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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 
feature 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 .
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 .
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 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°.

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.

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.     

Direction Buttons – The direction a star moves in the eyepiece varies 
depending on the accessories being used . This can create confusion when 

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Страница 1: ...InstructionManual 11007 11008 11009...

Страница 2: ...www celestron com...

Страница 3: ...20 22 CELESTIAL OBSERVING 23 24 CELESTIAL PHOTOGRAPHY 25 29 TELESCOPE MAINTENANCE 30 31 OPTIONAL ACCESSORIES 31 32 APPENDIX A TECHNICAL SPECIFICATIONS 33 34 APPENDIX B GLOSSARY OF TERMS 34 36 APPENDI...

Страница 4: ...other high performance features TheCPC DeluxeHD s features combined withCelestron s legendary optical systems give amateur astronomers the most sophisticated and easy to use telescopes available on th...

Страница 5: ...onal 9 Schmidt Corrector Lens 14 Accessory Tray Center 4 Hand Control 10 Altitude Locking Knobs Support Bracket 5 Eyepiece 11 Carrying Handle 15 Focus Knob 6 Finderscope A Hand Control Port C PC Inter...

Страница 6: ...tached 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 s...

Страница 7: ...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 t...

Страница 8: ...erscope 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 mou...

Страница 9: ...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 dir...

Страница 10: ...unique list of some of the most recognizable star patterns in the sky CCDObjects A custom list of many interesting galaxy pairs trios and clusters that are well suited forCCD imaging with theCPC tele...

Страница 11: ...rmation downloaded from theGPS 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 co...

Страница 12: ...der 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 pressALIGN to accept this star as your second alignment star When t...

Страница 13: ...e EQ alignments gives you the choice of performing anAutoAlign Two Star alignment One Star alignment or Solar System alignment EQAutoAlign The EQAutoAlign uses all the same time site information as th...

Страница 14: ...amed Stars NamedObject Double Stars Variable Stars Asterisms andCCDObjects Selecting any one of these catalogs will display a numeric alphabetical listing of the objects under that list Pressing theUP...

Страница 15: ...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 th...

Страница 16: ...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 obje...

Страница 17: ...tions 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 C...

Страница 18: ...acklash compensation values initial date and time longitude latitude along with slew and filter limits will be reset The hand control will ask you to press the 0 key before returning to the factory de...

Страница 19: ...ection 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 astrophotogra...

Страница 20: ...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 a...

Страница 21: ...e apparent field of the eyepiece supplied by the eyepiece manufacturer by the magnification In equation format the formula looks like this As you can see before determining the field of view you must...

Страница 22: ...oving toward the west Motionof theStars 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 t...

Страница 23: ...y bright star in the telescope s database select the AlignWedge option The telescope will then re slew to the same star 1 Center the star in the finderscope and press ENTER 2 Then accurately center th...

Страница 24: ...one 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...

Страница 25: ...te power PlanetaryObserving 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...

Страница 26: ...ance 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 pollute...

Страница 27: ...models are available ShortExposurePrimeFocusPhotography Short exposure prime focus photography is the best way to begin recording celestial objects It is done with the camera attached to the telescope...

Страница 28: ...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 commen...

Страница 29: ...s 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 pos...

Страница 30: ...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 candi...

Страница 31: ...view 5 times larger and the object size 1 5 compared to that of f 10 see Figure 8 8 FIGURE 8 8 Telescope Standard f 10 f 2 Model Configuration Configuration 8 80 2032 mm 16 406 4 mm 9 25 93 2350 mm 1...

Страница 32: ...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 second...

Страница 33: ...direction than simply repeat steps 2 through 6 as described above for the new direction FIGURE 9 3 A collimatedtelescope should appear symmetrical withthe central obstruction centered inthe star s di...

Страница 34: ...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 pris...

Страница 35: ...122x Resolution Rayleigh Criterion 68 arc seconds 59 arc seconds 50 arc seconds Dawes Limit 57 arc seconds 49 arc seconds 42 arc seconds Light Gathering Power 843x 1127x 1593x Near Focus with Standard...

Страница 36: ...tude star or other celestial object as perceived by an observer on Earth Arc minute A unit of angular size equal to 1 60 of a degree Arc second A unit of angular size equal to 1 3 600 of a degree or 1...

Страница 37: ...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 celes...

Страница 38: ...anet U Universe The totality of astronomical things events relations and energies capable of being described objectively V VariableStar A star whose brightness varies over time due to either inherent...

Страница 39: ...a Dec R34AB 12CE Scope must be aligned If command conflicts with slew limits there will be no action Get Azm Alt Z 12AB 4000 10 characters returned 12AB Azm comma 4000 Alt Get RA Dec E 34AB 12CE Scope...

Страница 40: ...38 www celestron com APPENDIXD MAPSOFTIMEZONES...

Страница 41: ...www celestron com 39...

Страница 42: ...40 www celestron com APPENDIXE SKYMAPS...

Страница 43: ...www celestron com 41...

Страница 44: ...42 www celestron com...

Страница 45: ...www celestron com 43...

Страница 46: ...44 www celestron com...

Страница 47: ...www celestron com 45...

Страница 48: ...EclipseType Duration Location 2001 Dec 14 Annular 03m53s North America Hawaii 2001 Jun 21 Total 04m57s South Africa Madagascar 2002 Dec 04 Total 02m04s S Africa Indonesia Australia 2002 Jun 10 Annula...

Страница 49: ...cted to abuse misuse mishandling or unauthorized repair Further product malfunction or deterioration due to normal wear is not covered by this warranty CELESTRON DISCLAIMSANYWARRANTIES EXPRESSOR IMPLI...

Страница 50: ...ars of age and older 2835 Columbia Street Torrance CA 90503 U S A Telephone 310 328 9560 Fax 310 212 5835 FCC Statement This device complies with Part 15 of FCC Rules Operation is subject to the follo...

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