Knowledge Base

  • LX90 GPS mount

    The mount's drive base is made of die-cast aluminum. The light-weight, but rigid, die-cast aluminum dual fork arms are shaped to damp vibrations quickly. There is a carrying handle on each fork arm. Both manual and electric slow motion controls are provided for both right ascension and declination. In addition to the digital readout of the scope's aiming point in right ascension and declination on the AutoStar computer hand control, there are analog setting circles on the mount (5" in declination and 8.75" in right ascension). The drive base has a 4-port control panel, including two RS-232 serial interface ports for communication with an external computer and other ancillary equipment.

    A 16-channel Sony GPS (Global Positioning System) receiver is built into the top of one of the fork arms. When the scope is turned on, the GPS receiver locks onto the network of orbiting GPS satellites to determine your observing location's latitude, longitude, date, and time. It uses this information to tell the scope's AutoStar computer where and when on earth the scope is located. Once the computer has this information, it orients the scope to the sky and slews at 6.5 degrees per second to the first of two alignment stars. If that star is not precisely centered in the finderscope or main scope optics, a touch or two on the Autostar hand control's directional push buttons quickly centers it. Do the same with the second alignment star the scope moves to and the scope is then accurately aligned on the sky and ready to locate and track any celestial object you choose.

    The mount includes servo-controlled 12VDC slewing and tracking motors with 4.9" worm gear drives in both altitude and azimuth. The drive system has individually selectable drive speeds in both right ascension and declination - 6.5°/sec, 3°/sec, and 1.5°/sec for slewing and centering; as well as 128x, 64x, 16x, 8x, and 2x the sidereal rate for centering and astrophotographic guiding. In addition, there are standard solar, lunar, and sidereal tracking rates with 2000 precision-selected incremental rates that permit observatory-level precision in tracking the Moon and planets.

    The scope is powered by eight user-supplied C-cell batteries that store in the drive base so you can use the LX90 in the field or your backyard without the need for a separate battery pack or AC power supply. The usable life of the batteries is up to 60 hours, depending on the ambient temperature (colder temperatures reduce usable battery life). An optional #RCXAC adapter is available to allow you to power the scope from 110-120volt 60Hz AC household current in your backyard to conserve battery life. An optional #607 cigarette lighter plug cable is available to power the scope from your car's cigarette lighter plug or from a rechargeable battery for extended use in the field.

  • Canon Image Stabilization

    Large aperture high power binoculars are a very useful tool for astronomy. They
    complement the close up view of a telescope by letting you see the big picture -
    of open star clusters, galaxies like Andromeda, comets, and more. But it's hard
    to hold a conventional big binocular steady enough to examine the sky at length.
    Your arms soon get tired and you develop unavoidable hand tremors that blur the
    images and fuzz the details. No more. Canon active image-stabilized binoculars make
    those blurred high power images obsolete. Their rock-steady and unblurred images
    mean there is not only more detail to see, and see clearly, but there is also minimal
    eye fatigue to tire you out and bring on headaches.

    The Canon IS (Image Stabilized) binoculars have two Vari-Angle Prisms located between
    the objective lenses and the image-erecting prisms. If the binocular tilts quickly
    (from even minor hand tremors, for example), horizontal and vertical sensors detect
    the motion. A microprocessor adjusts the Vari-Angle Prisms in the right and left
    sides of the binocular independently to compensate for a tilt up to +/- 0.7° - far
    more motion than any fatigue-induced tremor.

    Each prism expands or contracts in a bellows motion to redirect the light path and
    compensate for the tilt. This instantly and precisely adjusts the direction of the
    visual path through the binoculars to maintain a perfectly steady and centered image,
    even while the binocular moves. The result is a clear, high power, hand-held image
    at the push of a button.

    The diagram below shows the action of the Vari-Angle Prisms and the results you
    can expect. You can see the changing "bellows" action of the Vari-Angle Prisms (yellow
    in the diagram) as the tilt of the binocular changes.

  • 16" LX200 mount

    The mount's drive base and dual fork arm assembly is made of heavy-duty die-cast aluminum. For added strength and rigidity the base and forks are cast in one continuous U-shaped piece, rather than being a less-rigid three-piece assembly of two vertical arms bolted to the sides of the drive base. The optical tube has two factory-installed declination housings which bolt to the tops of the one-piece U-shaped fork to complete the very rigid optical assembly.

    There are two carrying handles on each declination housing for lifting the tube. At least two people are needed to lift the 125 pound optical tube up onto the fork arms and bolt it into place. Analog setting circles are provided on the mount (12" in declination and 17" in right ascension, both with verniers), in addition to the digital r.a. and dec readouts on the AutoStar computer hand control. The drive base has a 7-port multi-function control panel, including two RS-232 serial interface ports for communication with an external computer and other ancillary equipment.

    The mount includes servo-controlled 18VDC high torque slewing and tracking motors with 11" worm gear drives in both altitude and azimuth. The declination axis is supported by four 80mm roller bearings (two per side). Two additional roller bearings, one 100mm and one 150mm, provide smooth motion in right ascension.

    The drive system has over 2000 individually selectable drive speeds in both right ascension and declination to permit observatory-level precision in tracking, guiding, and slewing. You can choose from 0.01x to 1.0x sidereal, variable in 0.01x increments; 2x, 8x, 16x, 64x, or 128x the sidereal rate; as well as 1°/sec. to 6°/sec., variable in 0.1° increments. You can also select either a pre-set sidereal or lunar tracking rate, or you can custom-select a drive speed from 2000 incremental rates to match solar or planetary motions.

    There is a supplied adapter with a 25' cord that lets you power the scope from 110-120 volt 60 Hz AC household current in your back yard or observatory. An optional #1812A adapter lets you power the 18VDC scope from your car's 12VDC cigarette lighter plug or a rechargeable 12 volt battery for extended use in the field. Maximum power draw is 2 amps, so choose a battery with a sufficiently high power capacity to last for a full night's observing.

  • MAX mount on tripod

    The Meade MAX go-to robotic German equatorial mount can handle a payload of up to 250 pounds (excluding counterweights) with ease and precision. It has a periodic error of only 2 arc seconds, less than half that of a star's Airy disc on nights of sub-par seeing, and sub arc minute pointing accuracy during go-to operation.

    It uses 13.625" diameter right ascension and declination drive gears with 652 teeth on each. Each gear is driven by a high torque Pittman DC servo motor turning a clutchless 1.1667" diameter fully-enclosed and permanently precision-adjusted spring-loaded worm. The massive right ascension shaft is a full 3.84" in diameter. It is supported by two high payload ball bearing races. The declination shaft is 2.90" in diameter. It is also supported by two high payload ball bearing races.

    The mount can be operated over a 0° to 90° latitude range for use anywhere in the world. Internal cabling eliminates the potential cable tangles possible with lesser mounts that use external cabling to the drive motors. The mount uses a proprietary quick-release dovetail plate, rather than a standard Losmandy-type D plate. P>Electronic features include local control while standing at the scope through two multi-function/multi-port panels; remote control through a LAN from a nearby location (from inside your warm house, for example, while the mount works flawlessly outside in your observatory building in sub-freezing temperatures); or remote control from any distant location via the internet, even from another continent. The mount's main control panel is identical to the main control panel on Meade large aperture LX400-ACF optical tubes. The mount's saddle panel has the same connections as those on the LX400-ACF OTA panel. This includes three USB connectors for accessories such as cameras and auto-guiders. A cable connects between the LX400-ACF OTA and the mount's saddle panel to let the AutoStar controller (handbox) operate the optical tube's focuser and collimation motors, fan, and dew heater. There are no dangling cables between the LX400-ACF optical tube and the body of the mount,

    The MAX mount has a software-controlled meridian limit of 8 degrees beyond the zenith to prevent accidental pier damage when the telescope and its equipment are aimed at the zenith. The user can decrease this if a custom set-up limits this further. There are also horizon limits built into the software that are user-definable if you have trees or buildings blocking your view of the horizon.

    The mount has open loop tracking; 3 USB 2.0 ports; an AutoStar II hand control with a 147,541 star and object library. The hand control has expanded AutoStar II-based software features, such as AutoAlign and an electronic mount balancing program. There's a built-in 16-channel GPS system using a Sony GPS receiver that can be disabled if the mount is permanently installed in an observatory dome. The GPS system can also be left enabled in an observatory to provide an accurate time/date reference, even if the latitude/longitude function is not used. Built-in Smart Mount Technology constantly trains and improves the already high pointing accuracy of the telescope with every object that you center precisely and synchronize on during a night's observing. The Smart Drive system has a new advanced PPEC (Permanent Periodic Error Correction) circuit to improve the already superb two arc second tracking accuracy for astrophotography and more.

    The mount slews in RA and Dec at the following user-selected speeds: 0.01x to 1.0x sidereal, variable in 0.01x increments; 2x, 8x, 16x, 64x, and 128x sidereal; and 1°/second to 2°/second, variable in 0.1°/second increments. In addition, you can select from pre-set sidereal or lunar tracking rates, or any of 2000 custom-selected incremental rates (for tracking the Sun for solar observing, for example).

    The MAX mount requires an optional 110 volt AC to 12 volt DC power adapter (#RCXAC). This AC adapter is rated for a 5 amp capacity. This is enough current to run the fan and the dew heater of an LX400-ACF optical tube, in addition to operating the mount.

    The MAX mount has a heavy duty 26.5" tall tripod for use in the field. When aimed 45° above the horizon, the tripod puts the eyepiece of a typical 16" catadioptric scope approximately 5'8" above ground level. The tripod can also be used semi-permanently in an observatory building, with the tripod giving you the option to also take the mount into the field. The mount is transportable, as opposed to being truly portable, since the various components of the mount and tripod weigh in at a 329 pound total - without counterweights or optical tube. The tripod itself weighs 81 pounds. The mount's pedestal (wedge) weighs 66 pounds. The right ascension assembly is 66 pounds. The declination assembly is 75 pounds. The counterweight shaft assembly weighs 32 pounds. One very motivated person can set up the mount on his own, but a minimum of two people is strongly recommended. The setup time is heavily dependant upon the strength, skill, and experience of the person(s) assembling the components.

    The mount comes with the appropriate number of 35 pound counterweights to balance your particular optical tube. There are optional 20 and 35 pound counterweights available to balance the weight of heavy accessories. The counterweight shaft is a stainless steel threaded rod with a thread 1.5" in diameter and 6 threads per inch. The counterweights are equipped with a pushbutton for quick release to let you slide the counterweight(s) to the approximate correct location on the shaft. Once positioned in the rough location, the pushbutton is released and the counterweight(s) spin on the threaded shaft for fine balance.

    Once the MAX mount is turned on, it goes through the normal AutoStar setup routine. The AutoStar software is expanded for the MAX Mount, however. For example, there are no clutches and no way of disengaging the worm screw from the worm gear. This is for safety reasons, to avoid the potential damage that could be caused by an unbalanced 130-140 pound optical tube swinging unexpectedly, along with the potential for stripped teeth on the drive gear when an unbalanced OTA starts jumping over gear teeth. Accordingly, the new software includes an electronic balancing routine that takes literally only seconds to balance the mount.

  • MAX mount on permanent pier

    The Meade MAX go-to robotic German equatorial mount on a permanent pier can handle a payload of up to 250 pounds (excluding counterweights) with ease and precision. It has a periodic error of only 2 arc seconds, less than half that of a star's Airy disc on nights of sub-par seeing, and sub arc minute pointing accuracy during go-to operation.

    It uses 13.625" diameter right ascension and declination drive gears with 652 teeth on each. Each gear is driven by a high torque Pittman DC servo motor turning a clutchless 1.1667" diameter fully-enclosed and permanently precision-adjusted spring-loaded worm. The massive right ascension shaft is a full 3.84" in diameter. It is supported by two high payload ball bearing races. The declination shaft is 2.90" in diameter. It is also supported by two high payload ball bearing races.

    The mount can be operated over a 0° to 90° latitude range for use anywhere in the world. Internal cabling eliminates the potential cable tangles possible with lesser mounts that use external cabling to the drive motors. The mount uses a proprietary quick-release dovetail plate, rather than a standard Losmandy-type D plate. P>Electronic features include local control while standing at the scope through two multi-function/multi-port panels; remote control through a LAN from a nearby location (from inside your warm house, for example, while the mount works flawlessly outside in your observatory building in sub-freezing temperatures); or remote control from any distant location via the internet, even from another continent. The mount's main control panel is identical to the main control panel on the Meade LX400-ACF optical tubes. The mount's saddle panel has the same connections as those on the LX400-ACF OTA panel. This includes three USB connectors for accessories such as cameras and auto-guiders. A cable connects between the LX400-ACF OTA and the mount's saddle panel to let the AutoStar controller (handbox) operate the optical tube's focuser and collimation motors, fan, and dew heater. There are no dangling cables between the LX400-ACF optical tube and the body of the mount,

    The MAX mount has a software-controlled meridian limit of 8 degrees beyond the zenith to prevent accidental pier damage when the telescope and its equipment are aimed at the zenith. The user can decrease this if a custom set-up limits this further. There are also horizon limits built into the software that are user-definable if you have trees or buildings blocking your view of the horizon.

    The mount has open loop tracking; 3 USB 2.0 ports; an AutoStar II hand control with a 147,541 star and object library. The hand control has expanded AutoStar II-based software features, such as AutoAlign and an electronic mount balancing program. There's a built-in 16-channel GPS system using a Sony GPS receiver that can be disabled if the mount is permanently installed in an observatory dome. The GPS system can also be left enabled in an observatory to provide an accurate time/date reference, even if the latitude/longitude function is not used. Built-in Smart Mount Technology constantly trains and improves the already high pointing accuracy of the telescope with every object that you center precisely and synchronize on during a night's observing. The Smart Drive system has a new advanced PPEC (Permanent Periodic Error Correction) circuit to improve the already superb two arc second tracking accuracy for astrophotography and more.

    The mount slews in RA and Dec at the following user-selected speeds: 0.01x to 1.0x sidereal, variable in 0.01x increments; 2x, 8x, 16x, 64x, and 128x sidereal; and 1°/second to 2°/second, variable in 0.1°/second increments. In addition, you can select from pre-set sidereal or lunar tracking rates, or any of 2000 custom-selected incremental rates (for tracking the Sun for solar observing, for example).

    The MAX mount requires an optional 110 volt AC to 12 volt DC power adapter (#RCXAC). This AC adapter is rated for a 5 amp capacity. This is enough current to run the fan and the dew heater of an LX400-ACF optical tube, in addition to operating the mount.

    The standard MAX mount pier for permanent mounting in an observatory building is 22" tall and weighs 39 pounds. When aimed 45° above the horizon, the MAX mount/pier combination puts the eyepiece of a typical 16" catadioptric scope at a height of approximately 5'4" above ground level.

    The mount comes with the appropriate counterweights to balance your particular optical tube. There are optional 20 and 35 pound counterweights available to balance the weight of heavy accessories. The counterweight shaft is a stainless steel threaded rod with a thread 1.5" in diameter and 6 threads per inch. The counterweights are equipped with a pushbutton for quick release to let you slide the counterweight(s) to the approximate correct location on the shaft. Once positioned in the rough location, the pushbutton is released and the counterweight(s) spin on the threaded shaft for fine balance.

    Once the MAX mount is turned on, it goes through the normal AutoStar setup routine. The AutoStar software is expanded for the MAX Mount, however. For example, there are no clutches and no way of disengaging the worm screw from the worm gear. This is for safety reasons, to avoid the potential damage that could be caused by an unbalanced 130-140 pound optical tube swinging unexpectedly, along with the potential for stripped teeth on the drive gear when an unbalanced OTA starts jumping over gear teeth. Accordingly, the new software includes an electronic balancing routine that takes literally only seconds to balance the mount.

  • Tip-to-Tip Distance

    To be sure that your mount will fit a particular Wheeley Bar product, it may be
    necessary to verify the tip-to-tip distance of the mount. Usually, this measurement
    is made with the legs of a tripod fully retracted (the shortest length) and spread
    out completely. Alternately, you can measure at your preferred viewing height, but
    be sure to allow for the height of the Wheeley Bars (listed with each product).
    The tip-to-tip distance is the measurement from the outside edge of the end of one
    tripod leg or pier foot (where it touches the ground) to the outside edge of another
    tripod leg or pier foot as illustrated below.

    The left-hand illustration shows the tripod footprint and the correct tip-to-tip
    measurement to the outside of the legs. The center illustration shows a tape measure
    being used to determine the tip-to-tip distance. The arrow in the right-hand illustration
    shows the correct measuring point at the outside of the leg.

    Here are some examples of different types of tripod feet. The tick marks show where
    to measure on the outside of the leg to find the tip-to-tip distance. You also need
    to be sure that your tripod leg or foot is not too large to fit into the receptacles
    cut into the Wheeley Bars. Measure the diameter of the leg or foot and be sure it
    is smaller than the listed receptacle size.

      For leg style A, with a tubular tip, you need to measure the leg diameter.

      For leg style B, with a flat circular foot plate, you need to measure the diameter
      of the foot plate.

      For leg style C, with a rounded tip, you need to measure the leg diameter.

      For leg style D, with a pointed tip, you also need to measure the leg diameter.

      For leg style E, with a flat circular leveling foot, you need to measure the leveling
      foot diameter.

  • Takahashi triplet lens

    Takahashi has been the acknowledged leader in ultra-premium apochromatic optics for almost three decades. The new TOA and TSA Series of triplet refractor optical systems keep up that proud tradition.

    Apochromatic means "free from spurious color" - a design that drastically reduces the faint violet halos of out-of-focus light that you see around the planets, the limb of the Moon, and all the bright stars in an ordinary achromatic (crown and flint glass) refractor. Orthoscopic means "visually correct," and is most commonly is associated with an eyepiece design widely regarded as having the most accurate and aberration-free images available.

    All Takahashi TOA and TSA Series triplet refractors are true apochromatic optical systems, with virtually perfect correction of spurious violet color. Their colors are highly saturated, full of contrast, and true to life. They combine these vanishingly low levels of spurious color with equally low levels of optical distortion. Accordingly, they are called "Ortho-Apochromats" to distinguish them from ordinary apochromatic scopes. The term embodies their unrivalled high level of optical performance in both color correction and freedom from aberrations. It's an apt term that is well deserved.

    The Takahashi ortho-apochromatic refractors use a newly developed lens design that uses three air-spaced lenses in three groups. A low dispersion crown glass element is positioned between two FPL-53 ED (Extra-low Dispersion) glass elements to produce images of very high quality . All lens surfaces are fully multicoated with state-of-the-art antireflection materials for maximum light transmission. Takahashi color correction and contrast equals, or exceeds, that of other triplet lens systems, regardless of cost or brand name, even costly oil-spaced triplet systems. Light loss is only about 0.5% at each multicoated lens surface in the Takahashi air-spaced system, versus about 2% at each surface in an oil-spaced triplet. Maintenance is less than oil-spaced designs, since there is no oil to potentially leak or become cloudy with age.

    The simple, yet sophisticated, lens cells provide good stability for the optical system during the rigors of transport. The lens cells are fully collimatable for peak optical performance by using a simple optional Cheshire-type collimating eyepiece and the locking collimating screws on the lens cell. The lens cell design, combined with the tight spacing between the lens elements, allows the optics to quickly reach thermal equilibrium with changing ambient temperatures during the course of an evening's observing.

    The Strehl ratio of a telescope is a numerical value that represents the percentage of the light of a star's image that actually falls into the Airy disk, compared to the theoretical maximum possible. A Strehl ratio of 0.95 is within 95% of perfection and is generally considered excellent. It equates to a 1/8th wave system accuracy. A Strehl ratio of 0.978 equates to a 1/12th wave accuracy. The Strehl ratio of the Takahashi triplet design is 0.992. This means that the Takahashi TOA and TSA objectives are within 99.2% of perfection. This compares with a Strehl ratio of 0.946 for a best-selling fluorite doublet system that has long been considered one of the very best telescopes available.

    Previous apochromatic systems were optimized photographically for the state-of-the-art imaging media available at the time - the silver emulsion of Kodak Technical Pan 35mm film (TP-2415) and the small array/large pixel CCD sensors (less blue-sensitive than current models) that were just coming available to the amateur astronomer. The small residual blue halo seen around bright stars at high powers and off-axis in even the best apo systems of the time was not an issue.

    Today, however, the imaging landscape has changed. Film imaging is becoming a dying art. Technical Pan film is no longer made. CCD sensors with larger arrays of smaller pixels demand tighter stellar images, both on and off-axis, to provide accurate and realistic images. The increased blue sensitivity of modern CCD sensors likewise demands a drastic reduction in the tiny residual blue halo around brighter stars that may not be visible to the eye, but glares like a searchlight onto the blue-sensitive CCD pixels.

    The Takahashi triplets reduce the residual deviation from a flat line response over the blue to green portion of the visible spectrum of previous apo designs (even fluorite systems) by a third. The maximum deviation from all colors coming to a focus in precisely the same plane is no more than +/- 0.01mm from the blue end of the spectrum (436nm) to the H-alpha line at 656nm. The violet halo of chromatic aberration vanishes, and the tiny residual blue halation around bright stars at high powers essentially disappears. Stellar images are tight, with stars in the 12~20µm range, even at the very edges of the fully-illuminated image circle. CCD images are crisp and realistic, and visual observing is unparalleled in its clarity. Quite simply put, the Takahashi TOA and TSA optics have no equal.

  • NexStar 8i Computer

        The NexStar computer hand control has a built-in database of more
    than 45,000 stars, deep space objects, and solar system objects it can locate for
    you. The computer's memory contains the following objects:

    • the entire RNGC (Revised New General Catalog) of 7840 nebulas, galaxies, and star
      clusters

    • the IC (Index Catalog) of 5386 nebulas, galaxies, and star clusters
    • the Messier Catalog of the 110 best known deep sky objects
    • the Caldwell Catalog of 109 fascinating objects that Messier missed
    • 20 famous asterisms
    • the Abell Catalog of 2712 galaxy clusters
    • 25 selected CCD imaging objects

    • 29,500 selected SAO stars, including variable stars and multiple star systems.

        Also included are the eight major planets out to Pluto, as well as
    the Moon, for a total database more than 45,000 stars and objects. It's enough fascinating
    objects to keep you busy observing for the rest of your life.

        You can also store and edit the right ascension and declination of
    up to 400 objects of your own choosing, such as the comet and asteroid coordinates
    published monthly in Astronomy and Sky & Telescope magazines. The
    computer control can quickly find any of those objects at your command, and track
    them with high accuracy for visual observing or casual astrophotography.

        A review in Sky & Telescope magazine commented, "To quantify
    the Go To pointing accuracy, I spent several nights slewing to 50 objects selected
    from the NexStar's database. About one-third of them ended up dead center in the
    field, another third landed within ½° of the center, and the remaining third were
    within 1° of the center."

        All of the database and scope operation information is displayed on
    a double line, 16-character, liquid crystal display on the hand control. This display
    leads you through the steps necessary to line up the scope on the sky, locate objects,
    control scope functions like the brightness of the hand control display, and much
    more. It shows you basic information about the object being viewed (such as the
    object's name, catalog designation, type, magnitude, and so forth). In addition
    to this basic information, there is enhanced information on over 200 of the most
    note-worthy objects. When it's not displaying menus or object information, the display
    also shows you the constantly updated right ascension and declination coordinates
    at which the scope is aimed.

        The Sky & Telescope review said, "After using several NexStar-equipped
    telescopes in recent years, I can attest to the quality of the software and hardware
    for Celestron's Go To system. The package is reliable and offers quick access to
    an excellent array of databases. I especially like Celestron's Tour mode, which
    steps a user through an eclectic choice of deep-sky objects, quirky asterisms, and
    fine double stars, the latter being a class of objects great for urban observing
    that many Go To systems ignore. Using NexStar scopes, I've been introduced to many
    fine double stars."

        There are 19 fiber optic backlit LED buttons that glow a soft red in
    the dark to make it easy for you to control the computer without affecting your
    dark-adapted vision. An RS-232 communication port on the hand control allows you
    to operate the telescope via a personal computer. The Sky & Telescope review
    said, "The author tried Windows and Mac programs, including Desktop Universe, ECU,
    MegaStar, SkyMap Pro, Starry Night,
    and TheSky, and all controlled
    the mount without any problems."

        You have to know where you are in order to find your destination. That
    is what aligning a computerized telescope is all about. The software for the telescope
    needs to know the exact orientation of the telescope in relation to the night sky
    in order to find the tens of thousands of celestial objects that are programmed
    into the hand control.

        Other methods for aligning a computerized telescope require the user
    to confirm what star the telescope is pointing at in order to align. If you're a
    newcomer to astronomy - one who in unfamiliar with the sky and isn't sure which
    star really is Arcturus or Sirius - how can you confirm that information?
    The best you can do is guess. SkyAlign is the only alignment method where
    you truly do not have to know the night sky - and it's only available from Celestron.

        The operation of the NexStar with SkyAlign is simplicity itself. Once
    you mount the scope on its tripod in the altazimuth mode, turn on the power. Enter
    the date and time and your location (the scope's computer will remember up to ten
    different observing sites for you to choose from, and will automatically default
    to the last site you observed from). Then, simply point the scope at any three bright
    stars, or at two bright stars and a planet or the Moon (you don't even have to know
    which stars and planet you're looking at, and you don't have to know and locate
    specific stars as you do with other alignment programs). Using the scope's hand
    control, center the stars in the finderscope crosshairs. There is no need to first
    point the telescope north or to level the optical tube as in other alignment methods.
    The initial position of the telescope is irrelevant. This makes for a fast and very
    easy method for aligning the telescope.

        The NexStar SkyAlign computer system automatically determines
    which objects you chose and generates an internal map of the sky that it uses to
    guide its automatic moves to any star or object you select for the rest of the night.
    It does it by calculating the angles and distances between the objects you've chosen
    and compares them to the known separations between objects. The display tells you
    which three objects you aligned on for confirmation.

        Only two of the alignment objects will actually be used for calculating
    the model of the sky that the computer uses for locating objects. The third object
    simply provides a positive identification of the other two. Therefore, at least
    two of the three alignment objects should be spaced at least 60 degrees apart in
    the sky if possible, and the third object should not fall in a straight line between
    the first two alignment stars.

        Since the brightest stars appear first as the sky darkens at dusk,
    the SkyAlign system is exceptionally easy to set up and use as night comes
    on. You don't have to guess which stars are brightest, as only the brightest will
    be visible in the early evening. The same holds true for observers from a light-polluted
    suburban site, where only the brightest stars are visible to the unaided eye.

        Once the scope has aligned itself with the sky, it takes only a few
    keystrokes on the computer hand control to have the scope move automatically to
    your night's first observing target and start tracking it so you can observe at
    your leisure. You can find hundreds of fascinating deep space objects your first
    night out, even if you have never used a telescope before. No matter what level
    of experience you start from, your NexStar SkyAlign scope will unfold all
    the wonders of the Universe for you, your family, and your friends.

        If you're using an optional equatorial wedge to polar align the scope
    for long exposure astrophotography, two polar alignment programs in the scope's
    computer (one for the Northern hemisphere and one for the Southern hemisphere) make
    quick work of accurate alignment on the appropriate celestial pole. SkyAlign
    does not work in the equatorial mode.

        Several different alignment methods are built into the NexStar computer
    in addition to SkyAlign, allowing you to choose a level of computer accuracy
    in automatically finding objects with which you are comfortable. Both the Auto Two-Star
    "quick align" procedure and two accurate three star alignment methods (one computer-guided)
    are easily accomplished in only a few short minutes. You can be observing in less
    than 10 minutes after you first take the scope outdoors, including telescope set-up
    time.

        For example, if you're familiar with the sky, you can use the new Auto
    Two-Star Align method. Enter the date, time, and the latitude and longitude of your
    observing location into the hand control. If you don't know your latitude and longitude
    or can't determine them from the grid lines on your state's road map, you can use
    the coordinates of the nearest city from the list of hundreds in the instruction
    manual. The scope will keep up to ten observing locations stored in its memory (backyard,
    vacation home, favorite dark sky site, etc.), so you only have to enter the latitude
    and longitude once. Next, align the scope manually on a single bright star from
    a list of 40 in its memory. The scope will then automatically choose and slew to
    a second alignment star. Check to be sure the second star is centered in the telescope
    eyepiece and that's it. You've aligned the scope on the sky, ready for a night's
    go-to observing.

        In addition, the NexStar computer hand control is GPS-compatible (using
    an optional inexpensive CN16 GPS module) for full GPS (Global Positioning System)
    satellite accuracy. Adding GPS to the computer is something no competitive scope
    can do. Once the scope is approximately polar aligned, the 16-channel CN16 GPS system
    uses signals from government satellites to calculate the scope's location on earth
    with an accuracy measured in meters. The system also calculates the current time
    based on the split second accuracy of the GPS time signals. After the CN16 quickly
    completes these calculations and enters the information into the computer control
    for you automatically, the computer then orients the scope with the sky, slews to
    a pair of guide stars, asks you to confirm that the stars are in the center of the
    field (and center them if they're not precisely aligned), and then starts finding
    and tracking over 45,000 objects for you at your command. With the NexStar go-to
    mount and the CN16, orienting the scope in time and space on earth and aligning
    the scope on the sky becomes almost as easy a task as simply turning the scope on.

        You can click on the link below to download a brief RealPlayer movie
    showing how quick and easy it is to line up your scope on the sky with SkyAlign.
    There is also a link to download RealPlayer for free if your PC does not already
    have the program.



  • NexStar computer with SkyAlign

        The NexStar computer hand control has a built-in database of more
    than 40,000 stars, deep space objects, and solar system objects it can locate for
    you. The computer's memory contains the following objects:

    • the entire RNGC (Revised New General Catalog) of 7840 nebulas, galaxies, and star
      clusters

    • the IC (Index Catalog) of 5386 nebulas, galaxies, and star clusters
    • the Messier Catalog of the 110 best known deep sky objects
    • the Caldwell Catalog of 109 fascinating objects that Messier missed
    • 20 famous asterisms
    • the Abell Catalog of 2712 galaxy clusters
    • 25 selected CCD imaging objects

    • 29,500 selected SAO stars, including variable stars and multiple star systems.

        Also included are the eight major planets out to Pluto, as well as
    the Moon, for a total database more than 45,000 stars and objects. It's enough fascinating
    objects to keep you busy observing for the rest of your life.

        You can also store and edit the right ascension and declination of
    up to 400 objects of your own choosing, such as the comet and asteroid coordinates
    published monthly in Astronomy and Sky & Telescope magazines. The
    computer control can quickly find any of those objects at your command, and track
    them with high accuracy for visual observing or casual astrophotography.

        A review in Sky & Telescope magazine commented, "To quantify
    the Go To pointing accuracy, I spent several nights slewing to 50 objects selected
    from the NexStar's database. About one-third of them ended up dead center in the
    field, another third landed within ½° of the center, and the remaining third were
    within 1° of the center."

        All of the database and scope operation information is displayed on
    a double line, 16-character, red-illuminated liquid crystal display on the hand
    control. This display leads you through the steps necessary to line up the scope
    on the sky, locate objects, control scope functions like the brightness of the hand
    control display, and much more. It shows you basic information about the object
    being viewed (such as the object's name, catalog designation, type, magnitude, and
    so forth). In addition to this basic information, there is enhanced information
    on over 200 of the most note-worthy objects. When it's not displaying menus or object
    information, the display also shows you the constantly updated right ascension and
    declination coordinates at which the scope is aimed.

        The Sky & Telescope review said, "After using several NexStar-equipped
    telescopes in recent years, I can attest to the quality of the software and hardware
    for Celestron's Go To system. The package is reliable and offers quick access to
    an excellent array of databases. I especially like Celestron's Tour mode, which
    steps a user through an eclectic choice of deep-sky objects, quirky asterisms, and
    fine double stars, the latter being a class of objects great for urban observing
    that many Go To systems ignore. Using NexStar scopes, I've been introduced to many
    fine double stars."

        There are 19 fiber optic backlit LED buttons that glow a soft red in
    the dark to make it easy for you to control the computer without affecting your
    dark-adapted vision. An RS-232 communication port on the hand control allows you
    to operate the telescope remotely via a personal computer, using the supplied RS-232
    cable and CD-ROM that contains Celestron's NexRemote control software program.

        NexRemote provides an on-screen image of the computer hand control
    with full control of all the hand control functions from your computer keyboard.
    In addition to emulating the NexStar hand control, NexRemote adds powerful new features
    that let you keep your eyes on the stars instead of the hand control. It provides
    talking computer speech support using your computer's built-in speaker; lets you
    control the objects you want to see and the order in which you see them; lets you
    create and save custom sky tours; lets you take wireless control of the telescope
    with optional gamepad support; lets you connect your personal GPS device to the
    NexRemote; downloads NexRemote updates online to use the latest features; lets you
    download software upgrades to your NexStar computer at no charge from Celestron's
    website via the Internet; lets you use third-party planetarium programs to control
    the scope; and more.

        The Sky & Telescope review said, "The author tried Windows and
    Mac programs, including Desktop Universe, ECU, MegaStar, SkyMap Pro, Starry Night,
    and TheSky, and all controlled the mount without any problems." The telescope
    comes with a CD-ROM of TheSky Level 1 planetarium and star charting software. This
    Windows-based program will let explore the Universe on your PC and print out custom
    star charts of the sky to help you find faint objects that are not in the scope
    computer's database.

        A high precision pointing subroutine ("precise go-to") in the computer
    lets you point accurately at objects that you want to photograph that are too dim
    to be seen though the scope. Built-in programmable permanent periodic error correction
    allows sharper astrophotographic images, with fewer guiding corrections needed during
    long exposure photos through scopes with enough aperture to make such imaging practicable.
    Built-in adjustable backlash compensation permits precise corrections during astrophotography
    and when observing visually at high powers.

        The operation of the NexStar with SkyAlign is simplicity itself. You
    don't have to level the scope or point it north with SkyAlign, or even know
    Polaris from the Pleiades. After turning on the scope, enter the date and time and
    your location. The scope's computer will remember up to ten different observing
    sites for you to choose from, and will automatically default to your last observing
    site (very helpful if you invariably observe from one location, such as your back
    yard). Then, simply point the scope at any three bright stars, or at two bright
    stars and a planet or the Moon (you don't even have to know which stars and planet
    you're looking at, and you don't have to know and locate specific stars as you do
    with other alignment programs). Using the scope's hand control, center the stars
    in the finderscope crosshairs.

        The NexStar SkyAlign computer system automatically determines
    which objects were chosen and generates an internal map of the sky that it uses
    to guide its automatic moves to any star or object you select for the rest of the
    night. It does it by calculating the angles and distances between the objects you've
    chosen and compares them to the known separations between objects. Using this method,
    the telescope determines what objects were chosen. The display tells you which three
    objects you aligned to for confirmation.

        Only two of the alignment objects will actually be used for calculating
    the model of the sky that the computer uses for locating objects. The third object
    simply provides a positive identification of the other two. Therefore, at least
    two of the three alignment objects should be spaced at least 60 degrees apart in
    the sky if possible, and the third object should not fall in a straight line between
    the first two alignment stars.

        Since the brightest stars appear first as the sky darkens at dusk,
    the SkyAlign system is exceptionally easy to set up and use as night comes
    on. You don't have to guess which stars are brightest, as only the brightest will
    be visible in the early evening. The same holds true for observers from a light-polluted
    suburban site, where only the brightest stars are visible to the unaided eye.

        Several additional alignment methods are built into the NexStar computer
    - auto two-star alignment, manual two-star alignment, solar system alignment for
    daytime observing, and a one-star manual alignment - allowing you to choose a level
    of computer accuracy in automatically finding objects with which you are comfortable.
    If you're more familiar with the sky, you can use the new Auto Two-Star Align method.
    Enter the date, time, and the latitude and longitude of your observing location
    into the hand control. If you don't know your latitude and longitude or can't determine
    them from the grid lines on your state's road map, you can use the coordinates of
    the nearest city from the list of hundreds in the instruction manual. The scope
    will keep up to ten observing locations stored in its memory (backyard, vacation
    home, favorite dark sky site, etc.), so you only have to enter the latitude and
    longitude once.

        Next, align the scope manually on a single bright star from a list
    of 40 in its memory. The NexStar will then automatically choose and slew to a second
    alignment star. Check to be sure the second star is centered in the telescope eyepiece
    and that's it. You've aligned the scope on the sky, ready for a night's go-to observing.

        In addition to moving the scope to any of the 45,000 objects in its
    memory and tracking the object while you observe, the computer is loaded with useful
    features. It has user-defined slew limits, which prevent the scope from moving to
    objects below any horizon that you define. That makes it ideal for observing locations
    that have the normal horizon view blocked by houses or trees. The computer has a
    hibernate mode that lets you power down the scope without losing your astronomical
    alignment. This feature allows you to find planets in the daytime after aligning
    the scope the night before. The computer has a wedge align program that helps aligns
    the scope on the celestial pole when you're using a tripod and wedge for long exposure
    astrophotography.

        Once the scope has aligned itself with the sky, it takes only a few
    keystrokes on the computer hand control to have the scope move automatically to
    your night's first observing target and start tracking it so you can observe at
    your leisure. You can find hundreds of fascinating deep space objects your first
    night out, even if you have never used a telescope before. No matter what level
    of experience you start from, your NexStar SkyAlign scope will unfold all
    the wonders of the Universe for you, your family, and your friends.

        If you're using an optional equatorial wedge to polar align the scope
    for long exposure astrophotography, two polar alignment programs in the scope's
    computer (one for the Northern hemisphere and one for the Southern hemisphere) make
    quick work of accurate alignment on the appropriate celestial pole. SkyAlign
    does not work in the equatorial mode.

        You can click on the link below to download a brief RealPlayer movie
    showing how quick and easy it is to line up your scope on the sky with SkyAlign.
    There is also a link to download RealPlayer for free if your PC does not already
    have the program.



  • 5" Starbright XLT optics

    Starbright XLT multicoated optics: This advanced optical coatings package includes high reflectivity mirrors coated with multiple layers of vacuum-deposited aluminum. The mirror coatings are enhanced with titanium dioxide for maximum reflectivity and overcoated with a protective layer of silicon monoxide (quartz) for long life.

    A unique combination of magnesium fluoride and hafnium dioxide antireflection coatings is vacuum-deposited on both sides of the Schmidt corrector lens for maximum light throughput and contrast. The corrector lens itself is made of high transmission water white float glass instead of the conventional soda lime glass (which has 3.5% lower transmission) used in other telescopes.

    The Starbright XLT multicoatings give you higher light transmission for brighter deep space images and shorter exposure times during CCD and 35mm photography. Across the total visual/photographic spectrum from 400nm to 750nm, independent laboratory tests show the new Starbright XLT coatings are 16% brighter overall than even the original industry-standard Starbright multicoatings. They also visibly increase the contrast on subtle lunar, planetary, and nebula details when compared with a scope with standard multicoatings.

    NASA, and your tax dollars, can afford to purchase any optics in the world for use on the Space Shuttle. In the face of such very stiff competition, it is interesting to note that Celestron 5" Schmidt-Cassegrain optics have been chosen by NASA for scientific use on several Space Shuttle flights, proving that Celestron's 5" SCT optical performance is unmatched on Earth and in space.

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