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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:

Sidereal 

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 . 

Lunar 

Used for tracking the Moon when observing the  

 

lunar landscape .

Solar 

Used for tracking the Sun when solar observing .

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.

  Enter R.A. - Dec – 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.

  GoTo Object – To go to any of the user defined objects stored in the 

database, scroll down to either GoTo Sky Obj or GoTo Land Obj and 
enter the number of the object you wish to select and press ENTER. 
The 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. The 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 . 

2 . Choose Database to select the object that you want to observe from 

any of the database catalogs listed   

3 . Choose RA/DEC to enter a set of celestial coordinates that you wish 

to slew to .

4.  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 .

5 .  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 .

Summary of Contents for 11007

Page 1: ...InstructionManual 11007 11008 11009...

Page 2: ...www celestron com...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

Page 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...

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

Page 41: ...www celestron com 39...

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

Page 43: ...www celestron com 41...

Page 44: ...42 www celestron com...

Page 45: ...www celestron com 43...

Page 46: ...44 www celestron com...

Page 47: ...www celestron com 45...

Page 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...

Page 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...

Page 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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