INTRODUCTION... 4 ... 4 ARNING ASSEMBLY... 6 ... 6 SSEMBLING THE Powering the NexStar... 6 The Hand Control... 6 The Eyepiece... 7 The Star Pointer Finderscope ... 7 HAND CONTROL... 10 ... 11 ONTROL PERATION Alignment Procedure... 11 Sky Align... 12 Auto Two-Star Align...
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Get Axis Position ...24 Goto Axis Postion ...24 Hibernate ...24 Sun Menu ...24 Scrolling Menu ...24 Calibrate Goto...24 Set Mount Position...25 Hand Control Command Tree ... 26 TELESCOPE BASICS ... 26 ... 27 MAGE RIENTATION ... 28 OCUSING ... 28 ALCULATING AGNIFICATION ...
Congratulations on your purchase of the Celestron NexStar! The NexStar ushers in a whole new generation of computer automated technology. Simple and friendly to use, the NexStar is up and running after locating just three bright objects. It’s the perfect combination of power and portability.
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NexStar 4 SE Optical Tube Star Pointer Finderscope Eyepiece Focuser Knob Threaded Photographic Adapter Flip Mirror Control Battery Compartment Tripod Accessory Tray / Leg Brace ON/OFF Switch Hand Control Liquid Crystal Display...
Computerized Hand Control with nearly 40,000 Object Database Start by removing the telescope from its shipping carton and setting the round base on a flat table or surface. It is best to carry the telescope by holding it from the lower portion of the fork arm and from the bottom of the base. Remove all of the accessories from their individual boxes.
The Star Pointer Finderscope The Star Pointer is the quickest and easiest way to point your telescope exactly at a desired object in the sky. It's like having a laser pointer that you can shine directly onto the night sky. The Star Pointer is a zero magnification pointing tool that uses a coated glass window to superimpose the image of a small red dot onto the night sky.
The star pointer is powered by a long life 3-volt lithium battery (#CR2032) located underneath the front portion of the Star Pointer. Like all finderscopes, the Star Pointer must be properly aligned with the main telescope before it can be used. This is a simple process using the azimuth and altitude control knobs located on the side and bottom of the Star Pointer.
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Tighten the locking lever to hold the tilt plate securely in place. Set the base of the telescope on the wedge tilt plate so that the hole in the center of the base goes over the positioning pin on top of the tilt plate.
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. Align: Instructs the NexStar to use a selected star or object as an alignment position.
This section describes the basic hand control procedures needed to operate the NexStar. 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 and tracking rate;...
You may even select a planet or the moon. The NexStar is then ready to start finding and tracking any of the objects in its 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 with Sky Align, Auto Two-Star Align requires you to enter all the necessary time/site information as before. entered, NexStar will prompt you to select and point the telescope at one known star in the sky. The NexStar now has all the information it needs to automatically choose a second star that will assure the best possible alignment.
Once in position, the NexStar will model the sky based on this information and display Align Successful. ote: 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.
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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: •...
The telescope 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. Then, center the object in the eyepiece and press ALIGN.
Your telescope’s pointing accuracy will now be improved in that area of the sky. NOTE: Sync can improve your telescope’s pointing accuracy over a wide area or over smaller areas of the sky depending on the quality of the initial alignment, as well as where the telescope was pointing when the Sync was done.
Constellation Tour In addition to the Tour Mode, the NexStar 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).
The NexStar has four direction buttons in the center of the hand control which control the telescope motion in altitude (up and down) and azimuth (left and right). The telescope can be controlled at nine different speed rates. 1 = .5x...
The camera feature comes with an easy to use Camera Wizard that allows you to save a list of as many as nine targets. Then with a DSLR attached or piggyback mounted to your telescope, NexStar will automatically slew to the specified targets and take an exposure of each one.
The Camera Wizard is the quickest way to build an imaging sequence of targets and exposure times. The Wizard will ask you to point the telescope/camera to up to 9 objects. After the user selects 9 objects or presses UNDO it asks you whether the sequence should repeat forever (perhaps for security monitoring) or whether it should stop when it gets to the end.
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.
Slew Limits – Sets the limits in altitude that the telescope can slew without displaying a warning message. The slew limits prevent the telescope tube from slewing to an object below the horizon. The slew limits can be customized depending on your needs. For example, if you would like to slew to an object that is close to the zenith but you have a camera attached that prevents it from pointing straight up, you can set the maximum altitude to 80 or 85 degrees to prevent the tube from ever pointing straight up.
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.
Set Mount Position from the Utilities menu. Since the telescope has been moved, the pointing accuracy will be diminished. But now you can slew to a new set of alignment stars and replace any of...
MENU ALIGNMENT TRACKING MODE ALT-AZ EQ NORTH EQ SOUTH RATE SIDEREAL SOLAR LUNAR VIEW TIME-SITE SCOPE SETUP SETUP TIME-SITE ANTI-BACKLASH SLEW LIMITS FILTER LIMITS DIRECTION BUTTONS GOTO APPROACH CORDWRAP UTILITIES LIGHT CONTROL FACTORY SETTING VERSION GET AXIS POSITION GOTO AXIS POSITION HIBERNATE SUN MENU SCROLLING TEXT...
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 Maksutov-Cassegrain optical system uses a combination of mirrors and lenses and is referred to as a compound or catadioptric telescope.
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: Magnification = Let’s say, for example, you are using the 25mm eyepiece.
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.
Up to this point, this manual covered the assembly and basic operation of your NexStar 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 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.
After performing either an EQ AutoAlign or Two-Star Alignment, Wedge Align will slew the telescope to where Polaris should be. By adjusting the tripod’s tilt plate to center Polaris in the eyepiece, the fork arm (polar axis) will then be pointing towards the actual North Celestial Pole.
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.
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.
This can damage the telescope and/or any accessories attached to the telescope. For safe solar viewing, use a Celestron solar filter (see Optional Accessories section of manual) 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.
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. •...
This will prevent contaminants from entering the optical tube. Internal adjustments and cleaning should be done only by the Celestron service department. If your telescope is in need of internal cleaning,...
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Celestron offers the Car Battery Adapter that allows you to run the NexStar drive off an external Diagonal, 45 degree, erect image (#94116) – Threads on to the back of the NexStar 4. This design allows you to look into the telescope at a 45°...
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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.
Near Focus standard eyepiece or camera Field of View: Standard Eyepiece : 35mm Camera Linear Field of View (at 1000 yds) Magnification: Standard Eyepiece : Camera Optical Tube Length Weight of Telescope Weight of Tripod Input Voltage Batteries Required Power Supply Requirements Motor: Type Resolution...
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.
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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.
RS-232 cable . For information about using NexRemote to control your telescope, refer to the help files located on the disk. In addition to NexRemote, the telescope can be controlled using other popular astronomy software programs.
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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.
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Celestron 2835 Columbia Street Torrance, CA 90503 Tel. (310) 328-9560 Fax. (310) 212-5835 Web site at http//www.celestron.com Copyright 2006 Celestron All rights reserved. (Products or instructions may change without notice or obligation.) This device complies with Part 15 of the FCC Rule. Operation is subject to the...