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Manual de usuario Celestron, modelo C8-S

Fabricar: Celestron
Tamaño del archivo: 4.03 mb
Nombre del archivo:
Idioma del manual:en
Fotos y especificaciones  Celestron  C8-S
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Resumen del manual


22 = 6 = 64x = 7 = .5. / sec = 8 = 2. / sec = 9 = 3. / sec = Nine available slew speeds = 6 = 64x = 7 = .5. / sec = 8 = 2. / sec = 9 = 3. / sec = Nine available slew speeds S SSe eet ttu uup pp P PPr rro ooc cce eed ddu uur rre ees ss The Advanced GT 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 telescope has three different tracking modes: EQ North Used to track the sky when the telescope is polar aligned in the Northern Hemisphere. EQ South Used to track the sky when the telescope is polar aligned in the Southern Hemisphere. Off 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, your telescope 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. Lunar Used for tracking the moon when observing the lunar landscape. Solar Used for tracking the Sun when solar observing with the proper filter. View Time-Site -Displays the current time and longitude/latitude downloaded from the optional CN-16 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 or not present, the hand control will only display the last saved time and location. User Defined Objects -Your telescope 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: 23 Helpful Hint Helpful Hint 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 telescope will automatically retrieve and display the coordinates before slewing to the object. Save Sky Object: Your telescope 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. 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. Save Land Object: The telescope 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. To replace the contents of any of the user defined objects, simply save a new object using one of the existing identification numbers; the telescope 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. To store a set of coordinates (R.A./Dec) permanently into the database, save it as a User Defined Object as described above. Identify Identify Mode will search any of the telescope's database catalogs or lists and dis...

Otros modelos de este manual:
Instrumentos de óptica - C5-S (4.03 mb)
Instrumentos de óptica - C9.25-S (4.03 mb)

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