Celestron Advanced Series C5-S, C8-S, C9.25-S, Advanced GT, OMNI Plossl 4mm, 6mm, 9mm, 12.5mm, 5mm, 20mm, 25mm, 32mm and 40mm, X-Cel 2.3mm, 5mm, 8mm, 10mm, 12.5mm, 8mm, 21mm, 25mm, Ultima 5mm, 7.5mm, 10mm, 12.5mm, 18mm, 30mm, 35mm, and 42mm User guide
Below you will find brief information for telescope Advanced Series C5-S, telescope Advanced Series C8-S, telescope Advanced Series C9.25-S, telescope Advanced GT, eyepieces OMNI Plossl 4mm, 6mm, 9mm, 12.5mm, 5mm, 20mm, 25mm, 32mm and 40mm, eyepieces X-Cel 2.3mm, 5mm, 8mm, 10mm, 12.5mm, 8mm, 21mm, 25mm, eyepieces Ultima 5mm, 7.5mm, 10mm, 12.5mm, 18mm, 30mm, 35mm, and 42mm, eyepieces Axiom. This document describes proper care and maintenance for your Celestron telescope and its accessories.
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While your 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 1s 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 ie optical performance of your telescope is directly related to its collimation, that is the alignment of its optical system. Your telescope was collimated at the factory after it was compietely assembled. However, 1f 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. 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. | Fig ure 81 - CL | . ; . The three | pe screws are > lncated. | To verify collimation, view a star near the zenith. Use a medium to high power ocular on the front of the secondary mirror — 12mm to 6mm focal length. It is important to center a star in the center of the field to “housing: = 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. 47 Figure 8-2 -- Even though the star pattern appears the same on both sides of focus, they are asymmetric. 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 in the secondary mirror holder (see figure 8-1). 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: L. 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 8-2). Center the de-focused star and notice in which direction the central shadow 1s 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). | 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). (sa 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 18 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 1s skewed in Figure 8-3 a different direction, than simply repeat steps 2 through 6 as described above for the new A collimated telescope direction | | should appear о symmetrical with the . o I | central obstruction Perfect collimation will yield a star image very symmetrical just inside and outside of focus. In centered in the star's addition, perfect collimation delivers the optimal optical performance specifications that your p p p p Р diffraction pattern. telescope is built to achieve. 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. 48 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. Adapter AC (#18773) - Allow DC (battery powered) telescopes to be converted for use with 120 volt AC power. Auxiliary Port Accessory (#93965) — This accessory plugs into the auxiliary port of the telescopes control panel to provide additional ports for accessories like the CN-16 GPS as well as a PC programming port. 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. 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. The OMNI Barlow (#93326) 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. e OMNI Plgssl - Plossl eyepieces have a 4-element lens designed for low-to-high power observing. The Plôssis 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: 4mm, 6mm, 9mm, [2.5mm, 5mm, 20mm, 25mm, 32mm and 40mm. e X-Cel - This 6 element design allows each X-Cel Eyepiece to have 20mm of eye relief, 55° field of view and more than 25mm of lens aperture (even with the 2.3mm). In order to maintain razor sharp, color corrected images across its 55° field of view, extra-low dispersion glass is used for the most highly curved optical elements. The excellent refractive properties of these high grade optical elements, make the X-Cel line especially well suited for high magnification planetary viewing where sharp, color-free views are most appreciated. X-Cel eyepiece come in the following focal lengths: 2.3mm, 5mm, 8mm, 10mm, 12.5mm, 8mm, 21mm, 25mm. е Ultima - Ultima is our 5-element, wide 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 70° extra wide field of view (except the 50mm). All are fully multicoated and contain all the features of the Ultimas. Filters Sets, Eyepiece - Celestron offers four convenient filter sets, which contain four different filters per set. Not only are these highly useful filter combinations, but they also offer an economical way to add versatility to your filter collection. Series 1 —#94119-10 Orange, Light Blue, ND13%T, Polarizing (#s 21, 80A, #15, Polarizing) 49 Series 2 — #94119-20 Deep Yellow, Red, Light Green, ND25% T (#s 12, 25, 56, 96ND-25) Series 3 — #941 19-30 Light Red, Blue, Green, ND50% T (#s 23A, 38A, 58, 96ND-50) Series 4 — #94119-40 Yellow, Deep Yellow, Violet, Pale Blue (#s 8, 47, 82A, ND96-13) 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). CN16 GPS Accessory (#93963) - Plug in this 16-channel GPS module into your telescopes drive base port to link up and automatically download information from one of many global positioning satellites. Controlled with the computerized hand control, the CN-16 will greatly improve the accuracy of your star alignments. CN16 GPS Bracket {#93964) — Support your CN-16 GPS accessory with this bracket and strap combination that securely wraps around any of the tripod legs and holds the GPS module in place . Light Pollution Reduction (LPR) Filters - These filters arc 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 hght, 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 (#94126A) and a model that attaches to the rear cell ahead of the star diagonal and visual back (#94127A). Micro Guide Evepiece (#94171) - This multipurpose 2.5mm 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 163 power with the C8-S and 188 power with the C9.25-S. Moon Filter (#94119-A) - Celesiron’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%. Motor Drive, Single Axis (#93518) — This motor drive is a single axis (R.A.), DC motor drive. It is powered by four D- cell batteries (not included). 2x and 4x sidereal speeds are available through the included hand controller. For non- computerized Advanced Series Mounts. Motor Drive, Dual Axis (#93523) - This dual axis motor drive, with drive corrector capabilities, are designed for Celestron's Advanced CG-5 mounts. They precisely control the telescope's tracking speed during long, timed exposures of celestial objects, producing the best possible image sharpness. Four speeds are available—1x (sidereal), 2x for guiding, 4x, and 8x for centering. These precision, state-of-the-art DC motor drives operate from 4 D-cell batteries (not included). The hand controller module is very compact and fits easily in the palm of your hand. Motors for both axes are included, along with brackets, clutches and hardware. For non-computerized Advanced Series Mounts. 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. Polar Axis Finderscope (#94220) — This useful accessory speeds accurate polar alignment by providing a means of visually aligning your German equatorial mount with Polaris and true north. As a result, you can spend more time observing and less time setting up. The finderscope has an easy to use cross hair reticle. PowerTank (#18774) — 12v 7Amp hour rechargeable power supply. Comes with two 12v output cigarette outlets, built-in red flash light , Halogen emergency spotlight. Switchable 110v/220v AC adapter and cigarette lighter adapter included. 50 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 C8-S a 1280mm {/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 1s 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. RS-232 Cable (#93920) — Allows your Advanced Series telescope to be controlled using a laptop computer or PC. Once connected, the telescope can be controlled using popular astronomy software programs. 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 1s used on the Celestron 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 1s minimal. Solar Filter - The Baader 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 the C5-S (#94139) and C8-S (494162). T-Adapter (#93633-A) - T-Adapter (with additional T-Ring) allows you to attach your SLR camera to the rear cell of your Celestron telescope. This turns your telescope 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 1s 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. A full description of all Celestron accessories can be found in the Celestron Accessory Catalog (#93685) 51 Appendix A — Technical Specifications Advanced Series 11071/11072 11025/11026 11045/11046 C5-S C8-S C9.25-S Specifications: Optical Design 127mm(5") Schmidt-Cassegrain 203mm (8") Schmidt-Cassegrain 235mm (9.25") Schmidt-Cassegrain Focal Length [250mm F/10 2032mm E/10 2350mm F/10 Finderscope 6x30 6x30 6x30 Mount CG-5 Equatorial CG-5 Equatorial CG-5 Equatorial Eyepiece 25mm Plossl (50x) 25mm Plossl (81x) 25mm Plossl (94x) Star Diagonal 1,25" 1.25" 1.25" Accessory tray Yes Yes Yes Tripod 2" Stainless Steel 2" Stainless Steel 2" Stainless Steel Technical Specs Highest Useful Magnication 300x 480x 555x Lowest Useful Magnification 18x 29x 34x Limiting Stellar Magnitude 13 14 14.4 Resolution: Rayleigh I. larc seconds .68 arc seconds .59 arc seconds Dawes Limit 91 arc seconds 37 arc seconds 49 arc seconds Photographic Resolution 200 line/mm 200 line/mm 200 tine/mm Light Gathering Power 329x unaided eye 843x unaided eye [127% unaided eye Field of View: standard eyepiece 19 ‚64° 55° Linear FOV (@1000 yds) 52.5 ft. 33.6 ft. 29 ft. Optical Coatings - Standard Starbright Coating Starbright Coating Starbright Coating Secondary Mirror Obstruction 1.75" 2.7" 3.35" by Area 12% 11% 13% by Diameter 35% 34% 36% Optical tube length 14 inches 17 inches 22 inches Telescope Weight 48 155 54.5 165 73 lbs Advanced GT Additional Specifications Hand Control Double line, 16 character Liquid Crystal Display; 19 fiber optic backlit LED buttons Motor: Type DC Servo motors with encoders, both axes Max Slew Speed 3°/second Software Precision 24bit, 0.08 arcsec calculation Hand Control Ports RS-232 communication port on hand control Motor Ports Aux Port, Autoguide Ports Tracking Rates Sidereal, Solar and Lunar Tracking Modes EQ North & EQ South Alignment Procedures AutoAlign, 3-Star Alignment, Quick Align, Last Align 40,000+ objects, 400 user defined programmable objects, Database Enhanced information on over 200 objects Complete Revised NGC Catalog 7,840 Complete Messier Catalog 110 Complete IC Catalog 5,386 Complete Caldwell 109 Abell Galaxies 2,712 Solar System objects 9 Famous Asterisms 20 Selected CCD Imaging Objects 25 Selected SAO Stars 29,500 Total Object Database 45,492 52 Appendix B - Glossary of Terms А- Absolute magnitude Airy disk Alt-Azimuth Mounting Altitude Aperture Apparent Magnitude Arcminute Arcsecond Asterism Asteroid Astrology Astronomical unit (AU) Aurora Azimuth В - Binary Stars С - Celestial Equator Celestial pole Celestial Sphere Collimation D - Declination (DEC) Е - Ecliptic Equatorial mount Е - Focal length 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. A telescope mounting using two independent rotation axis allowing movement of the instrument in Altitude and Azimuth. In astronomy, the altitude of a celestial object is its Angular Distance above or below the celestial horizon. the diameter of a telescope's primary lens or mirror; the larger the aperture, the greater the telescope's light-gathering power. A measure of the relative brightness of a star or other celestial object as perceived by an observer on Earth. 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. The pseudoscientific belief that the positions of stars and planets exert an influence on human affairs; astrology has nothing in common with astronomy. 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. 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. . 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. The projection of the Earth's equator on to the celestial sphere. It divides the sky into two equal hemispheres. 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. 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. 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". 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. The distance between a lens (or mirror) and the point at which the image of an object at infinity 18 brought to focus. The focal length divided by the aperture of the mirror or lens 1s termed the focal ratio. | 53 J - Jovian Planets K - Kuiper Belt L - Light-Year (LY) M - Magnitude Meridian Messier N - Nebula North Celestial Pole Nova O - Open Cluster P- Parallax Parfocal Parsec Point Source В - Reflector Resolution Right Ascension: (RA) S - Schmidt Telescope Sidereal Rate Any of the four gas giant planets that are at a greater distance form the sun than the terrestrial planets. A region beyond the orbit of Neptune extending to about 1000 AU which is a source of many short period comets. 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). 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 | 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, 1s -26.78. The zero point of the apparent magnitude scale is arbitrary. 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. Interstellar cloud of gas and dust. Also refers to any celestial object that has a cloudy appearance. The point in the Northern hemisphere around which all the stars appear to rotate. This 1s 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. 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. 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 1f 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. 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.) 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. 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. 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). This is the angular speed at which the Earth is rotating. Telescope tracking motors drive the 54 T - Terminator U- Universe V- Variable Star W - Waning Moon Waxing Moon 7 - Zenith Zodiac 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. The totality of astronomical things, events, relations and energies capable of being described objectively. 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. The period of the moon's cycle between full and new, when its illuminated portion 1s decreasing. The period of the moon's cycle between new and full, when its illuminated portion 1s increasing. 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. 55 APPENDIX C LONGITUDES AND LATITUDES ALABAMA Anniston Auburn Birmingham Centreville Dothan Fort Rucker Gadsden Huntsville Maxwell AFB Mobile Mobile Aeros Montgomery Muscle Shoal Selma Troy Tuscaloosa ALASKA Anchorage Barrow Fairbanks Haines Hrbor Homer Juneau Ketchikan Kodiak Nome Sitka Sitkinak Skagway Valdez “ARIZOI Davis-M AFB Deer Valley Douglas Falcon Fid Flagstaff Fort Huachuc Gita Bend Goodyear GrandCanyon Kingman Luke Page Payson Phoenix Prescott Safford Awrs Scotisdale Show Low Tucson Williams AFB Winslow Yuma Yuma Mcas Yur Blytheville Camden El Dorado Fayetteville Fi Smith Harrison Hot Springs Jonesboro Litile Rock Pine Bluff Springdale Texarkana Walnut Ridge d CA Alturas Arcata Bakersfield Beale AFB Beaumont Bicycle Lk Big Bear Bishop Blue Canyon - degrees LONGITUDE 85 85 86 87 85 85 86 86 86 88 88 86 87 86 86 156 147 135 151 134 131 152 165 135 154 135 110 112 109 111 111 110 113 112 112 113 112 111 111 112 112 109 111 110 110 111 110 115 114 114 89 92 92 94 94 93 93 90 92 91 94 94 90 122 120 124 119 121 116 116 116 118 120 26.4 45 15 27 43.2 5.4 46.2 22.2 15 4.2 2.4 37.2 59.4 19.2 31.8 0.6 27 57 37.2 40.8 3.6 4.2 LATITUDE min - degrees 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 Blythe Burbank Campo Carlsbad Castle AFB Chico China Lake Chino Concord Crescent Cty Daggett Edwards AFB El Centro El Monte El Toro Eureka Fort Hunter ’ Fort Ord Fresno Fullerton George AFB Hawthorne Hayward Imperial imperial Bch La Verne Lake Tahoe Lancaster Livermore Long Beach Los Alamitos Los Angeles Mammoth March AFB Marysville Mather AFB Mcclellan Merced Miramar NAS Modesto Moffet Mojave Montague Monterey Mount Shasta Mount Wilson Napa Needies North ls Norton AFB Oakland Ontario Int! 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 Clemente San Diego San Francisco San Jose San Luis Obi San Mateo San Miguel Sandburg Santa Ana Santa Barb Santa Maria Santa Monica Santa Rosa 56 LONGITUDE LATITUDE degrees min degrees 114 43.2 33 118 22.2 34 116 28.2 32 117 16.8 33 120 34.2 37 121 51 39 117 40.8 35 117 37.8 33 122 3 37 124 13.8 41 116 46.8 34 117 52.8 34 115 40.8 32 118 1.8 34 117 43.8 33 124 16.8 41 121 19.2 36 121 46.2 36 119 43.2 36 117 58.2 33 117 22.8 34 118 19.8 33 122 7.2 37 115 34.2 32 117 7.2 32 117 46.8 34 120 0 38 118 13.2 34 121 49.2 37 118 9 33 118 3 33 118 24 33 118 55.2 37 117 16.2 33 121 34.2 39 121 1.8 38 121 2.4 38 120 31.2 37 117 9 32 120 57 37 122 3 37 118 9 35 122 31.8 41 121 51 36 122 19.2 41 118 4.2 34 122 16.8 38 114 37.2 34 117 1.2 32 117 13.8 34 122 13.2 37 117 37.2 34 119 1.2 34 116 3 33 118 7.8 35 122 7.2 37 120 37.8 35 122 49.8 37 119 7.2 34 124 13.2 39 121 7.2 34 121 16.8 35 122 15 40 122 1.8 40 117 27 33 121 3 38 121 3.6 36 122 15 37 117 37.2 33 117 7.8 32 122 22.8 37 121 55.2 37 120 39 35 117 34.8 33 120 2.4 34 118 43.8 34 117 52.8 33 119 49.8 34 120 27 34 118 27 34 122 49.2 38 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 40.8 46.2 52.2 34.8 55.2 39 49.8 34.2 54 43.8 42 49.2 46.8 55.8 37.8 52.8 34.2 40.2 16.8 52.2 37.8 25.2 43.8 34.8 19.2 13.8 13.2 46.2 42 43.8 12 49.8 28.2 40.2 49.8 7.2 34.8 57 40.2 30 57 31.2 40.2 31.2 25.2 49.2 37.2 22.2 13.8 22.8 1.8 45 40.2 25.8 54 1.2 31.2 LONGITUDE LATITUDE degrees min degrees min Shelter Cove 124 4.2 40 1.8 Siskiyou 122 28.2 41 46.8 Stockton 121 1b 37 54 Superior Val 117 0.6 35 19.8 Susanville 120 57 40 37.8 Thermal 116 10.2 33 37.8 Torrance 118 19.8 33 48 Travis AFB 121 55.8 38 16.2 Tahoe 120 7.8 39 19.2 Tustin Mcas 117 49.8 33 42 Ukiah 123 1.2 39 7.8 Van Nuys 118 28.8 34 13.2 Vandenberg 120 57 35 12 Visalia 119 2.4 36 192. Air Force A 105 39 31.2 Akron 103 40 10.2 Alamosa 105 37 27 Aspen 106 39 13.2 Brmfield/Jef 105 39 54 Buckley 104 39 43.2 Colo Sprgs 104 38 49.2 Cortez 108 37 18 Craig-Moffat 107 40 30 Denver . 104 39 45 Durango 107 37 9 Eagle 106 39 39 Englewood 104 39 34.2 Fort Carson 104 38 40.8 Fraser 105 39 34.2 Ft Col/Lovel 105 40 27 Ft Collins 105 40 34.8 Grand Jct 108 39 7.2 Greeley-WId 104 40 25.8 Gunnison 106 38 33 La Junta 103 36 3 Lamar 102 38 7.2 Leadville 106 39 15 Limon 103 39 10.8 Montrose 107 38 30 Pueblo 104 38 16.8 Rifle 107 39 31.8 Salida 106 38 31.8 Trinidad 104 37 15 Winter Park 105 40 0 “CONNECTICUT = Bridgeport Danbury Groton Hartford New Haven New London ‘Windsor Loc DELAWARE Dover Wilmington D ASI Washington E Apalachicola 85 Astor NAS 81 Avon Park G 81 Cape 80 28 28.2 Canaveral Cecil 81 52.8 30 13.2 Crestview 86 31.2 30 46.8 Cross City 83 0.6 29 37.2 Daytona Bch 81 3 29 10.8 Duke Fld 86 31.2 30 39 Eglin AFB 86 31.8 30 28.8 Egmont Key 82 46.2 27 36 Fort Myers 81 52.2 26 34.8 Ft Lauderdale 80 9 26 4.2 Ft Myers 81 52.2 26 39 Gainesville 82 16.2 29 40.8 Homestead 80 22.8 25 28.8 Hurlburt Fid 86 40.8 30 25.8 Jacksonville 81 40.8 30 13.8 Key West 81 45 24 33 Lakeland 81 57 28 1.8 Macdill AFB 82 31.2 27 51 Marianna 85 10.8 30 50.4 Mayport NAS 81 25.2 30 24 LONGITUDE Melbourne Miami Naples Nasa Shuttle Orlando Panama City Patrick AFB Pensacola Ruskin Saint Peters Sanford Sarasota Tallahassee Tampa Intl Titusville Tyndall AFB Vero Beach West Palm Beach ‘Whiting FId Albany Alma Athens Atlanta Augusta/Bush Brunswick Columbus Dobbins AFB Fort Benning Ft Stewart Hunter Aaf La Grange Macon/Lewis Moody AFB Robins AFB Rome/Russell Valdosta _Waycro Barking San Fr Frigate Hito Honolulu Int Kahului Maui Kaneohe Mca Kilauea Pt Lanai-Lanai Lihue-Kauai Maui Molokai Upolo PtLn Waimea- Burley Chailis Coeur d'Alene Eik City Gooding Grangeville Idaho Falls Lewiston Malad City Malta Mccall Mullan Pocatello Salmon Soda Springs Sun Valley Aurora Bistate Park Bloomington Bradford Cairo Carbondale Centralia Champaign Chicago Danville DeKalb Decatur Du Page Galesburg degrees 80 80 81 80 81 85 80 87 82 82 81 82 84 . 82 80 - 85 80 80 87 160 166 155 157 156 158 159 156 159 156 157 156 156 113 114 116 115 115 116 112 117 112 113 116 115 112 113 411 min 37.8 16.8 4.8 40.8 19.2 40.8 3.6 19.2 3.6 40.8 15 33 22.2 31.8 4.8 34.8 25.2 7.2 1.2 10.8 31.2 19.2 25.2 58.2 22.8 55.8 31.2 34.2 4.2 39 1.2 3.6 10.2 16.8 1.8 28.2 4.2 55.8 25.8 16.8 40.2 57 21 49.8 0.6 28.2 7.2 46.2 13.2 49.2 25.8 10.2 7.8 4.2 1.2 18.2 22.2 0.6 4.8 3.6 54 34.8 ... LATITUD ‘degrees 28 25 26 28 28 30 28 30 27 27 28 27 30 27 28 30 27 26 30 21 22 24 19 21 20 21 20 21 20 21 20 20 42 44 47 45 43 45 43 46 42 42 44 47 42 45 42 E min 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 40.8 43.2 Glenview NAS Kankakee Macomb Marion Marseilles Mattoon Moline/Quad Mount Vernon Peoria Quincy Rockford Salem Scott AFB Springfield Sterling Taylorville alia Bloomington Elkhart Evansville Fort Wayne Gary Grissom AFB indianapolis Muncie South Bend Terre Haute W Lafayette 10} Burlington Cedar Rapids Des Moines Dubuque Estherville Fort Dodge Lamoni Mason City Ottumwa Sioux City Spencer Waterloo Mun Chanute Col. J Jabar Concordia Dodge City Eikhart Emporia Ft Leavnwrth Ft Riley Garden City Goodland Hays Hill City Hutchinson Johnson Cnty Liberal Manhatten Mcconnell Af Medicine Ldg Olathe Russell Salina Topeka Topeka/Forbe Wichit Bowling Gren Ft Campbell Ft Knox Jackson Lexington London Louisville Owensboro Paducah Pikeville Alexandria Barksdale Baton Rouge Boothville Cameron Heli Claiborne R England AFB Eugene ls. Fort Polk LONGITUDE degrees 87 87 90 89 88 88 90 88 89 91 89 88 89 89 89 89 86 86 86 87 85 87 86 86 85 86 87 86 91 93 90 94 94 93 93 92 96 95 92 95 97 97 99 101 96 94 96 100 101 99 99 97 94 100 96 97 98 94 98 97 95 95 97 86 87 85 83 85 84 85 87 88 82 92 93 91 89 93 92 92 91 93 57 LATITUDE min degrees 49.2 51 39.6 0 40.8 16.8 31.2 51.6 40.8 1.2 0.6 57.6 51 40.2 40.2 19.8 42 41 40 37 41 39 41 38 40 39 42 38 38 39 41 39 min 4.8 4.2 31.2 45 22.2 28.8 19.2 40.2 46.2 19.8 22.2 55.8 22.2 51 22.8 4.2 49.2 37.2 18 51 52.2 48 4.2 57 39 58.2 40.2 54 36 4.8 13.8 22.8 30 31.8 33 46.8 13.2 19.8 28.2 ter Ann Arbor Battle Creek Benton Harbor 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 Peliston Pontiac Saginaw Sault Ste M Sawyer AFB Selfridge Seul Choix Traverse Cty min 4.2 2.4 39 7.2 0 13.2 0.6 1.2 16.8 55.2 1.8 58.2 3.6 16.6 7.2 37.2 4.2 58.2 10.8 31.2 10.8 55.6 43.2 31.8 52.2 -- LONGITUDE... degrees Grand Isle 90 High Island 94 Houma a0 Intercoastal 92 Lafayette 92 Lake Charles 93 Lk Palourde 91 Missippi Can 89 Monroe 92 Morgan City 91 New Iberia 91 New Orleans 90 S Marsh lsl 91 Shreveport 93 _Slidel _ 89 Augusta Bangor Bar Harbor 68 Brunswick 69 Caribou Mun 68 Greenville 69 Houiton 67 Loring AFB 67 Portland 70 Presque Isle 68 Rockland 69 Rumford (MARYLAN Andrews AF Baltimore Fort Meade Hagerstown Ocean City Patuxent Phillips Salisbury MASSACHUSETT: Bedford 71 Beverly 70 Boston 71 Cape Cod 70 Chatham 69 Fort Devens 71 Hyannis 70 Lawrence 71 Marthas Vine 70 Nantucket 70 New Bedford 70 Norwood 71 Otis ANGB 70 Pittsfield 73 S Weymouth 70 Westfield 72 Westover 72 _Worces 71 13.8 25.8 28.2 57 51 4.8 45 31.2 31.8 40.8 7.2 7.8 28.2 33 15 57 37.8 15 4.8 25.2 4.8 22,2 . 2.4 49.8 55.2 34.8 29 28 29 29 30 30 29 28 32 29 30 29 28 32 44 44 44 43 46 45 46 46 43 46 44 42 42 42 41 41 42 41 42 41 41 41 42 41 42 42 42 42 42 42 42 46 43 47 42 45 42 42 47 43 44 45 46 42 42 42 44 46 45 43 45 42 43 46 46 42 45 44 LATITUDE ‘degrees min 10.8 7.8 34.2 43.8 12 7.2 42 46.8 31.2 42 1.8 58.8 18 31.2 48 27 52.8 52.2 27 7.8 57 39 40.8 4.2 52.8 10.8 4.8 42 33 16.8 28.2 19.8 28.2 34.8 22.2 46.8 40.2 34.2 40.2 43.2 24 15 40.8 10.8 39 15.6 10.2 12 16.2 13.2 18 7.8 15 4.2 28.2 25.2 43.8 58.2 52.8 10.2 49.8 22.2 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 37.2 55.2 43.8 © LONGITUDE ““ degrees Wurtsmith Alexandria Bemidji Muni Brainerd-Crw Detroit Laks Duluth Ely Fairmont Fergus Falls Grand Rapids Hibbing Intl Falls Litchfield Mankato Marshall Arpt Minneapolis Park Rapids Pequot Lake Rochester Saint Paul St Cloud Thief River Tofte Warroad Worthington Columbus AFB Golden Trian Greenville Greenwood Gulfport Hattiesburg Jackson Keesler AFB Laurel Mccomb Meridian NAS Meridian/Key Natchez Oxford Tupel Columbia Cape Girardeau Ft Leonard Jefferson City Joplin Kansas City Kirksville Monett Muskogee Poplar Bluff Richards-Geb Spickard Springfield St Joseph St Louis Vichy/Rolla West Plains Whiteman Bozeman Broadus Butte Cut Bank Dillon Drummond Glasgow Glendive Great Falls Harlowton Havre Helena Jordan Kalispell Lewiston Livingston Maimstrom Miles City Missoula Monida Sidney W Yellowston 83 83 88 88 90 90 89 90 88 89 90 88 88 91 89 92 89 92 92 94 94 92 94 95 90 94 93 93 95 90 91 92 93 111 105 112 112 112 113 106 104 111 109 109 112 106 114 109 110 111 105 114 112 104 111 2.4 31.8 55.8 7.8 52.8 10.8 49.2 25.2 13.2 34.8 7.8 10.2 43.2 33 21 21.6 28.2 33 43.2 22.8 31.8 22.2 46.2 25.2 33 — LATITUDE. min. degrees 44 42 44 46 46 43 44 45 48 47 48 43 33 33 33 33 31 32 30 31 31 32 32 31 34 38 37 37 38 37 39 40 37 35 36 38 40 37 40 38 38 37 38 45 45 45 48 45 46 48 47 47 46 48 46 47 48 47 45 47 46 46 44 47 44 49.8 55.2 55.8 33 4.2 34.8 55.8 39 43.8 46.8 40.2 57 36 15 40.2 13.2 7.8 28.8 25.8 33 19.8 18 42 30 25.8 55.2 34.2 43.2 39 NE Yucca Flat Berlin Atlantic Ainsworth Alliance Beatrice Broken Bow Burwell Chadron Columbus Cozad Falls City Grand island Hastings Imperial Kearney Lincoln Muni Mecook Muilen Norfolk North Omaha North Platte O'neill Offutt AFB Omaha Ord/Sharp Scottsbluff Sidney Muni Valentine Austin Battle Mtn Caliente Elko Ely/Y elland Eureka Fallon NAS Hawthorne ind Sprng Rn Las Vegas Lovelock Mercury Nellis AFB Owyhee Reno Tonopah Wildhorse Winnemucca Concord Jaffrey Keene Laconia Lebanon Manchester Mt Washingtn Nashua Pease AFB Wolfeboro N Barnegat Ls Fairfield Lakehurst Mcguire AFB Millville Morristown Newark Inti Teterboro Albuquerqu Cannon Carlsbad Clayton Arpt Corona Deming Farmington Galtup/Clark Grants Hobbs Holioman AFB Las Cruces Las Vegas Los Alamos Moriarity Northrup Str Raton Roswell 101 100 101 97 96 100 98 95 95 98 103 102 100 117 116 114 115 114 115 118 118 115 115 118 116 115 116 119 117 116 117 116 106 103 104 103 105 107 108 108 107 103 106 106 105 106 106 106 104 104 58 58.8 10.2 55.2 1.2 1.8 10.2 46.8 4.8 15 4.8 4.8 46.2 16.8 2.4 31.8 LATITUDE 34.2 37.8 55.8 16.2 46.8 4.8 16.8 52.2 22.8 19.8 27 15 45 31.2 10.2 40.8 51 18 39 52.8 58.8 54 44.4 18 e degrees. Santa Fe Silver City Socorro Taos Truth Or Con Tucumcari White Sands Albany Ambrose Binghamton Buffalo Dansville Elmira Farmingdale Fort Drum Glens Falls Griffiss AFB Islip Ithaca Jamestown Massena Monticello New York Newburgh Niagara Fall Ogdensburg Oneonta Plattsburgh Rochester Saranac Lk Schenectady Syracuse Utica Watertown Westhampton Pl Whi Asheville 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- Salem Devil's Lake Dickenson Fargo Grand Forks Jamestown Lidgerwood Minot Roseglen Athens Canton Cincinnati Cleveland Columbus Dayton Findlay Mansfield Rickenbacker Toledo Willoughby Youngstown Zanesville 106 108 106 105 107 103 106 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 13 82 75 80 76 76 75 76 78 78 79 81 82 77 77 79 75 77 77 79 78 77 79 77 80 102 96 97 98 97 101 DE LATITUDE... 4.8 10.2 5.4 34.2 16.2 3.6 2.4 4.8 22.2 58.8 43.8 10.8 40.8 16.8 13.8 25.8 40.2 40.8 52.8 1.2 40.2 31.2 55.8 4.8 2.4 40.2 5.4 min: degrees 35 32 34 36 33 35 32 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 35 35 35 34 36 35 36 35 35 36 35 35 34 35 35 35 35 34 35 35 35 35 34 36 39 40 39 41 40 41 40 39 41 41 41 39 “min 37.2 37.8 4.2 25.2 13.8 10.8 37.8 45 45 13.2 55.8 58.2 10.2 43.8 21 13.8 46.8 28.8 95.6 42 46.2 30 40.8 52.2 39 7.2 22.8 25.8 16.2 13.2 54 7.8 15 16.2 7.8 4.8 45 54 49.2 19.2 1.8 55.2 4.8 42 10.2 52.2 51 14.4 16.2 7.8 49.2 37.8 16.2 57 - LONGITUDE ~~ LATITUDE ~~ LONGITUD — LATITUDE LONGITUDE : ... LATITUDE degrees... min degrees i - degrees. . min degrees min degrees min degrees min OKLAHOMA >>> Myrtle Beach 78 55.8 33 San Angelo 100 3 31 22.2 Altus AFB 99 16.2 34 40.2 Shaw AFB 80 28.2 33 San Antonio 98 28.2 29 31.8 Ardmore 97 1.2 34 18 Spartanburg 81 57.6 34 Sanderson 102 25.2 30 10.2 Bartlesville 96 0 36 45 ‘SOUTH DAKOTA South Brazos 95 52.2 28 1.8 Clinton 99 1.2 35 21 Aberdeen 25.8 45 27 Stephenville 98 10.8 32 13.2 Enid 97 4.8 36 22.8 Brookings 4.8 44 18 Temple 97 252 31 9 Fort Sili 98 2.4 34 - 39 Chamberlain 19.2 43 48 Tyler/Pounds 95 2.4 32 22.2 Gage 99 46.2 36 18 Custer 103 3.6 43 46.2 Victoria 96 55.2 28 51 Hobart 99 3 35 0 Ellsworth 103 0.6 44 9 Wichita Flis 98 3 33 58.8 Lawton 98 25.2 34 34.2 Huron 98 13.2 44 22.8 Wink 103 1.2 31 Mcalester 95 46.8 34 52.8 Lemmon 102 10.2 45 55.8 ‘UTAH 0 Norman 97 28.2 35 13.8 Mitchell 98 1.8 43 46.2 Blanding 109 46.8 38 1.8 Oklahoma 97 3.6 35 24 Mobridge 100 25.8 45 31.8 Bullfrog Mar 110 4.2 37 30 Page 94 37.2 34 40.8 Philip 101 3.6 44 3 Cedar City 113 0.6 37 42 Ponca City 97 0.6 36 43.8 Pierre 100 16.8 44 22.8 Delta 112 34.8 39 19.8 Stillwater 97 54 36 9.6 Rapid City 103 4.2 44 3 Eagle Range 113 4.2 41 3 т Tinker AFB 97 22.8 35 25.2 Redig 103 19.2 45 9.6 Green River 110 9 39 0 ne Tulsa 95 5.4 36 12 Sioux Falls 96 43.8 43 34.8 Hanksville 110 43.2 38 22.2 Vance AFB 97 55.2 36 19.8 Watertown Hill AFB 111 58.2 41 7.2 OREGON | Yankton Logan 111 51 41 46.8 Astoria TENNESSEE Milford 113 1.8 38 43.2 Aurora Bristol Moab 109 45 38 46.2 Baker 117 49.2 44 49.8 Chattanooga Ogden 112 1.2 41 10.8 Brookings 124 28.2 42 4.8 Clarksville 87 25.2 36 37.2 Price/Carbon 110 45 39 37.2 Burns Arpt 118 57 43 36 Crossville 85 4.8 35 57 Provo 111 43.2 40 13.2 Cape Blanco 124 57 43 22.8 Dyersburg 89 2.4 36 1.2 Roosevelt 110 37.8 40 30 Cascade 121 52.8 45 40.8 Jackson 88 55.2 35 36 Saint George 113 3.6 37 4.8 Corvallis 123 16.8 44 30 Knoxville 83 58.8 35 49.2 Salt Lake Ct 411 58.2 40 46.8 Eugene 123 13.2 44 7.2 Memphis Int! 90 0 35 3 Tooele 112 1.2 40 10.2 Hillsboro 122 57 45 31.8 Monteagle 85 30.6 35 9 Vernal 109 31.2 40 27 Klamath Fali 121 43.8 42 9 Nashville 86 40.8 36 7.2 Wendover 114 3 41 132 La Grande 118 0 45 16.8 0 "VERMONT > _ о Lake View 120 21 42 10.8 TEXAS о Burlington Meacham 118 2.4 45.. 30 Abilene 99 40.8 32 25.2 Montpelier Medford 122 52.2 42 22.2 Alice 98 1.8 27 43.8 Newport Newport 124 3 44 37.8 Amarillo 101 4.2 35 13.8 Rutland 73 57 43 31.8 North Bend 124 15 43 25.2 Austin 97 4.2 30 18 St Johnsbury 72 1.2 44 25.2 Ontario 117 1.2 44 1.2 Bergstrom Af 97 40.8 30 12 Wilmington 52.8 42 Pendieton 118 51 45 40.8 Big Sky 101 28.8 32 234 VIRGINIA © EEE Portland 122 3.6 45 36 Big Spring 101 27 32 18 Charlottes 38 Redmond 121 9 44 16.2 Brownsville 97 25.8 25 54 Chesapeake 76 1.2 37 Roseburg 123 22.2 43 13.8 Brownwood 98 57.6 31 47.4 Danville 79 19.8 36 34.2 Salem 123 0 44 55.2 Carswell AFB 97 25.8 32 46.8 Fort Belvoir 77 10.8 38 43.2 Sexton 123 22.2 42 37.2 Chase NAS 97 40.2 28 22.2 Fort Eustis 76 37.2 37 7.8 The Dalles 121 9 45 37.2 Childress 100 16.8 34 25.8 Hot Springs 79 49.2 37 57 Troutdale Coliege Stn 96 22.2 30 34.8 Langley AFB 76 22.2 37 4.8 PENNSYLVANIA Corpus Chrst 97 3 27 46.2 Lynchburg 79 1.2 37 19.8 Allentown Cotulla 99 13.2 28 27 Newport 76 3 37 7.8 Altoona Dalhart 102 33 36 1.2 News Beaver Falls Dallas/FW 97 1.8 32 54 Norfolk NAS 76 16.8 36 55.8 Blairsville Del Rio 100 55.2 29 22.2 Norfolk Rgni 76 1.2 36 54 Bradford Dyess AFB 99 51 32 25.8 Oceana NAS 76 1.8 36 49.2 Dubois El Paso 106 2.4 31 48 Quantico Mca 77 1.8 38 30 Erie Ellington Af 95 10.2 29 37.2 Richmond 77 19.8 37 30 Franklin Fort Worth 97 21 32 49.2 Roanoke 79 58.2 37 19.2 Harrisburg Ft Hood Aaf 97 43.2 31 9 Muni Johnstown Galveston 94 52.2 29 16.2 Staunton 78 38 16.2 Lancaster Gray AFB 97 49.8 31 4.2 Volens Latrobe Greenville 96 4.2 33 4.2 Wallops Sta —— Middletown Guadalupe 104 4.8 31 49.8 ‘WASHINGTON Muir Harlingen 97 40.2 26 13.8 Bellingham Nth Philadel Hondo 99 10.2 29 21 Bremerton 122 46.2 47 28.8 Philadelphia Houston 95 21 29 58.2 Burlington 122 19.8 48 30 Philipsburg Junction 99 46.2 30 30 Colville 118 28.2 48 52.8 Pittsburgh Kelly AFB 98 34.8 29 22.8 Ephrata 119 31.2 47 19.2 Reading Kerrville 99 4.8 29 58.8 Everet/Paine 122 16.8 47 55.2 Site R Killeen 97 40.8 31 4.8 Fairchild 117 39 47 37.2 State Colleg Kingsville 97 49.2 27 30 Fort Lewis 122 34.8 47 4.8 Wilkes-Barre Laredo Intl 99 28.2 27 31.8 Hanford 119 3.6 46 34.2 Williamsport Laughlin AFB 100 46.8 29 22.2 Hoquiam 123 58.2 46 58.2 Willow Grove. Longview 94 43.2 32 22.8 Mcchord AFB 122 28.8 47 9 Lubbock 101 49.2 33 39 Moses Lake 119 19.2 47 12 Block Island 71 34.8 41 10.2 Lufkin 94 45 31 13.8 Oak Harbor 122 40.8 48 15 Nth Kingston 71 25.2 41 36 Marfa 104 1.2 30 22.2 Olympia 122 5.4 46 58.2 Providence... — 41 43.8 Mcallen 98 13.8 26 10.8 Omak 119 31.8 48 25.2 Midland 102 10.8 31 57 Pasco 119 7.2 46 16.2 Anderson 82 43.2 34 30 Mineral Wils 98 4.2 32 46.8 Port Angeles 123 3 48 7.2 Beaufort 80 43.2 32 28.8 Palacios 96 15 28 43.2 Puliman 117 7.2 46 45 Charleston 80 1.8 32 54 Paris/Cox 95 27 33 37.8 Quillayute 124 33 47 57 Columbia 81 7.2 33 57 Plainview 101 42.6 34 10.2 Renton 122 13.2 47 30 Florence 79 43.2 34 10.8 Port Arthur 94 1.2 30 34.8 Seattle 122 1.8 47 27 Greenville 82 21 34 51 Reese AFB 102 3 33 36 Shelton 123 9 47 15 Mcentire 80 4.8 33 55.2 Rockport 97 1.8 28 4.8 Spokane 117 31.8 47 37.8 Tacoma 122 34.8 47 16.2 Toledo 122 4.8 46 28.8 59 60 LONGITUDE LATITUDE LONGITUDE = ~~ LATITUDE. LONGITUDE - ~~ LATITUDE degrees min degrees min ЩЕ —. min: degrees o degrees min - de Walla Walla 118 16.8 46 6 WISCONSIN WYOMIN Wenatchee 120 1.2 47 24 Appleton 88 31.2 44 15 Big Piney 110 0.6 42 34.2 Whidbey Is 122 39 48 21 Eau Claire 91 28.8 44 52.2 Casper 106 28.2 42 55.2 Yakima 120 8 46 34.2 Green Bay 88 7.8 44 28.8 Cheyenne 104 49.2 41 9 WEST VIRGINIA о о Janesville 89 1.8 42 37.2 Cody 109 1.2 44 31.2 Beckley 81 7.2 37 46.8 La Crosse 91 15 43 52.2 Douglas 105 22.8 42 45 Bluefield 81 13.2 37 18 Lone Rock 90 10.8 43 12 Evanston 111 0 41 19.8 Charleston 81 3.6 38 22.2 Madison 89 19.8 43 7.8 Gillette 105 31.8 44 21 Clarksburg 80 13.8 39 16.8 Manitowac 87 40.2 44 7.8 Jackson 110 43.8 43 36 Elkins 79 51 38 52.8 Milwaukee 87 5.4 42 57 Lander 108 43.8 42 49.2 Huntington 82 33 38 22.2 Mosinee 89 40.2 44 46.8 Laramie 105 40.8 41 19.2 Lewisburg 80 2.4 37 52.2 Neenah 88 31.8 44 13.2 Moorcroft 104 48.6 44 21 Martinsburg 77 58.8 39 24 Oshkosh 88 34.2 44 0 Rawlins 107 1.2 41 48 Morgantown 79 55.2 39 39 Rhinelander 89 27 45 37.8 Riverton 108 27 43 3 Parkersburg 81 25.8 39 21 Rice Lake 91 43.2 45 28.8 Rock Springs 109 4.2 41 36 Wheeling 80 39 40 10.8 Volk Fld 90 16.2 43 55.8 Sheridan 106 58.2 44 46.2 Wh Sulphur 80 1.2 37 27.6 Wausau 89 37.2 44 55.2 Worland 107 58.2 43 58.2 Yellowstone 110 25.2 44 33 CANADA CITY PROVINCE LONGITUDE LATITUDE CITY COUNTRY LONGITUDE LATITUDE - Calgary Alberta 114 7 51 14 Glasgow Scotland 4 15w 55 50n Churchill Newfoundland 94 0 58 45 Guatemala City Guatemala 90 31 w 14 37n Coppermine Northwest Terr. 115 21 67 49 Guayaquil Ecuador 79 56 w 2 10s Edmonton Alberta 113 25 53 34 Hamburg Germany 10 2e 53 33n Frederickton New Brunswick 66 40 45 57 Hammerfest Norway 23 38 e 70 38n Ft Mcpherson Northwest Terr 134 50 67 29 Havana Cuba 82 23w 23 8n Goose Bay Newfoundland 60 20 53 15 Helsinki Finland 25 0e 60 10n Halifax Nova Scotia 63 34 44 39 Hobart Tasmania 147 19e 42 52s Hazelton BC 127 38 55 15 iquique Chile 70 7w 20 10s Kenora Ontario 94 29 49 47 Irkutsk Russia 104 20e 52 30n Labrador City Labrador 66 52 52 56 Jakarta Indonesia 106 48 e 6 16s Montreal Quebec 73 39 45 32 Johannesburg South Africa 28 4е 26 12 5 Mt. Logan Yukon 140 24 60 34 Kingston Jamaica 76 49 w 17 San Nakina Yukon 132 48 59 12 La Paz Bolivia 68 22 W 16 27s Ottawa Ontario 75 45 45 18 Leeds England 1 30 w 53 45n Peace River Alberta 117 18 56 15 Lima Peru 77 2w 12 Os Pr. Edward Isl Nova Scotia 63 9 46 14 Liverpool England 3 Ow 53 25n Quebec Quebec 71 15 46 50 London England 0 5 w 51 32n Regina Saskatchewan 104 38 50 30 Lyons France 4 50 e 45 45n Saskatoon Saskatchewan 101 32 52 10 Madrid Spain 3 42 w 40 26 n St. Johns Newfoundiand 52 43 47 34 Manchester England 2 15 w 53 30n Toronto Ontario 79 23 43 39 Manila Phillipines 120 57e 14 35n Vancouver BC 123 7 49 16 Marseilles France 5 20e 43 20n Victoria BC 123 20 48 26 Mazatlan Mexico 106 25w 23 12n Whitehorse Yukon 135 3 60 43 Mecca Saudi Arabia 39 45e 21 23n Winnipeg Manitoba 97 g 49 53 Melbourne Australia 144 58 e 37 47 s INTERNA TIONAL Mexico City Mexico 99 7w 19 26n Milan Italy 9 10e 45 27n Montevideo Uruguay 56 10w 34 538 Aberdeen Scotland 2 9 w 57 9n Moscow Russia 37 36 e 55 45n Adelaide Australia 138 36e 34 55s Munich Germany 11 35e 48 8n Amsterdam Holland 4 53e 52 22Nn Nagasaki Japan 129 57 e 32 48n Ankara Turkey 32 55e 39 55n Nagoya Japan 136 56 e 35 7n Asuncion Paraguay 57 40 w 25 15s Nairobi Kenya 36 55 е 1 25s Athens Greece 23 43 e 37 58n Nanjing China 118 53e 32 3n Auckland New Zealand 174 45 e 36 52s Naples italy 14 15e 40 50n Bangkok Thailand 100 30e 13 45n Newcastle England 1 37W 54 58n Barcelona Spain 2 9e 41 23n Odessa Ukraine 30 48 e 46 27n Belém Brazil 48 29 w 1 28s Osaka Japan 135 30e 34 32n Belfast Northern Ireland 5 56 w 54 37n Oslo Norway 10 42 e 59 57n Belgrade Yugoslavia 20 32e 44 52n Panama City Panama 79 32 \м 8 58n Berlin Germany 13 25e 52 30n Paramaribo Surinam 55 15w 5 45n Birmingham England 1 55 w 52 26n Paris France 2 20 e 4 48n Bombay India 72 48 e 19 On Beijing China 116 256 39 55n Bordeaux France 0 31 w 44 sûn Perth Australia 115 52 е 31 57s Bremen Germany 8 49 e 53 an Plymouth England 4 5 w 50 25n Brisbane Australia 153 Se 27 29s Rio de Janeiro Brazil 43 12w 22 57 $ Bristol England 2 35 w 51 28n Rome Italy 12 27 e 41 54 n Brussels Belgium 4 22e 50 52n Salvador Brazit 38 27 W 12 56s Bucharest Romania 26 7e 44 25n Santiago Chile 70 45 w 33 28s Budapest Hungary 19 5e 47 30n St. Petersburg Russia 30 18e 59 56n Buenos Aires Argentina 58 22 W 34 35s Sao Paulo Brazil 46 31w 23 31s Cairo Egypt 31 21e 30 2n Shanghai China 121 28 e 31 10 n Canton China 113 15e 23 7n Sofia Bulgaria 23 20e 42 40n Cape Town South Africa 18 22e 33 55 s Stockhoim Sweden 18 3e 59 17n Caracas Venezuela 67 2w 10 28n Sydney Australia 151 Oe 34 Os Chihuahua Mexico 106 5w 28 З/п Tananarive Madagascar 47 33e 18 50s Chongqing China 106 34 e 23 46n Teheran Iran 51 45 e 35 45n Copenhagen Denmark 12 34e 55 40n Tokyo Japan 139 45e 35 40n Cordoba Argentina 64 10 w 31 285 Tripoli Libya 13 12e 32 57n Darwin Australia 130 ble 12 28s Venice italy 12 20e 45 26n Dublin Ireland 6 15w 53 Z0n Veracruz Mexico 96 10w 19 10n Durban South Africa 30 53e 29 53s Vienna Austria 16 20e 48 14 Edinburgh Scotland 3 10w 55 B55n Warsaw Poland 21 Oe 52 14 n Frankfurt Germany 8 41 e 50 7n Wellington New Zealand 174 47 e 41 17s Georgetown Guyana 58 15 w 6 45n Zúrich Switzerland 8 31e 47 21n Appendix D - RS-232 Connection You can control your telescope with a computer via the RS-232 port on the computerized hand control and using an optional RS-232 cable (#93920). Once connected, the telescope can be controlled using popular astronomy software programs. Communication Protocol: The Advanced GT communicates at 9600 bits/sec, No parity and a stop bit. All angles are communicated with 16 bit angle and communicated using ASCII hexadecimal. Description | PC Command ASCII | Hand Control Response | Notes Echo Kx X# Useful to check communication Goto Azm-Alt B12AB, 4000 # 10 characters sent. B=Command, 12AB=Azm, comma, 4000=Alt. If command conflicts with slew limits, there will be no action. Goto Ra-Dec R34AB, 12CE # Scope must be aligned. If command conflicts with slew limits, there will be no action. Get Azm-Alt Z 12AB, 40004 10 characters returned, | 12AB=Azm, comma, 4000=Alt, # Get RA-Dec E 34AB, 12CE# Scope must be aligned Cancel Goto M # Is Goto in Progress L O# or 1# O=No, 1=Yes; "0" is ASCII character zero Is Alignment Complete J O# or 1# O=No, 1=Yes Commands below available on version 1.6 or later HC version V 22 Two bytes representing V2.2 Stop/Start Tracking TX # Alt-Az tracking requires alignment x = 0 (Tracking off) x = 1 (AIt-AZ on) x = 2 (EQ-N) x = 3 (EQ-S) 32-bit goto RA-Dec r34AB0500,12CE0500 # 32-bit get RA-Dec e 34AB0500,12CE0500# The last two characters will always be zero. Commands below available on version 2.2 or later 32-bit goto Azm-Alt b34AB0500,12CE0500 # 32-bit get Azm-Alt Z 34AB0500,12CE0500# The last two characters will always be zero. The cable required to interface to the telescope has an RS-232 male plug at one end and a 4-4 telephone jack at the other end. The wiring is as follows: 4-4 Modular Phone Jack / / DB9 Pin 3 J PC Transmit DB9 Pin 5 Ground DB9 Pin? PC Receive 61 Additional RS232 Commands Send Any Track Rate Through RS232 To The Hand Control 1. Multiply the desired tracking rate (arcseconds/second) by 4. Example: if the desired trackrate is 150 arcseconds/second, then TRACKRATE = 600 2. Separate TRACKRATE into two bytes, such that (TRACKRATE = TrackRateHigh*256 + rackRateLow). Example: TrackRateHigh =2 TrackRateLow = 88 3. To send a tracking rate, send the following 8 bytes: a. Positive Azm tracking: 80, 3, 16, 6, TrackRateHigh, TrackRateLow, 0, 0 b. Negative Azm tracking:80, 3, 16, 7, TrackRateHigh, TrackRateLow, 0, 0 c. Positive Alt tracking: 80, 3, 17, 6, TrackRateHigh, TrackRateLow, 0, 0 d. Negative Alt tracking: 80, 3, 17, 7, TrackRateHigh, TrackRateLow, 0, 0 4. The number 35 is returned from the handcontrol Send A Slow-Goto Command Through RS232 To The Hand Control (note: Only valid for motorcontrol version 4.1 or greater) 1. Convert the angle position to a 24bit number. Example: if the desired position 1s 220°, then POSITION 24BIT = (220/360)*2** = 10,252,743 | 2. Separate POSITION 24BIT into three bytes such that (POSITION 24BIT = PosHigh*65536 + PosMed*256 + PosLow). Exampe: PosHigh = 156, PosMed = 113, PosLow = 199 3. Send the following $ bytes: a. Azm Slow Goto: 80, 4, 16, 23, PosHigh, PosMed, PosLow, 0 b. Alt Slow Goto: 80, 4, 17,23, PosHigh, PosMed, PosLow, 0 4. The number 35 15 returned from the handcontrol Reset The Position Of Azm Or Alt 1. Convert the angle position to a 24bit number, same as Slow-Goto example. 2. Send the following 8 bytes: a. Azm Set Position: 80, 4, 16, 4, PosHigh, PosMed, PosLow, 0 b. Alt Set Position: 80, 4, 17, 4, PosHigh, PosMed, PosLow, 0 3. The number 35 1s returned from the handcontrol 4. Note: Ifusing Motorcontrol version less than 4.1, then send: a. Azm Set Position: 80, 3, 16, 4, PosHigh, PosMed, PosLow, 0 b. Alt Set Position: 80, 3, 17, 4, PosHigh, PosMed, PosLow, 0 62 APPENDIX E — MAPS OF TIME ZONES "2 ASSET Fa us AAN Farms arn rs, q aii 1 % ® * + \ % KERIB ATE % NE % ve Seto 1-85,000.000 à 9 & 800 1000 Rigen о 800 $000 Misa 100 00| 200 300 4:00 — 50 6:00 700. 8:00 8:00 | 1000 1 0 9 8 7 6 5 4 3 2 Hawaii Alaska Pacific Mountain Central Eastern 63 ct HI OL seLo7 SWL ¿ —9 5 ани) jesisaAiun L- Tok Hen 20 BRM Ok MP TE at YT A peter “pri Mal plena TS pitt ue DEEE LATE Meda perdiera = ACA 1 E TT LOAD Ate MET MEA T TO ZE | ZE FT OT 6 8 £ | 9 Hi 0000 | 2 DO ЕЁ > E DOE Aa mél EL NE UPS ung и > - 7 72 a Ka B rey a i Era bu ; BON 3 au ge 7 pam 3 Edy Pa É PAR § rw ha Я акне Hes . : Ч Tt 5 gE чт iL 8 4 id : J 8 [rm i 8 py = = à Rite AN eva vas 4% e [5 wpa Serena Or N TESTA | ; в к +. * - . 3 - N . тян | Th, pri Let RED By an mm] - ura i y i $ 3 Al © dl A i Этот бк - £elvYElHiNa - о wen WET nn Tm Ln TT ET — YE > FL - TEEN TL PIE G EXA MDI RRA Ff TOIT EAT 5 1543 © 1534 * = 4] + + a : зол р в ; CE! ME oz] Le E LIO) ei DOY Yen Aso (DLA) BURL ERISA PR LER CESS EPR : Came! SLI SALA PAT SEAN Gs redes wir Eo E à © WER PE FRESTÍ FO YI SA BILL ue FEE PRE rend DREGE, 64 January - February Sky Trianguium 9 Perseus Años Canis Minor Crater Procyon 65 March - April Sky innela ® CassioP Navi ° “Cepheus To 66 May - June Sky Corona o й > o Borealis Arctyrus . e A \ y e AN A e, | Serpens d ° * Ophiuchus (caput) | a x у 3 ; / NS Libra * Y A 7 В / N + а ° \ ; Ne e /Е © Hydra Y 67 July - August Sky 1 Auriga Perseus Ursa Minor Major Navi Cassiopeia Andromeda Bootes Draco °° | ES Pegasus e Pisces, Rasalhague « \ N | u o Dephinus] ° y Ophiuchus ° / № Aquarius . a . Ne, Tau, fm в © Capricornus ес © y Serpens Hercules , э ® (сари) ® « Sagittarius 68 1 y \ \ РВ A Idebaran ON Taurus \ 69 Triangulum | “ à co pe 70 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. В. 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 1s 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 U.S.A. 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. Celestron 2835 Columbia Street Torrance, CA 90503 U.S.A. Tel. (310) 328-9560 Fax. (310) 212-5835 Web site at http//www.celestron.com Copyright 2003 Celestron All rights reserved. (Products or instructions may change without notice or obligation.) Item # 11025-INST $10.00 08-03 ">
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Key Features
- Care and Cleaning of the Optics
- Collimation
- Accessories
- Technical Specifications
- Glossary of Terms
- Longitudes and Latitudes
Frequently Answers and Questions
How do I clean the corrector plate of my telescope?
Remove dust with a camel's hair brush or pressurized air. Use optical cleaning solution and white tissue paper to remove remaining debris.
What do I do if moisture condenses on the inside of the corrector?
Remove accessories, place the telescope in a dust-free environment, point it down.
How do I collimate my telescope?
Use a light source, center a star in the center of the field, slowly cross in and out of focus and judge the symmetry of the star. If needed, tighten the secondary collimation screw(s) to move the star toward the direction of the skewed light.