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Celestron CGEM II 1100 SCT

SKU CEL-12012
Original price CA$5,976.00 - Original price CA$5,976.00
Original price
CA$5,976.00
CA$5,976.00 - CA$5,976.00
Current price CA$5,976.00
Price Match Policy!
  • 11-inch (279.4mm) Schmidt-Cassegrain Optical Tube
  • 40 lb (18 kg) Instrument Payload Capacity
  • CGEM II Computerized Equatorial Mount
  • StarBright XLT Optical Coatings
  • 0.42 Arc Second Dawes Resolution
  • NexStar+ Hand Control with 40,000+ Object Database
  • All-Star Polar Alignment and Permanent Periodic Error Correction (PEC)
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Framing Simulator
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See exactly how your targets fit with the Celestron CGEM II 1100 SCT, on real sky survey data.

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Preview your eyepiece's FOV

See exactly what the Celestron CGEM II 1100 SCT shows you, on real sky survey data.

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  • Description
  • FAQ
  • Specifications
  • In the Box
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  • Celestron CGEM II 1100 SCT

    The Celestron CGEM II 1100 pairs a 279.4mm (11") f/10 Schmidt-Cassegrain with StarBright XLT coatings and the CGEM II computerized equatorial mount. With the tube weighing only 27.5 lbs, it is still portable enough to be taken to dark skies, with 89% more light gathering power than an 8" telescope and more than 40% more than the 9.25". The tube gathers 1593 times more light than the eye and resolves 0.42 arc seconds (Dawes); the mount carries 40 lbs, and the complete kit weighs 105.5 lbs.

    11" Schmidt-Cassegrain Optics: 2800mm at f/10

    The telescope is especially at home as a solid platform for long exposure photography with optional cameras. The C11 provides excellent, high-contrast views and can perform at very high magnifications. The aluminum tube is 610mm (24") long and 312.42mm (12.3") in diameter, weighs 27.5 lbs (12.4 kg) and mounts with its CGE dovetail bar.

    The 279.4mm aperture and 2800mm focal length give 1593x the light gathering power of the eye, a limiting stellar magnitude of 14.7 and a resolution of 0.5 arc seconds (Rayleigh) or 0.42 arc seconds (Dawes). The secondary obstruction is 34% by diameter and 12% by area.

    The included 40mm eyepiece gives 70x; the highest useful magnification is 660x and the lowest is 40x. A 9x50 finderscope and a 1.25" star diagonal are included.

    StarBright XLT Coatings, Focusing and Collimation

    StarBright XLT is Celestron's coating system, built from three parts: enhanced multi-layer mirror coatings of aluminum, SiO2 and TiO2, with reflectivity fairly flat across the spectrum for both imaging and visual use; multi-layer anti-reflective coatings of magnesium fluoride and hafnium dioxide; and water white glass instead of soda lime glass for the corrector. Water white glass transmits about 90.5% of light uncoated, 3.5% more than soda lime glass, and reaches an average transmission of 97.4% with the StarBright XLT anti-reflective coatings. These coatings let you discern subtle details while viewing the Moon and planets as well as faint galaxies and nebulae.

    Focusing moves the primary mirror, which slides on the primary baffle tube; the focus knob sits on the rear cell just below the star diagonal, and it takes about 30 turns to go from close focus to infinity. Make the final focus turn counterclockwise so the mirror moves against gravity, which minimizes any mirror shift, and start on a bright object such as the Moon or a planet, since out-of-focus stars are very diffuse.

    Celestron collimates every telescope at the factory and checks it before shipping. If it is jarred in transport, you can adjust the tilt of the secondary mirror with the three collimation screws on the secondary housing, the only adjustment available to the user. To check, defocus a star at least 20 degrees above the horizon with a high-power eyepiece: the dark shadow of the secondary should sit centered in the bright rings on both sides of focus. If you are unsure whether it needs adjustment, it is likely fine and best left alone. Before checking collimation, let the telescope reach thermal equilibrium with its surroundings, allowing 45 minutes if you move it between large temperature extremes, such as from a heated house into the cold night air.

    The CGEM II Mount: 40 lb Payload and Permanent PEC

    The CGEM II is a fresh update to the venerable CGEM mount, capable of carrying Celestron's higher-end SCT optical tubes, up to 11", securely and vibration free, for both imaging and visual observing. The CGEM II carries 40 lbs. Its features include high-torque motors to smoothly drive heavier loads, low-cog DC servo motors, permanently programmable periodic error correction (PPEC), a dedicated autoguider port, large, easy-to-access polar alignment knobs and an ergonomic design that disassembles into compact, portable pieces. The latitude range is 15° to 70°, and the mount slews at nine speeds, tracking at sidereal, solar and lunar rates.

    Celestron designed the CGEM II to be ergonomically friendly, with large altitude and azimuth adjustment knobs for quick and easy polar alignment, and internal R.A. and DEC motor wiring for a clean look and an easy, trouble-free setup. The saddle connects directly to both CG-5 and CGE dovetail bars.

    To balance in R.A., loosen the R.A. lock lever with the counterweight bar horizontal and move the counterweight until the telescope stays put; in Dec, loosen the DEC clutch with the tube level and slide the tube in the saddle. Celestron's tip for imaging is a very slight imbalance, toward the counterweight side when the tube is west of the mount and toward the tube when it is east, so the worm gear always pushes against a slight load.

    Tripod, Polar Alignment and All-Star

    The steel tripod has 2" (50.8mm) legs with graduated markings on the lower section and weighs 20 lbs (9 kg); with the mount, the height range is 1346mm to 1651mm (53" to 65"). The equatorial head weighs 40 lbs (18.14 kg). This kit includes two 17 lb counterweights.

    Polar alignment is done not by moving the telescope in R.A. or Dec but with the mount's altitude and azimuth adjustments; both azimuth knobs push against the alignment peg on the tripod head, so you may have to loosen one while tightening the other. A bubble level built into the mount helps you level the tripod.

    All-Star Polar Alignment lets you polar align accurately using any bright star, even when the celestial pole cannot be seen. After a two-star alignment with at least one calibration star, you slew to a bright star from the Named Star list, ideally high in the sky and near the meridian, and choose Polar Align, then Align Mount. The mount syncs on the star and slews to where it should be if accurately polar aligned, and you center it with the mount's latitude and azimuth adjustments, not the hand control's direction buttons.

    NexStar+ Hand Control and Software

    The NexStar+ hand control has a 2 line, 18 character backlit LCD and 19 LED backlit buttons, and its database holds over 40,000 objects, 100 user defined programmable objects and enhanced information on over 200 objects. New observers can start with the built-in Sky Tour, which finds the most interesting objects in the sky and slews to each one.

    The mount slews at 9 speeds up to 4.5° per second and tracks at sidereal, solar and lunar rates in EQ North and EQ South modes. Alignment procedures are 2-Star, 1-Star, Solar System, Last Alignment and Quick Align; after a two-star alignment you can add calibration stars to improve pointing accuracy.

    The hand control's USB port connects to a computer for point-and-click slewing from software and for firmware updates; updating the hand control with Celestron Firmware Manager may resolve some problems. The mount's software is Starry Night Special Edition and the SkyPortal app.

    Imaging: Permanent PEC, Autoguiding and Tracking Past the Meridian

    Periodic Error Correction improves tracking by reducing the amplitude of the worm errors. It works in three steps: the mount indexes its worm gear, you guide with an autoguider for at least 10 minutes (one full worm revolution) while it records your corrections, and then you play them back. The mount retains the recording, and PEC is for advanced astrophotography and still needs careful guiding.

    The CGEM II tracks well past the meridian for uninterrupted imaging through the best part of the sky. The R.A. slew limits can be set anywhere from 40° above level to 20° below, so the mount can keep tracking past the meridian without flipping, or stop before an imaging cable runs out of length, and the Meridian setting (Favor Current, Favor West, Favor East or Disable) chooses which side of the mount the tube stays on.

    The mount has a hand control port, one AUX port for optional accessories and a dedicated autoguider port on its electronics panel. Built-in calibration routines compensate for the mechanical variation found in every German equatorial mount; they are worth running, and most need doing only once.

    The 11" tube is Fastar/HyperStar compatible: the secondary mirror can be removed and replaced with a lens assembly, sold separately and not included, so that a camera works at the f/2 focus of the primary mirror at the front of the telescope. At f/2, exposures are about 25 times shorter than at f/10, with a field of view 5 times larger and the object 1/5 the size. The secondary mirror should never be removed except to install the Fastar lens assembly. The optional Celestron Reducer/Corrector f/6.3 is the matching reducer for this tube.

    Power

    Power is 12V DC at 3.2 amps. The supplied car battery adapter plugs into a car's cigarette lighter outlet or a portable power supply, or you can use one of Celestron's optional AC to DC adapters; use only adapters Celestron supplies, as others may damage the electronics and void the warranty.

  • What magnification does the included eyepiece give?

    The 40mm eyepiece gives 70x (2800mm / 40mm). The highest useful magnification is 660x and the lowest is 40x.

    How do I keep the corrector clean?

    Dust on the corrector can be removed with a camel hair brush or pressurized air, then an optical cleaning solution and white tissue. Dew on the corrector can be cleared with a hair dryer on a low setting or by pointing the telescope at the ground until it evaporates. Internal cleaning and adjustments should be done only by Celestron's repair department.

    Does the telescope need collimating?

    Celestron collimates every telescope at the factory and checks it before shipping. If it is jarred in transport, you can adjust the tilt of the secondary mirror with the three collimation screws on the secondary housing, the only adjustment available to the user. To check, defocus a star at least 20 degrees above the horizon with a high-power eyepiece: the dark shadow of the secondary should sit centered in the bright rings on both sides of focus. If you are unsure whether it needs adjustment, it is likely fine and best left alone.

    Is the 11" tube Fastar compatible?

    The 11" tube is Fastar/HyperStar compatible: the secondary mirror can be removed and replaced with a lens assembly, sold separately and not included, so that a camera works at the f/2 focus of the primary mirror at the front of the telescope. Celestron's SCT manual says f/2 needs exposures about 25 times shorter than f/10, with a field of view 5 times larger and the object 1/5 the size. The secondary mirror should never be removed except to install the Fastar lens assembly.

    Can I polar align the CGEM II if I can't see the celestial pole?

    Yes. All-Star Polar Alignment lets you polar align accurately using any bright star, even when the celestial pole cannot be seen. After a two-star alignment with at least one calibration star, you slew to a bright star from the Named Star list, ideally high in the sky and near the meridian, and choose Polar Align, then Align Mount. The mount syncs on the star and slews to where it should be if accurately polar aligned, and you center it with the mount's latitude and azimuth adjustments, not the hand control's direction buttons.

    How does Permanent PEC work?

    Periodic Error Correction improves tracking by reducing the amplitude of the worm errors. It works in three steps: the mount indexes its worm gear, you guide with an autoguider for at least 10 minutes (one full worm revolution) while it records your corrections, and then you play them back. The mount retains the recording, and PEC is for advanced astrophotography and still needs careful guiding.

    Will the CGEM II track past the meridian?

    The CGEM II tracks well past the meridian for uninterrupted imaging through the best part of the sky. The R.A. slew limits can be set anywhere from 40° above level to 20° below, so the mount can keep tracking past the meridian without flipping, or stop before an imaging cable runs out of length, and the Meridian setting (Favor Current, Favor West, Favor East or Disable) chooses which side of the mount the tube stays on.

    How do I balance the telescope on the CGEM II?

    To balance in R.A., loosen the R.A. lock lever with the counterweight bar horizontal and move the counterweight until the telescope stays put; in Dec, loosen the DEC clutch with the tube level and slide the tube in the saddle. Celestron's tip for imaging is a very slight imbalance, toward the counterweight side when the tube is west of the mount and toward the tube when it is east, so the worm gear always pushes against a slight load.

    What power does the CGEM II need?

    Power is 12V DC at 3.2 amps. The supplied car battery adapter plugs into a car's cigarette lighter outlet or a portable power supply, or you can use one of Celestron's optional AC to DC adapters; use only adapters Celestron supplies, as others may damage the electronics and void the warranty.

    Can I control the CGEM II from a computer?

    The hand control's USB port connects to a computer for point-and-click slewing from software and for firmware updates; updating the hand control with Celestron Firmware Manager may resolve some problems. The mount's software is Starry Night Special Edition and the SkyPortal app.

  • Optical Design Schmidt-Cassegrain
    Aperture 279.4mm (11")
    Focal Length 2800mm (110")
    Focal Ratio f/10
    Optical Coatings StarBright XLT
    Finderscope 9x50
    Star Diagonal 1.25" Star Diagonal
    Included Eyepiece 40mm (70x Magnification)
    Highest Useful Magnification 660x
    Lowest Useful Magnification 40x
    Limiting Stellar Magnitude 14.7
    Resolution (Rayleigh) 0.5 arc seconds
    Resolution (Dawes) 0.42 arc seconds
    Light Gathering Power 1593x (Compared to human eye)
    Secondary Mirror Obstruction 34% by Diameter, 12% by Area
    Optical Tube Length 610mm (24")
    Optical Tube Weight 27.5 lbs (12.4 kg)
    Dovetail CGE Dovetail Bar
    Mount Type Computerized Equatorial
    Instrument Load Capacity 40 lbs (18 kg)
    Motor Drive DC servo motors
    Slew Speeds 9 speeds, max 4.5°/second
    Tracking Rates Sidereal, Solar and Lunar
    Tracking Modes EQ North & EQ South
    Alignment Procedures 2-Star, 1-Star, Solar System, Last, Quick
    Periodic Error Correction Yes
    Dovetail Compatibility Dual saddle (CG-5 and CGE)
    Tripod 2" Steel Legs with graduated markings
    Latitude Adjustment Range 15° - 70°
    Power Requirements 12V DC, 3.2 amps
    Hand Control NexStar+, USB Port for PC connection
    Database 40,000+ objects
    Autoguide Port Yes
    Auxiliary Ports 2 (1 for Hand Control, 1 for accessories)
    Mount Head Weight 40 lbs (18.14 kg)
    Tripod Weight 20 lbs (9.07 kg)
    Counterweights 2 x 17 lbs
    Total Kit Weight 105.5 lbs (47.8 kg)
    Tube outer diameter 312.42mm (12.3")
    Focuser type Moving primary mirror
    Matching flattener / reducer Celestron Reducer/Corrector f/6.3
    • 11" Schmidt-Cassegrain OTA

      × 1

    • CGEM II Equatorial Head

      × 1

    • Tripod with Accessory Tray

      × 1

    • 17 lb Counterweight

      × 2

    • NexStar+ Hand Control

      × 1

    • 9x50 Finderscope with Bracket

      × 1

    • 1.25" Star Diagonal

      × 1

    • 40mm Eyepiece (1.25")

      × 1

    • DC Power Cable

      × 1

  • Celestron 2-Year Telescope Warranty