
You can do this while the tripod legs are still folded together.
Remember that the higher the tripod legs are extended, the less stable it is. For casual observing, this may not pose a problem.
However, if you plan on doing photography, the tripod should be set low to ensure stability. A recommended height is to set the tripod
in such a manner that you can look directly into the eyepiece on
the telescope with a diagonal while seated.
Attaching the CPC to the Tripod
After the tripod is set up, you are now ready to attach the
telescope. The bottom of the CPC base has three threaded
holes that mount to the tripod head and one hole in the center
that goes over the positioning pin on the tripod head.
Positioning
Pin
Mounting
Bolts
1. Place the center hole in the bottom of the telescope
base over the positioning pin in the center of the
tripod head.
Figure 3-2 Mounting the Telescope
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2. Rotate the telescope base on the tripod head until the three feet on the bottom of the base fall into the feet recesses on the top
of the tripod head.
3. Thread the three attached mounting bolts from underneath the tripod head into the bottom of the telescope base. Tighten all
three bolts.
You are now ready to attach the visual accessories onto the telescope optical tube.
Adjusting the Clutches
The CPC has a dual axis clutch system. This allows you to move the telescope manually even when the telescope is not powered on.
However, both clutches need to be tightened down for the telescope to be aligned for "goto" use. Any manual movement of the
telescope will invalidate your telescope's alignment.
Before attaching your visual accessories, first loosen the altitude locking knob while holding the telescope tube by the rear cell handle.
Rotate the tube upwards until it is level with the ground and tighten the locking knob.
Note: When transporting your telescope, make sure that both clutches are somewhat loose; this will diminish the load placed
on the worm gear assemblies and protect them from damage.
Azimuth
Locking Knob
Altitude
Locking
Knob
Figure 3-4 - The CPC has an altitude locking knobs (right) located on the fork arm and an
azimuth locking knob (left) located on the top of the base.
The Star Diagonal
The star diagonal diverts the light at a right angle from the light path of the telescope. For astronomical observing, this allows you to
observe in positions that are more comfortable than if you were to look straight through. To attach the star diagonal:
Finderscope
Mounting
Bracket
Eyepiece
1.
Turn the thumbscrew on the visual back until its tip no
longer extends into (i.e., obstructs) the inner diameter of
the visual back.
2.
3.
Slide the chrome portion of the star diagonal into the
visual back.
Tighten the thumbscrew on the visual back to hold the
star diagonal in place.
Star
Diagonal
If you wish to change the orientation of the star diagonal,
loosen the thumbscrew on the visual back until the star
diagonal rotates freely. Rotate the diagonal to the desired
position and tighten the thumbscrew.
Visual Back
Figure 3-5 - The Visual Accessories
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The Eyepiece
The eyepiece, is the optical element that magnifies the image focused by the telescope. The eyepiece fits into either the visual back
directly or the star diagonal. To install the eyepiece:
1. Loosen the thumbscrew on the star diagonal so it does not obstruct the inner diameter of the eyepiece end of the diagonal.
2. Slide the chrome portion of the eyepiece into the star diagonal.
3. Tighten the thumbscrew to hold the eyepiece in place.
To remove the eyepiece, loosen the thumbscrew on the star diagonal and slide the eyepiece out.
Eyepieces are commonly referred to by focal length and barrel diameter. The focal length of each eyepiece is printed on the eyepiece
barrel. The longer the focal length (i.e., the larger the number) the lower the eyepiece power or magnification; and the shorter the focal
length (i.e., the smaller the number) the higher the magnification. Generally, you will use low-to-moderate power when viewing. For
more information on how to determine power, see the section on “Calculating Magnification.”
Barrel diameter is the diameter of the barrel that slides into the star diagonal or visual back. The CPC uses eyepieces with a standard
1-1/4" barrel diameter.
The Finderscope
The CPC telescope comes with an 8x50 finderscope. The specifications for a finderscope stand for the magnification and the
aperture, in millimeters, of the scope. So, an 8x50 finder magnifies objects eight times and has a 50mm objective lens.
Finderscope Installation
The finderscope must first be mounted in the included quick-release bracket then attached to the rear cell of the telescope. To
install the finderscope:
1. Locate the finderscope mounting bracket attached to the bottom portion of the finder bracket. Loosen the two thumb screws
to slide the mounting bracket from the finderscope bracket.
2. Find the two holes in the rear cell of the telescope on the top left, when looking from the back of the tube.
3. Place the mounting bracket over the two holes of the rear cell as shown in the figure 3-7.
4. Insert the screws through the bracket and into the rear cell.
Figure 3-6
WARNING: If you remove the mounting bracket, do not completely thread the screws back into the rear cell of the telescope. The
screws may be long enough to obstruct the movement of, and possibly damage the primary mirror.
Figure 3-7
The finderscope bracket comes in two pieces; the mounting bracket (left) and the finder bracket (right)
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With the bracket firmly attached to the telescope, you are ready to attach the finder to the bracket.
1. Slide the O-Ring over the back of the finderscope and position it on the tube toward the objective end of the finderscope.
Alignment Screws
2. Slide the eyepiece end of the finderscope into the front
ring of the bracket (the front ring is the one without the
adjustment screws), then through the back ring. It may
be necessary to push down the spring loaded pivot
screw so that the finder will pass through the back ring
(see figure 3-8)
Pivot
Screw
Quick release
Screws
3. Push the finder back until the O-Ring is snug inside the
front ring of the finder bracket.
4. Hand tighten the two adjustment thumb screws until
they make contact with the findersocpe.
Figure 3-8
Aligning the Finderscope
The finderscope is adjusted using two adjustment screws, located on the top and on the right (when looking though the finder) of the
finder bracket and a spring loaded pivot screw (located on the left side of the bracket). This allows you to turn the top adjustment
screw to move the finderscope up and down, and turn the right adjustment screw to move the finderscope right to left. The spring
loaded pivot screw puts constant pressure on the finder so that the adjustment screws are always making contact with the finder.
To make the alignment process a little easier, you should perform this task in the daytime when it is easier to locate objects in the
telescope without the finder. To align the finder:
1. Choose a conspicuous object that is in excess of one mile away. This will eliminate any possible parallax effect between the
telescope and the finder.
2. Point your telescope at the object you selected and center it in the main optics of the telescope.
3. Lock the azimuth and altitude clamps to hold the telescope in place.
4. Check the finder to see where the object is located in the field of view.
5. Adjust the thumb screws on the finder bracket, until the cross hairs are centered on the target.
Remember that the image orientation through the finder is inverted (i.e., upside down and reversed from left-to-right). Because of this,
it may take a few minutes to familiarize yourself with the directional change each screw has on the finder
Attaching the Hand Control
In order to protect your CPC telescope during shipping, the hand control unit has been packaged along with the other telescope
accessories and will need to be plugged in to the drive base of your telescope. The hand control cable has a phone jack style connector
that will plug into the designated jack outlet located on the top of the drive base (see figure 3-10). Your telescope also comes with a
hand control holder that must be attached to the fork arm. To connect the hand control to the
fork arm:
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Locate the hand control holder and slide it down into the slot located on the
fork arm (see figure 3-9)
•
Push the connector into the jack until it clicks into place.
The hand control can now rest in the holder on the fork arm of the telescope.
Figure 3-9
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Powering the CPC
The CPC can be powered by the supplied 12v car battery adapter or optional power supply (see Optional Accessories section in the
back of this manual).
1. To power the CPC with the car battery adapter, simply plug the round post into the designated 12v power outlet located on
the drive base.
2. Turn on the power to the CPC by flipping the switch, located next to the 12v outlet, to the "On" position.
Hand Control
Port
On/Off Switch
12v Input Jack
Figure 3-10
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The CPC is controlled by Celestron’s NexStar hand controller designed to give you instant access to all the functions the
CPC has to offer. With automatic slewing to over 40,000 objects, and common sense menu descriptions, even a beginner
can master its variety of features in just a few observing sessions. Below is a brief description of the individual components
of the CPC’s NexStar hand controller:
1. Liquid Crystal Display (LCD) Window: Has a dual-line, 16 character display screen that is backlit for
comfortable viewing of telescope information and scrolling text.
2. Align: Instructs the CPC to use a selected star or object as an alignment position.
3. Direction Keys: Allows complete control of the CPC in any direction. Use the direction keys to move the
telescope to the initial alignment stars or for centering objects in the eyepiece.
4. Catalog Keys: The NexStar hand control has keys to allow direct access to each of the catalogs in its database.
The hand control contains the following catalogs in its database:
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10
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5
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6
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Figure 4-1
The NexStar Hand Control
Messier– Complete list of all Messier objects.
NGC – Complete list of all the deep-sky objects in the Revised New General Catalog.
Caldwell – A combination of the best NGC and IC objects.
Planets - All 8 planets in our Solar System plus the Moon and the Sun.
Stars – A compiled list of the brightest stars from the SAO catalog.
List – For quick access, all of the best and most popular objects in the NexStar database have been broken
down into lists based on their type and/or common name:
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Common name listing of the brightest stars in the sky.
Alphabetical listing of over 50 of the most popular deep
sky objects.
Named Stars
Named Objects
Numeric-alphabetical listing of the most visually stunning
double, triple and quadruple stars in the sky.
Select list of the brightest variable stars with the shortest
period of changing magnitude.
A unique list of some of the most recognizable star
patterns in the sky.
Double Stars
Variable Stars
Asterisms
A custom list of many interesting galaxy pairs, trios and
clusters that are well suited for CCD imaging with the
CPC telescope.
CCD Objects
A complete list of all the Index Catalog deep-sky objects.
A complete list of all the Abell Catalog deep-sky objects.
IC Objects
Abell Objects
5. Info: Displays coordinates and useful information about objects selected from the NexStar database.
6. Tour: Activates the tour mode, which seeks out all the best objects for the current date and time, and
automatically slews the CPC to those objects.
7. Enter: Pressing Enter allows you to select any of the CPC functions and accept entered parameters.
8. Undo: Undo will take you out of the current menu and display the previous level of the menu path. Press Undo
repeatedly to get back to a main menu or use it to erase data entered by mistake.
9. Menu: Displays the many setup and utilities functions such as tracking rate and user defined objects and many
others.
10. Scroll Keys: Used to scroll up and down within any of the menu lists. A double-arrow will appear on the right
side of the LCD when there are sub-menus below the displayed menu. Using these keys will scroll through those
sub-menus.
11. Rate: Instantly changes the rate of speed of the motors when the direction buttons are pressed.
12. RS-232 Jack: Allows you to interface with a computer and control the CPC remotely.
Hand Control Operation
This section describes the basic hand control procedures needed to operate the CPC. These procedures are grouped into
three categories: Alignment, Setup and Utilities. The alignment section deals with the initial telescope alignment as well as
finding objects in the sky; the setup section discusses changing parameters such as tracking mode, tracking rate and setting
filter and slew limits; finally, the last section reviews all of the utilities functions such as PEC, polar alignment and
hibernating the telescope.
Alignment Procedures
In order for the CPC to accurately point to objects in the sky, it must first be aligned to known positions (stars) in the sky.
With this information, the telescope can create a model of the sky, which it uses to locate any object with known
coordinates. There are many ways to align the CPC with the sky depending on what information the user is able to provide:
SkyAlign use the internal GPS receiver to acquire all the necessary time/site information needed for the CPC to create an
accurate model of the sky. Then the user can simply point the telescope to any three bright celestial objects to accurately
align the telescope with the sky. Auto Two-Star Align will ask the user to choose and center the first alignment star, then
the CPC will automatically select and slew to a second star for alignment. Two-Star Alignment requires the user to identify
and manually slew the telescope to the two alignment stars. One-Star Align is the same as Two-Star Align however only
requires you to align to one known star. Although not as accurate as the other alignment methods, One-Star Align is the
quickest way to find and track bright planets and objects in Altazimuth mode. Solar System Align will display a list of
visible daytime objects (planets and the moon) available to align the telescope. Finally, EQ North and EQ South
alignments are designed to assist you in aligning the CPC when polar aligned using an equatorial wedge. Each alignment
method is discussed in detail below.
Definition
"Altazimuth" or "Alt-Az" refers to a type of mounting that allows a telescope to move in both altitude (up and down)
and azimuth (left and right) with respect to the ground. This is the simplest form of mounting in which the telescope is attached
directly to a tripod without the use of an equatorial wedge.
Sky Align
Sky Align must be used with the telescope mounted in altazimuth. With Sky Align, the GPS receiver links with and acquires
information from 3 of the orbiting GPS satellites. With this information, the built-in GPS system calculates the scope’s
location on Earth with an accuracy of a few meters and calculates universal time down to the second. After quickly making
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all these calculations and automatically entering the information for you, the user simply needs to aim the telescope to any
three bright celestial objects in the sky. Since Sky Align requires no knowledge of the night sky it is not necessary to know
the name of the stars that you are aiming. You may even select a planet or the moon. The CPC is then ready to start finding
and tracking any of the objects in its 40,000+ object database. Before the telescope is ready to be aligned, it should be set up
in an outside location with all accessories (eyepiece, diagonal and finderscope) attached and lens cover removed as
described in the Assembly section of the manual. To begin Sky Align:
1. Power on the CPC by flipping the switch located on the
control panel of the drive base, to the "on" position. Once
turned on the hand control display will say CPC Ready.
Press ENTER to choose Sky Align or use the UP/Down
scroll keys (10) to select a different method of alignment.
Pressing the ALIGN key will bypass the other alignment
options and the scrolling text and automatically begins Sky
Align.
A Few Words on GPS:
The CPC uses an on-board GPS to take the
guesswork out of aligning your telescope with the
sky. Once an alignment method is selected, the
CPC automatically initiates the internal GPS
module. However, there are a few things you
should be aware of in order to get full use of its
many capabilities:
2. Once Sky Align has been selected, the hand control will
display “Enter if OK”, “Undo to edit” and “GPS Linking”.
The bottom line of the LCD will display either the current
time or the time when you last used the telescope. The GPS
will quickly link up and display the current date, time and
location. Additionally you have the option of pressing
UNDO and manually updating the time/site information.
Press ENTER to accept the time/site information
downloaded the GPS.
GPS alignment will only work when the
telescope is set-up outdoors with an
unobstructed view of the sky. If the CPC
is set-up in a location that has a limited
horizon in any direction it may take
longer for the telescope to find and link
with the needed satellites.
When using the GPS for the first time, it
may take 3-5 minutes for the CPC to
link-up with its satellites. Once the
telescope is successfully linked, leave the
telescope powered on for at least 20
minutes. During this time the CPC will
download the complete almanac of
orbital elements (called the ephemeris)
for the orbiting GPS satellites. Once this
information is received it will be stored
for future alignments.
3. The hand control will display a message reminding you to
level the tripod if you already haven’t done so. Press
ENTER to continue.
4. Use the arrow buttons on the hand control to slew (move)
the telescope towards any bright celestial object in the sky.
Center the object in the crosshairs of the finderscope and
press ENTER.
5. If the finderscope has been properly aligned with the
telescope tube, the alignment star should now be visible
inside the field of view of the eyepiece. The CPC will ask
that you center the bright alignment star in the center of the
eyepiece and press the ALIGN button. This will accept the
star as the first alignment position. (There is no need to
adjust the slewing rate of the motors after each alignment
step. The CPC automatically selects the best slewing rate
for aligning objects in both the finderscope and the
eyepiece).
If your CPC is transported over a long
distance (say from the northern to the
southern hemisphere) it may take as long
as one hour to establish a satellite link
from its new location. Observers wishing
to travel long distances with their
telescope are advised to turn on their
telescope in advance to allow the GPS to
acquire the necessary data.
6. For the second alignment object, choose a bright star or
planet as far as possible from the first alignment object.
Once again use the arrow button to center the object in the
finderscope and press ENTER. Then once centered in the
eyepiece press the ALIGN button.
7. Repeat the process for the third alignment star. When the telescope has been aligned to the final stars, the display
will read "Match Confirmed". Press UNDO to display the names of the three bright objects you aligned
to, or press ENTER to accept these three objects for alignment. You are now ready to find your first object.
Tips for Using Sky Align
Remember the following alignment guidelines to make using Sky Align as simple and accurate as possible.
•
•
Be sure to level the tripod before you begin alignment. The time/site information along with a level tripod will help
the telescope better predict the available bright stars and planets that are above the horizon.
Remember SkyAlign does not care where the optical tube is pointed at the beginning of the alignment. So to make
the alignment process even faster it is acceptable to move the telescope to the first alignment star manually by
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loosening both clutches. However the following alignment stars still need to found and centered using the hand
control.
•
•
Remember to select alignment stars that are as far apart in the sky as possible. For best results make sure that the
third alignment star does not lie in a straight line between the first two stars. This may result in a failed alignment.
Don’t worry about confusing planets for stars when selecting alignment objects. SkyAlign works with the four
brightest planets (Venus, Jupiter, Saturn and Mars) as well as the Moon. In addition to the planets, the hand control
has over 80 bright alignment stars to choose from (down to 2.5 magnitude).
•
•
Rarely SkyAlign will not be able to determine what three alignment objects were centered. This sometime happens
when a bright planet or the Moon passes near one of the brighter stars. In situations like these it is best to try to avoid
aligning to either object if possible.
For the best possible pointing accuracy, always center the alignment stars using the same final movements as the
direction of the GoTo Approach (by default this will be using the up arrow button and the right arrow button).
Approaching the star from this direction when looking through the eyepiece will eliminate much of the backlash
between the gears and assure the most accurate alignment possible.
Auto Two-Star Align
As with Sky Align, Auto Two-Star Align downloads all the necessary time/site information from orbiting GPS satellites.
Once this information is received, CPC will prompt you to slew the telescope and point at one known star in the sky. The
CPC now has all the information it needs to automatically choose a second star that will assure the best possible alignment.
Once selected the telescope will automatically slew to that second alignment star to complete the alignment. With the CPC
set up outside with all accessories attached and the tripod leveled, follow the steps below to align the telescope:
1. Once the CPC is powered on , Press ENTER to begin alignment.
2. Use the Up and Down scroll keys (10) to select Auto Two-Star Align and press ENTER.
3. The hand control will display the last time and location information that was entered or downloaded from the
GPS. Use the Up and Down buttons to scroll through the information. Press ENTER to accept the downloaded
information or press UNDO to manually edit the information.
4. The display will now prompt you to select a bright star from the displayed list on the hand control. Use Up and
Down buttons (6 and 9 on the keypad) to scroll to the desired star and then press ENTER.
5. Use the arrow buttons to slew the telescope to the star you selected. Center the star in the crosshairs of the
finderscope and press ENTER. Finally, center the star in the eyepiece and press ALIGN.
6. Based on this information, the CPC will automatically display the most suitable second alignemnt star that is
above the horizon. Press ENTER to automatically slew the telescope to the displayed star. If for some reason you
do not wish to select this star (perhaps it is behind a tree or building), you can either:
•
•
Press the UNDO button to display the next most suitable star for alignment.
Use the UP and DOWN scroll buttons to manually select any star you wish from the entire list of available
stars.
Once the desired star is displayed press ENTER to automatically slew the telescope to the displayed star. When
finished slewing, the display will ask you to use the arrow buttons to align the selected star with the cross hairs in the
center of the finderscope. Once centered in the finder, press ENTER. The display will then instruct you to center the
star in the field of view of the eyepiece. When the star is centered, press ALIGN to accept this star as your second
alignment star. When the telescope has been aligned to both stars the display will read Alignment Success, and
you are now ready to find your first object.
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Two Star Alignment
With the two-star alignment method, the CPC requires the user to know the positions of two bright stars in order to
accurately align the telescope with the sky and begin finding objects. Here is an overview of the two-star alignment
procedure:
1. Once the CPC is powered on, use the Up and Down scroll keys (10) to select Two-Star Align, and press ENTER.
2. Press ENTER to accept the time/site information displayed on the display, or wait until the telescope has
downloaded the information from the GPS satellites.
3. The SELECT STAR 1 message will appear in the top row of the display. Use the Up and Down scroll keys (10) to
select the star you wish to use for the first alignment star. Press ENTER.
4. CPC then asks you to center in the eyepiece the alignment star you selected. Use the direction arrow buttons to
slew the telescope to the alignment star and carefully center the star in the finderscope. Press ENTER when
centered.
5. Then, center the star in the eyepiece and press ALIGN
Helpful
Hint
In order to accurately center the alignment star in the eyepiece, you may wish to decrease the slew rate of the motors for
fine centering. This is done by pressing the RATE key (11) on the hand controller then selecting the number that
corresponds to the speed you desire. (9 = fastest , 1 = slowest).
6. CPC will then ask you to select and center a second alignment star and press the ALIGN key. It is best to choose
alignment stars that are a good distance away from one another. Stars that are at least 40º to 60º apart from each
other will give you a more accurate alignment than stars that are close to each other.
Once the second star alignment is completed properly, the display will read Alignment Successful, and you should
hear the tracking motors turn-on and begin to track.
One-Star Align
One-Star Align allows you to download all the same information as you would for the Two-Star Align procedure. However,
instead of slewing to two alignment stars for centering and alignment, the CPC uses only one star to model the sky based on
the information given. This will allow you to roughly slew to the coordinates of bright objects like the moon and planets
and gives the CPC the information needed to track objects in altazimuth in any part of the sky. Quick-Align is not meant to
be used to accurately locate small or faint deep-sky objects or to track objects accurately for photography.
To use One-Star Align:
1.
2.
Select One-Star Align from the alignment options.
Press ENTER to accept the time/site information displayed on the display, or wait until the telescope has
downloaded the information from the GPS satellites.
3.
4.
The SELECT STAR 1 message will appear in the top row of the display. Use the Up and Down scroll keys (10)
to select the star you wish to use for the first alignment star. Press ENTER.
CPC then asks you to center in the eyepiece the alignment star you selected. Use the direction arrow buttons to
slew the telescope to the alignment star and carefully center the star in the finderscope. Press ENTER when
centered.
5.
6.
Then, center the star in the eyepiece and press ALIGN
Once in position, the CPC will model the sky based on this information and display Alignment
Successful.
Note: Once a One-Star Alignment has been done, you can use the Re-alignment feature (later in this section ) to improve your
telescope’s pointing accuracy.
Solar System Align
Solar System Align is available in alt-az mode (scope mounted directly on the tripod) and equatorial mode (scope mounted
on a wedge). Solar System Align is designed to provide excellent tracking and GoTo performance by using solar system
objects (Sun, Moon and planets) to align the telescope with the sky. Solar System Align is a great way to align your
telescope for daytime viewing as well as a quick way to align the telescope for night time observing.
Never look directly at the sun with the naked eye or with a telescope (unless you have the proper solar filter).
Permanent and irreversible eye damage may result.
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1. Select Solar System Align from the alignment options.
2. Press ENTER to accept the time/site information displayed on the display, or wait until the telescope has
downloaded the information from the GPS satellites.
3. The SELECT OBJECT message will appear in the top row of the display. Use the Up and Down scroll keys (10) to
select the daytime object (planet, moon or sun) you wish to align. Press ENTER.
4. CPC then asks you to center in the eyepiece the alignment object you selected. Use the direction arrow buttons to
slew the telescope to the alignment object and carefully center it in the finderscope. Press ENTER when centered.
5. Then, center the object in the eyepiece and press ALIGN.
Once in position, the CPC will model the sky based on this information and display Alignment Successful.
Tips for Using Solar System Align
•
For safety purposes, the Sun will not be displayed in any of the hand control’s customer object lists unless it is
enabled from the Utilities Menu. To allow the Sun to be displayed on the hand control, do the following:
1. Press the UNDO button until the display reads “CPC Ready”
2. Press the MENU button and use the Up and Down keys to select the Utilities menu. Press ENTER.
3. Use the UP and Down keys to select Sun Menu and press ENTER.
4. Press ENTER again to allow the Sun to appear on the hand control display.
The Sun can be removed from the display by using the same procedure as above.
•
To improve the telescope pointing accuracy, you can use the Re-Align feature as described below.
EQ North / EQ South Alignment
EQ North and EQ South Alignments assist the user in aligning the telescope when polar aligned on an optional equatorial
wedge. Similar to the Altazimuth alignments described earlier, the EQ alignments gives you the choice of performing an
AutoAlign, Two-Star alignment, One-Star alignment or Solar System alignment.
EQ AutoAlign
The EQ AutoAlign uses all the same time/site information as the Alt-Az alignments, however it also requires you to position
the tube so that the altitude index markers are aligned (see figure 4-2), and then rotate the telescope base until the tube is
pointed towards the Meridian (see figure 4-3). Based on this information the CPC will automatically slew to two selected
alignment stars to be centered and aligned. To use EQ Auto-Align:
1. Select EQ North or South Align from the alignment options and press ENTER
2. Press ENTER to accept the time/site information displayed on the display, or wait until the telescope has
downloaded the information from the GPS satellites.
3. Select EQ AutoAlign method and press ENTER
4. Use the up and down arrow buttons to move the telescope tube upwards until the altitude index markers are
aligned. The altitude index markers are located at the top of the fork arm. See figure 4-2.
5. Use the left and right arrow buttons to move the telescope base until the fork arms are horizontally parallel and the
tube is pointing towards the Meridian.
6. Based on this information, the CPC will automatically display the most suitable alignment stars that are above the
horizon. Press ENTER to automatically slew the telescope to the displayed star. If for some reason you do not
wish to select one of these stars (perhaps it is behind a tree or building), you can either:
•
•
Press the UNDO button to display the next most suitable star for alignment.
Use the UP and DOWN scroll buttons to manually select any star you wish from the entire list of available
stars.
7. CPC then asks you to center in the eyepiece the alignment object you selected.
Use the direction arrow buttons to slew the telescope to the alignment object and
carefully center it in the finderscope. Press ENTER when centered.
8. Then, center the object in the eyepiece and press ALIGN.
9. Once you press the ALIGN button the telescope will automatically slew to a
second alignment star. Repeat steps 6 and 7 to complete alignment.
Figure 4-2 - Altitude Index Markers
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EQ Two-Star Align
The EQ Two-Star Align follows most of the same steps as the Alt-Az Two-Star Align. This alignment method does not
require the user to align the altitude index markers or point towards the Meridian, but it does require the user to locate and
align the telescope on two bright stars. When selecting alignment stars it is best to choose stars that, a) have a large
separation in azimuth and b) both are either positive or negative in declination. Following these two guidelines will result in
a more accurate EQ Two-Star alignment.
EQ One-Star Align
EQ One-Star Align operates much the same way as EQ Two-Star Align however it only relies on the alignment of one star
to align the telescope. To use EQ One-Star Align follow steps 1 through 7 under the EQ Two-Star Align section.
EQ Solar System Align
This alignment method allows you use only one solar system object to
equatorially align the telescope for daytime use. To align your telescope
using a solar system object follow steps 1 through 7 under the EQ Two-Star
Align section.
CPC Re-Alignment
The CPC has a re-alignment feature which allows you to replace
either of the original alignment stars with a new star or celestial
object. This can be useful in several situations:
•
•
If you are observing over a period of a few hours, you may
notice that your original alignment stars have drifted towards
the west considerably. (Remember that the stars are moving
at a rate of 15º every hour). Aligning on a new star that is in
the eastern part of the sky will improve your pointing
accuracy, especially on objects in that part of the sky.
If you have aligned your telescope using the One-Star or
Solar System alignment method, you can use re-align to
align to additional objects in the sky. This will improve the
pointing accuracy of your telescope without having to re-
enter addition information.
Figure 4-3
The Meridian is an imaginary line in the sky that
starts at the North celestial pole and ends at
the South celestial pole and passes through the
zenith. If you are facing South, the meridian
starts from your Southern horizon and passes
directly overhead to the North celestial pole.
To replace an existing alignment star with a new alignment star:
1. Select the desired star (or object) from the database and slew to it.
2. Carefully center the object in the eyepiece.
3. Once centered, press the UNDO button until you are at the main menu.
4. With CPC Readydisplayed, press the ALIGN key on the hand control.
5. The display will then ask you which alignment star you want to replace. Use the UP and Down scroll keys to
select the alignment star to be replaced. It is usually best to replace the star closest to the new object. This will
space out your alignment stars across the sky. If you have used one of the single object alignment methods then it
is always best to replace the object that is “unassigned” with an actual object.
6. Press ALIGN to make the change.
Selecting an Object
Now that the telescope is properly aligned, you can choose an object from any of the catalogs in the CPC's extensive
database. The hand control has a key (4) designated for each of the catalogs in its database. There are two ways to select
objects from the database: scrolling through the named object lists and entering object numbers.
Helpful
Hint
Pressing the LIST key on the hand control will access all objects in the database that have common names or types. Each list
is broken down into the following categories: Named Stars, Named Object, Double Stars, Variable Stars, Asterisms and
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CCD Objects. Selecting any one of these catalogs will display a numeric-alphabetical listing of the objects under that list.
Pressing the Up and Down keys (10) allows you to scroll through the catalog to the desired object.
When scrolling through a long list of objects, holding down either the Up or Down key will allow you to scroll through the
catalog at a rapid speed.
Pressing any of the other catalog keys (M, CALD, NGC, or STAR) will display a blinking cursor below the name of the catalog chosen.
Use the numeric key pad to enter the number of any object within these standardized catalogs. For example, to find the Orion Nebula, press
the "M" key and enter "042".
When entering the number for a SAO star, you are only required to enter the first four digits of the objects six digit SAO
number. Once the first four digits are entered, the hand control will automatically list all the available SAO objects
beginning with those numbers. This allows you to scroll through only the SAO stars in the database. For example, in
searching for the SAO star 40186 (Capella), the first four digits would be "0401". Entering this number will display the
closest match from the SAO stars available in the database. From there you can scroll down the list and select the desired
object.
Slewing to an Object
Once the desired object is displayed on the hand control screen, choose from the following options:
•
•
Press the INFO Key. This will give you useful information about the selected object such as R.A. and
declination, magnitude size and text information for many of the most popular objects.
Press the ENTER Key. This will automatically slew the telescope to the coordinates of the object.
Caution: Never slew the telescope when someone is looking into the eyepiece. The telescope can move at fast slew
speeds and may hit an observer in the eye.
If you manually enter an object that is below the horizon, CPC will notify you by displaying a message reminding you that
you have selected an object outside of your slew limits (see Slew Limits in the Scope Setup section of the manual). Press
UNDO to go back and select a new object. Press ENTER to ignore the message and continue the slew.
Object information can be obtained without having to do a star alignment. After the telescope is powered on, pressing any
of the catalog keys allows you to scroll through object lists or enter catalog numbers and view the information about the
object as described above.
Finding Planets
The CPC can located all 8 of our solar systems planets plus the Sun and Moon. However, the hand control will only display
the solar system objects that are above the horizon (or within its filter limits). To locate the planets, press the PLANET key
on the hand control. The hand control will display all solar system objects that are above the horizon:
•
•
•
Use the Up and Down keys to select the planet that you wish to observe.
Press INFO to access information on the displayed planet.
Press ENTER to slew to the displayed planet.
To allow the Sun to be displayed as an option in the database, see Sun Menu in the Utilities section of the manual.
Tour Mode
The CPC includes a tour feature which automatically allows the user to choose from a list of interesting objects based on the
date and time in which you are observing. The automatic tour will display only those objects that are within your set filter
limits (see Filter Limits in the Setup Procedures section of the manual). To activate the Tour mode, press the TOUR key (6)
on the hand control. The CPC will display the best objects to observe that are currently in the sky.
•
•
•
To see information and data about the displayed object, press the INFO key.
To slew to the object displayed, press ENTER.
To see the next tour object, press the Up key.
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Constellation Tour
In addition to the Tour Mode, the CPC telescope has a Constellation Tour that allows the user to take a tour of all the best
objects within a particular constellation. Selecting Constellation from the LIST menu will display all the constellation
names that are above the user defined horizon (filter limits). Once a constellation is selected, you can choose from any of
the database object catalogs to produce a list of all the available objects in that constellation.
•
•
•
To see information and data about the displayed object, press the INFO key.
To slew to the object displayed, press ENTER.
To see the next tour object, press the Up key.
Direction Buttons
The CPC has four direction buttons (3) in the center of the hand control which control the telescope's motion in altitude (up
and down) and azimuth (left and right). The telescope can be controlled at nine different speed rates.
Rate Button
Pressing the RATE key (11) allows you to instantly change the speed rate of the motors from high speed slew rate to precise
guiding rate or anywhere in between. Each rate corresponds to a number on the hand controller key pad. The number 9 is
the fastest rate (3º per second, depending on power source) and is used for slewing between objects and locating alignment
stars. The number 1 on the hand control is the slowest rate (.5x sidereal) and can be used for accurate centering of objects in
the eyepiece and photographic guiding. To change the speed rate of the motors:
•
•
Press the RATE key on the hand control. The LCD will display the current speed rate.
Press the number on the hand control that corresponds to the desired speed. The number will
appear in the upper-right corner of the LCD display to indicate that the rate has been changed.
The hand control has a "double button" feature that allows you to instantly speed up the motors without having to choose a
speed rate. To use this feature, simply press the arrow button that corresponds to the direction that you want to move the
telescope. While holding that button down, press the opposite directional button. This will increase the slew rate to the
maximum slew rate.
When pressing the Up and Down arrow buttons in the slower slew rates (6 and lower) the motors will move the telescope in
the opposite direction than the faster slew rates (7 thru 9). This is done so that an object will move in the appropriate
direction when looking into the eyepiece (i.e. pressing the Up arrow button will move the star up in the field of view of the
eyepiece). However, if any of the slower slew rates (rate 6 and below) are used to center an object in the finderscope, you
may need to press the opposite directional button to make the telescope move in the correct direction.
1 = .5x*
6 = 64x
2 = 1x (sidereal)*
3 = 4x
4 = 8x
7 = .5º / sec
8 = 2º / sec
9 = 3º / sec
5 = 16x
Nine available slew speeds
*Rate 1 and 2 are photographic guide rates and are meant to be used when the telescope is set up on a wedge in equatorial
mode. These rates can be used while set up in altazimuth, however the actual speed rate may differ slightly.
Setup Procedures
The CPC contains many user defined setup functions designed to give the user control over the telescope's many advanced
features. All of the setup and utility features can be accessed by pressing the MENU key and scrolling through the options:
Tracking Mode This allows you to change the way the telescope tracks depending on the type of mount being
used to support the telescope. The CPC has three different tracking modes:
This is the default tracking rate and is used when the telescope is placed on
Alt-Az
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a flat surface or tripod without the use of an equatorial wedge. The
telescope must be aligned with two stars before it can track in altazimuth
(Alt-Az).
Used to track the sky when the telescope is polar aligned using an
equatorial wedge in the Northern Hemisphere.
EQ North
EQ South
Off
Used to track the sky when the telescope is polar aligned using an
equatorial wedge in the Southern Hemisphere.
When using the telescope for terrestrial (land) observation, the tracking
can be turned off so that the telescope never moves.
Tracking Rate In addition to being able to move the telescope with the hand control buttons, the CPC will
continually track a celestial object as it moves across the night sky. The tracking rate can be
changed depending on what type of object is being observed:
This rate compensates for the rotation of the Earth by moving the
telescope at the same rate as the rotation of the Earth, but in the opposite
direction. When the telescope is polar aligned, this can be accomplished
by moving the telescope in right ascension only. When mounted in Alt-
Az mode, the telescope must make corrections in both R.A. and
declination.
Sidereal
Used for tracking the moon when observing the lunar landscape.
Used for tracking the Sun when solar observing.
Lunar
Solar
View Time-Site - Displays the current time and longitude/latitude downloaded from the GPS receiver. It will also
display other relevant time-site information like time zone, daylight saving and local sidereal time. Local sidereal time
(LST) is useful for knowing the right ascension of celestial objects that are located on the meridian at that time. View Time-
Site will always display the last saved time and location entered while it is linking with the GPS. Once current information
has been received, it will update the displayed information. If GPS is switched off, the hand control will only display the
last saved time and location.
User Defined Objects - The CPC can store up to 400 different user defined objects in its memory. The objects can be
daytime land objects or an interesting celestial object that you discover that is not included in
the regular database. There are several ways to save an object to memory depending on what
type of object it is:
Save Sky Object:
The CPC stores celestial objects to its database by saving its right ascension and declination
in the sky. This way the same object can be found each time the telescope is aligned. Once a
desired object is centered in the eyepiece, simply scroll to the "Save Sky Obj" command
and press ENTER. The display will ask you to enter a number between 1-200 to identify the
object. Press ENTER again to save this object to the database.
Save Land Object:
The CPC can also be used as a spotting scope on terrestrial objects. Fixed land objects can
be stored by saving their altitude and azimuth relative to the location of the telescope at the
time of observing. Since these objects are relative to the location of the telescope, they are
only valid for that exact location. To save land objects, once again center the desired object
in the eyepiece. Scroll down to the "Save Land Obj" command and press ENTER. The
display will ask you to enter a number between 1-200 to identify the object. Press ENTER
again to save this object to the database.
Save Database (Db)
Object:
This feature allows you to create your own custom tour of database objects by allowing you
to record the current position of the telescope and save the name of the object by selecting it
from any one of the database catalogs. These objects then can be accessed by selecting GoTo
Sky Object.
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Enter R.A. - Dec:
GoTo Object:
You can also store a specific set of coordinates for an object just by entering the R.A. and
declination for that object. Scroll to the "Enter RA-DEC " command and press ENTER.
The display will then ask you to enter first the R.A. and then the declination of the desired
object.
To go to any of the user defined objects stored in the database, scroll down to either GoTo
Sky Objor Goto Land Objand enter the number of the object you wish to select and
press ENTER. CPC will automatically retrieve and display the coordinates before slewing to
the object.
To replace the contents of any of the user defined objects, simply save a new object using one of the existing identification
numbers; CPC will replace the previous user defined object with the current one.
Get RA/DEC - Displays the right ascension and declination for the current position of the telescope.
Goto R.A/ Dec - Allows you to input a specific R.A. and declination and slew to it.
Identify
Identify Mode will search any of the CPC database catalogs or lists and display the name and offset distances to the nearest
matching objects. This feature can serve two purposes. First, it can be used to identify an unknown object in the field of
view of your eyepiece. Additionally, Identify Mode can be used to find other celestial objects that are close to the objects
you are currently observing. For example, if your telescope is pointed at the brightest star in the constellation Lyra,
choosing Identify and then searching the Named Star catalog will no doubt return the star Vega as the star you are observing.
However, by selecting Identify and searching by the Named Object or Messier catalogs, the hand control will let you know
that the Ring Nebula (M57) is approximately 6° from your current position. Searching the Double Star catalog will reveal
that Epsilon Lyrae is only 1° away from Vega. To use the Identify feature:
•
•
•
Press the Menu button and select the Identify option.
Use the Up/Down scroll keys to select the catalog that you would like to search.
Press ENTER to begin the search.
Note: Some of the databases contain thousands of objects, and can therefore take a minute or two to return the closest object.
Precise GoTo
The CPC has a precise goto function that can assist in finding extremely faint objects and centering objects closer to the
center of the field of view for astrophotography and CCD imaging. Precise Goto automatically searches out the closest
bright star to the desired object and asks the user to carefully center it in the eyepiece. The hand control then calculates the
small difference between its goto position and its centered position. Using this offset, the telescope will then slew to the
desired object with enhanced accuracy. To use Precise Goto:
1. Press the MENU button and use the Up/Down keys to select Precise Goto.
•
•
Choose Database to select the object that you want to observe from any of the database catalogs listed
Choose RA/DEC to enter a set of celestial coordinates that you wish to slew to.
2. Once the desired object is selected, the hand control will search out and display the closest bright star to your
desired object. Press ENTER to slew to the bright alignment star.
3. Use the direction buttons to carefully center the alignment star in the eyepiece.
Press ENTER to slew to the desired object.
To store a set of coordinates (R.A./Dec) permanently into the CPC database, save it as a User Defined Object as described
above.
Helpful
Hint
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Scope Setup Features
Setup Time-Site - Allows the user to customize the CPC display by changing time and location parameters (such as
time zone and daylight savings).
Anti-backlash – All mechanical gears have a certain amount of backlash or play between the gears. This play is evident
by how long it takes for a star to move in the eyepiece when the hand control arrow buttons are pressed (especially when
changing directions). The CPC's anti-backlash features allows the user to compensate for backlash by inputting a value
which quickly rewinds the motors just enough to eliminate the play between gears. The amount of compensation needed
depends on the slewing rate selected; the slower the slewing rate the longer it will take for the star to appear to move in the
eyepiece. There are two values for each axis, positive and negative. Positive is the amount of compensation applied when
you press the button, in order to get the gears moving quickly without a long pause. Negative is the amount of
compensation applied when you release the button, winding the motors back in the other direction to resume tracking. You
will need to experiment with different values (from 0-99); a value between 20 and 50 is usually best for most visual
observing, whereas a higher value may be necessary for photographic guiding. Positive backlash compensation is applied
when the mount changes its direction of movement from backwards to forwards. Similarly, negative backlash compensation
is applied when the mount changes its direction of movement from forwards to backwards. When tracking is enabled, the
mount will be moving in one or both axes in either the positive or negative direction, so backlash compensation will always
be applied when a direction button is released and the direction moved is opposite to the direction of travel.
MENU
To set the anti-backlash value, scroll down to the anti-backlash option and press
ENTER. While viewing an object in the eyepiece, observe the responsiveness of each of
the four arrow buttons. Note which directions you see a pause in the star movement after
the button has been pressed. Working one axis at a time, adjust the backlash settings
high enough to cause immediate movement without resulting in a pronounced jump
when pressing or releasing the button. Now, enter the same values for both positive and
negative directions. If you notice a jump when releasing the button, but setting the values
lower results in a pause when pressing the button, go with the higher value for positive,
but use a lower value for negative. CPC will remember these values and use them each
time it is turned on until they are changed.
SCOPE SETUP
SETUP TIME-SITE
ANTI-BACKLASH
AZM POSITIVE
AZM NEGATIVE
ALT POSITIVE
ALT NEGATIVE
SLEW LIMITS
Slew Limits – Sets the limits in altitude that the telescope can slew without
displaying a warning message. By default the slew limits are set to 0º to 90º and will only
display a warning message if an object is below the horizon. However, the slew limits
can be customized depending on your needs. For example, if you have certain
photographic accessories attached to your telescope preventing it from pointing straight-
up, you can set the maximum altitude limit to read 80º, thus preventing the telescope
from pointing to any objects that are greater than 80º in altitude without warning.
SLEW ALT MAX
SLEW ALT MIN
FILTER LIMITS
ALTMAX IN LIST
ALTMIN IN LIST
DIRECTION BUTTONS
GOTO APPROACH
Slew limits are applied relative to the base of the mount not the actual horizon.
So when setting the slew limits when using the telescope on an equatorial wedge
remember that a minimum slew limit of 0° would prevent the telescope from
slewing down past the celestial equator not the horizon. To set the slew limit so
that the telescope will slew to the horizon while on a wedge, you must set the minimum
slew limit to equal your latitude minus 90°.
AZM APPROACH
ALT APPROACH
AUTOGUIDE RATES
Helpful
Hint
AZM RATE
ALT RATE
CORDWRAP
UTILITIES
Filter Limits – When an alignment is complete, the CPC automatically knows which
celestial objects are above the horizon. As a result, when scrolling through the database
lists (or selecting the Tour function), the CPC hand control will display only those
objects that are known to be above the horizon when you are observing. You can
customize the object database by selecting altitude limits that are appropriate for your
location and situation. For example, if you are observing from a mountainous location
where the horizon is partially obscured, you can set your minimum altitude limit to read
+20º. This will make sure that the hand control only displays objects that are higher in
altitude than 20º. If you manually enter an object that is below the horizon using the
numeric keypad, the hand control will display a warning message before slewing to the
object.
GPS ON/OFF
WEDGE ALIGN
PEC
PLAYBACK
RECORD
LIGHT CONTROL
FACTORY SETTING
PRESS UNDO
PRESS "0"
VERSION
GET ALT-AZ
GOTO ALT-AZ
HIBERNATE
SUN MENU
SCROLLING MENU
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If you want to explore the entire object database, set the maximum altitude limit to 90º and the minimum limit to –90º. This
will display every object in the database lists regardless of whether it is visible in the sky from your location.
Observing
Tip!
Direction Buttons –The direction a star moves in the eyepiece varies depending on the accessories being used. This
can create confusion when guiding on a star using an off-axis guider versus a straight through guide scope. To compensate
for this, the direction of the drive control keys can be changed. To reverse the button logic of the hand control, press the
MENU button and select Direction Buttons from the Utilities menu. Use the Up/Down arrow keys (10) to select either the
azimuth (left and right) or altitude (up and down) button direction and press ENTER. Pressing ENTER again will reverse
the direction of the hand control buttons from their current state. Direction Buttons will only change the eyepiece rates (rate
1-6) and will not affect the slew rates (rate 7-9).
Goto Approach - lets the user define the direction that the telescope will approach when slewing to an object. This
allows the user the ability to minimize the effects of backlash For example, if your telescope is back heavy from using
heavy optical or photographic accessories attached to the back, you would want to set your altitude approach to the negative
direction. This would ensure that the telescope always approaches an object from the opposite direction as the load pulling
on the scope. Similarly, if using the CPC polar aligned on a wedge, you would want to set the azimuth approach to the
direction that allows the scope to compensate for different load level on the motors and gears when pointing in different
parts of the sky.
To change the goto approach direction, simply choose Goto Approach from the Scope Setup menu, select either Altitude or
Azimuth approach, choose positive or negative and press Enter.
Autoguide Rate – Allows the user to set an autoguide rate as a percentage of sidereal rate. This is helpful when
calibrating your telescope to a CCD autoguider for long exposure photography.
Cordwrap - – Cord wrap safeguards against the telescope slewing more than 360º in azimuth and wrapping accessory
cables around the base of the telescope. This is useful when autoguiding or any time that cables are plugged into the base of
the telescope. By default, the cord wrap feature is turned off when the telescope is aligned in altazimuth and turn on when
aligned on a wedge.
Utility Features
Scrolling through the MENU (9) options will also provide access to several advanced utility functions within the CPC such
as; Compass Calibration, Periodic Error Correction, Hibernate as well as many others.
GPS On/Off - Allows you to turn off the GPS module. When aligning the telescope, the CPC still receives information,
such as current time, from the GPS. If you want to use the CPC database to find the coordinates of a celestial object for a
future date you would need to turn the GPS module off in order to manually enter a date and time other than the present.
Wedge Align – The CPC has two equatorial alignment modes (one for the northern hemisphere and one for the southern)
that will help you to polar align your telescope when using an optional equatorial wedge. See the Astronomy Basics section
of the manual for more information on the Wedge Align feature.
Periodic Error Correction (PEC) - PEC is designed to improve photographic quality by reducing the amplitude of
the worm gear errors and improving the tracking accuracy of the drive. This feature is for advanced astrophotography and is
used when your telescope is polar aligned with the optional equatorial wedge. For more information on using PEC, see the
section on “Celestial Photography”.
Light Control – This feature allows you to turn off both the red key pad light and LCD display for daytime use to
conserve power and to help preserve your night vision.
Factory Setting – Returns the CPC hand control to its original factory setting. Parameters such as backlash
compensation values, initial date and time, longitude/latitude along with slew and filter limits will be reset. However, stored
parameters such as PEC and user defined objects will remain saved even when Factory Settings is selected. The hand
control will ask you to press the "0" key before returning to the factory default setting.
Version - Selecting this option will allow you to see the current version number of the hand control and motor control
software. The first set of numbers indicate the hand control software version. For the motor control, the hand control will
display two sets of numbers; the first numbers are for azimuth and the second set are for altitude.
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Get Alt-Az - Displays the relative altitude and azimuth for the current position of the telescope.
Goto Alt-Az - Allows you to enter a specific altitude and azimuth position and slew to it.
Hibernate - Hibernate allows the CPC to be completely powered down and still retain its alignment when turned back
on. This not only saves power, but is ideal for those that have their telescopes permanently mounted or leave their
telescope in one location for long periods of time. To place your telescope in Hibernate mode:
1. Select Hibernate from the Utility Menu.
2. Move the telescope to a desire position and press ENTER.
3. Power off the telescope. Remember to never move your telescope manually while in Hibernate mode.
Once the telescope is powered on again the display will read Wake Up. After pressing Enter you have the option of
scrolling through the time/site information to confirm the current setting. Press ENTER to wake up the telescope.
Helpful
Hint
Pressing UNDO at the Wake Up screen allows you to explore many of the features of the hand control without waking the
telescope up from hibernate mode. To wake up the telescope after UNDO has been pressed, select Hibernate from the
Utility menu and press ENTER. Do not use the direction buttons to move the telescope while in hibernate mode.
Sun Menu
For safety purposes the Sun will not be displayed as a database object unless it is first enabled. The enable the Sun, go to the
Sun Menu and press ENTER. The Sun will now be displayed in the Planets catalog as can be used as an alignment object
when using the Solar System Alignment method. To remove the Sun from displaying on the hand control, once again select
the Sun Menu from the Utilities Menu and press ENTER.
Scrolling Menu
This menus allows you to change the rate of speed that the text scrolls across the hand control display.
•
•
Press the Up (number 6) button to increase the speed of the text.
Press the Down (number 9) button to decrease the speed of the text.
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CPC Ready
MENU
ALIGNMENT
LIST
NAMED STAR
NAMED OBJECT
ASTERISM
TOUR
TRACKING
MODE
SKY ALIGN
GPS LINKING...
VARIABLE STAR
DOUBLE STAR
CCD OBJECTS
ABELL
IC CATALOG
CALDWELL
MESSIER
NGC
SAO
SOLAR SYSTEM
CONSTELLATION
Center Alignment Object 1
Center Alignment Object 2
Center Alignment Object 3
ALT-AZ
EQ NORTH
EQ SOUTH
OFF
RATE
AUTO TWO-STAR ALIGN
SIDEREAL
SOLAR
LUNAR
GPS LINKING...
Select Star 1
VIEW TIME-SITE
SCOPE SETUP
Center Star 1
Center Star 2
TWO-STAR ALIGNMENT
SETUP TIME-SITE
ANTI-BACKLASH
SLEW LIMITS
FILTER LIMITS
DIRECTION BUTTONS
GOTO APPROACH
AUTOGUIDE RATE
CORDWRAP
GPS LINKING...
SELECT STAR 1
UTILITIES
CENTER STAR 1
SELECT STAR 2
GPS ON/OFF
WEDGE ALIGN
PEC
LIGHT CONTROL
FACTORY SETTING
VERSION
GET ALT-AZ
GOTO ALT-AZ
HIBERNATE
CENTER STAR 2
ONE-STAR ALIGNMENT
GPS LINKING...
Select Star 1
SUN MENU
SCROLLING TEXT
USER OBJECTS
Center Star 1
SOLAR SYSTEM ALIGN
GPS LINKING...
Select Object
GOTO SKY OBJ
SAVE SKY OBJ
SAVE DB OBJ
ENTER RA & DEC
SAVE LAND OBJ
GOTO LAND OBJ
GET RA-DEC
Center Object
EQ ALIGNMENT
GOTO RA-DEC
INDENTIFY
GPS LINKING...
EQ AUTOALIGN
SELECT CATALOG
PRECISE GOTO
EQ TWO-STAR ALIGN
EQ ONE-STAR ALIGN
EQ SOLAR SYSTEM ALIGN
DATABASE
RA / DEC
CPC Menu Tree:
The following figure is a menu tree showing the sub-menus associated with the
primary command functions
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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. The Schmidt-Cassegrain
optical system (or Schmidt-Cass for short) uses a combination of mirrors and lenses and is referred to as a compound or
catadioptric telescope. This unique design offers large-diameter optics while maintaining very short tube lengths, making them
extremely portable. The Schmidt-Cassegrain system consists of a zero power corrector plate, a spherical primary mirror, and a
secondary mirror. Once light rays enter the optical system, they travel the length of the optical tube three times.
Figure 5-1
A cutaway view of the light path of the Schmidt-Cassegrain optical design
The optics of the CPC have Starbright coatings - enhanced multi-layer coatings on the primary and secondary mirrors for
increased reflectivity and a fully coated corrector for the finest anti-reflection characteristics.
Inside the optical tube, a black tube extends out from the center hole in the primary mirror. This is the primary baffle tube and it
prevents stray light from passing through to the eyepiece or camera.
Image Orientation
The image orientation changes depending on how the eyepiece is inserted into the telescope. When using the star diagonal, the
image is right-side-up, but reversed from left-to-right (i.e., mirror image). If inserting the eyepiece directly into the visual back
(i.e., without the star diagonal), the image is upside-down and reversed from left-to-right (i.e., inverted). This is normal for the
Schmidt-Cassegrain design.
Actual image orientation as seen
with the unaided eye
Inverted image, as viewed with
the eyepiece directly in telescope
Reversed from left to right, as
viewed with a Star Diagonal
Figure 5-2
Focusing
The CPC'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
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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.
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:
Figure 5-3
The emblem on the end of
the focus knob shows the
correct rotational direction
Focal Length of Telescope (mm)
for focusing the CPC.
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 CPC 8 for example has a focal length of 2032mm) by the focal length of the eyepiece, 40mm.
Dividing 2032 by 40 yields a magnification of 51 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 CPC 8 is 8 inches in diameter. Multiplying 8 by
60 gives a maximum useful magnification of 480 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 160 to 280 times for the CPC 8 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 51 power. This yields an actual field of .9°, or 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 example, multiply the angular field .9° by 52.5. This produces a linear field width of 47 feet at a distance of one
thousand yards. The apparent field of each eyepiece that Celestron manufactures is found in the Celestron Accessory Catalog
(#93685).
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 affect 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.
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•
•
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 difficult to focus when viewing terrestrially. The amount of detail seen under
these conditions is greatly reduced. Also, when photographing under these conditions, the processed film may come out a
little grainier than normal with lower contrast and underexposed.
•
If you wear corrective lenses (specifically 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.
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Up to this point, this manual covered the assembly and basic operation of your CPC telescope. However, to understand your
telescope more thoroughly, you need to know a little about the night sky. This section deals with observational astronomy
in general and includes information on the night sky and polar alignment.
The Celestial Coordinate System
To help find objects in the sky, astronomers use a celestial coordinate system that is similar to our geographical coordinate
system here on Earth. The celestial coordinate system has poles, lines of longitude and latitude, and an equator. For the
most part, these remain fixed against the background stars.
The celestial equator runs 360 degrees around the Earth and separates the northern celestial hemisphere from the southern.
Like the Earth's equator, it bears a reading of zero degrees. On Earth this would be latitude. However, in the sky this is
referred to as declination, or DEC for short. Lines of declination are named for their angular distance above and below the
celestial equator. The lines are broken down into degrees, minutes of arc, and seconds of arc. Declination readings south of
the equator carry a minus sign (-) in front of the coordinate and those north of the celestial equator are either blank (i.e., no
designation) or preceded by a plus sign (+).
The celestial equivalent of longitude is called Right Ascension, or R.A. for short. Like the Earth's lines of longitude, they
run from pole to pole and are evenly spaced 15 degrees apart. Although the longitude lines are separated by an angular
distance, they are also a measure of time. Each line of longitude is one hour apart from the next. Since the Earth rotates
once every 24 hours, there are 24 lines total. As a result, the R.A. coordinates are marked off in units of time. It begins with
an arbitrary point in the constellation of Pisces designated as 0 hours, 0 minutes, 0 seconds. All other points are designated
by how far (i.e., how long) they lag behind this coordinate after it passes overhead moving toward the west.
Figure 6-1
The celestial sphere seen from the outside showing R.A. and DEC.
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Motion of the Stars
The daily motion of the Sun across the sky is familiar to even the most casual observer. This daily trek is not the Sun
moving as early astronomers thought, but the result of the Earth's rotation. The Earth's rotation also causes the stars to do
the same, scribing out a large circle as the Earth completes one rotation. The size of the circular path a star follows depends
on where it is in the sky. Stars near the celestial equator form the largest circles rising in the east and setting in the west.
Moving toward the north celestial pole, the point around which the stars in the northern hemisphere appear to rotate, these
circles become smaller. Stars in the mid-celestial latitudes rise in the northeast and set in the northwest. Stars at high
celestial latitudes are always above the horizon, and are said to be circumpolar because they never rise and never set. You
will never see the stars complete one circle because the sunlight during the day washes out the starlight. However, part of
this circular motion of stars in this region of the sky can be seen by setting up a camera on a tripod and opening the shutter
for a couple hours. The processed film will reveal semicircles that revolve around the pole. (This description of stellar
motions also applies to the southern hemisphere except all stars south of the celestial equator move around the south
celestial pole.)
Figure 6-2
All stars appear to rotate around the celestial poles. However, the appearance of this motion
varies depending on where you are looking in the sky. Near the north celestial pole the stars
scribe out recognizable circles centered on the pole (1). Stars near the celestial equator also
follow circular paths around the pole. But, the complete path is interrupted by the horizon.
These appear to rise in the east and set in the west (2). Looking toward the opposite pole, stars
curve or arc in the opposite direction scribing a circle around the opposite pole (3).
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Polar Alignment (with optional Wedge)
Even though the CPC can precisely track a celestial object while in the Alt-Az position, it is still necessary to align the polar
axis of the telescope (the fork arm) to the Earth's axis of rotation in
order to do long exposure astrophotography. To do an accurate polar
alignment, the CPC requires an optional equatorial wedge between
the telescope and the tripod. This allows the telescope's tracking
motors to rotate the telescope around the celestial pole, the same
way as the stars. Without the equatorial wedge, you would notice
the stars in the eyepiece would slowly rotate around the center of the
field of view. Although this gradual rotation would go unnoticed
when viewing with an eyepiece, it would be very noticeable on
film.
Polar alignment is the process by which the telescope's axis of
rotation (called the polar axis) is aligned (made parallel) with the
Earth's axis of rotation. Once aligned, a telescope with a clock drive
will track the stars as they move across the sky. The result is that
objects observed through the telescope appear stationary (i.e., they
will not drift out of the field of view). If not using the clock drive,
all objects in the sky (day or night) will slowly drift out of the field.
This motion is caused by the Earth's rotation.
Wedge Align
The CPC has two equatorial wedge alignment modes (one for the
northern hemisphere and one for the southern) that will help you
polar align your telescope when using an optional equatorial wedge.
After performing either an EQ AutoAlign or Two-Star Alignment,
Wedge Align will slew the telescope to where Polaris should be. By
using the tripod and wedge to center Polaris in the eyepiece, the fork
arm (polar axis) will then be pointing towards the actual North
Celestial Pole. Once Wedge Align is complete, you must re-align
your telescope using any of the EQ alignment methods. Follow these
steps to Wedge Align the CPC in the Northern Hemisphere:
Figure 6-3
This is how the telescope is to be set up for polar
alignment. The tube should be parallel to the
fork arm and the mount should point to Polaris.
1. With the telescope set up on an optional equatorial wedge and roughly positioned towards Polaris, align the CPC
using either the EQ AutoAlign or Two-Star Alignment method.
2. Select Wedge Align from the Utilities menu and press Enter.
Based on your current alignment, the CPC will slew to where it thinks Polaris should be. Use the tripod and wedge
adjustments to place Polaris in the center of the eyepiece. Do not use the direction buttons to position Polaris. Once
Polaris is centered in the eyepiece press ENTER; the polar axis should then be
pointed towards the North Celestial Pole.
Finding the North Celestial Pole
In each hemisphere, there is a point in the sky around which all the other stars appear to
rotate. These points are called the celestial poles and are named for the hemisphere in
which they reside. For example, in the northern hemisphere all stars move around the
north celestial pole. When the telescope's polar axis is pointed at the celestial pole, it is
parallel to the Earth's rotational axis.
Many methods of polar alignment require that you know how to find the celestial pole by
identifying stars in the area. For those in the northern hemisphere, finding the celestial
pole is not too difficult. Fortunately, we have a naked eye star less than a degree away.
This star, Polaris, is the end star in the handle of the Little Dipper. Since the Little Dipper
Figure 6-5
(technically called Ursa Minor) is not one of the brightest constellations in the sky, it may
be difficult to locate from urban areas. If this is the case, use the two end stars in the bowl
of the Big Dipper (the pointer stars). Draw an imaginary line through them toward the
Little Dipper. They point to Polaris (see Figure 6-6). The position of the Big Dipper
The position of the Big
Dipper changes throughout
the year and the night.
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changes during the year and throughout the course of the night (see Figure 6-5). When the Big Dipper is low in the sky (i.e.,
near the horizon), it may be difficult to locate. During these times, look for Cassiopeia (see Figure 6-6). Observers in the
southern hemisphere are not as fortunate as those in the northern hemisphere. The stars around the south celestial pole are
not nearly as bright as those around the north. The closest star that is relatively bright is Sigma Octantis. This star is just
within naked eye limit (magnitude 5.5) and lies about 59 arc minutes from the pole.
Definition
The north celestial pole is the point in the northern hemisphere around which all stars appear to rotate.
The counterpart in the southern hemisphere is referred to as the south celestial pole.
Figure 6-6
The two stars in the front of the bowl of the Big Dipper point to Polaris which is less than
one degree from the true (north) celestial pole. Cassiopeia, the “W” shaped constellation,
is on the opposite side of the pole from the Big Dipper. The North Celestial Pole (N.C.P.)
is marked by the “+” sign.
Declination Drift Method of Polar Alignment
This method of polar alignment allows you to get the most accurate alignment on the celestial pole and is required if you want to do long
exposure deep-sky astrophotography through the telescope. The declination drift method requires that you monitor the drift of selected
stars. The drift of each star tells you how far away the polar axis is pointing from the true celestial pole and in what direction. Although
declination drift is simple and straight-forward, it requires a great deal of time and patience to complete when first attempted. The
declination drift method should be done after any one of the previously mentioned methods has been completed.
To perform the declination drift method you need to choose two bright stars. One should be near the eastern horizon and one due south
near the meridian. Both stars should be near the celestial equator (i.e., 0° declination). You will monitor the drift of each star one at a time
and in declination only. While monitoring a star on the meridian, any misalignment in the east-west direction is revealed. While
monitoring a star near the east/west horizon, any misalignment in the north-south direction is revealed. It is helpful to have an illuminated
reticle eyepiece to help you recognize any drift. For very close alignment, a Barlow lens is also recommended since it increases the
magnification and reveals any drift faster. When looking due south, insert the diagonal so the eyepiece points straight up. Insert the cross
hair eyepiece and align the cross hairs so that one is parallel to the declination axis and the other is parallel to the right ascension axis.
Move your telescope manually in R.A. and DEC to check parallelism.
First, choose your star near where the celestial equator and the meridian meet. The star should be approximately within 1/2 an hour of the
meridian and within five degrees of the celestial equator. Center the star in the field of your telescope and monitor the drift in declination.
•
•
If the star drifts south, the polar axis is too far east.
If the star drifts north, the polar axis is too far west.
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Make the appropriate adjustments to the polar axis to eliminate any drift. Once you have eliminated all the drift, move to the star near the
eastern horizon. The star should be 20 degrees above the horizon and within five degrees of the celestial equator.
•
•
If the star drifts south, the polar axis is too low.
If the star drifts north, the polar axis is too high.
Again, make the appropriate adjustments to the polar axis to eliminate any drift. Unfortunately, the latter adjustments interact with the prior
adjustments ever so slightly. So, repeat the process again to improve the accuracy checking both axes for minimal drift. Once the drift has
been eliminated, the telescope is very accurately aligned. You can now do prime focus deep-sky astrophotography for long periods.
NOTE: If the eastern horizon is blocked, you may choose a star near the western horizon, but you must reverse the polar high/low error
directions. Also, if using this method in the southern hemisphere, the direction of drift is reversed for both R.A. and DEC.
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With your telescope set up, you are ready to use it for observing. This section covers visual observing hints for both solar system and deep
sky objects as well as general observing conditions which will affect your ability to observe.
Observing the Moon
Often, it is tempting to look at the Moon when it is full. At this time, the face we see is fully
illuminated and its light can be overpowering. In addition, little or no contrast can be seen
during this phase.
One of the best times to observe the Moon is during its partial phases (around the time of
first or third quarter). Long shadows reveal a great amount of detail on the lunar surface.
At low power you will be able to see most of the lunar disk at one time. The optional
Reducer/Corrector lens allows for breath-taking views of the entire lunar disk when used
with a low power eyepiece. Change to higher power (magnification) to focus in on a
smaller area. Choose the lunar tracking rate from the CPC's MENU tracking rate options to
keep the moon centered in the eyepiece even at high magnifications.
Lunar Observing Hints
To increase contrast and bring out detail on the lunar surface, use filters. A yellow filter works well at improving contrast while a neutral
density or polarizing filter will reduce overall surface brightness and glare.
Observing the Planets
Other fascinating targets include the five naked eye planets. You can see Venus go through
its lunar-like phases. Mars can reveal a host of surface detail and one, if not both, of its polar
caps. You will be able to see the cloud belts of Jupiter and the great Red Spot (if it is visible
at the time you are observing). In addition, you will also be able to see the moons of Jupiter
as they orbit the giant planet. Saturn, with its beautiful rings, is easily visible at moderate
power.
Planetary Observing Hints
•
Remember that atmospheric conditions are usually the limiting factor on how
much planetary detail will be visible. So, avoid observing the planets when they
are low on the horizon or when they are directly over a source of radiating heat,
such as a rooftop or chimney. See the "Seeing Conditions" section later in this section.
To increase contrast and bring out detail on the planetary surface, try using Celestron eyepiece filters.
•
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Observing the Sun
Although overlooked by many amateur astronomers, solar observation is both rewarding and fun. However, because
the Sun is so bright, special precautions must be taken when observing our star so as not to damage your eyes or your
telescope.
Never project an image of the Sun through the telescope. Because of the folded optical design, tremendous heat build-
up will result inside the optical tube. This can damage the telescope and/or any accessories attached to the telescope.
For safe solar viewing, use a solar filter that reduces the intensity of the Sun's light, making it safe to view. With a
filter you can see sunspots as they move across the solar disk and faculae, which are bright patches seen near the Sun's
edge.
Solar Observing Hints
•
•
The best time to observe the Sun is in the early morning or late afternoon when the air is cooler.
To center the Sun without looking into the eyepiece, watch the shadow of the telescope tube until it forms a
circular shadow.
•
To ensure accurate tracking, be sure to select the solar tracking rate.
Observing Deep Sky Objects
Deep-sky objects are simply those objects outside the boundaries of our solar system. They include star clusters,
planetary nebulae, diffuse nebulae, double stars and other galaxies outside our own Milky Way. Most deep-sky objects
have a large angular size. Therefore, low-to-moderate power is all you need to see them. Visually, they are too faint to
reveal any of the color seen in long exposure photographs. Instead, they appear black and white. And, because of their
low surface brightness, they should be observed from a dark-sky location. Light pollution around large urban areas
washes out most nebulae making them difficult, if not impossible, to observe. Light Pollution Reduction filters help
reduce the background sky brightness, thus increasing contrast.
Seeing Conditions
Viewing conditions affect what you can see through your telescope during an observing session. Conditions include
transparency, sky illumination, and seeing. Understanding viewing conditions and the effect they have on observing
will help you get the most out of your telescope.
Transparency
Transparency is the clarity of the atmosphere which is affected by clouds, moisture, and other airborne particles. Thick
cumulus clouds are completely opaque while cirrus can be thin, allowing the light from the brightest stars through.
Hazy skies absorb more light than clear skies making fainter objects harder to see and reducing contrast on brighter
objects. Aerosols ejected into the upper atmosphere from volcanic eruptions also affect transparency. Ideal conditions
are when the night sky is inky black.
Sky Illumination
General sky brightening caused by the Moon, aurorae, natural airglow, and light pollution greatly affect transparency.
While not a problem for the brighter stars and planets, bright skies reduce the contrast of extended nebulae making
them difficult, if not impossible, to see. To maximize your observing, limit deep sky viewing to moonless nights far
from the light polluted skies found around major urban areas. LPR filters enhance deep sky viewing from light
polluted areas by blocking unwanted light while transmitting light from certain deep sky objects. You can, on the other
hand, observe planets and stars from light polluted areas or when the Moon is out.
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Seeing
Seeing conditions refers to the stability of the atmosphere and directly affects the amount of fine detail seen in extended
objects. The air in our atmosphere acts as a lens which bends and distorts incoming light rays. The amount of bending
depends on air density. Varying temperature layers have different densities and, therefore, bend light differently. Light
rays from the same object arrive slightly displaced creating an imperfect or smeared image. These atmospheric
disturbances vary from time-to-time and place-to-place. The size of the air parcels compared to your aperture
determines the "seeing" quality. Under good seeing conditions, fine detail is visible on the brighter planets like Jupiter
and Mars, and stars are pinpoint images. Under poor seeing conditions, images are blurred and stars appear as blobs.
The conditions described here apply to both visual and photographic observations.
Figure 7-1
Seeing conditions directly affect image quality. These drawings represent a point source
(i.e., star) under bad seeing conditions (left) to excellent conditions (right). Most often,
seeing conditions produce images that lie some where between these two extremes.
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After looking at the night sky for a while you may want to try photographing it. Several forms of celestial photography are possible with
your telescope, including short exposure prime focus, eyepiece projection, long exposure deep sky, terrestrial and even CCD imaging.
Each of these is discussed in moderate detail with enough information to get you started. Topics include the accessories required and some
simple techniques. More information is available in some of the publications listed at the end of this manual.
In addition to the specific accessories required for each type of celestial photography, there is the need for a camera - but not just any
camera. The camera does not have to have many of the features offered on today's state-of-the-art equipment. For example, you don't
need auto focus capability or mirror lock up. Here are the mandatory features a camera needs for celestial photography. First, a “B”
setting which allows for time exposures. This excludes point and shoot cameras and limits the selection to SLR cameras, the most
common type of 35mm camera on the market today.
Second, the “B” or manual setting should NOT run off the battery. Many new electronic cameras use the battery to keep the shutter open
during time exposures. Once the batteries are drained, usually after a few minutes, the shutter closes, whether you were finished with the
exposure or not. Look for a camera that has a manual shutter when operating in the time exposure mode. Olympus, Nikon, Minolta,
Pentax, Canon and others have made such camera bodies.
The camera must have interchangeable lenses so you can attach it to the telescope and so you can use a variety of lenses for piggyback
photography. If you can't find a new camera, you can purchase a used camera body that is not 100-percent functional. The light meter, for
example, does not have to be operational since you will be determining the exposure length manually.
You also need a cable release with a locking function to hold the shutter open while you do other things. Mechanical and air release
models are available.
Short Exposure Prime Focus Photography
Short exposure prime focus photography is the best way to begin recording celestial objects. It is done with the camera attached to the
telescope without an eyepiece or camera lens in place. To attach your camera you need the Celestron T-Adapter (#93633-A) and a T-Ring
for your specific camera (i.e., Minolta, Nikon, Pentax, etc.). The T-Ring replaces the 35mm SLR camera's normal lens. Prime focus
photography allows you to capture the majority of the lunar disk or solar disk. To attach your camera to your telescope.
1. Remove all visual accessories.
2. Thread the T-Ring onto the T-Adapter.
3. Mount your camera body onto the T-Ring the same as you would any other lens.
4. Thread the T-Adapter onto the back of the telescope while holding the camera in the desired orientation (either vertical or horizontal).
With your camera attached to the telescope, you are ready for prime focus photography. Start with an easy object like the Moon. Here's
how to do it:
1. Load your camera with film that has a moderate-to-fast speed (i.e., ISO rating). Faster films are more desirable when the Moon is a
crescent. When the Moon is near full, and at its brightest, slower films are more desirable. Here are some film recommendations:
•
•
•
•
•
T-Max 100
T-Max 400
Any 100 to 400 ISO color slide film
Fuji Super HG 400
Ektar 25 or 100
2. Center the Moon in the field of your CPC telescope.
3. Focus the telescope by turning the focus knob until the image is sharp.
4. Set the shutter speed to the appropriate setting (see table below).
5. Trip the shutter using a cable release.
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6. Advance the film and repeat the process.
Lunar Phase
Crescent
Quarter
Full
ISO 50
1/2
1/15
1/30
ISO 100
1/4
1/30
ISO 200
1/8
1/60
ISO 400
1/15
1/125
1/250
1/60
1/125
Table 8-1
Above is a listing of recommended exposure times when photographing the Moon at the
prime focus of your CPC telescope.
The exposure times listed in table 8-1 should be used as a starting point. Always make exposures that are longer and shorter than the
recommended time. Also, take a few photos at each shutter speed. This will ensure that you will get a good photo.
•
•
If using black and white film, try a yellow filter to reduce the light intensity and to increase contrast.
Keep accurate records of your exposures. This information is useful if you want to repeat your results or if you want to
submit some of your photos to various astronomy magazines for possible publication!
•
This technique is also used for photographing the Sun with the proper solar filter.
Eyepiece Projection
This form of celestial photography is designed for objects with small angular sizes, primarily the Moon and planets. Planets, although
physically quite large, appear small in angular size because of their great distances. Moderate to high magnification is, therefore, required
to make the image large enough to see any detail. Unfortunately, the camera/telescope combination alone does not provide enough
magnification to produce a usable image size on film. In order to get the image large enough, you must attach your camera to the telescope
with the eyepiece in place. To do so, you need two additional accessories; a deluxe tele-extender (#93643), which attaches to the visual
back, and a T-ring for your particular camera make (i.e., Minolta, Nikon, Pentax, etc.).
Because of the high magnifications during eyepiece projection, the field of view is quite small which makes it difficult to find and center
objects. To make the job a little easier, align the finder as accurately as possible. This allows you to get the object in the telescope's field
based on the finder's view alone.
Another problem introduced by the high magnification is vibration. Simply tripping the shutter ⎯ even with a cable release ⎯ produces
enough vibration to smear the image. To get around this, use the camera's self-timer if the exposure
time is less than one second ⎯ a common occurrence when photographing the Moon. For exposures
over one second, use the "hat trick." This technique incorporates a hand-held black card placed over
the aperture of the telescope to act as a shutter. The card prevents light from entering the telescope
while the shutter is released. Once the shutter has been released and the vibration has diminished (a
few seconds), move the black card out of the way to expose the film. After the exposure is complete,
place the card over the front of the telescope and close the shutter. Advance the film and you're ready
for your next shot. Keep in mind that the card should be held a few inches in front of the telescope,
and not touching it. It is easier if you use two people for this process; one to release the camera shutter
and one to hold the card. Here's the process for making the exposure.
1. Find and center the desired target in the viewfinder of your camera.
Figure 8-1 - Accessories for
Projection Photography
2. Turn the focus knob until the image is as sharp as possible.
3. Place the black card over the front of the telescope.
4. Release the shutter using a cable release.
5. Wait for the vibration caused by releasing the shutter to diminish. Also, wait for a moment of good seeing.
6. Remove the black card from in front of the telescope for the duration of the exposure (see accompanying table).
7. Replace the black card over the front of the telescope.
8. Close the camera's shutter.
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Advance the film and you are ready for your next exposure. Don't forget to take photos of varying duration and keep accurate records of
what you have done. Record the date, telescope, exposure duration, eyepiece, f/ratio, film, and some comments on the seeing conditions.
The following table lists exposures for eyepiece projection with a 10mm eyepiece. All exposure times are listed in seconds or fractions of
a second.
Planet
Moon
Mercury
Venus
Mars
ISO 50
4
16
1/2
16
8
ISO 100
2
8
1/4
8
ISO 200
1
4
1/8
4
ISO 400
1/2
2
1/15
2
1
4
8
2
4
Jupiter
Saturn
16
2
Table 8-2
Recommended exposure time for photographing planets.
The exposure times listed here should be used as a starting point. Always make exposures that are longer and shorter than the
recommended time. Also, take a few photos at each shutter speed. This will ensure that you get a good photo. It is not uncommon to go
through an entire roll of 36 exposures and have only one good shot.
NOTE: Don't expect to record more detail than you can see visually in the eyepiece at the time you are photographing.
Once you have mastered the technique, experiment with different films, different focal length eyepieces, and even different filters.
Long Exposure Prime Focus Photography
This is the last form of celestial photography to be attempted after others have been mastered. It is intended primarily for deep sky objects,
that is objects outside our solar system which includes star clusters, nebulae, and galaxies. While it may seem that high magnification is
required for these objects, just the opposite is true. Most of these objects cover large angular areas and fit nicely into the prime focus field
of your telescope. The brightness of these objects, however, requires long exposure times and, as a result, are rather difficult.
There are several techniques for this type of photography, and the one chosen will determine the standard accessories needed. The best
method for long exposure deep sky astrophotography is with an off-axis guider. This device allows you to photograph and guide through
the telescope simultaneously. Celestron offers a very special and advanced off-axis guider, called the Radial Guider (#94176). In
addition, you will need a T-Ring to attach your camera to the Radial Guider.
Other equipment needs include a guiding eyepiece. Unlike other forms of astrophotography which allows for fairly loose guiding, prime
focus requires meticulous guiding for long periods. To accomplish this you need a guiding ocular with an illuminated reticle to monitor
your guide star. For this purpose, Celestron offers the Micro Guide Eyepiece (#94171) Here is a brief summary of the technique.
1. Polar align the telescope using an optional equatorial wedge. To polar align the CPC you must select EQ North Align (or EO South
Align) from the alignment options. For more information on polar aligning, see the Polar Alignment section earlier in the manual.
2. Remove all visual accessories.
3. Thread the Radial Guider onto your telescope.
4. Thread the T-Ring onto the Radial Guider.
5. Mount your camera body onto the T-Ring the same as you would any other lens.
6. Set the shutter speed to the "B" setting.
7. Focus the telescope on a star.
8. Center your subject in the field of your camera.
9. Find a suitable guide star in the telescope field. This can be the most time consuming process.
10. Open the shutter using a cable release.
11. Monitor your guide star for the duration of the exposure using the buttons on the hand controller to make the needed corrections.
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12. Close the camera's shutter.
Periodic Error Correction (PEC)
PEC for short, is a system that improves the tracking accuracy of the drive by reducing the number of user corrections needed to keep a
guide star centered in the eyepiece. PEC is designed to improve photographic quality by reducing the amplitude of the worm errors.
Using the PEC function is a three-step process. First, the CPC needs to know the current position of its worm gear so that it has a
reference when playing back the recorded error. Next, you must guide for at least 8 minutes during which time the system records the
correction you make. (It takes the worm gear 8 minutes to make one complete revolution, hence the need to guide for 8 minutes). This
“teaches” the PEC chip the characteristics of the worm. The periodic error of the worm gear drive will be stored in the PEC chip and used
to correct periodic error. The last step is to play back the corrections you made during the recording phase. Keep in mind, this feature is
for advanced astrophotography and still requires careful guiding since all telescope drives have some periodic error.
Using Periodic Error Correction
Once the telescope has been polar aligned using the EQ North Align (or EQ South for southern hemisphere) method, select PEC from the
Utilities menu and press ENTER to begin recording your periodic error. Here’s how to use the PEC function.
1. Find a bright star relatively close to the object you want to photograph.
2. Insert a high power eyepiece with illuminated cross hairs into your telescope. Orient the guiding eyepiece cross hairs so that one
is parallel to the declination while the other is parallel to the R.A. axis.
3. Center the guide star on the illuminated cross hairs, focus the telescope, and study the periodic movement.
4. Before actually recording the periodic error, take a few minutes to practice guiding. Set the hand control slew rate to an
appropriate guide rate (rate 1 = .5x, rate 2 = 1x) and practice centering the guide star in the cross hairs for several minutes. This
will help you familiarize yourself with the periodic error of the drive and the operation of the hand control. Remember to ignore
declination drift when programming the PEC.
Note: When recording PEC only the photo guide rates (rates 1 and 2) will be operational. This eliminates the possibility of moving the
telescope suddenly while recording.
5. To begin recording the drive's periodic error, press the MENU button and select PEC from the Utilities menu. Use the Up/Down
scroll buttons to display the Record option and press ENTER. You will have 5 seconds before the system starts to record. The
first time each observing session that PEC record or play is selected, the worm gear must rotate in order to mark its starting
position. If the rotation of the worm gear moves your guide star outside the field of view of the eyepiece, it will have to be re-
centered before the recording begins.
Helpful
Hint
Once the worm gear is indexed, it will not need to be positioned again until the telescope is turned-off. So, to give yourself more time
to prepare for guiding, it is best to restart PEC recording after the worm gear has found its index.
6. After 8 minutes PEC will automatically stop recording.
7. Point the telescope at the object you want to photograph and center the guide star on the illuminated cross hairs and you are
ready to play back the periodic error correction.
8. Once the drive's periodic error has been recorded, use the Playback function to begin playing back the correction for future
photographic guiding. If you want to re-record the periodic error, select Record and repeat the recording processes again. The
previously recorded information will be replaced with the current information. Repeat steps 7 and 8 to playback the PEC
corrections for your next object.
Does the PEC function make unguided astrophotography possible? Yes and no. For solar (filtered), lunar, and piggyback (up to 200mm),
the answer is yes. However, even with PEC, off-axis guiding is still mandatory for long exposure, deep sky astrophotography. The
optional Reducer/Corrector lens reduces exposure times making the task of guiding a little easier.
When getting started, use fast films to record as much detail in the shortest possible time. Here are proven recommendations:
•
Ektar 1000 (color print)
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•
•
•
•
•
•
Konica 3200 (color print)
Fujichrome 1600D (color slide)
3M 1000 (color slide)
Scotchchrome 400
T-Max 3200 (black and white print)
T-Max 400 (black and white print)
As you perfect your technique, try specialized films, that is films that are designed or specially treated for celestial photography. Here are
some popular choices:
•
•
•
•
Ektar 125 (color print)
Fujichrome 100D (color slide)
Tech Pan, gas hypered (black and white print)
T-Max 400 (black and white print)
There is no exposure determination table to help you get started. The best way to determine exposure length is look at previously
published photos to see what film/exposure combinations were used. Or take unguided sample photos of various parts of the sky while the
drive is running. Always take exposures of various lengths to determine the best exposure time.
Terrestrial Photography
Your CPC makes an excellent telephoto lens for terrestrial (land) photography. Terrestrial photography is best done will the telescope in
Alt-Az configuration and the tracking drive turned off. To turn the tracking drive off, press the MENU (9) button on the hand control and
scroll down to the Tracking Mode sub menu. Use the Up and Down scroll keys (10) to select the Off option and press ENTER. This will
turn the tracking motors off, so that objects will remain in your camera's field of view.
Metering
The CPC has a fixed aperture and, as a result, fixed f/ratios. To properly expose your subjects photographically, you need to set your
shutter speed accordingly. Most 35mm SLR cameras offer through-the-lens metering which lets you know if your picture is under or
overexposed. Adjustments for proper exposures are made by changing the shutter speed. Consult your camera manual for specific
information on metering and changing shutter speeds.
Reducing Vibration
Releasing the shutter manually can cause vibrations, producing blurred photos. To reduce vibration when tripping the shutter, use a cable
release. A cable release keeps your hands clear of the camera and lens, thus eliminating the possibility of introducing vibration.
Mechanical shutter releases can be used, though air-type releases are best.
Blurry pictures can also result from shutter speeds that are too slow. To prevent this, use films that produce shutter speeds greater than
1/250 of a second when hand-holding the lens. If the lens is mounted on a tripod, the exposure length is virtually unlimited.
Another way to reduce vibration is with the Vibration Suppression Pads (#93503). These pads rest between the ground and tripod feet.
They reduce the vibration amplitude and vibration time.
The following is a brief description of the advantages of imaging at each f-number configuration and the proper equipment needed to use
the telescope in any of its many settings
F/6.3 with Reducer/Corrector
When imaging some objects like planetary nebula (for example M57, the Ring Nebula) and small galaxies (M104, the Sombrero Galaxy),
larger image scale is needed to resolve finer detail. These objects are better shot at f/6.3 or even f/10.
Medium size to small galaxies --
f/6.3 imaging gives you finer resolution then at f/2, but the slower f-number will usually require you to guide the image while you are
taking longer exposures. Guiding can be accomplished by using an optional Radial Guider or a piggyback guide scope. The exposure
times are about 10 times longer but the results can be worth the extra effort. There are some objects that are small enough and bright
enough that they work great at f/6.3. M104 (the Sombrero Galaxy) can be imaged under dark skies with a series of short exposures using
Track and Accumulate. Ten exposures at 15 seconds each will yield a nice image and is short enough that you may not need to guide the
exposure at all. For f/6.3 imaging the optional Reducer/Corrector is needed. (See Optional Accessory section at the end of this manual).
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Lunar or small planetary nebulae--
f/10 imaging is more challenging for long exposure, deep-sky imaging. Guiding needs to be very accurate and the exposure times need to
be much longer, about 25 times longer than f/2. There are only a select few objects that work well at f/10. The moon images fine
because it is so bright, but planets are still a bit small and should be shot at f/20. The Ring nebula is a good candidate because it is small
and bright. The Ring Nebula (M57) can be imaged in about 30-50 seconds at f/10. The longer the exposure the better.
Planetary or Lunar--
f/20 is a great way to image the planets and features on the moon. When imaging the planets, very short exposures are needed. The
exposure lengths range from .03 to .1 seconds on planetary images. Focus is critical as is good atmospheric conditions. Generally you will
take one image after another until one looks good. This is due to the atmospheric “seeing” conditions. For every 10 exposures you might
save 1. To image at f/20 you need to purchase a 2x Barlow and a T-adapter or Radial Guider.
Auto Guiding
The CPC has a designated auto guiding port for use with a CCD autoguider. The diagram below may be useful when connecting the CCD
camera cable to the CPC and calibrating the autoguider. Note that the four outputs are active-low, with internal pull-ups and are capable of
sinking 25 mA DC.
No Connect
Figure 8-7 – Pin out diagram for Autoguider port.
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While your CPC telescope requires little maintenance, there are a few things to remember that will ensure your telescope
performs at its best.
Care and Cleaning of the Optics
Occasionally, dust and/or moisture may build up on the corrector plate of your telescope. Special care should be taken when
cleaning any instrument so as not to damage the optics.
If dust has built up on the corrector plate, remove it with a brush (made of camel’s hair) or a can of pressurized air. Spray at an
angle to the lens for approximately two to four seconds. Then, use an optical cleaning solution and white tissue paper to remove
any remaining debris. Apply the solution to the tissue and then apply the tissue paper to the lens. Low pressure strokes should
go from the center of the corrector to the outer portion. Do NOT rub in circles!
You can use a commercially made lens cleaner or mix your own. A good cleaning solution is isopropyl alcohol mixed with
distilled water. The solution should be 60% isopropyl alcohol and 40% distilled water. Or, liquid dish soap diluted with water (a
couple of drops per one quart of water) can be used.
Occasionally, you may experience dew build-up on the corrector plate of your telescope during an observing session. If you want
to continue observing, the dew must be removed, either with a hair dryer (on low setting) or by pointing the telescope at the
ground until the dew has evaporated.
If moisture condenses on the inside of the corrector, remove the accessories from the rear cell of the telescope. Place the
telescope in a dust-free environment and point it down. This will remove the moisture from the telescope tube.
To minimize the need to clean your telescope, replace all lens covers once you have finished using it. Since the rear cell is NOT
sealed, the cover should be placed over the opening when not in use. This will prevent contaminants from entering the optical
tube.
Internal adjustments and cleaning should be done only by the Celestron repair department. If your telescope is in need of internal
cleaning, please call the factory for a return authorization number and price quote.
Collimation
The optical performance of your CPC telescope is directly related to its collimation,
that is the alignment of its optical system. Your CPC was collimated at the factory
after it was completely assembled. However, if the telescope is dropped or jarred
severely during transport, it may have to be collimated. The only optical element that
may need to be adjusted, or is possible, is the tilt of the secondary mirror.
To check the collimation of your telescope you will need a light source. A bright star
near the zenith is ideal since there is a minimal amount of atmospheric distortion. Make
sure that tracking is on so that you won’t have to manually track the star. Or, if you do
not want to power up your telescope, you can use Polaris. Its position relative to the
celestial pole means that it moves very little thus eliminating the need to manually
track it.
Figure 9-1
Collimation Adjustment Screws
Before you begin the collimation process, be sure that your telescope is in thermal equilibrium with the surroundings. Allow 45
minutes for the telescope to reach equilibrium if you move it between large temperature extremes.
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 re-collimation is needed.
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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.
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 on the secondary mirror holder (see figure 9-1). To access the collimation
screws you will need remove the collimation screw cover to expose the three collimation screws underneath. To remove the
cover place the tip of flat screwdriver underneath the cover and twist until the cover lifts off. Make only small 1/6 to 1/8
adjustments to the collimation screws 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.
Usually 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
Figure 9-3
is skewed in a different direction, than simply repeat steps 2 through 6 as described
A collimated telescope
above for the new direction.
should appear
symmetrical with the
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.
central obstruction
centered in the star's
diffraction pattern.
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.
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You will find that additional accessories enhance your viewing pleasure and expand the usefulness of your telescope. For
ease of reference, all the accessories are listed in alphabetical order.
Barlow Lens - A Barlow lens is a negative lens that increases the focal length of a telescope. Used with any eyepiece, it doubles the
magnification of that eyepiece. Celestron offers two Barlow lens in the 1-1/4" size for the CPC. The 2x Ultima Barlow (#93506) is a
compact triplet design that is fully multicoated for maximum light transmission and parfocal when used with the Ultima eyepieces.
Model #93507 is a compact achromatic Barlow lens that is under three inches long and weighs only 4 oz. It works very well with all
Celestron eyepieces.
Erect Image Diagonal (#94112-A) - This accessory is an Amici prism arrangement that allows you to look into the telescope at a 45°
angle with images that are oriented properly (upright and correct from left-to-right). It is useful for daytime, terrestrial viewing.
Eyepieces - Like telescopes, eyepieces come in a variety of designs. Each design has its own advantages and disadvantages. For the 1-
1/4" barrel diameter there are four different eyepiece designs available.
•
OMNI Plössl - Plössl eyepieces have a 4-element lens designed for low-to-high power
observing. All are fully multi-coated for maximum light transmission. These Plössls offer razor
sharp views across the entire field, even at the edges! In the 1-1/4" barrel diameter, they are
available in the following focal lengths: 3.6mm, 6mm, 8mm, 10mm, 13mm, 17mm, 25mm,
32mm and 40mm.
•
X-CEL - Fully Multi-coated. All air-to-glass surfaces have 5 layer multi-coating. Field of view
55°. Six element optical design using ED glass on most curved elements. Parfocal – little to no
focusing adjustments are needed when switching from a low power to high power eyepiece.
20mm eye relief and soft rubber eyecups. Blackened lens edges to minimizes internal reflection
and improved contrast. Each eyepiece comes in a durable plastic case.
•
Ultima - Ultima is our 5-element, wider field eyepiece design. In the 1-1/4" barrel diameter,
they are available in the following focal lengths: 5mm, 7.5mm, 10mm, 12.5mm, 18mm, 30mm, 35mm, and 42mm. These eyepieces
are all parfocal. The 35mm Ultima gives the widest possible field of view with a 1-1/4" diagonal.
• Axiom – As an extension of the Ultima line, a new wide angle series is offered – called the Axiom series. All units are seven element
designs and feature a 70º extra wide field of view ( except the 50mm). All are fully multicoated and contain all the feature of the
Ultimas.
Eyepiece, Micro Guide (#94171) - This multipurpose 12.5mm illuminated reticle can be used for guiding
deep-sky astrophotos, measuring position angles, angular separations, and more. The laser etched reticle
provides razor sharp lines and the variable brightness illuminator is completely cordless. The micro guide
eyepiece produces 224 power when used with the CPC 11 at f/10 and 163 power with the CPC 8.
Filters, Eyepiece - To enhance your visual observations of solar system objects, Celestron offers a wide
range of colored filters that thread into the 1-1/4" oculars. Available individually are: #12 deep yellow, #21
orange, #25 red, #58 green, #80A light blue, #96 neutral density - 25%T, #96 neutral density - 13%T, and
polarizing. These and other filters are also sold in sets.
Flashlight, Night Vision - (#93588) - Celestron’s premium model for astronomy, using two red LED's to
preserve night vision better than red filters or other devices. Brightness is adjustable. Operates on a single 9 volt battery (included).
Light Pollution Reduction (LPR) Filters - These filters are designed to enhance your views of deep sky astronomical objects when
viewed from urban areas. LPR Filters selectively reduce the transmission of certain wavelengths of light, specifically those produced by
artificial lights. This includes mercury and high and low pressure sodium vapor lights. In addition, they also block unwanted natural
light (sky glow) caused by neutral oxygen emission in our atmosphere. Celestron offers a model for 1-1/4" eyepieces (#94123) and 2"
eyepieces (#94124)
46
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Moon Filter (#94119-A) - Celestron’s Moon Filter is an economical eyepiece filter for reducing the brightness of the moon and
improving contrast, so greater detail can be observed on the lunar surface. The clear aperture is 21mm and the transmission is about
18%.
PowerTank (#18774) – 12v 7Amp hour rechargeable power supply. Comes with two 12v output
cigarette outlets, built-in red flash light , Halogen emergency spotlight. 120v AC adapter and cigarette
lighter adapter included. Celestron also offers a 17 amp hour models (#18777).
Polarizing Filter Set (#93608) - The polarizing filter set limits the transmission of light to a specific
plane, thus increasing contrast between various objects. This is used primarily for terrestrial, lunar and
planetary observing.
®
Radial Guider (#94176) - The Celestron Radial Guider is specifically
designed for use in prime focus, deep sky astrophotography and takes the
place of the T-Adapter. This device allows you to photograph and guide
simultaneously through the optical tube assembly of your telescope. This type of guiding produces the
best results since what you see through the guiding eyepiece is exactly reproduced on the processed film.
The Radial Guider is a “T”-shaped assembly that attaches to the rear cell of the telescope. As light from
the telescope enters the guider, most passes straight through to the camera. A small portion, however, is
diverted by a prism at an adjustable angle up to the guiding eyepiece. This guider has two features not
found on other off-axis guiders; first, the prism and eyepiece housing rotate independently of the camera
orientation making the acquisition of a guide star quite easy. Second, the prism angle is tunable allowing
you to look at guide stars on-axis. This accessory works especially well with the Reducer/Corrector.
Reducer/Corrector (#94175) - This lens reduces the focal length of the telescope by 37%, making your CPC 11 a 1764mm f/6.3
instrument and the CPC 800 a 1280mm f/6.3 instrument. In addition, this unique lens also corrects
inherent aberrations to produce crisp images all the way across the field when used visually. When
used photographically, there is some vignetting that produces a 26mm circular image on the processed
film. It also increases the field of view significantly and is ideal for wide-field, deep-space viewing. It
is also perfect for beginning prime focus, long-exposure astro photography when used with the radial
guider. It makes guiding easier and exposures much shorter.
Sky Maps (#93722) - Celestron Sky Maps are the ideal teaching guide for learning the night sky. You
wouldn’t set off on a road trip without a road map, and you don’t need to try to navigate the night sky
without a map either. Even if you already know your way around the major constellations, these maps
can help you locate all kinds of fascinating objects.
Skylight Filter (#93621) - The Skylight Filter is used on the Celestron CPC telescope as a dust seal. The filter threads onto the rear cell
of your telescope. All other accessories, both visual and photographic (with the exception of Barlow lenses), thread onto the skylight
filter. The light loss caused by this filter is minimal.
Solar Filter - The AstroSolar® filter is a safe and durable filter that covers the front opening of the telescope. View sunspots and other
solar features using this double-sided metal coated filter for uniform density and good color balance across the entire field. The Sun
offers constant changes and will keep your observing interesting and fun. Celestron offers filters for CPC 800 (#94162).
T-Adapter (#93633-A) - T-Adapter (with additional T-Ring) allows you to attach your SLR camera to the rear cell of your Celestron
CPC. This turns your CPC into a high power telephoto lens perfect for terrestrial photography and short exposure lunar and filtered solar
photography.
T-Ring - The T-Ring couples your 35mm SLR camera body to the T-Adapter, radial guider, or tele-extender. This accessory is
mandatory if you want to do photography through the telescope. Each camera make (i.e., Minolta, Nikon, Pentax, etc.) has its own
unique mount and therefore, its own T-Ring. Celestron has 8 different models for 35mm cameras.
Tele-Extender, Deluxe (#93643) - The tele-extender is a hollow tube that allows you to attach a camera to the telescope when the
eyepiece is installed. This accessory is used for eyepiece projection photography which allows you to capture very high power views of
the Sun, Moon, and planets on film. The tele-extender fits over the eyepiece onto the visual back. This tele-extender works with
eyepieces that have large housings, like the Celestron Ultima series.
Wedge, Heavy Duty (#93655) – The wedge allows you to tilt the telescope so that its polar axis is parallel to the earth's axis of rotation.
Ideal for using your CPC for guided astrophotography.
A full description of all Celestron accessories can be found in the Celestron Accessory Catalog (#93685).
47
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Appendix A - Technical Specifications
Optical Specification
CPC 800 - #11073
Schmidt-Cassegrain Catadioptric
8" (203.2mm)
CPC 925 - #11074
Schmidt-Cassegrain Catadioptric
9.25" (235mm)
CPC 1100 - #11075
Schmidt-Cassegrain Catadioptric
11" (279mm)
Design
Aperture
Focal Length
2032mm
2350mm
2800mm
F/ratio of the Optical System
10
10
10
Primary Mirror:
Material
Coatings
Fine Annealed Pyrex
Starbright Coatings - 5 step multi-
layer process
Fine Annealed Pyrex
Starbright Coatings - 5 step multi-
layer process
Fine Annealed Pyrex
Starbright Coatings - 5 step multi-
layer process
Optional:Starbright XLT Coating
Optional:Starbright XLT Coating
Optional:Starbright XLT Coating
Central Obstruction
Corrector Plate:
2.5"
3..35"
3.75"
Material
Coatings
Optical Quality Crown Glass
A-R Coatings both sides
480x (~4mm eyepiece)
29x (~70mm eyepiece)
Optical Quality Crown Glass
A-R Coatings both sides
555x (~4mm eyepiece)
34x (~70mm eyepiece)
Optical Quality Crown Glass
A-R Coatings both sides
660x (~4mm eyepiece)
40x (~70mm eyepiece)
Highest Useful Magnification
Lowest Useful Magnification
(7mm exit pupil)
Magnification: Standard Eyepiece (40mm Pl)
51x
59x
70x
Resolution: Rayleigh Criterion
Dawes Limit
Light Gathering Power
.68 arc seconds
.57 arc seconds
843x
.59 arc seconds
.49 arc seconds
1127x
.50 arc seconds
.42 arc seconds
1593x
Near Focus w/ standard eyepiece or camera
Field of View: Standard Eyepiece
: 35mm Camera
Linear Field of View (at 1000 yds)
Optical Tube Length
~25 feet
.9º
1º x .68º
47 ft.
17"
~40 feet
.78º
.9º x .6º
41 ft.
22"
~60 feet
.65º
.72º x .50º
34.5 ft.
23"
Weight of Telescope
42 lbs
58 lbs
65 lbs
Weight of Tripod
19 lbs
19 lbs
19 lbs
Electronic Specifications
Input Voltage
12 V DC Nominal
Maximum
Minimum
15 V DC Max.
9 V DC Min.
Power Supply Requirements
GPS
12 VDC-1.5A (Tip positive)
Internal 16 channel
Mechanical Specifications
Motor: Type
DC Servo motors with encoders, both axes
.1406 arc sec
Resolution
Slew speeds
Hand Control
Nine slew speeds: 3º /sec, 2º /sec, .5º/sec, 64x, 16x, 8x, 4x, 1x, .5x
Double line, 16 character Liquid Crystal Display
19 fiber optic backlit LED keypad
Fork Arm
Gears
Bearings
Optical Tube
Dual Fork tine cast aluminum with detachable HC holder
5.625", precision aluminum gears on both axes, 180 tooth. Brass worm gear
9.8" Azimuth Bearing
Aluminum
Software Specifications
Software Precision
Ports
24 bit, .08 arc sec. calculations
RS-232 communication port on hand control, Autoguider Port, 2 Auxiliary Port
Period Error Correction
Tracking Rates
Permanently programmable
Sidereal, Solar, Lunar
Tracking Modes
Alt-Az, EQ North & EQ South
Alignment Procedures
Sky Align, Auto Two-Star Align, Two-Star Align, Solar System Align, EQ North
Align & EQ South Align
Database
40,000+ objects, 99 user defined programmable objects.
Enhanced information on over 200 objects
Complete Revised NGC Catalog
Complete Messier Catalog
Complete IC Catalog
Complete Caldwell
7,840
110
5,386
109
Abell Galaxies
Solar System objects
Famous Asterisms
2,712
9
20
Selected CCD Imaging Objects
Selected SAO Stars
25
29,500
48
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Appendix B - Glossary of Terms
A-
Absolute magnitude
The apparent magnitude that a star would have if it were observed from a standard distance of 10
parsecs, or 32.6 light-years. The absolute magnitude of the Sun is 4.8. at a distance of 10 parsecs, it
would just be visible on Earth on a clear moonless night away from surface light.
The apparent size of a star's disk produced even by a perfect optical system. Since the star can never
be focused perfectly, 84 per cent of the light will concentrate into a single disk, and 16 per cent into
a system of surrounding rings.
Airy disk
Alt-Azimuth Mounting
A telescope mounting using two independent rotation axis allowing movement of the instrument in
Altitude and Azimuth.
Altitude
In astronomy, the altitude of a celestial object is its Angular Distance above or below the celestial
horizon.
Aperture
the diameter of a telescope's primary lens or mirror; the larger the aperture, the greater the
telescope's light-gathering power.
Apparent Magnitude
A measure of the relative brightness of a star or other celestial object as perceived by an observer on
Earth.
Arcminute
Arcsecond
Asterism
Asteroid
A unit of angular size equal to 1/60 of a degree.
A unit of angular size equal to 1/3,600 of a degree (or 1/60 of an arcminute).
A small unofficial grouping of stars in the night sky.
A small, rocky body that orbits a star.
Astrology
The pseudoscientific belief that the positions of stars and planets exert an influence on human
affairs; astrology has nothing in common with astronomy.
Astronomical unit (AU)
Aurora
The distance between the Earth and the Sun. It is equal to 149,597,900 km., usually rounded off to
150,000,000 km.
The emission of light when charged particles from the solar wind slams into and excites atoms and
molecules in a planet's upper atmosphere.
Azimuth
The angular distance of an object eastwards along the horizon, measured from due north, between
the astronomical meridian (the vertical line passing through the center of the sky and the north and
south points on the horizon) and the vertical line containing the celestial body whose position is to
be measured. .
B -
Binary Stars
Binary (Double) stars are pairs of stars that, because of their mutual gravitational attraction, orbit
around a common Center of Mass. If a group of three or more stars revolve around one another, it is
called a multiple system. It is believed that approximately 50 percent of all stars belong to binary or
multiple systems. Systems with individual components that can be seen separately by a telescope are
called visual binaries or visual multiples. The nearest "star" to our solar system, Alpha Centauri, is
actually our nearest example of a multiple star system, it consists of three stars, two very similar to
our Sun and one dim, small, red star orbiting around one another.
C -
Celestial Equator
The projection of the Earth's equator on to the celestial sphere. It divides the sky into two equal
hemispheres.
Celestial pole
Celestial Sphere
Collimation
D -
The imaginary projection of Earth's rotational axis north or south pole onto the celestial sphere.
An imaginary sphere surrounding the Earth, concentric with the Earth's center.
The act of putting a telescope's optics into perfect alignment.
Declination (DEC)
The angular distance of a celestial body north or south of the celestial equator. It may be said to
correspond to latitude on the surface of the Earth.
E -
Ecliptic
The projection of the Earth's orbit on to the celestial sphere. It may also be defined as "the apparent
yearly path of the Sun against the stars".
Equatorial mount
A telescope mounting in which the instrument is set upon an axis which is parallel to the axis of the
Earth; the angle of the axis must be equal to the observer's latitude.
F -
Focal length
The distance between a lens (or mirror) and the point at which the image of an object at infinity is
brought to focus. The focal length divided by the aperture of the mirror or lens is termed the focal
ratio.
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J -
Jovian Planets
Any of the four gas giant planets that are at a greater distance form the sun than the terrestrial
planets.
K -
Kuiper Belt
A region beyond the orbit of Neptune extending to about 1000 AU which is a source of many short
period comets.
L -
Light-Year (LY)
A light-year is the distance light traverses in a vacuum in one year at the speed of 299,792 km/ sec.
With 31,557,600 seconds in a year, the light-year equals a distance of 9.46 X 1 trillion km (5.87 X 1
trillion mi).
M -
Magnitude
Magnitude is a measure of the brightness of a celestial body. The brightest stars are assigned
magnitude 1 and those increasingly fainter from 2 down to magnitude 5. The faintest star that can be
seen without a telescope is about magnitude 6. Each magnitude step corresponds to a ratio of 2.5 in
brightness. Thus a star of magnitude 1 is 2.5 times brighter than a star of magnitude 2, and 100 times
brighter than a magnitude 5 star. The brightest star, Sirius, has an apparent magnitude of -1.6, the
full moon is -12.7, and the Sun's brightness, expressed on a magnitude scale, is -26.78. The zero
point of the apparent magnitude scale is arbitrary.
Meridian
Messier
A reference line in the sky that starts at the North celestial pole and ends at the South celestial pole
and passes through the zenith. If you are facing South, the meridian starts from your Southern
horizon and passes directly overhead to the North celestial pole.
A French astronomer in the late 1700’s who was primarily looking for comets. Comets are hazy
diffuse objects and so Messier cataloged objects that were not comets to help his search. This
catalog became the Messier Catalog, M1 through M110.
N -
Nebula
Interstellar cloud of gas and dust. Also refers to any celestial object that has a cloudy appearance.
North Celestial Pole
The point in the Northern hemisphere around which all the stars appear to rotate. This is caused by
the fact that the Earth is rotating on an axis that passes through the North and South celestial poles.
The star Polaris lies less than a degree from this point and is therefore referred to as the "Pole Star".
Although Latin for "new" it denotes a star that suddenly becomes explosively bright at the end of its
life cycle.
Nova
O -
Open Cluster
One of the groupings of stars that are concentrated along the plane of the Milky Way. Most have an
asymmetrical appearance and are loosely assembled. They contain from a dozen to many hundreds
of stars.
P -
Parallax
Parallax is the difference in the apparent position of an object against a background when viewed by
an observer from two different locations. These positions and the actual position of the object form a
triangle from which the apex angle (the parallax) and the distance of the object can be determined if
the length of the baseline between the observing positions is known and the angular direction of the
object from each position at the ends of the baseline has been measured. The traditional method in
astronomy of determining the distance to a celestial object is to measure its parallax.
Refers to a group of eyepieces that all require the same distance from the focal plane of the
telescope to be in focus. This means when you focus one parfocal eyepiece all the other parfocal
eyepieces, in a particular line of eyepieces, will be in focus.
Parfocal
Parsec
The distance at which a star would show parallax of one second of arc. It is equal to 3.26 light-years,
206,265 astronomical units, or 30,8000,000,000,000 km. (Apart from the Sun, no star lies within
one parsec of us.)
Point Source
An object which cannot be resolved into an image because it to too far away or too small is
considered a point source. A planet is far away but it can be resolved as a disk. Most stars cannot
be resolved as disks, they are too far away.
R -
Reflector
Resolution
A telescope in which the light is collected by means of a mirror.
The minimum detectable angle an optical system can detect. Because of diffraction, there is a limit
to the minimum angle, resolution. The larger the aperture, the better the resolution.
The angular distance of a celestial object measured in hours, minutes, and seconds along the
Celestial Equator eastward from the Vernal Equinox.
Right Ascension: (RA)
S -
Schmidt Telescope
Rated the most important advance in optics in 200 years, the Schmidt telescope combines the best
features of the refractor and reflector for photographic purposes. It was invented in 1930 by
Bernhard Voldemar Schmidt (1879-1935).
Sidereal Rate
This is the angular speed at which the Earth is rotating. Telescope tracking motors drive the
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telescope at this rate. The rate is 15 arc seconds per second or 15 degrees per hour.
The boundary line between the light and dark portion of the moon or a planet.
T -
Terminator
U -
Universe
The totality of astronomical things, events, relations and energies capable of being described
objectively.
V -
Variable Star
A star whose brightness varies over time due to either inherent properties of the star or something
eclipsing or obscuring the brightness of the star.
W -
Waning Moon
The period of the moon's cycle between full and new, when its illuminated portion is decreasing.
The period of the moon's cycle between new and full, when its illuminated portion is increasing.
Waxing Moon
Z -
Zenith
Zodiac
The point on the Celestial Sphere directly above the observer.
The zodiac is the portion of the Celestial Sphere that lies within 8 degrees on either side of the
Ecliptic. The apparent paths of the Sun, the Moon, and the planets, with the exception of some
portions of the path of Pluto, lie within this band. Twelve divisions, or signs, each 30 degrees in
width, comprise the zodiac. These signs coincided with the zodiacal constellations about 2,000 years
ago. Because of the Precession of the Earth's axis, the Vernal Equinox has moved westward by
about 30 degrees since that time; the signs have moved with it and thus no longer coincide with the
constellations.
51
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APPENDIX C
LONGITUDES AND
LATITUDES
LONGITUDE
degrees
LATITUDE
min degrees
LONGITUDE
degrees
114
118
116
117
120
121
117
117
122
124
116
117
115
118
117
124
121
121
119
117
117
118
122
115
117
117
120
118
121
118
118
118
118
117
121
121
121
120
117
120
122
118
122
121
122
118
122
114
117
117
122
117
119
116
118
122
120
122
119
124
121
121
122
122
117
121
121
122
117
LATITUDE
min degrees
LONGITUDE
degrees
124
LATITUDE
min degrees
min
min
37.2
12
37.2
7.8
22.8
46.8
40.8
58.2
58.8
46.8
52.2
54
49.2
4.8
40.2
19.8
0
40.8
46.2
52.2
34.8
55.2
39
49.8
34.2
6
min
1.8
46.8
54
19.8
37.8
37.8
48
16.2
19.2
42
ALABAMA
Anniston
Auburn
Blythe
Burbank
Campo
43.2
22.2
28.2
16.8
34.2
51
40.8
37.8
3
13.8
46.8
52.8
40.8
1.8
43.8
16.8
19.2
46.2
43.2
58.2
22.8
19.8
7.2
34.2
7.2
46.8
0
13.2
49.2
9
3
2.4
55.2
16.2
34.2
1.8
2.4
31.2
9
57
3
9
31.8
51
19.2
4.2
16.8
37.2
1.2
13.8
13.2
37.2
1.2
3
7.8
33
34
32
33
37
39
35
33
37
41
34
34
32
34
33
41
36
36
36
33
34
33
37
32
32
34
38
34
37
33
33
33
37
33
39
38
38
37
32
37
37
35
41
36
41
34
38
34
32
34
37
34
34
33
35
37
35
37
34
39
34
35
40
40
33
38
36
37
33
Shelter Cove
Siskiyou
Stockton
Superior Val
Susanville
Thermal
Torrance
Travis AFB
Tahoe
Tustin Mcas
Ukiah
Van Nuys
Vandenberg
Visalia
COLORADO
Air Force A
Akron
Alamosa
Aspen
Brmfield/Jef
Buckley
Colo Sprgs
Cortez
4.2
28.2
15
0.6
57
10.2
19.8
55.8
7.8
49.8
1.2
28.8
57
2.4
40
41
37
35
40
33
33
38
39
33
39
34
35
36
85
85
86
87
85
85
86
86
86
88
88
86
87
86
86
87
51
26.4
45
15
27
43.2
5.4
46.2
22.2
15
4.2
2.4
37.2
59.4
1.2
33
32
33
32
31
31
33
34
32
30
30
32
34
32
31
33
34.8
40.2
34.2
54
19.2
16.8
58.2
39
22.8
40.8
37.8
18
122
121
117
120
116
118
121
120
117
123
118
120
Birmingham
Centreville
Dothan
Fort Rucker
Gadsden
Huntsville
Maxwell AFB
Mobile
Mobile Aeros
Montgomery
Muscle Shoal
Selma
Carlsbad
Castle AFB
Chico
China Lake
Chino
Concord
Crescent Cty
Daggett
Edwards AFB
El Centro
El Monte
El Toro
Eureka
7.8
13.2
12
45
119
19.2
20.4
52.2
13.8
Troy
105
103
105
106
105
104
104
108
107
104
107
106
104
104
105
105
105
108
104
106
103
102
106
103
107
104
107
106
104
105
21
39
40
37
39
39
39
38
37
40
39
37
39
39
38
39
40
40
39
40
38
38
38
39
39
38
38
39
38
37
40
31.2
10.2
27
13.2
54
43.2
49.2
18
30
45
9
39
34.2
40.8
34.2
27
34.8
7.2
25.8
33
3
7.2
15
10.8
30
16.8
31.8
31.8
15
Tuscaloosa
ALASKA
Anchorage
Barrow
Fairbanks
Haines Hrbor
Homer
Juneau
Ketchikan
Kodiak
Nome
Sitka
Sitkinak
Skagway
Valdez
ARIZONA
Davis-M AFB
Deer Valley
Douglas
Falcon Fld
Flagstaff
Fort Huachuc
Gila Bend
Goodyear
GrandCanyon
Kingman
Luke
37.2
Fort Hunter
Fort Ord
Fresno
13.2
52.2
52.2
7.2
149
156
147
135
151
134
131
152
165
135
154
135
146
51
61
71
64
59
59
58
55
57
64
57
56
59
61
13.2
18
46.8
52.2
25.8
3
34.8
4.2
3
25.8
21
1.2
31.8
21
Fullerton
49.2
13.8
37.8
22.2
21
45
30
4.2
52.8
45
George AFB
Hawthorne
Hayward
45
43.2
37.8
31.8
52.2
45
55.2
49.8
46.2
3
Imperial
Craig-Moffat
Denver
Durango
Eagle
Imperial Bch
La Verne
Lake Tahoe
Lancaster
Livermore
Long Beach
Los Alamitos
Los Angeles
Mammoth
March AFB
Marysville
Mather AFB
Mcclellan
Merced
54
43.8
42
Englewood
Fort Carson
Fraser
Ft Col/Lovel
Ft Collins
Grand Jct
Greeley-Wld
Gunnison
La Junta
Lamar
Leadville
Limon
Montrose
Pueblo
Rifle
Salida
49.2
46.8
55.8
37.8
52.8
6
34.2
40.2
16.8
52.2
37.8
25.2
3
43.8
34.8
19.2
13.8
13.2
46.2
42
6
43.8
3
12
49.8
3
28.2
40.2
49.8
7.2
34.8
57
40.2
9
30
7.8
1.2
4.8
110
112
109
111
111
110
113
112
112
113
112
111
111
112
112
109
111
110
110
111
110
115
114
114
52.8
4.8
3.6
43.8
40.2
21
10.2
22.8
9
57
22.8
27
19.8
1.2
25.8
40.8
55.2
0
32
33
31
33
35
31
33
33
35
35
33
36
34
33
34
32
33
34
32
33
35
33
32
32
10.2
40.8
27
28.2
7.8
36
33
25.2
57
16.2
31.8
55.8
13.8
25.8
39
49.2
37.2
16.2
7.2
31.8
37.8
55.8
31.2
3.6
1.8
4.2
52.8
31.2
4.8
Miramar NAS
Modesto
Moffet
Mojave
Montague
Monterey
Mount Shasta
Mount Wilson
Napa
Needles
North Is
Norton AFB
Oakland
Ontario Intl
Oxnard
Palm Springs
Palmdale
Palo Alto
Paso Robles
Pillaro Pt
Point Mugu
Pt Arena
Pt Arguello
Pt Piedras
Red Bluff
Redding
Riverside
Sacramento
Salinas
San Carlos
San
3
19.8
52.2
Page
Payson
Phoenix
Prescott
Safford Awrs
Scottsdale
Show Low
Tucson
Williams AFB
Winslow
Trinidad
Winter Park
CONNECTICUT
0
Bridgeport
Danbury
Groton
73
73
72
72
72
72
72
7.8
28.8
3
41
41
41
41
41
41
41
10.2
22.2
19.8
43.8
13.2
18
Hartford
39
55.8
40.2
43.8
0
37.2
2.4
New Haven
New London
Windsor Loc
DELAWARE
Dover
Wilmington
D.C. WASH
Washington
FLORIDA
Apalachicola
Astor NAS
Avon Park G
Cape
Canaveral
Cecil
Crestview
Cross City
Daytona Bch
Duke Fld
Eglin AFB
Egmont Key
Fort Myers
Ft Lauderdale
Ft Myers
Gainesville
Homestead
Hurlburt Fld
Jacksonville
Key West
Lakeland
40.2
4.8
40.8
18
1.2
6
39
55.8
Yuma
Yuma Mcas
Yuma Prv Gd
ARKANSAS
Blytheville
Camden
El Dorado
Fayetteville
Ft Smith
75
75
28.2
3.6
39
39
7.8
40.2
51
7.2
37.8
49.8
7.2
13.2
7.2
16.8
15
1.8
27
3
3.6
15
89
92
92
94
94
93
93
90
92
91
94
94
90
57
35
33
33
36
35
36
34
35
35
34
36
33
36
58.2
31.2
13.2
0
19.8
16.2
28.8
49.8
13.2
10.2
10.8
27
77
27.6
38
57
2.4
4.8
10.2
22.2
9
0.6
39
22.8
55.8
7.8
0
85
81
81
80
1.8
34.2
33
29
29
28
28
43.8
7.2
4.8
Harrison
33
28.2
Hot Springs
Jonesboro
Little Rock
Pine Bluff
Springdale
Texarkana
Walnut Ridge
CALIFORNIA
Alameda
Alturas
57
81
86
83
81
86
86
82
81
80
81
82
80
86
81
81
81
82
85
81
52.8
31.2
0.6
30
30
29
29
30
30
27
26
26
26
29
25
30
30
24
28
27
30
30
13.2
46.8
37.2
10.8
39
28.8
36
34.8
4.2
31.2
40.2
31.2
25.2
3
37.2
31.2
31.8
46.2
52.2
9
52.2
16.2
22.8
40.8
40.8
45
55.8
7.8
Clemente
San Diego
San
117
122
7.8
22.8
32
37
49.2
37.2
122
120
124
119
121
116
116
116
118
120
19.2
31.8
0.6
3
27
57
37.2
40.8
3.6
4.2
37
41
40
35
39
33
35
34
37
39
46.8
28.8
58.8
25.8
7.8
55.8
16.8
16.2
36
Francisco
San Jose
San Luis Obi
San Mateo
San Miguel
Sandburg
Santa Ana
Santa Barb
Santa Maria
Santa Monica
Santa Rosa
Arcata
121
120
117
120
118
117
119
120
118
122
55.2
39
34.8
2.4
43.8
52.8
49.8
27
37
35
33
34
34
33
34
34
34
38
22.2
13.8
22.8
1.8
39
Bakersfield
Beale AFB
Beaumont
Bicycle Lk
Big Bear
40.8
28.8
25.8
13.8
33
1.8
51
50.4
24
45
40.2
25.8
54
1.2
31.2
Bishop
Blue Canyon
57
16.8
Macdill AFB
Marianna
Mayport NAS
31.2
10.8
25.2
27
49.2
52
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LONGITUDE
degrees
80
LATITUDE
min degrees
LONGITUDE
degrees
87
LATITUDE
min degrees
LONGITUDE
degrees
90
LATITUDE
min degrees
min
6
49.2
7.8
37.2
25.8
12
13.8
21
58.2
55.2
46.8
24
22.8
58.2
31.2
4.2
min
4.8
min
10.8
7.8
Melbourne
Miami
37.8
16.8
4.8
40.8
19.2
40.8
3.6
19.2
3.6
40.8
15
28
25
26
28
28
30
28
30
27
27
28
27
30
27
28
30
27
26
Glenview
NAS
Kankakee
Macomb
Marion
Marseilles
Mattoon
Moline/Quad
Mount
Vernon
Peoria
Quincy
Rockford
Salem
Scott AFB
Springfield
Sterling
Taylorville
Vandalia
INDIANA
Bakalar
Bloomington
Elkhart
Evansville
Fort Wayne
Gary
Grissom AFB
Indianapolis
Muncie
South Bend
Terre Haute
W Lafayette
IOWA
Burlington
Cedar Rapids
Des Moines
Dubuque
Estherville
Fort Dodge
Lamoni
Mason City
Ottumwa
Sioux City
Spencer
Waterloo Mun
KANSAS
Chanute
Col. J Jabar
Concordia
Dodge City
Elkhart
49.2
42
Grand Isle
High Island
Houma
Intercoastal
Lafayette
Lake Charles
Lk Palourde
Missippi Can
Monroe
Morgan City
New Iberia
New Orleans
S Marsh Isl
Shreveport
Slidel
4.2
2.4
39
7.2
0
13.2
0.6
3
29
28
29
29
30
30
29
28
32
29
30
29
28
32
30
80
81
80
81
85
80
87
82
82
81
82
84
82
80
85
80
94
90
92
92
93
91
89
92
91
91
90
91
93
89
Naples
Nasa Shuttle
Orlando
87
90
89
88
88
90
88
51
39.6
0
40.8
16.8
31.2
51.6
41
40
37
41
39
41
38
4.2
31.2
45
22.2
28.8
27
34.2
43.8
12
Panama City
Patrick AFB
Pensacola
Ruskin
Saint Peters
Sanford
7.2
42
46.8
31.2
42
19.2
3
1.2
52.8
15
58.8
45
89
91
89
88
89
89
89
89
89
40.8
1.2
0.6
57.6
51
40.2
40.2
19.8
10.2
40
39
42
38
38
39
41
39
38
40.2
55.8
12
37.8
33
1.8
Sarasota
Tallahassee
Tampa Intl
Titusville
Tyndall AFB
Vero Beach
West Palm
Beach
33
58.8
18
31.2
21
22.2
31.8
4.8
34.8
25.2
7.2
49.2
51
MAINE
Augusta
Bangor
39
40.8
44.4
31.8
59.4
69
68
68
69
68
69
67
67
70
68
69
70
4.8
44
44
44
43
46
45
46
46
43
46
44
44
19.2
48
27
80
49.2
22.2
55.8
1.2
Bar Harbor
Brunswick
Caribou Mun
Greenville
Houlton
Loring AFB
Portland
Presque Isle
Rockland
Rumford
MARYLAND
Andrews AFB
Baltimore
Fort Meade
Hagerstown
Ocean City
Patuxent
Whiting Fld
GEORGIA
Albany
87
1.2
30
43.2
52.8
52.2
27
86
86
86
87
85
87
86
86
85
86
87
86
3
37.2
0
39
39
41
38
41
41
40
39
40
41
39
40
22.8
7.8
43.2
3
0
37.2
39
43.8
13.8
42
27
25.2
84
82
83
84
81
81
84
84
85
81
81
85
83
83
83
85
83
82
10.8
31.2
19.2
25.2
58.2
22.8
55.8
31.2
0
34.2
9
4.2
39
1.2
31
31
33
33
33
31
32
33
32
31
32
33
32
30
32
34
30
31
31.8
31.8
57
39
22.2
9
31.2
55.2
19.8
52.8
1.2
33
Alma
Athens
46.8
52.8
19.2
3
7.2
52.8
7.8
57
31.8
1.2
25.2
9
16.2
22.8
19.2
1.8
55.8
Atlanta
39
Augusta/Bush
Brunswick
Columbus
Dobbins AFB
Fort Benning
Ft Stewart
Hunter Aaf
La Grange
Macon/Lewis
Moody AFB
Robins AFB
Rome/Russell
Valdosta
Waycross
HAWAII
Barbers Pt
Barking San
Fr Frigate
Hilo
Honolulu Int
Kahului Maui
Kaneohe Mca
Kilauea Pt
Lanai-Lanai
Lihue-Kauai
Maui
40.8
4.2
52.8
76
76
76
77
75
76
76
75
52.2
40.2
46.2
43.2
7.8
2.4
10.2
3
38
39
39
39
38
38
39
38
49.2
10.8
4.8
42
33
16.8
28.2
19.8
0.6
42
91
91
93
90
94
94
93
93
92
96
95
92
7.2
4.2
39
4.2
45
10.8
55.8
19.8
27
22.8
9
40
41
41
42
43
42
40
43
41
42
43
42
46.8
52.8
31.8
24
24
33
37.2
9
6
24
10.2
33
58.2
37.8
21
46.8
15
3.6
Phillips
Salisbury
10.2
16.8
2.4
MASSACHUSETTS
Bedford
71
70
71
70
69
71
70
71
70
70
70
71
70
73
70
72
72
71
16.8
55.2
1.8
3
58.2
3.6
16.8
7.2
37.2
4.2
58.2
10.8
31.2
10.8
55.8
43.2
31.8
52.2
42
42
42
41
41
42
41
42
41
41
41
42
41
42
42
42
42
42
28.2
34.8
22.2
46.8
40.2
34.2
40.2
43.2
24
Beverly
Boston
Cape Cod
Chatham
Fort Devens
Hyannis
Lawrence
Marthas Vine
Nantucket
New Bedford
Norwood
158
160
166
155
157
156
158
159
156
159
156
157
156
156
7.2
1.8
28.2
4.2
55.8
25.8
16.8
40.2
57
21
49.8
0.6
21
22
24
19
21
20
21
22
20
21
20
21
20
20
31.8
3
27
43.2
21
54
45
22.8
48
58.8
58.2
9
25.2
0
2.4
95
97
97
99
101
96
94
96
100
101
99
99
97
94
100
96
97
98
94
98
97
95
95
97
28.8
13.2
39
58.2
52.8
1.2
55.2
46.2
43.2
4.2
16.2
49.8
52.2
52.8
58.2
40.2
16.2
34.8
5.4
37
37
39
37
37
38
39
39
37
39
38
39
38
38
37
39
37
37
38
38
38
39
38
37
40.2
45
33
46.2
0
19.8
22.2
3
55.8
22.2
51
22.8
4.2
49.2
3
9
37.2
18
15
40.8
10.8
39
Otis ANGB
Pittsfield
Molokai
Emporia
Ft Leavnwrth
Ft Riley
Garden City
Goodland
Hays
15.6
9
10.2
12
Upolo Pt Ln
Waimea-
Koha
28.2
7.2
S Weymouth
Westfield
Westover
Worcester
MICHIGAN
Alpena
Ann Arbor
Battle Creek
Benton
IDAHO
16.2
Boise
116
113
114
116
13.2
46.2
13.2
49.2
43
42
44
47
34.2
31.8
31.2
46.2
Burley
Challis
Coeur
Hill City
83
83
85
86
34.2
45
13.8
25.8
45
42
42
42
4.2
13.2
18
Hutchinson
Johnson Cnty
Liberal
Manhatten
Mcconnell Af
Medicine Ldg
Olathe
Russell
Salina
Topeka
Topeka/Forbe
Wichita
KENTUCKY
Bowling Gren
Ft Campbell
Ft Knox
Jackson
Lexington
London
Louisville
Owensboro
Paducah
Pikeville
LOUISIANA
Alexandria
Barksdale
Baton Rouge
Boothville
Cameron Heli
Claiborne R
England AFB
Eugene Is.
Fort Polk
d'Alene
7.8
Elk City
115
115
116
112
117
112
113
116
115
112
113
111
114
114
25.8
10.2
7.8
4.2
1.2
19.2
22.2
0.6
4.8
3.6
45
43
45
43
46
42
42
44
47
42
45
42
43
42
49.2
0
Harbor
Gooding
Chippewa
Coopersville
Copper Harb
Detroit
Escanaba
Flint/Bishop
Grand Rapids
Hancock
Harbor Beach
Houghton
Lake
Iron Mtn
Ironwood
Jackson
Kalamazoo
Lansing
Manistee
Marquette
Menominee
Muskegon
Pellston
84
85
87
83
87
83
85
88
82
84
28.2
57
51
1.2
4.8
45
31.2
3
46
43
47
42
45
42
42
47
43
44
15
Grangeville
Idaho Falls
Lewiston
Malad City
Malta
Mccall
Mullan
Pocatello
Salmon
55.2
31.2
22.8
10.2
18
52.8
28.2
55.2
10.8
39
4.2
51
52.2
48
4.2
57
39
28.2
25.2
43.8
58.2
52.8
10.2
49.8
22.2
49.2
39
37.2
40.2
25.8
31.8
40.8
5.4
34.8
1.8
86
87
85
83
85
84
85
87
88
82
25.8
3
58.2
19.2
0
36
36
37
37
38
37
38
37
37
37
58.2
40.2
54
36
3
4.8
13.8
45
4.2
28.8
Soda Springs
Sun Valley
Twin Falls
ILLINOIS
Alton
30
28.8
88
90
84
85
84
86
87
87
86
84
83
84
84
87
82
85
85
7.2
7.8
28.2
33
3.6
15
57
37.8
15
4.8
25.2
4.8
22.2
2.4
49.8
55.2
34.8
45
46
42
42
42
44
46
45
43
45
42
43
46
46
42
45
44
49.2
31.8
16.2
13.8
46.2
16.2
52.8
7.2
10.2
34.2
40.2
31.8
28.2
21
28.8
90
88
90
88
89
89
89
89
88
87
87
88
88
88
90
3
19.2
9
55.8
3.6
13.2
15
5.4
16.8
39
38
41
38
40
41
37
37
38
40
41
40
41
39
41
40
52.8
46.2
34.2
28.8
9.6
4.2
Aurora
40.2
10.2
46.2
31.2
Bistate Park
Bloomington
Bradford
Cairo
Carbondale
Centralia
Champaign
Chicago
4.2
46.8
30.6
1.8
54
12
55.8
49.8
55.2
55.8
92
93
91
89
93
92
92
91
93
1.8
40.2
9
40.2
1.8
57
33
46.8
1.2
31
32
30
29
29
31
31
28
31
22.8
30
31.8
33
46.8
13.2
19.8
28.2
3
Pontiac
Saginaw
Sault Ste M
Sawyer AFB
Selfridge
Seul Choix
Traverse Cty
Danville
3.6
43.2
52.2
15
DeKalb
Decatur
Du Page
Galesburg
37.2
55.2
43.8
25.8
53
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LONGITUDE
degrees
83
LATITUDE
min degrees
LONGITUDE
degrees
LATITUDE
min degrees
LONGITUDE
degrees
106
LATITUDE
min degrees
min
27
13.8
min
min
37.2
37.8
4.2
25.2
13.8
10.8
37.8
Wurtsmith
Ypsilanti
2.4
31.8
44
42
NEBRASKA
Ainsworth
Alliance
Beatrice
Broken Bow
Burwell
Chadron
Columbus
Cozad
Falls City
Grand Island
Hastings
Imperial
Kearney
Lincoln Muni
Mccook
Santa Fe
Silver City
Socorro
4.8
10.2
5.4
34.2
16.2
3.6
35
32
34
36
33
35
32
83
99
102
96
99
99
103
97
100
95
98
98
101
99
96
100
101
97
96
100
98
95
95
58.8
4.8
45
39
9
4.8
21
0
34.8
19.2
25.8
23.4
0
42
42
40
41
41
42
41
40
40
40
40
40
40
40
40
42
41
41
41
42
41
41
41
41
41
42
34.8
3
108
106
105
107
103
106
MINNESOTA
Albert Lea
Alexandria
Bemidji Muni
Brainerd-Crw
Detroit Laks
Duluth
93
95
94
94
95
92
91
94
96
93
92
93
94
93
95
93
95
94
92
93
94
96
90
95
95
22.2
22.8
55.8
7.8
52.8
10.8
49.2
25.2
4.2
43
45
47
46
46
46
47
43
46
47
47
48
45
44
44
44
46
46
43
44
45
48
47
48
43
40.8
52.2
30
19.2
25.8
46.8
49.8
27
52.2
4.2
58.2
36
19.8
43.8
51
13.2
3
58.8
22.2
7.8
28.2
7.2
Taos
Truth Or Con
Tucumcari
White Sands
NEW YORK
Albany
Ambrose
Binghamton
Buffalo
24
2.4
49.2
49.8
54
39
18
13.2
22.8
34.2
7.8
13.2
27
49.8
54
36
73
74
75
78
78
76
73
75
73
75
73
76
79
74
74
73
74
78
75
75
73
77
74
73
76
75
76
72
73
4.8
42
40
42
42
42
42
40
44
43
43
40
42
42
44
41
40
41
43
44
42
44
43
44
42
43
43
44
40
41
45
Ely
22.2
58.8
43.8
1.2
45
Fairmont
Fergus Falls
Grand Rapids
Hibbing
Intl Falls
Litchfield
Mankato
13.2
55.8
58.2
10.2
43.8
3
31.2
51
Dansville
Elmira
5.4
22.8
31.2
55.2
49.2
28.2
4.2
19.2
3
3
45
34.8
3
Farmingdale
Fort Drum
Glens Falls
Griffiss AFB
Islip
25.8
43.8
37.2
2.4
0.6
28.2
15
51
4.8
58.8
0.6
57
Mullen
Norfolk
21
Marshall Arpt
Minneapolis
Park Rapids
Pequot Lake
Rochester
Saint Paul
St Cloud
25.8
1.2
40.8
40.8
55.2
5.4
57
3.6
58.8
33
13.8
46.8
28.8
9
55.8
42
46.2
30
6
North Omaha
North Platte
O'neill
Offutt AFB
Omaha
Ord/Sharp
Scottsbluff
Sidney Muni
Valentine
NEVADA
Austin
Battle Mtn
Caliente
Elko
Ely/Yelland
Eureka
Fallon NAS
Hawthorne
Ind Sprng Rn
Las Vegas
Lovelock
Mercury
Nellis AFB
Owyhee
Reno
Tonopah
Wildhorse
Winnemucca
Yucca Flat
Ithaca
Jamestown
Massena
Monticello
New York
Newburgh
Niagara Fall
Ogdensburg
Oneonta
Plattsburgh
Rochester
Saranac Lk
Schenectady
Syracuse
Utica
55.2
55.8
33
18
4.2
98
37.2
52.2
6
Thief River
Tofte
10.8
49.8
21
4.2
103
102
100
34.8
55.8
39
Warroad
52.2
2.4
7.2
40.8
52.2
39
7.2
22.8
51
7.2
9
0
Worthington
MISSISSIPPI
Columbus
AFB
Golden Trian
Greenville
Greenwood
Gulfport
34.8
117
116
114
115
114
115
118
118
115
115
118
116
115
116
119
117
116
117
116
7.8
39
40
37
40
39
39
39
38
36
36
40
36
36
42
39
38
41
40
37
49.8
37.2
37.2
49.8
16.8
30
25.2
33
31.8
4.8
28.2
40.2
1.2
55.8
7.2
22.8
1.2
37.8
43.2
88
27
33
39
52.2
31.2
46.8
51
58.2
4.2
37.8
34.2
10.2
55.2
1.2
88
90
90
89
89
90
88
89
90
88
88
91
89
88
34.8
58.8
4.8
4.2
19.8
4.8
55.2
10.2
28.2
34.2
45
15
32.4
46.2
33
33
33
30
31
32
30
31
31
32
32
31
34
34
27
28.8
30
24
Watertown
Westhampton
White Plains
Hattiesburg
Jackson
28.2
19.2
25.2
40.2
10.8
33
19.8
37.2
23.4
16.2
51
4.2
Keesler AFB
Laurel
Mccomb
Meridian NAS
Meridian/Key
Natchez
NORTH CAROLINA
Asheville
6
82
75
80
76
76
75
76
78
78
79
81
82
77
77
79
75
77
77
79
78
77
79
77
80
33
33
55.8
52.8
3
35
35
35
34
36
35
36
35
35
36
35
35
34
35
35
35
35
34
35
35
35
35
34
36
25.8
16.2
13.2
54
37.2
13.8
34.8
30
4.2
19.8
54
Cape Hattera
Charlotte
Cherry Point
Dare Co Gr
Diamond Sho
Elizabeth
Fayetteville
Fort Bragg
Greensboro
Hickory
Hot Springs
Jacksonville
Kinston
Mackall Aaf
Manteo Arpt
New Bern
New River
Pope AFB
Raleigh-Durh
Rocky Mt
Southern Pin
Wilmington
Winston-
1.8
10.2
46.8
4.8
15
4.8
7.8
Oxford
3
15
Tupelo
10.8
52.8
55.8
57
22.8
49.2
37.2
37.8
3
40.8
3
25.8
1.2
16.2
0
7.8
MISSOURI
Columbia
Cape
92
89
13.2
34.8
38
37
49.2
13.8
4.8
34.8
NEW HAMPSHIRE
Berlin
4.8
Girardeau
Ft Leonard
Jefferson City
Joplin
Kansas City
Kirksville
Monett
71
71
72
72
71
72
71
71
71
70
71
10.8
3
0
16.2
25.8
1.8
25.8
1.8
44
43
42
42
43
43
42
44
42
43
44
34.8
12
48
45
54
92
92
94
94
92
94
95
90
94
93
93
95
90
91
92
93
7.8
10.2
3
43.2
33
21
21.6
28.2
33
43.2
22.8
31.8
22.2
46.2
25.2
33
37
38
37
39
40
37
35
36
38
40
37
40
38
38
37
38
45
36
Concord
Jaffrey
Keene
Laconia
49.2
19.2
1.8
55.2
4.8
10.2
19.2
6
19.8
39.6
46.2
51
54
34.2
37.8
55.8
16.2
46.8
4.8
Lebanon
Manchester
Mt Washingtn
Nashua
Pease AFB
Wolfeboro
NEW JERSEY
Atlantic CtIy
Barnegat Ls
Fairfield
Lakehurst
Mcguire AFB
Millville
Morristown
Newark Intl
Teterboro
Trenton
Muskogee
Poplar Bluff
Richards-Geb
Spickard
42
31.2
49.2
22.8
10.2
52.2
51
46.8
52.8
23.4
55.2
13.8
15
0
Springfield
St Joseph
St Louis
13.8
16.8
45
7.8
13.2
43.8
14.4
16.2
7.8
74
74
74
74
74
75
74
74
74
74
34.2
16.8
16.8
21
3.6
4.2
25.2
10.2
3
39
40
40
40
40
39
40
40
40
40
27
16.8
52.2
1.8
1.2
22.2
48
42
51
16.8
Vichy/Rolla
West Plains
Whiteman
AFB
MONTANA
Billings
Salem
NORTH DAKOTA
Bismarck
Devil's Lake
Dickenson
Fargo
Grand Forks
Jamestown
Lidgerwood
Minot
Roseglen
Williston
OHIO
Athens
Canton
100
98
102
96
97
98
45
5.4
4.8
4.8
10.8
40.8
9
16.8
49.8
37.8
46
48
46
46
47
46
46
48
47
48
46.2
7.2
46.8
54
108
111
105
112
112
112
113
106
104
111
109
109
112
106
114
109
110
111
105
114
112
104
111
31.8
9
40.2
3
22.2
33
9
37.2
4.8
22.2
49.8
46.2
0
55.8
16.2
27
25.8
10.8
52.2
4.8
45
45
45
45
48
45
46
48
47
47
46
48
46
47
48
47
45
47
46
46
44
47
44
48
Bozeman
Broadus
Butte
46.8
40.2
57
36
15
40.2
13.2
7.8
28.8
25.8
33
36
19.8
18
3
42
30
25.8
55.2
34.2
43.2
39
57
55.2
6
49.2
NEW MEXICO
Albuquerque
Cannon
Carlsbad
Clayton Arpt
Corona
97
Cut Bank
Dillon
106
103
104
103
105
107
108
108
107
103
106
3.6
35
34
32
36
34
32
36
35
35
32
32
3
101
101
103
16.2
45
19.2
16.2
9
40.8
4.2
13.8
46.8
5.4
22.8
19.8
27
6
15
Drummond
Glasgow
10.8
Glendive
Great Falls
Harlowton
Havre
82
81
84
81
82
84
83
82
82
83
81
80
81
13.8
25.8
40.2
40.8
52.8
1.2
40.2
31.2
55.8
4.8
39
40
39
41
40
39
41
40
39
41
41
41
39
12.6
55.2
3
31.2
0
Deming
Farmington
Gallup/Clark
Grants
Hobbs
Holloman
AFB
Las Cruces
Las Vegas
Los Alamos
Moriarity
Northrup Str
Raton
45
Cincinnati
Cleveland
Columbus
Dayton
31.2
10.2
40.8
51
Helena
Jordan
1.2
0.6
54
Kalispell
Findlay
1.2
49.2
49.2
36
37.8
16.2
57
Lewiston
Livingston
Malmstrom
Miles City
Missoula
Monida
Mansfield
Rickenbacker
Toledo
Willoughby
Youngstown
Zanesville
106
105
106
106
106
104
104
46.2
9
16.8
3
2.4
3
31.8
32
35
35
34
32
36
33
18
39
52.8
58.8
54
44.4
18
2.4
40.2
5.4
19.2
10.8
0.6
Sidney
W Yellowston
Roswell
54
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LONGITUDE
degrees
LATITUDE
min degrees
LONGITUDE
degrees
LATITUDE
min degrees
LONGITUDE
LATITUDE
min degrees
min
min
40.8
58.2
55.2
degrees
100
98
min
22.2
31.8
10.2
1.8
13.2
9
22.2
51
OKLAHOMA
Altus AFB
Ardmore
Bartlesville
Clinton
Enid
Fort Sill
Gage
Hobart
Lawton
Mcalester
Norman
Oklahoma
Page
Ponca City
Stillwater
Tinker AFB
Tulsa
Vance AFB
OREGON
Astoria
Aurora
Baker
Brookings
Burns Arpt
Cape Blanco
Cascade
Corvallis
Eugene
Hillsboro
Klamath Fall
La Grande
Lake View
Meacham
Medford
Newport
North Bend
Ontario
Pendleton
Portland
Redmond
Roseburg
Salem
Sexton
The Dalles
Troutdale
Myrtle Beach
Shaw AFB
Spartanburg
78
80
81
55.8
28.2
57.6
33
33
34
San Angelo
San Antonio
Sanderson
South Brazos
Stephenville
Temple
Tyler/Pounds
Victoria
Wichita Flls
Wink
3
31
29
30
28
32
31
32
28
33
31
99
97
96
99
97
98
99
99
98
95
97
97
94
97
97
97
95
97
16.2
1.2
0
1.2
4.8
2.4
46.2
3
25.2
46.8
28.2
3.6
37.2
0.6
34
34
36
35
36
34
36
35
34
34
35
35
34
36
36
35
36
36
40.2
18
45
21
22.8
39
28.2
25.2
52.2
10.8
25.2
2.4
55.2
3
1.2
102
95
98
97
95
96
98
103
SOUTH DAKOTA
Aberdeen
Brookings
Chamberlain
Custer
98
96
99
103
103
98
25.8
4.8
19.2
3.6
45
44
43
43
44
44
45
43
45
44
44
44
45
43
44
42
27
18
48
46.2
9
22.8
55.8
46.2
31.8
3
22.8
3
9.6
34.8
55.2
55.2
18
0
Ellsworth
Huron
Lemmon
Mitchell
Mobridge
Philip
Pierre
Rapid City
Redig
Sioux Falls
Watertown
Yankton
0.6
58.8
46.8
34.2
52.8
13.8
24
40.8
43.8
9.6
25.2
12
13.2
10.2
1.8
25.8
3.6
16.8
4.2
19.2
43.8
9
102
98
UTAH
Blanding
109
110
113
112
113
110
110
111
111
113
109
112
110
111
110
113
111
112
109
114
46.8
4.2
0.6
34.8
4.2
9
43.2
58.2
51
1.8
45
1.2
45
43.2
37.8
3.6
58.2
1.2
31.2
3
38
37
37
39
41
39
38
41
41
38
38
41
39
40
40
37
40
40
40
41
1.8
30
42
19.8
3
0
22.2
7.2
46.8
43.2
46.2
10.8
37.2
13.2
30
100
101
100
103
103
96
Bullfrog Mar
Cedar City
Delta
Eagle Range
Green River
Hanksville
Hill AFB
Logan
Milford
Moab
Ogden
Price/Carbon
Provo
Roosevelt
Saint George
Salt Lake Ct
Tooele
5.4
22.8
5.4
55.2
19.8
97
97
22.8
123
122
117
124
118
124
121
123
123
122
121
118
120
118
122
124
124
117
118
122
121
123
123
123
121
122
52.8
45
49.2
28.2
57
46
45
44
42
43
43
45
44
44
45
42
45
42
45
42
44
43
44
45
45
44
43
44
42
45
45
9
15
49.8
4.8
36
22.8
40.8
30
7.2
31.8
9
16.8
10.8
30
22.2
37.8
25.2
1.2
TENNESSEE
Bristol
82
85
87
85
89
88
83
90
85
86
86
2.4
1.2
25.2
4.8
2.4
55.2
58.8
0
36
35
36
35
36
35
35
35
35
36
36
28.8
1.8
37.2
57
1.2
36
49.2
3
9
Chattanooga
Clarksville
Crossville
Dyersburg
Jackson
Knoxville
Memphis Intl
Monteagle
Nashville
Smyrna
TEXAS
Abilene
Alice
Amarillo
Austin
Bergstrom Af
Big Sky
Big Spring
Brownsville
Brownwood
Carswell AFB
Chase NAS
Childress
College Stn
Corpus Chrst
Cotulla
Dalhart
Dallas/FW
Del Rio
Dyess AFB
El Paso
Ellington Af
Fort Worth
Ft Hood Aaf
Galveston
Gray AFB
Greenville
Guadalupe
Harlingen
Hondo
Houston
Junction
Kelly AFB
Kerrville
Killeen
57
52.8
16.8
13.2
57
43.8
0
4.8
46.8
10.2
27
30.6
40.8
3
Vernal
7.2
0
Wendover
VERMONT
Burlington
Montpelier
Newport
13.2
21
73
72
72
73
72
72
9
44
44
45
43
44
42
28.2
12
33
31.8
25.2
52.8
2.4
52.2
3
15
1.2
51
3.6
9
22.2
0
22.2
9
2.4
99
98
101
97
40.8
1.8
4.2
32
27
35
30
30
32
32
25
31
32
28
34
30
27
28
36
32
29
32
31
29
32
31
29
31
33
31
26
29
29
30
29
29
31
27
27
29
32
33
31
30
26
31
32
28
33
34
30
33
28
25.2
43.8
13.8
18
12
23.4
18
34.2
19.8
57
1.2
52.8
Rutland
4.2
St Johnsbury
Wilmington
VIRGINIA
Charlottes
Chesapeake
Danville
Fort Belvoir
Fort Eustis
Hot Springs
Langley AFB
Lynchburg
Newport
97
40.8
28.8
27
25.8
57.6
25.8
40.2
16.8
22.2
3
13.2
33
1.8
55.2
51
2.4
40.8
36
101
101
97
98
97
97
100
96
97
99
102
97
100
99
106
95
97
97
94
97
96
104
97
99
95
99
98
99
97
97
99
100
94
101
94
104
98
102
98
96
95
101
94
78
76
79
77
76
79
76
79
76
27
1.2
38
37
36
38
37
37
37
37
37
7.8
30
34.2
43.2
7.8
57
4.8
19.8
7.8
16.2
13.8
55.2
37.2
37.2
33
54
47.4
46.8
22.2
25.8
34.8
46.2
27
19.8
10.8
37.2
49.2
22.2
1.2
PENNSYLVANIA
Allentown
Altoona
75
78
80
79
78
78
80
79
76
78
76
79
76
76
75
75
78
79
75
77
77
75
76
75
25.8
19.2
19.8
5.4
37.8
5.4
10.8
52.2
51
49.8
1.8
40
40
40
40
41
41
42
41
40
40
40
40
40
40
40
39
41
40
40
39
40
41
41
40
39
18
45
16.2
48
10.8
4.8
22.8
13.2
19.2
7.8
16.8
12
25.8
4.8
52.8
28.2
21
22.8
43.8
51
19.8
15
12
3
1.2
54
News
Beaver Falls
Blairsville
Bradford
Dubois
Erie
Norfolk NAS
Norfolk Rgnl
Oceana NAS
Quantico Mca
Richmond
Roanoke
Muni
76
76
76
77
77
79
16.8
1.2
1.8
1.8
19.8
58.2
36
36
36
38
37
37
55.8
54
49.2
30
30
19.2
22.2
25.8
48
37.2
49.2
9
16.2
4.2
4.2
49.8
13.8
21
58.2
30
22.8
58.8
4.8
10.2
21
43.2
52.2
49.8
4.2
Franklin
Harrisburg
Johnstown
Lancaster
Latrobe
Middletown
Muir
Nth Philadel
Philadelphia
Philipsburg
Pittsburgh
Reading
Staunton
Volens
78
78
75
51
58.8
28.8
38
36
37
16.2
57
51
2.4
Wallops Sta
WASHINGTON
Bellingham
Bremerton
Burlington
Colville
46.2
34.2
1.2
15
7.8
55.8
58.2
25.8
49.8
43.8
55.2
9
4.8
40.2
10.2
21
46.2
34.8
4.8
40.8
49.2
28.2
46.8
43.2
49.2
45
122
122
122
118
119
122
117
122
119
123
122
119
122
122
119
119
123
117
124
122
122
123
117
122
122
31.8
46.2
19.8
28.2
31.2
16.8
39
34.8
3.6
58.2
28.8
19.2
48
47
48
48
47
47
47
47
46
46
47
47
48
46
48
46
48
46
47
47
47
47
47
47
46
48
28.8
30
52.8
19.2
55.2
37.2
4.8
34.2
58.2
9
12
15
58.2
25.2
16.2
7.2
Ephrata
Everet/Paine
Fairchild
Fort Lewis
Hanford
Hoquiam
Mcchord AFB
Moses Lake
Oak Harbor
Olympia
Omak
Pasco
Port Angeles
Pullman
Quillayute
Renton
Seattle
Shelton
Spokane
Tacoma
Toledo
Site R
State Colleg
Wilkes-Barre
Williamsport
Willow Grove
RHODE ISLAND
Block Island
Nth Kingston
Providence
SOUTH CAROLINA
Anderson
Beaufort
Kingsville
Laredo Intl
Laughlin AFB
Longview
Lubbock
Lufkin
Marfa
Mcallen
Midland
30
31.8
22.2
22.8
39
13.8
22.2
10.8
57
46.8
43.2
37.8
10.2
34.8
36
71
71
71
34.8
25.2
25.8
41
41
41
10.2
36
43.8
40.8
1.2
5.4
31.8
7.2
3
7.2
33
13.2
1.8
9
31.8
34.8
4.8
13.8
10.8
4.2
15
27
42.6
1.2
3
82
80
80
81
79
82
80
43.2
43.2
1.8
7.2
43.2
21
34
32
32
33
34
34
33
30
28.8
54
57
10.8
51
Mineral Wlls
Palacios
45
57
30
27
Charleston
Columbia
Florence
Greenville
Mcentire
Paris/Cox
Plainview
Port Arthur
Reese AFB
Rockport
102
97
15
4.8
55.2
1.8
4.8
37.8
16.2
28.8
55
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LONGITUDE
degrees
118
LATITUDE
min degrees
LONGITUDE
degrees
LATITUDE
min degrees
LONGITUDE
degrees
LATITUDE
min degrees
min
6
24
21
34.2
min
min
Walla Walla
Wenatchee
Whidbey Is
Yakima
16.8
1.2
39
46
47
48
46
WISCONSIN
Appleton
WYOMING
Big Piney
Casper
Cheyenne
Cody
Douglas
Evanston
Gillette
Jackson
Lander
Laramie
Moorcroft
Rawlins
Riverton
Rock Springs
Sheridan
Worland
Yellowstone
120
122
120
88
91
88
89
91
90
89
87
87
89
88
88
89
91
90
89
31.2
28.8
7.8
44
44
44
42
43
43
43
44
42
44
44
44
45
45
43
44
15
110
106
104
109
105
111
105
110
108
105
104
107
108
109
106
107
110
0.6
28.2
49.2
1.2
42
42
41
44
42
41
44
43
42
41
44
41
43
41
44
43
44
34.2
55.2
9
31.2
45
19.8
21
36
49.2
19.2
21
48
3
Eau Claire
Green Bay
Janesville
La Crosse
Lone Rock
Madison
Manitowac
Milwaukee
Mosinee
Neenah
Oshkosh
Rhinelander
Rice Lake
Volk Fld
52.2
28.8
37.2
52.2
12
7.8
7.8
57
46.8
13.2
0
37.8
28.8
55.8
55.2
31.8
WEST VIRGINIA
Beckley
1.8
15
81
81
81
80
79
82
80
77
79
81
80
80
7.2
13.2
3.6
13.8
51
33
2.4
58.8
55.2
25.8
39
37
37
38
39
38
38
37
39
39
39
40
37
46.8
18
22.8
0
Bluefield
10.8
19.8
40.2
5.4
Charleston
Clarksburg
Elkins
Huntington
Lewisburg
Martinsburg
Morgantown
Parkersburg
Wheeling
22.2
16.8
52.8
22.2
52.2
24
39
21
10.8
27.6
31.8
43.8
43.8
40.8
48.6
1.2
40.2
31.8
34.2
27
27
4.2
43.2
16.2
37.2
36
58.2
58.2
25.2
46.2
58.2
33
Wh Sulphur
1.2
Wausau
CANADA
CITY
Calgary
Churchill
PROVINCE
Alberta
Newfoundland
Northwest Terr.
Alberta
New Brunswick
Northwest Terr
Newfoundland
Nova Scotia
BC
Ontario
Labrador
Quebec
Yukon
Yukon
LONGITUDE
LATITUDE
CITY
Glasgow
Guatemala City Guatemala
COUNTRY
Scotland
LONGITUDE
LATITUDE
114
7
51
58
67
53
45
67
53
44
55
49
52
45
60
59
45
56
46
46
50
52
47
43
49
48
60
49
14
45
49
34
57
29
15
39
15
47
56
32
34
12
18
15
14
50
30
10
34
39
16
26
43
53
4
15 w
31 w
56 w
2 e
38 e
23 w
0 e
19 e
7 w
20 e
48 e
4 e
55
14
2
50 n
37 n
10 s
33 n
38 n
8 n
10 n
52 s
10 s
30 n
16 s
12 s
59 n
27 s
45 n
0 s
25 n
32 n
45 n
26 n
30 n
35 n
20 n
12 n
29 n
47 s
26 n
27 n
53 s
45 n
8 n
94
0
90
79
10
23
82
25
147
70
104
106
28
76
68
1
Coppermine
Edmonton
Frederickton
Ft Mcpherson
Goose Bay
Halifax
Hazelton
Kenora
Labrador City
Montreal
Mt. Logan
Nakina
Ottawa
Peace River
Pr. Edward Isl
Quebec
115
113
66
134
60
63
127
94
21
25
40
50
20
34
38
29
52
39
24
48
45
18
9
Guayaquil
Hamburg
Hammerfest
Havana
Helsinki
Hobart
Ecuador
Germany
Norway
Cuba
Finland
Tasmania
Chile
53
70
23
60
42
20
52
6
Iquique
Irkutsk
Russia
66
73
Jakarta
Indonesia
South Africa
Jamaica
Bolivia
Johannesburg
Kingston
La Paz
26
17
16
53
12
53
51
45
40
53
14
43
23
21
37
19
45
34
55
48
32
35
1
140
132
75
117
63
49 w
22 w
30 w
2 w
Ontario
Alberta
Leeds
Lima
England
Peru
77
3
Nova Scotia
Quebec
Saskatchewan
Saskatchewan
Newfoundland
Ontario
BC
BC
Yukon
Manitoba
Liverpool
London
Lyons
England
England
France
Spain
0 w
71
15
38
32
43
23
7
20
3
9
0
5 w
Regina
104
101
52
4
3
2
120
5
50 e
42 w
15 w
57 e
20 e
25 w
45 e
58 e
7 w
10 e
10 w
36 e
35 e
57 e
56 e
55 e
53 e
15 e
37 w
48 e
30 e
42 e
32 w
15 w
20 e
25 e
52 e
5 w
Saskatoon
St. Johns
Toronto
Vancouver
Victoria
Madrid
Manchester
Manila
Marseilles
Mazatlán
Mecca
Melbourne
Mexico City
Milan
England
Phillipines
France
Mexico
Saudi Arabia
Australia
Mexico
Italy
79
123
123
135
97
106
39
144
99
9
56
37
11
129
136
36
118
14
1
30
135
10
79
55
2
116
115
4
Whitehorse
Winnipeg
INTERNATIONAL
Montevideo
Moscow
Munich
Nagasaki
Nagoya
Nairobi
Uruguay
Russia
Germany
Japan
Japan
Kenya
Aberdeen
Scotland
2
9 w
57
9 n
Adelaide
Amsterdam
Ankara
Asunción
Athens
Auckland
Bangkok
Barcelona
Belém
Belfast
Belgrade
Berlin
Birmingham
Bombay
Bordeaux
Bremen
Brisbane
Bristol
Australia
Holland
Turkey
Paraguay
Greece
New Zealand
Thailand
Spain
138
4
36 e
53 e
55 e
40 w
43 e
45 e
30 e
9 e
34
52
39
25
37
36
13
41
1
55 s
22 n
55 n
15 s
58 n
52 s
45 n
23 n
28 s
37 n
52 n
30 n
25 n
0 n
48 n
7 n
25 s
3 n
32
57
23
174
100
2
Nanjing
Naples
China
Italy
32
40
54
46
34
59
8
50 n
58 n
27 n
32 n
57 n
58 n
45 n
48 n
55 n
57 s
25 n
57 s
54 n
56 s
28 s
56 n
31 s
10 n
40 n
17 n
0 s
Newcastle
Odessa
Osaka
England
Ukraine
Japan
Brazil
48
5
20
13
1
72
0
8
29 w
56 w
32 e
25 e
55 w
48 e
31 w
49 e
8 e
Northern Ireland
Yugoslavia
Germany
England
India
54
44
52
52
19
44
53
27
51
50
44
47
34
30
23
33
10
28
29
55
31
12
53
29
55
50
6
Oslo
Norway
Panama
Surinam
France
China
Panama City
Paramaribo
Paris
5
48
39
31
50
22
41
12
33
59
23
31
42
59
34
18
35
35
32
45
19
48
52
41
47
Beijing
France
50 n
5 n
Perth
Plymouth
Australia
England
Germany
Australia
England
Belgium
Romania
Hungary
Argentina
Egypt
153
2
4
29 s
28 n
52 n
25 n
30 n
35 s
2 n
Rio de Janeiro Brazil
43
12
38
70
30
46
121
23
18
151
47
51
139
13
12
96
16
21
174
8
12 w
27 e
27 w
45 w
18 e
31 w
28 e
20 e
3 e
35 w
22 e
7 e
Rome
Italy
Brussels
Bucharest
Budapest
Buenos Aires
Cairo
Salvador
Santiago
St. Petersburg
Sao Paulo
Shanghai
Sofia
Stockholm
Sydney
Tananarive
Teheran
Tokyo
Brazil
Chile
Russia
Brazil
China
Bulgaria
Sweden
Australia
Madagascar
Iran
26
19
58
31
113
18
67
106
106
12
64
130
6
5 e
22 w
21 e
15 e
22 e
2 w
Canton
China
7 n
Cape Town
Caracas
Chihuahua
Chongqing
Copenhagen
Córdoba
Darwin
Dublin
Durban
Edinburgh
Frankfurt
Georgetown
South Africa
Venezuela
Mexico
55 s
28 n
37 n
46 n
40 n
28 s
28 s
20 n
53 s
55 n
7 n
0 e
5 w
33 e
45 e
45 e
12 e
20 e
10 w
20 e
0 e
50 s
45 n
40 n
57 n
26 n
10 n
14 n
14 n
17 s
21 n
China
34 e
34 e
10 w
51 e
15 w
53 e
10 w
41 e
15 w
Denmark
Argentina
Australia
Ireland
South Africa
Scotland
Germany
Guyana
Japan
Tripoli
Libya
Venice
Italy
Veracruz
Vienna
Warsaw
Wellington
Zürich
Mexico
Austria
Poland
New Zealand
Switzerland
30
3
8
47 e
31 e
58
45 n
56
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Appendix D - RS-232 Connection
Using the included NexRemote software you can control your CPC telescope with a computer via the RS-232 port
located on the computerized hand control and using the RS-232 cable (#93920). For information about using
NexRemote to control your telescope, refer to the instruction sheet that came with the NexRemote CD and the help
files located on the disk. In addition to NexRemote, the CPC can be controlled using other popular astronomy software
programs. For detailed information about controlling the CPC via the RS-232 port, Communication protocols and the
57
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APPENDIX E – MAPS OF TIME ZONES
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Observational Data Sheet
Yearly
Meteor Showers
Shower
Date
Peak
4-Jan
Hourly Rate
60-200
15
Quadrantids
Lyrids
pi-Puppids
eta-Aquarids
June Bootids
July Phoenicids
Southern delta-Aquarids
Perseids
Jan 01-Jan 05
Apr 16-Apr 25
Apr 15-Apr 28
Apr 19-May 28
Jun 26-Jul 02
Jul 10-Jul 16
Jul 12-Aug 19
Jul 17-Aug 24
Aug 25-Sep 05
Oct 06-Oct 10
Oct 02-Nov 07
Nov 14-Nov 21
Nov 15-Nov 25
Nov 28-Dec 09
Dec 01-Dec 15
Dec 07-Dec 17
Dec 17-Dec 26
21-Apr
23-Apr
5-May
27-Jun
13-Jul
27-Jul
12-Aug
31-Aug
8-Oct
21-Oct
17-Nov
21-Nov
6-Dec
7-Dec
13-Dec
22-Dec
Var.
60
Var.
Var.
20
120-160
10
Var*.
20
100*
Var.
Var.
10
120
10
alpha-Aurigids
Draconids
Orionids
Leonids
alpha-Monocerotids
Phoenicids
Puppid-Velids
Geminids
Ursids
* These meteor showers have the potential of becoming meteor storms with displays of thousands of meteors per hour.
Solar Eclipses in North America plus Total Eclipses Around the World
Date
Eclipse Type
Annular
Total
Duration Location
2001 Dec 14
2001 Jun 21
2002 Dec 04
2002 Jun 10
2003 May 31
2003 Nov 23
2005 Apr 08
2006 Mar 29
2008 Aug 01
2009 Jul 22
2010 Jul 11
2012 May 20
2012 Nov 13
2013 May 10
2014 Oct 23
2015 Mar 20
2016 Mar 09
2017 Aug 21
2019 Jul 02
2020 Dec 14
03m53s
04m57s
02m04s
00m23s
03m37s
01m57s
00m42s
04m07s
02m27s
06m39s
05m20s
05m46s
04m02s
06m03s
-
North America, Hawaii
South Africa, Madagascar
S. Africa, Indonesia, Australia
West, Midwest, Hawaii, Alaska
Alaska
Australia, New Zealand, S. America
Florida, Southwest
Africa, Europe, Asia
Europe, Asia
Total
Annular
Annular
Total
Partial
Total
Total
Total
Total
Annular
Total
Annular
Partial
Total
Partial
Total
Asia, Hawaii
South America
West, Hawaii, Alaska
Australia, S. America
Australia, N.Z.
West, Midwest, Alaska
Europe, N. Africa, Asia
Hawaii, Alaska
02m47s
04m09s
02m40s
04m33s
02m10s
Across the U.S.!
S. America
S. America
Total
Total
66
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CELESTRON TWO YEAR WARRANTY
A. Celestron warrants this telescope to be free from defects in materials and workmanship for two years. Celestron will repair or
replace such product or part thereof which, upon inspection by Celestron, is found to be defective in materials or workmanship.
As a condition to the obligation of Celestron to repair or replace such product, the product must be returned to Celestron
together with proof-of-purchase satisfactory to Celestron.
B. The Proper Return Authorization Number must be obtained from Celestron in advance of return. Call Celestron at (310) 328-
9560 to receive the number to be displayed on the outside of your shipping container.
All returns must be accompanied by a written statement setting forth the name, address, and daytime telephone number of the
owner, together with a brief description of any claimed defects. Parts or product for which replacement is made shall become
the property of Celestron.
The customer shall be responsible for all costs of transportation and insurance, both to and from the factory of
Celestron, and shall be required to prepay such costs.
Celestron shall use reasonable efforts to repair or replace any telescope covered by this warranty within thirty days of receipt. In
the event repair or replacement shall require more than thirty days, Celestron shall notify the customer accordingly. Celestron
reserves the right to replace any product which has been discontinued from its product line with a new product of comparable
value and function.
This warranty shall be void and of no force of effect in the event a covered product has been modified in design or
function, or subjected to abuse, misuse, mishandling or unauthorized repair. Further, product malfunction or
deterioration due to normal wear is not covered by this warranty.
CELESTRON DISCLAIMS ANY WARRANTIES, EXPRESS OR IMPLIED, WHETHER OF MERCHANTABILITY OF
FITNESS FOR A PARTICULAR USE, EXCEPT AS EXPRESSLY SET FORTH HEREIN.
THE SOLE OBLIGATION OF CELESTRON UNDER THIS LIMITED WARRANTY SHALL BE TO REPAIR OR
REPLACE THE COVERED PRODUCT, IN ACCORDANCE WITH THE TERMS SET FORTH HEREIN. CELESTRON
EXPRESSLY DISCLAIMS ANY LOST PROFITS, GENERAL, SPECIAL, INDIRECT OR CONSEQUENTIAL DAMAGES
WHICH MAY RESULT FROM BREACH OF ANY WARRANTY, OR ARISING OUT OF THE USE OR INABILITY TO
USE ANY CELESTRON PRODUCT. ANY WARRANTIES WHICH ARE IMPLIED AND WHICH CANNOT BE
DISCLAIMED SHALL BE LIMITED IN DURATION TO A TERM OF TWO YEARS FROM THE DATE OF ORIGINAL
RETAIL PURCHASE.
Some states do not allow the exclusion or limitation of incidental or consequential damages or limitation on how long an implied
warranty lasts, so the above limitations and exclusions may not apply to you.
This warranty gives you specific legal rights, and you may also have other rights which vary from state to state.
Celestron reserves the right to modify or discontinue, without prior notice to you, any model or style telescope.
If warranty problems arise, or if you need assistance in using your telescope contact:
Celestron
Customer Service Department
2835 Columbia Street
Torrance, CA 90503
Tel. (310) 328-9560
Fax. (310) 212-5835
Monday-Friday 8AM-4PM PST
This warranty supersedes all other product warranties.
NOTE: This warranty is valid to U.S.A. and Canadian customers who have purchased this product from an Authorized
Celestron Dealer in the U.S.A. or Canada. Warranty outside the U.S.A. and Canada is valid only to customers who purchased
from a Celestron Distributor or Authorized Celestron Dealer in the specific country and please contact them for any
warranty service.
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Celestron
2835 Columbia Street
Torrance, CA 90503
Tel. (310) 328-9560
Fax. (310) 212-5835
Copyright 2005 Celestron
All rights reserved.
(Products or instructions may change
without notice or obligation.)
Item # 11073-INST
$10.00
04-05
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