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Bintel Glebe
Usually ready for pickup in 24 hours
Bintel 84 Wentworth park road, Glebe, 2073, NSW
Phone:(02) 9518 7255
Hours:
Monday9:30 am–5:30 pm
Tuesday9:30 am–5:30 pm
Wednesday9:30 am–5:30 pm
Thursday9:30 am–5:30 pm
Friday9:30 am–5:30 pm
Saturday9:30 am–4 pm
SundayClosed
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From $4,890.00
Hubble UL12 – 12" Lightweight Reflector Telescope
Hubble UP12 – An Ultra-Portable 12" Dobsonian Telescope
The Hubble UP12 is a premium 12-inch Dobsonian designed for observers who want serious optical performance in an exceptionally compact and travel-friendly form. Weighing just 14.5 kg) fully assembled, the UP12 delivers true large-aperture performance in a package that can be transported, stored, and deployed with ease.
Once disassembled, the UP12 can be packed into airline-approved luggage, making it one of the most portable 12-inch telescopes available. This is a genuine “take anywhere” instrument for dark-sky trips, remote expeditions, and observers who value performance without bulk.
Light, Compact and Truly Portable
The UP12 is less than half the weight of a traditional 12-inch Dobsonian. Its modular construction allows the entire system to be assembled in just a few minutes, with no heavy components and no complex setup.
All major structural elements are made from precision-machined aluminium alloy, providing excellent rigidity while keeping weight to an absolute minimum. The result is a telescope that feels effortless to transport, yet remains mechanically stable at high magnifications.
Optical Performance
The UP12 uses a premium parabolic primary mirror, individually tested and finished to achieve diffraction-limited performance (Strehl 0.95+). The secondary mirror is specified to 1/10 wave or better, delivering high contrast and sharp stellar images across the field.
Both mirrors receive 96% enhanced reflective coatings, maximising light throughput and reducing scatter. From a dark sky site, the UP12 is capable of revealing most NGC objects, subtle structure in bright nebulae, fine planetary detail on Jupiter and Saturn, and even challenging targets such as the Horsehead Nebula when used with appropriate filters.
A Perfect Balance of Power and Portability
The UP12 gathers around 44% more light than a 10-inch telescope, yet remains dramatically smaller and lighter than traditional 12-inch designs. Its full 12-inch optical surface (with a generous 12.4-inch overall diameter) provides slightly more true light-gathering area than many mass-produced 12-inch mirrors.
This balance makes the UP12 a telescope that actually gets used. It is large enough to deliver meaningful deep-sky performance, yet portable enough to be taken out frequently without hesitation.
Specs:
| Specification | Details |
|---|---|
| Optical design | Reflector |
| Optical diameter | 12" (304.8 mm) |
| Focal length | 1372 mm |
| Focal ratio | f/4.5 |
| Eyepiece height at zenith | ~1320 mm |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ for primary 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | Lightweight low-profile 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 60 mm |
| Secondary mirror obstruction by diameter | 19.7% |
| Secondary mirror obstruction by area | 3.9% |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws all aluminium alloy structure |
| Weight, fully assembled | ~14.5 kg |
| Dawes Limit | 0.38″ |
| Rayleigh Limit | 0.44″ |
| Limiting Magnitude | 14.9 |
| Maximum Magnification | 600× |
| Additional / optional accessories | Red-dot finder 8×50 Finder Tube Shroud Vinyl foam cushioned grips |
| Other features | Stainless steel cable sling lateral support and deluxe push-pull brass knob collimation screws |
From $21,190.00
Hubble UL24 – A Lightweight 24" Dobsonian Telescope
The Hubble UL24 is a made-to-order 24-inch Dobsonian telescope, designed for experienced observers who want truly extreme aperture without sacrificing transportability.
With a huge 24-inch primary mirror, the UL24 delivers around nine times the light grasp of an 8-inch telescope and four times that of a 12-inch, revealing ultra-faint galaxies, subtle nebular structure, and fine detail in planetary nebulae that smaller instruments simply cannot reach.
Light, Strong, and Surprisingly Portable
The UL24 features a precision-machined all-metal construction with eight rigid aluminium truss tubes and an extremely strong folding altitude bearing structure. Despite its massive aperture, the complete telescope weighs only around 70 kg, making it dramatically lighter than traditional 24-inch Dobsonians.
A real mirror box protects the primary mirror during transport, while the modular design allows the telescope to be broken down into manageable components for storage and travel. The heaviest single component is the primary mirror at around 30 kg, allowing one person to realistically transport the system to dark-sky locations.
Optical Performance
At the heart of the UL24 is a premium parabolic primary mirror with a full 24-inch optical surface and an overall diameter of 24.4 inches. This provides around 4% more true optical area than many other 24-inch designs that use undersized optical surfaces.
Each mirror is individually tested and finished to achieve diffraction-limited performance, with a Strehl ratio of 0.95+ for the primary and 1/10 wave or better for the secondary. Both mirrors receive 96% enhanced reflective coatings, maximising light throughput and contrast while reducing scatter.
The fast f/3.3 focal ratio keeps the eyepiece height to just 1955 mm at zenith, allowing most observers to use the telescope without a ladder while still enjoying extreme aperture.
Choose Your Telescope Control
The UL24 can be customised to suit your observing style. You can use it fully manually, or opt for Guided Push-To or Automatic Go-To systems.
Manual Mode
Even without electronics, the UL24 remains a highly refined Dobsonian with smooth, stable motion and precise balance. Manual observing delivers the classic deep-sky experience at a scale few observers ever reach.
Guided Push-To Version
The Guided Push-To version uses the SkyHub2 digital setting circle system, providing accurate real-time positioning without motorised tracking. High-resolution encoders on both axes feed live position data into compatible planetarium software.
Alignment is quick and intuitive using one- or two-star alignment. The system works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices.
Power consumption is extremely low, allowing up to 100 hours of operation from a standard USB power bank. Both WiFi and Bluetooth are supported.
Automatic Go-To Version
The Go-To version adds fully motorised pointing and tracking for hands-free observing. A smart hand controller with a 30,000-object database supports multi-star alignment for highly accurate pointing.
Built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking. The system can be controlled via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android.
Adjustable slew and guide speeds, spiral search, and park/unpark functionality ensure smooth, precise operation during long observing sessions.
| Optical design | Reflector |
|---|---|
| Optical diameter | 24" |
| Focal length | ~2012 mm |
| Focal ratio | f/3.3 |
| Eyepiece height at zenith | ~1955 mm |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality |
Diffraction limited++ (Strehl 0.95+ for primary, 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford |
| Secondary mirror | 127 mm |
| Secondary obstruction (diameter) | 20.80% |
| Secondary obstruction (area) | 4.30% |
| Mirror coatings |
96% Enhanced coating on primary and secondary mirrors |
| Tube material |
6063-T6 aluminium alloy tubes Aluminium alloy OTA & mount Steel mirror cell |
| Weight (optical tube) | ~61 kg |
| Weight (fully assembled) | ~70 kg |
| Dawes Limit | 0.19" |
| Rayleigh Limit | 0.23" |
| Limiting magnitude | 16.4 |
| Maximum magnification | 1200× |
| Optional accessories |
8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features |
Sling lateral support Deluxe push-pull brass knob collimation screws |
From $249.00
Shroud
Crafted from premium Nylon/Lycra blended materials, the Hubble Shroud is a must-have for any Dobsonian. It keeps stray light out, reduces thermal currents around the tube, and helps protect your optics during transport or storage. Free shipping is included when purchased with your telescope.
Mirror Cover
Protect your primary mirror with this durable, high-quality plastic cover. It fits snugly over the mirror cell to shield the optics from dust, debris, and accidental contact when the telescope is not in use.
Light Baffle
The Hubble Light Baffle reduces stray and scattered light, improving contrast and detail in your night sky views. Designed to integrate seamlessly with the telescope tube, it is an essential addition for observing faint deep-sky objects or working under bright skies.
Note: Telescope not included.
$48,290.00
Hubble UL32 – 32" Lightweight Reflector Telescope
The Hubble UL32sg is a flagship 32-inch Dobsonian telescope designed for serious deep-sky observers, research-grade visual work, and advanced EAA applications. With a massive 32-inch primary mirror, the UL32sg delivers 16 times the light grasp of an 8-inch telescope and four times that of a 16-inch, revealing galaxies, nebulae, and fine structure at a level few instruments on Earth can match.
Despite its extraordinary aperture, the UL32sg is engineered to remain as compact and transportable as possible for its class. Fully assembled, the telescope weighs around 150 kg and features a modular, all-metal construction with sectional truss tubes and a folding altitude bearing structure. A real mirror box provides safe protection for the primary mirror during transport and storage.
Light, Strong, Compact and Still Portable
The UL32sg is built using precision-machined aluminium alloy components, extensively modelled with CAD and FEA to optimise structural rigidity while minimising weight. Eight rigid sectional truss tubes ensure excellent stiffness and collimation stability, even at extreme elevations.
While the UL32sg is not a casual backyard instrument, it remains one of the most compact and practical 32-inch class telescopes available, capable of being transported and assembled by a small team for dark-sky expeditions, observatories, and research installations.
Revolutionary Smart Go-To System
The UL32sg is supplied exclusively in a Smart Go-To configuration, built around the state-of-the-art OnStep control system. This advanced platform combines fully motorised Go-To, high-resolution encoders, and a revolutionary plate-solving smart finder for unmatched pointing accuracy.
Using the system is simple: select a target via the smart hand controller or third-party software such as SkySafari or Stellarium, then with a single button press the telescope captures an image, plate-solves its position, and automatically refines its pointing until the target is perfectly centred.
The system supports automated star alignment, automated “Star Shows” such as Messier Marathons, intelligent routing to reduce slewing time by 30–50%, and full EAA live stacking for electronically assisted observing.
Connectivity includes built-in WiFi and Bluetooth, INDI and ASCOM drivers, real-time clock, spiral search, park/unpark, and full sidereal, lunar, and solar tracking rates. Control is available via smart hand controller, desktop software, or mobile apps on Windows, macOS, Linux, iOS, and Android.
Exclusive Sandwich Mirror Technology
The UL32sg uses a lightweight sandwich primary mirror designed to reach thermal equilibrium far faster than traditional solid mirrors. Rapid cooling dramatically reduces mirror seeing and internal turbulence, allowing the telescope to achieve its full optical potential much sooner in real-world conditions.
Unlike thick solid mirrors that may never stabilise during changing temperatures, the sandwich design delivers sharp, stable images without the need for active cooling systems, avoiding vibration and mechanical complexity.
Enhanced Optical Coatings
Both primary and secondary mirrors receive 96% enhanced dielectric coatings with multiple precision-controlled layers. These coatings maximise reflectivity, reduce scatter, and provide excellent chemical and mechanical durability, delivering bright, high-contrast images even at extreme magnifications.
Real Mirror Cell in a Real Mirror Box
The UL32sg features a fully engineered 27-point flotation mirror cell with sling and 90-degree pivoting lateral supports. This system prevents mirror deformation and eliminates astigmatism commonly caused by simpler collimation designs.
The independent three-point rod-end collimation system allows precise adjustment without stressing the mirror edge, maintaining optical integrity under all observing orientations.
Dual-Speed 2" Linear Bearing Crayford Focuser
The UL32sg is fitted with a precision 2-inch dual-speed linear bearing Crayford focuser, capable of handling heavy modern eyepieces and imaging equipment. The fine focus control provides ten times finer adjustment for critical focusing at high power or during EAA use, with approximately 50 mm of travel.
Specifications (UL16)
| Optical design | Reflector |
|---|---|
| Optical diameter | 32" (812.8 mm) |
| Focal length | ~2683 mm |
| Focal ratio | f/3.3 |
| Eyepiece height at zenith | ~2570 mm |
| Optics type | Parabolic |
| Control system | State-of-the-art OnStep Smart Go-To |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ for primary 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 180 mm |
| Secondary mirror obstruction by diameter | 22.1% |
| Secondary mirror obstruction by area | 4.9% |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Length of optical tube | ~2600 mm |
| Weight, optical tube | ~120 kg |
| Weight, fully assembled | ~150 kg |
| Connectivity | Built-in WiFi and Bluetooth |
| Power supply | Control: 12 VDC 2A Motors: 24 VDC 5A |
| Dawes Limit | 0.14″ |
| Rayleigh Limit | 0.17″ |
| Limiting Magnitude | 17.3 |
| Maximum Magnification | 1600× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | 27-point flotation mirror cell sling lateral support deluxe push-pull brass knob collimation screws |
From $4,890.00
Hubble UL14g – 14" Lightweight Reflector Telescope
The Hubble UL14g is a premium 14-inch Dobsonian telescope designed for serious visual observers who want substantial aperture in a system that remains genuinely portable. Combining advanced mirror technology with precision-machined construction, the UL14g delivers impressive deep-sky and planetary performance in a compact, travel-friendly design.
Optical Performance
At the heart of the UL14g is a full 14-inch parabolic primary mirror featuring Hubble’s exclusive Sandwich Mirror Technology. This lightweight yet rigid design achieves diffraction-limited performance (Strehl 0.95+) while reaching thermal equilibrium up to ten times faster than traditional solid mirrors. Faster cooldown means reduced mirror seeing and sharper, more stable views shortly after setup.
Both primary and secondary mirrors feature 96% enhanced reflective coatings, maximising light throughput and contrast while minimising scatter. This results in brighter galaxies, improved nebular structure, and high-contrast planetary detail even at high magnifications.
Engineered for Precision
The UL14g uses a real mirror box and precision flotation mirror support system to evenly distribute load across the primary mirror, minimising deformation and preserving optical accuracy across the sky. The structure is built from CNC-machined aluminium components with a steel mirror cell, providing excellent rigidity while remaining exceptionally lightweight.
Eight rigid truss tubes ensure stable collimation, while the large altitude bearings provide smooth and predictable motion during tracking.
Smooth, Accurate Focusing
The UL14g is equipped with a 2-inch dual-speed Crayford focuser with linear bearings, delivering smooth, backlash-free focusing. Fine focus control makes it easy to achieve critical focus at high power and supports heavy wide-field eyepieces without flex or slippage.
Big Aperture, Exceptional Portability
Despite its 14-inch aperture, the UL14g is remarkably easy to transport and set up. The modular truss-tube design breaks down into compact components that can be assembled in just a few minutes without tools. The heaviest single component is the primary mirror, weighing around 7 kg, making solo transport realistic for most observers.
With its fast f/4.6 focal ratio, the eyepiece height remains accessible at all times — just 60 inches at zenith — allowing comfortable observing with both feet on the ground.
Unmatched Observing Potential
The UL14g collects approximately 36% more light than a 12-inch telescope and nearly double that of a 10-inch, allowing significantly fainter objects and finer details to be resolved. From dense globular clusters to delicate dust lanes in distant galaxies, the UL14g reveals a level of structure that smaller instruments simply cannot match.
From dark-sky sites, most NGC objects are within reach. Bright emission nebulae show subtle hints of colour, planetary nebulae display internal structure, and Jupiter reveals fine banding and atmospheric detail. With an H-beta filter, even challenging targets like the Horsehead Nebula become achievable under good conditions.
The UL14g strikes a rare balance between serious aperture and true portability, making it a telescope that gets used often, not one that stays in storage.
Push-To and Go-To Options
Guided Push-To Version
The UL16 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time positioning without motorised tracking. High-resolution (8192 PPR) encoders on both axes continuously update your telescope’s position in compatible planetarium software.
Alignment is quick and intuitive using a one-star or optional two-star alignment. The system works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices. Power consumption is extremely low, allowing up to 100 hours of operation from a 15,000 mAh USB power bank. WiFi and Bluetooth are supported (WiFi only for iOS).
Automatic Go-To Version
The UL16 Go-To version adds fully motorised pointing and tracking with a smart hand controller featuring a 30,000-object database. Multi-star alignment (1–9 stars) ensures precise pointing accuracy, while built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking rates.
Control the system via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android. Adjustable slew and guide speeds, spiral search, and park/unpark functionality provide smooth, precise operation for extended observing sessions.
Specifications (UL14)
| Optical design | Reflector |
|---|---|
| Optical diameter | 355.6 mm (14") |
| Focal length | 1635 mm |
| Focal ratio | f/4.6 |
| Eyepiece height at zenith | 1525 mm (60") |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ primary 1/10 λ PV secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford |
| Secondary mirror size | 70 mm |
| Secondary mirror obstruction by diameter | 19.7% |
| Secondary mirror obstruction by area | 3.9% |
| Mirror coatings / over-coatings | 96% enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 aluminium alloy tubes aluminium alloy structure steel mirror cell |
| Length of optical tube | 1525 mm (60") |
| Weight, optical tube | 18.1 kg (40 lb) |
| Weight, fully assembled | 26.8 kg (59 lb) |
| Built-in WiFi | Yes |
| Power supply | 12–15 V DC 2A centre positive |
| Dawes limit | 0.33″ |
| Rayleigh limit | 0.38″ |
| Limiting magnitude | 15.2 |
| Maximum magnification | 700× |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
From $5,290.00
Hubble UL16 – 16" Lightweight Reflector Telescope
The Hubble UL16 is a made-to-order 16-inch Dobsonian telescope built for serious visual observers who want maximum aperture without sacrificing portability. Combining advanced mirror technology with precision engineering, the UL16 delivers exceptional deep-sky and planetary performance in a surprisingly manageable package.
Optical Performance
At the heart of the UL16 is a full 16-inch parabolic primary mirror featuring Hubble’s exclusive Sandwich Mirror Technology. This lightweight yet rigid design achieves diffraction-limited performance (Strehl 0.95+) while reaching thermal equilibrium up to ten times faster than traditional solid mirrors. Faster cooldown means reduced mirror seeing and sharper, steadier views sooner after setup.
Both primary and secondary mirrors feature 96% enhanced reflective coatings, maximising light throughput and contrast while minimising scatter. The result is brighter galaxies, improved nebular detail, and high-contrast planetary views even at high magnification.
Engineered for Precision
A carefully designed flotation mirror support system combined with independent collimation ensures the primary mirror is evenly supported, minimising astigmatism and maintaining optical accuracy across the sky. The UL16’s robust construction uses CNC-machined aluminium structural components and a steel mirror cell, providing excellent rigidity without unnecessary mass.
Smooth, Accurate Focusing
The UL16 is equipped with a 2-inch dual-speed Crayford focuser featuring linear bearings for smooth, backlash-free operation. Fine focus control allows precise adjustment at high magnifications and works seamlessly with heavy eyepieces or imaging accessories.
Big Aperture, Thoughtful Portability
Despite its impressive aperture, the UL16 is designed with transport in mind. The truss-tube construction breaks down easily for travel, while the fast focal ratios keep eyepiece height within a comfortable range. Whether observing from your backyard or transporting to dark skies, the UL16 balances power with practicality.
Unmatched Observing Potential
With significantly more light-gathering power than a 14-inch telescope, the UL16 reveals faint galaxies, subtle nebular structure, and fine planetary detail that smaller instruments simply cannot match. From resolving globular clusters to tracking delicate dust lanes in distant galaxies, the UL16 is built for observers who want to go deeper.
Push-To and Go-To Options
Guided Push-To Version
The UL16 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time positioning without motorised tracking. High-resolution (8192 PPR) encoders on both axes continuously update your telescope’s position in compatible planetarium software.
Alignment is quick and intuitive using a one-star or optional two-star alignment. The system works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices. Power consumption is extremely low, allowing up to 100 hours of operation from a 15,000 mAh USB power bank. WiFi and Bluetooth are supported (WiFi only for iOS).
Automatic Go-To Version
The UL16 Go-To version adds fully motorised pointing and tracking with a smart hand controller featuring a 30,000-object database. Multi-star alignment (1–9 stars) ensures precise pointing accuracy, while built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking rates.
Control the system via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android. Adjustable slew and guide speeds, spiral search, and park/unpark functionality provide smooth, precise operation for extended observing sessions.
Choosing Your Focal Ratio: f/5 or f/4.5
The UL16 is available in f/5.0 or f/4.5, allowing you to tailor the telescope to your observing style.
Why choose f/5?
-
Approximately 30% less coma than the f/4.5 version
-
No coma corrector required for most observers
-
Lower cost, saving around $500
-
Smaller central obstruction (2.76" secondary vs 3.1" on f/4.5)
-
Optimised for observers seeking the cleanest possible visual performance
Why choose f/4.5?
-
Lower eyepiece height, no ladder required for most users
-
Wider true field of view, ideal for large nebulae and star fields
-
Slightly more compact overall system
-
Coma is mild and often unnoticed by most observers without a corrector
Both focal ratios deliver outstanding views. The f/5 prioritises ultimate optical cleanliness, while the f/4.5 emphasises comfort and wide-field observing. Thanks to Hubble’s two-section truss design for f/5 (single-section for f/4.5), both versions remain equally portable and rigid.
Please note that counterweights are required for the f/5 configuration and are not included.
Specifications (UL16)
| Optical design | Reflector |
|---|---|
| Optical diameter | 16" (406.4 mm) |
| Focal length | 1829 mm (f/4.5) 2032 mm (f/5) |
| Focal ratio | f/4.5, f/5 |
| Eyepiece height at zenith | ~1690 mm (f/4.5) ~1890 mm (f/5) |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ for primary 1/10 λ PV for secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 80 mm (f/4.5), 70 mm (f/5) |
| Secondary mirror obstruction by diameter | 19.7% (f/4.5), 17.3% (f/5) |
| Secondary mirror obstruction by area | 3.9% (f/4.5), 3.0% (f/5) |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Weight, optical tube | ~25 kg |
| Weight, fully assembled | ~29.5 kg |
| Dawes Limit | 0.29″ |
| Rayleigh Limit | 0.33″ |
| Limiting Magnitude | 15.5 |
| Maximum Magnification | 800× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
From $8,090.00
Hubble UL18 – A Lightweight 18" Dobsonian Telescope
The Hubble UL18 is a made-to-order 18-inch Dobsonian telescope, built specifically for serious visual observers who want true observatory-class performance in a portable, transportable design.
With a massive 18-inch primary mirror, the UL18 gathers over five times more light than an 8-inch telescope, and more than twice the light grasp of a 12-inch, unlocking faint galaxies, delicate nebular structure, and extreme planetary detail that simply isn’t possible with smaller apertures.
Light, Strong, and Surprisingly Portable
Each UL18 is custom built to order using precision-machined all-metal components. The truss construction uses eight rigid aluminium truss tubes and a folding altitude bearing structure to provide exceptional stiffness while keeping overall weight under control.
The large mirror box design protects the primary mirror during transport, while the modular layout allows the telescope to be broken down quickly for storage or travel. Fully assembled, the UL18 weighs just ~33 kg, making it one of the most portable 18-inch class Dobsonians available.
Optical Performance
At the heart of the UL18 is a premium parabolic primary mirror, individually tested and finished to achieve diffraction-limited performance (Strehl 0.95+). The secondary mirror is specified to 1/10 wave or better, ensuring excellent contrast and pinpoint stellar images across the field.
Both mirrors receive 96% enhanced reflective coatings, maximising light throughput while reducing scatter. This results in brighter deep-sky views, improved low-contrast detail, and excellent planetary performance even at extreme magnifications.
Choose Your Telescope Control
The UL18 can be customised to suit your observing style. You can use it fully manually, or opt for Guided Push-To or Automatic Go-To systems.
Manual Mode
Even without electronics, the UL18 is a precision Dobsonian with smooth, stable bearings and an easy-to-use truss design. You can enjoy the classic hands-on experience, exploring the night sky exactly as the great visual observers have for decades.
Guided Push-To Version
The UL18 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time telescope positioning without motorised tracking. High-resolution 8192 PPR encoders on both axes continuously update your telescope’s position in compatible planetarium software.
-
Alignment is fast and intuitive using a simple one-star alignment, with optional two-star alignment for increased accuracy.
-
Works with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM-compatible software on Windows, macOS, Android, and iOS devices.
-
Extremely low power consumption: up to 100 hours from a 15,000 mAh USB power bank.
-
WiFi and Bluetooth supported (WiFi only for iOS devices).
Automatic Go-To Version
The UL18 Go-To version adds fully motorised pointing and tracking for a completely hands-free observing experience. It includes a smart hand controller with a 30,000-object database and supports advanced 1–9 star alignment for precise pointing accuracy.
-
Built-in encoders and a real-time clock maintain accurate sidereal, lunar, and solar tracking rates.
-
Control via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI-compatible software on Windows, macOS, Linux, iOS, or Android.
-
Adjustable slew and guide speeds, spiral search, and park/unpark functionality provide smooth, precise movement for extended observing sessions.
Choosing Your Focal Ratio: f/4.0 or f/4.5
The UL18 is available in f/4.0 or f/4.5, allowing you to prioritise either maximum comfort or maximum optical refinement.
Why choose f/4.0?
-
Lower eyepiece height – no ladder required for most users
-
More compact overall system
-
Wider true field of view
-
Ideal for observers who value comfort and portability
Why choose f/4.5?
-
Reduced coma across the field
-
Slightly smaller secondary obstruction
-
Better suited to high-power planetary and lunar observing
-
Preferred by observers seeking ultimate optical purity
Both versions deliver extraordinary performance. The f/4.0 favours ergonomic comfort and wide-field observing, while the f/4.5 favours optical cleanliness and contrast. The choice ultimately comes down to observing style and personal preference.
Specifications (UL18)
| Optical design | Reflector |
|---|---|
| Optical diameter | 18" (457.2 mm) |
| Focal length | ~1860 mm (f/4.0) ~2058 mm (f/4.5) |
| Focal ratio | f/4.0, f/4.5 |
| Eyepiece height at zenith | ~1730 mm (f/4.0) ~1930 mm (f/4.5) |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ primary 1/10 λ PV secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 90 mm (f/4.0), 80 mm (f/4.5) |
| Secondary mirror obstruction by diameter | 19.7% (f/4.0), 17.2% (f/4.5) |
| Secondary mirror obstruction by area | 3.9% (f/4.0), 3.0% (f/4.5) |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Length of optical tube | ~1830 mm (f/4.0) ~2010 mm (f/4.5) |
| Weight, optical tube | ~28 kg |
| Weight, fully assembled | ~33 kg |
| Dawes Limit | 0.25″ |
| Rayleigh Limit | 0.30″ |
| Limiting Magnitude | 15.8 |
| Maximum Magnification | 900× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
From $10,690.00
Hubble UL20 – A Lightweight 20" Dobsonian Telescope
The Hubble UL20 is a made-to-order 20-inch Dobsonian telescope designed for observers who want truly extreme aperture without the bulk and weight of traditional large Dobsonians.
With its enormous 20-inch primary mirror, the UL20 gathers over six times more light than an 8-inch telescope, and almost three times the light grasp of a 12-inch, revealing galaxies, nebulae, and fine structure at a level normally reserved for permanent observatory installations.
A Premium, Light, Compact and Portable Design
Despite its size, the UL20 is engineered to remain practical and transportable. The precision-machined all-metal truss construction delivers exceptional rigidity while keeping overall weight to around half that of traditional 20-inch Dobsonians.
The modular truss design allows the telescope to be broken down for transport, while the reinforced mirror box protects the primary mirror during storage and travel. This makes the UL20 a genuine “portable observatory” for dedicated deep-sky observers.
Optical Performance
At the heart of the UL20 is a premium parabolic primary mirror, individually tested and finished to achieve diffraction-limited performance (Strehl 0.95+). The secondary mirror is specified to 1/10 wave or better, ensuring excellent contrast and pinpoint stellar images across the field.
Both mirrors receive 96% enhanced reflective coatings, maximising light throughput while reducing scatter. This results in breathtaking deep-sky views, extremely faint object detection, and exceptional planetary performance even at very high magnifications.
Choose Your Telescope Control
The UL20 can be customised to suit your observing style. You can use it fully manually, or opt for Guided Push-To or Automatic Go-To systems.
Manual Mode
Even without electronics, the UL20 remains a precision Dobsonian with smooth, stable bearings and a well-balanced truss structure. This allows for classic hands-on observing with direct control and intuitive sky navigation.
Guided Push-To Version
The UL20 Guided Push-To version features the SkyHub2 digital setting circle system, providing accurate real-time telescope positioning without motorised tracking. High-resolution 8192 PPR encoders on both axes continuously update your telescope’s position in compatible planetarium software.
-
Fast one-star alignment, with optional two-star alignment for higher accuracy
-
Compatible with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM software
-
Works on Windows, macOS, Android, and iOS devices
-
Extremely low power consumption, up to 100 hours from a 15,000 mAh USB power bank
-
WiFi and Bluetooth supported (WiFi only for iOS devices)
Automatic Go-To Version
The UL20 Go-To version adds fully motorised pointing and tracking for a hands-free observing experience. It includes a smart hand controller with a 30,000-object database and supports advanced 1–9 star alignment for high pointing accuracy.
-
Built-in encoders and real-time clock maintain accurate sidereal, lunar, and solar tracking rates
-
Control via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI software
-
Compatible with Windows, macOS, Linux, iOS, and Android
-
Adjustable slew and guide speeds, spiral search, and park/unpark functionality
Choosing Your Focal Ratio: f/3.3, f/3.7 or f/4.2
The UL20 is available in three focal ratios, allowing you to balance comfort, optical performance, and field of view.
Why choose f/4.2?
-
Sharper images with almost 50% less coma than f/3.7
-
Smaller central obstruction (3.5" secondary vs 4.0" on f/3.7)
-
Easier to achieve perfect collimation
-
Better suited for high-magnification lunar and planetary observing
-
A coma corrector is helpful but not essential for many users
Why choose f/3.3 or f/3.7?
-
No ladder required at all for f/3.3; only a small step may be needed for f/4.2 near zenith
-
Extremely wide true field of view, especially with f/3.3
-
Ideal for sweeping large nebulae and rich Milky Way fields
All three versions deliver extraordinary performance. A coma corrector is strongly recommended for the UL20 f/3.3, while the f/4.2 prioritises optical cleanliness and ease of use.
Thanks to Hubble’s two-section truss design for f/4.2 (single-section for f/3.3 and f/3.7), all versions remain equally rigid and transportable. Please note that counterweights may be required for balance, depending on configuration, and are not included.
Specifications (UL20)
| Optical design | Reflector |
|---|---|
| Optical diameter | 20" (508 mm) |
| Focal length | ~1676 mm (f/3.3) ~1880 mm (f/3.7) ~2134 mm (f/4.2) |
| Focal ratio | f/3.3, f/3.7, f/4.2 |
| Eyepiece height at zenith | ~1490 mm (f/3.3) ~1745 mm (f/3.7) ~2000 mm (f/4.2) |
| Optics type | Parabolic |
| Eyepieces | Not included |
| Optical quality | Diffraction limited++ (Strehl 0.95+ primary 1/10 λ PV secondary) |
| Finder scope | Not included |
| Focuser | 2" dual-speed linear bearing Crayford (50.8 mm) |
| Secondary mirror | 100 mm (f/3.3 f/3.7) 90 mm (f/4.2) |
| Secondary mirror obstruction by diameter | 19.7% (f/3.3 f/3.7) 17.7% (f/4.2) |
| Secondary mirror obstruction by area | 3.9% (f/3.3 f/3.7) 3.1% (f/4.2) |
| Mirror coatings / over-coatings | 96% Enhanced coating on primary and secondary mirrors |
| Tube material | 6063-T6 Aluminium Alloy tubes with black zinc-plated steel knob screws aluminium alloy main structure (OTA and mount) and steel mirror cell |
| Length of optical tube | ~1850 mm (f/3.3 f/3.7) ~2110 mm (f/4.2) |
| Weight, optical tube | ~34.5 kg (f/3.3 f/3.7) ~35 kg (f/4.2) |
| Weight, fully assembled | ~40 kg (f/3.3 f/3.7) ~40.5 kg (f/4.2) |
| Dawes Limit | 0.19″ |
| Rayleigh Limit | 0.23″ |
| Limiting Magnitude | 16.4 |
| Maximum Magnification | 1200× |
| Additional / optional accessories | 8×50 Finder Tube Shroud Wheelbarrow handles Vinyl foam cushioned grips |
| Other features | Sling lateral support and deluxe push-pull brass knob collimation screws |
$95.00
四个 M6 螺纹可为您的设备提供刚性且无弯曲的连接。中央通用 ¼” UNC 螺纹可连接到三脚架头和其他兼容的 UNC 螺钉。包括两个不锈钢支撑支柱,以保护螺纹免受重载,确保其使用寿命。
显示连接到 StellarMate Pro 计算机。
包括:
- 两件式夹具
- 2x 支撑柱
- 1x 中心螺纹
- 1x 拇指旋钮
- 1x 6mm 六角扳手
- 4x M6x12mm 螺丝
$179.00
iOptron 5kg 配重块
用于 iOptron 支架的 5kg 配重。
此 CW 专为以下 iOptron 接口而设计:
- CEM70/CEM70EC/CEM70G
- CEM60/CEM60EC
- GEM45/GEM45EC/GEM45G
- CEM40/CEM40EC/CEM40G*(适用于配备 28 毫米 CW 轴的后期版本)
- iEQ45专业版
- 艾格45
订购之前,请检查您的 CEM40 安装 CW 轴直径。
它可以用于其他带有直径 28 毫米配重轴的支架。
iOptron CW 5kg 规格
重量:5kg
外径:148mm
孔径:28.5mm
高度:38毫米
锁定机制:锁定螺钉
锁紧螺钉螺纹尺寸:M8
$199.00
iOptron 球形云台采用高性能球形云台,可实现平稳精确的移动。可独立控制其平移和倾斜移动。底座直径为 2 英寸,可实现 360 度精确平移测量。快装板系统通用,可与所有主要品牌兼容。冗余板锁和安全锁可确保相机安全安装。
iOptron 球形云台特点
- 铝结构
- 带相机板的快速释放装置
- 3 个螺丝位置相机板
- 盘子尺寸:1.5 英寸 x 2.375 英寸表面
- 重量:0.875 磅
- 工作高度:3.875 英寸
- 360 度平移
- 头部倾斜:+/- 90 度
- 2 个水平仪
- 负载能力:20磅。
- 还包括 1/4"-20 / 3/8"-16 三脚架适配器
$7,999.00
艾普创 CEM120
全新 iOptron CEM120
支架设计的非凡创新...现在有了新的有效载荷!
认识到市场对准确、稳定、能够承载更大仪器和更复杂成像阵列的赤道仪的需求日益增长,我们发明了 iOptron CEM120。它具有我们革命性的“中心平衡”设计的优势:稳定性、准确性和顺畅的机械操作,同时能够承载高达 52 公斤的有效载荷。“中心平衡”设计的自然稳定性源于其将赤道仪连同有效载荷的重量直接集中在支柱或三脚架的中心。
CEM120 的性能体现在其低周期跟踪误差 ±3.5 弧秒。除了稳定性方面,CEM120 还具有先进的电缆管理系统,该系统由更多位置的更多端口组成,可防止电缆缠绕并降低电缆断裂的可能性。它还为 CEM 系列增加了一些新功能,例如用于远程操作的 Wi-Fi 和 LAN,以及两个轴上易于使用、可靠的离合器。
可选附加功能
可选的重型Tri-Pier 360和永久码头可供订购。
/产品/ioptron-tri-pier-360
可选的轻型有效载荷三柱适配器 ( 8036-120 ) 售价为 239 美元。可对其进行修改以用于永久性柱式安装。
特征
- 采用全新设计的中央平衡赤道仪 (CEM),可实现最大有效载荷和自然稳定性
- 天文台天文摄影支架非常适合视觉摄影师和天文摄影师
- 有效载荷 52 公斤,安装重量 26 公斤
- 易于使用且可靠的齿轮离合器
- 精确的高度和方位角调整。
- 精密步进电机,精度达 0.07 角秒,可实现精确 GOTO 和精确跟踪
- 为无法看见北极星的人提供极地校准程序
- Go2Nova® 8407 V2 控制器采用先进的 GOTONOVA® GOTO 技术,内置加热器
- 高精度跟踪,低周期误差(PE)<±3.5角秒
- 永久周期误差校正(PPEC)
- 32 通道全球定位系统 (GPS)
- 内置 WiFi 和 LAN,可进行远程操作
- 集成 ST-4 自动导航端口
- 先进的线缆管理系统,更多选择
- 弹簧式、可单独调节的 Losmandy 鞍座
工厂提供美国电源
规格
| 山 | 中心平衡赤道仪 (CEM) |
| 有效载荷 | 52kg ,不包括配重* |
| 安装重量 | 26公斤 |
| 有效载荷/安装重量比 | 2 |
| 材料 | 全金属 |
| 纬度调整范围 | 0°~ 68°(0.5 弧分格)** |
| 方位调整范围 | ± 5°(3 弧分格) |
| PE(通过编码器) | < ±3.5 角秒*** |
| 蠕虫期 | 240 秒 |
| 聚乙烯醇 | 太平洋石油公司 |
| 赤经蜗轮 | φ216mm、360齿、零背隙 |
| 偏角蜗轮 | φ216mm、360齿、零背隙 |
| 蠕虫 | φ26毫米 |
| 赤经轴 | φ80mm,钢 |
| 偏角轴 | φ80mm,钢 |
| 赤经方位 | φ125毫米 |
| 偏角轴承 | φ125毫米 |
| 配重轴 | φ38.1×540mm(不锈钢、防滑、4.5kg) |
| 配重 | 10公斤 |
| 安装底座尺寸 | 210 x 230 毫米 |
| 电机驱动 | 精密步进电机,128 微步 |
| 解决 | 0.07 角秒 |
| 回转速度 | 最大 4°/秒(960x) |
| 手持控制器 | Go2Nova® 8407 V2,8 行 21 个字符 LCD |
| 电源要求 | 直流 12V,5A |
| 功耗 | 0.7A(跟踪),1.8A(GOTO) |
| 极地望远镜 | 可选电子极轴镜 |
| 经络治疗 | 停止(0-14°通过),自动翻转 |
| 零位 | 自动零点搜索 |
| 驻车位置 | 水平、垂直、电流、高度/方位角输入 |
| 液位指示器 | 是的 |
| 燕尾鞍座 | 洛斯曼迪 D,17.2 英寸(437 毫米) |
| 全球定位系统 | 是的 |
| 导向口 | ST-4 |
| 通信端口 | RS232、USB、LAN、WiFi |
| 电缆管理 | 2xDC12V(1A)、DC5V(1A)、2xDC(5A)、ST4、6P6C、4xUSB2.0、USB3.0(供电)、USB 用于 PS、AUX |
| 墩座/三脚架 | 可选码头 |
| 保修单 | 两年有限 |
手册和说明
库存单位:7300
$10,749.00
全新 iOptron CEM120EC
支架设计的非凡创新...现在有了新的有效载荷!
认识到市场对准确、稳定、能够承载更大仪器和更复杂成像阵列的赤道仪的需求日益增长,我们发明了 iOptron CEM120EC。它具有我们革命性的“中心平衡”设计的优势:稳定性、准确性和顺畅的机械操作,同时能够承载高达 52 公斤的有效载荷。“中心平衡”设计的自然稳定性源于其将赤道仪连同有效载荷的重量直接集中在支柱或三脚架的中心。
CEM120EC 的性能体现在其低周期跟踪误差 <0.15 弧秒 RMS。除了稳定性方面,CEM120EC 还具有先进的电缆管理系统,该系统由更多位置的更多端口组成,可防止电缆缠绕并降低电缆断裂的可能性。它还为 CEM 系列增加了一些新功能,例如用于远程操作的 Wi-Fi 和 LAN,以及两个轴上易于使用、可靠的离合器。
可选附加功能
可选的重型Tri-Pier 360和永久码头可供订购。
/产品/ioptron-tri-pier-360
可选的轻型有效载荷三柱适配器 ( 8036-120 ) 售价为 239 美元。可对其进行修改以用于永久性柱式安装。
特征
- 采用全新设计的中央平衡赤道仪 (CEM),可实现最大有效载荷和自然稳定性
- 天文台天文摄影支架非常适合视觉摄影师和天文摄影师
- 有效载荷 52 公斤,安装重量 26 公斤
- 易于使用且可靠的齿轮离合器
- 精确的高度和方位角调整。
- 精密步进电机,精度达 0.07 角秒,可实现精确 GOTO 和精确跟踪
- 为无法看见北极星的人提供极地校准程序
- Go2Nova® 8407 V2 控制器采用先进的 GOTONOVA® GOTO 技术,内置加热器
- 高精度跟踪,低周期误差 (PE)<0.15 角秒 RMS
- 实时周期误差校正(RPEC)
- 32 通道全球定位系统 (GPS)
- 内置 WiFi 和 LAN,可进行远程操作
- 集成 ST-4 自动导航端口
- 先进的线缆管理系统,更多选择
- 弹簧式、可单独调节的 Losmandy 鞍座
规格
| 山 | 中心平衡赤道仪 (CEM) |
| 有效载荷 | 52kg ,不包括配重* |
| 安装重量 | 26公斤 |
| 有效载荷/安装重量比 | 2 |
| 材料 | 全金属 |
| 纬度调整范围 | 0°~ 68°(0.5 弧分格)** |
| 方位调整范围 | ± 5°(3 弧分格) |
| PE(通过编码器) | < 0.15 角秒 RMS*** |
| 蠕虫期 | 240 秒 |
| 聚乙烯醇 | 实时 PEC(RPEC) |
| 赤经蜗轮 | φ216mm、360齿、零背隙 |
| 偏角蜗轮 | φ216mm、360齿、零背隙 |
| 蠕虫 | φ26毫米 |
| 赤经轴 | φ80mm,钢 |
| 偏角轴 | φ80mm,钢 |
| 赤经方位 | φ125毫米 |
| 偏角轴承 | φ125毫米 |
| 配重轴 | φ38.1×540mm(不锈钢、防滑、4.5kg) |
| 配重 | 10公斤 |
| 安装底座尺寸 | 210 x 230 毫米 |
| 电机驱动 | 精密步进电机,128 微步 |
| 编码器分辨率 | 0.035 角秒 |
| 电机分辨率 | 0.07 角秒 |
| 回转速度 | 最大 4°/秒(960x) |
| 手持控制器 | Go2Nova® 8407 V2,8 行 21 个字符 LCD |
| 电源要求 | 直流 12V,5A |
| 功耗 | 0.7A(跟踪),1.8A(GOTO) |
| 极地观测镜 | 可选电子极轴镜 |
| 经络治疗 | 停止(0-14°通过),自动翻转 |
| 零位 | 自动零点搜索 |
| 驻车位置 | 水平、垂直、电流、高度/方位角输入 |
| 液位指示器 | 是的 |
| 燕尾鞍座 | 洛斯曼迪 D,17.2 英寸(437 毫米) |
| 全球定位系统 | 是的 |
| 导向口 | ST-4 |
| 通信端口 | RS232、USB、LAN、WiFi |
| 电缆管理 | 2xDC12V(1A)、DC5V(1A)、2xDC(5A)、ST4、6P6C、4xUSB2.0、USB3.0(供电)、USB 用于 PS、AUX |
| 墩座/三脚架 | 可选码头 |
| 保修单 | 两年有限 |
工厂提供美国电源
手册和说明
库存单位:7301
$12,999.00
全新 iOptron CEM120EC2
支架设计的非凡创新...现在有了新的有效载荷!
认识到市场对精确、稳定、能够灵活地承载大型仪器和更复杂成像阵列的赤道仪的需求日益增长,我们创造了 iOptron CEM120EC2。它具有我们革命性的“中心平衡”设计的优势:稳定性、准确性和流畅的机械操作,同时能够承载高达 52 公斤的有效载荷。“中心平衡”设计的自然稳定性源于它将赤道仪连同有效载荷的重量直接集中在支柱或三脚架的中心。除了稳定性方面,CEM120 还具有先进的电缆管理系统,该系统由更多位置的更多端口组成,可防止电缆缠绕并降低电缆断裂的可能性。它们还为 CEM 系列添加了一些新功能,例如用于远程操作的 Wi-Fi 和 LAN,以及两个轴上易于使用、可靠的离合器。
CEM120EC2 使用两个高分辨率编码器,每个轴一个。两个编码器使支架能够执行双轴跟踪。借助先进的天空建模,CEM120EC2 将能够考虑和调整极轴对准误差以及大气(折射)失真的变化。每个轴上的固定主传感器允许支架在断电后保存对准模型,以便在未来的夜晚使用。
可选附加功能
可选的重型Tri-Pier 360和永久码头可供订购。
/产品/ioptron-tri-pier-360
可选的轻型有效载荷三柱适配器 ( 8036-120 ) 售价为 239 美元。可对其进行修改以用于永久性柱式安装。
特征
- 采用全新设计的中央平衡赤道仪 (CEM),可实现最大有效载荷和自然稳定性
- 天文台天文摄影支架非常适合视觉摄影师和天文摄影师
- 有效载荷为 115 磅(52 千克),安装重量为 57 磅(26 千克)
- 易于使用且可靠的齿轮离合器
- 精确的高度和方位角调整。
- 精密步进电机,精度达 0.07 角秒,可实现精确 GOTO 和精确跟踪
- 为无法看见北极星的人提供极地校准程序
- Go2Nova® 8407 V2 控制器采用先进的 GOTONOVA® GOTO 技术,内置加热器
- RA 和 DEC 上均配备双高精度编码器
- 高精度跟踪,低周期误差 (PE)<0.15 角秒 RMS
- 实时周期误差校正(RPEC)
- 32 通道全球定位系统 (GPS)
- 内置 WiFi 和 LAN,可进行远程操作
- 集成 ST-4 自动导航端口
- 先进的线缆管理系统,更多选择
- 弹簧式、可单独调节的 Losmandy 鞍座
工厂提供美国电源
规格
| 山 | 中心平衡赤道仪 (CEM) |
| 有效载荷 | 52 公斤(115 磅),不包括配重* |
| 安装重量 | 26公斤(57磅) |
| 有效载荷/安装重量比 | 2 |
| 材料 | 全金属 |
| 纬度调整范围 | 0°~ 68°(0.5 弧分格)** |
| 方位调整范围 | ± 5°(3 弧分格) |
| PE(通过编码器) | < 0.15 角秒 RMS*** |
| 蠕虫期 | 240 秒 |
| 聚乙烯醇 | 实时 PEC(RPEC) |
| 赤经蜗轮 | φ216mm、360齿、零背隙 |
| 偏角蜗轮 | φ216mm、360齿、零背隙 |
| 蠕虫 | φ26毫米 |
| 赤经轴 | φ80mm,钢 |
| 偏角轴 | φ80mm,钢 |
| 赤经方位 | φ125毫米 |
| 偏角轴承 | φ125毫米 |
| 配重轴 | φ38.1×540mm(不锈钢、防滑、4.5kg) |
| 配重 | 10 公斤(22 磅) |
| 安装底座尺寸 | 210 x 230 毫米 |
| 电机驱动 | 精密步进电机,128 微步 |
| 编码器分辨率 | 0.035 角秒 |
| 电机分辨率 | 0.07 角秒 |
| 回转速度 | 最大 4°/秒(960x) |
| 手持控制器 | Go2Nova® 8407 V2,8 行 21 个字符 LCD |
| 电源要求 | 直流 12V,5A |
| 功耗 | 0.7A(跟踪),1.8A(GOTO) |
| 极地望远镜 | 可选电子极轴镜 |
| 经络治疗 | 停止(0-14°通过),自动翻转 |
| 零位 | 自动零点搜索 |
| 驻车位置 | 水平、垂直、电流、高度/方位角输入 |
| 液位指示器 | 是的 |
| 燕尾鞍座 | 洛斯曼迪 D,17.2 英寸(437 毫米) |
| 全球定位系统 | 是的 |
| 导向口 | ST-4 |
| 通信端口 | RS232、USB、LAN、WiFi |
| 电缆管理 | 2xDC12V(1A)、DC5V(1A)、2xDC(5A)、ST4、6P6C、4xUSB2.0、USB3.0(供电)、USB 用于 PS、AUX |
| 墩座/三脚架 | 可选码头 |
| 保修单 | 两年有限 |
手册和说明
库存单位:7302
$2,479.00
和前代产品一样,CEM26 在设计时也充分考虑了便携性,重量仅为 4.5 公斤,可支撑高达 12 公斤的有效载荷,安装重量与有效载荷之比高达 2.6。实现这种比率的关键在于 CEM 设计将安装和有效载荷的重量直接集中在三脚架的中心,从而实现“自然稳定性”。
在早期 CEM 型号的基础上,我们增加了一些功能,以提高便利性和实用性。正向锁定齿轮啮合系统(即使戴着手套也易于使用)、内置 Wi-Fi,实现无与伦比的连接性,以及可记录的永久周期性误差校正 (PPEC),以重复最佳的 PEC 训练课程。在功能方面,CEM26 提供精确的指向和准确的跟踪。CEM26 为紧凑型赤道仪树立了新标准。
中心平衡设计的支架将有效载荷的重量置于重心,从而实现更大的自然稳定性。其他功能包括可调节的配重杆,以防止三脚架受阻。由于极轴镜不受偏角轴阻挡,因此极轴校准快速且随时可用。
CEM26 配备了最新的先进 GOTONOVA® GOTO 技术,使其成为目前最强大、最准确的 GOTO 支架之一。其数据库包含超过 212,000 个物体。Go2Nova® 手动控制器使用直观,其大型 4 行 LCD 屏幕简化了设置望远镜和定位物体的过程。
CEM26A 支架配有集成电子极地寻星镜(称为 iPolar)。此工具可确保望远镜准确对准,即使北极星被遮挡。它配有 1.5 英寸重型不锈钢三脚架和铝制手提箱。
装运箱 #1:C262A-CEM26 头部,带 iPolar/盒子/托盘 (C262A)
装运箱#2:8281-CEM26/GEM28 1.5英寸三脚架(无托盘)(C26/G28 1.5T)
特征
- 独特的设计,中心平衡赤道仪 (CEM),可实现最大有效载荷和最小安装重量
- 非常适合视觉观察和天文摄影
- 低周期误差(< ± 10 角秒)
- 有效载荷为 12 公斤(26 磅),仅安装重量为 4.5 公斤(10 磅)
- CNC 加工和铸造的金属机身
- 弹簧加载齿轮系统
- 大型、易于使用的快速锁齿轮离合器
- 可调节配重轴,适合 0º 纬度操作
- 低功耗步进电机
- 集成 iOptron iPolar TM电子极轴镜
- 为无法看见北极星的人提供极地校准程序
- 采用先进 GOTONOVA® GOTO 技术的 Go2Nova® 8409 控制器
- 集成 ST-4 自动导航端口
- 内置 Wi-Fi
- USB 端口用于固件升级和计算机控制
- 标准1.5英寸重型不锈钢三脚架(5kg)
- 带附件托盘的压铸金属三脚架扩展器
- 硬质便携包
- 可选 32 通道全球定位系统 (GPS)
- 可选 iGuider TM自动导航系统 #3360
工厂提供美国电源
| 山 | 中心平衡赤道仪 |
| 有效载荷 * | 26 磅(12 千克),不含配重 |
| 安装重量 | 10 磅(4.5 公斤) |
| 有效载荷/安装重量 | 2.60 |
| 结构材料 | 全金属,铸造+数控加工 |
| 外墙装饰 | 粉末涂料 |
| 周期性误差 (PE) ** | <±10 角秒 |
| 聚乙烯醇 | 是的,永久 PEC |
| 蠕虫期 | 600 秒 |
| 赤经蜗轮 | φ88mm、144齿铝 |
| 偏角蜗轮 | φ88mm、144齿铝 |
| 赤经轴 | φ35mm钢材 |
| 赤纬轴轴 | φ35mm钢材 |
| 赤经方位 | φ55mm滚珠轴承 |
| 偏角方位 | φ55mm滚珠轴承 |
| 蜗轮 | φ15.2mm, 黄铜 |
| 电机驱动 | 1.8º步进电机,128X细分 |
| 解决 | 0.17 角秒 |
| 传播 | 同步带 |
| 纬度调整范围 | 0º ~ 60º (若 <10° 则采用特殊的顺时针轴安装) |
| 方位调整范围 | ± 6° |
| 极地望远镜 | iPolar TM电子极轴镜 |
| 液位指示器 | 水准气泡 |
| 手持控制器 | Go2Nova® 8409 拥有约 212,000 个对象的数据库 |
| 追踪 | 自动的 |
| 回转速度 | 1×,2×,8×,16×,64×,128×,256×,512×,MAX(6度/秒) |
| 功耗 | 0.5A(跟踪),0.8A(GOTO) |
| 电源要求 | 12V 直流,5A |
| 交流适配器 | 100V~240V(含) |
| 掉电记忆 | 是的 |
| 无线上网 | 内置 |
| 通信端口 | 是(Wi-Fi 和 USB) |
| 自动导航端口 | 是(兼容 ST-4) |
| 固件升级 | 是的 |
| PC电脑控制 | 是 (ASCOM) |
| 配重轴 | φ20X200mm,带120mm延长杆(M16,SS) |
| 配重 | 10 磅(4.5 公斤) |
| 三脚架 | 1.5英寸不锈钢(5千克) |
| 燕尾鞍座 | 3.8 英寸 Vixen 风格,中心可调 |
| 便携包 | 包括 |
| 全球定位系统 | 可选外置32通道GPS |
| 自动导航 | 可选外置 iGuider 1 |
| 操作温度 | -10℃~40℃ |
| 保修单 | 两年有限 |
$2,699.00
与其前代产品一样,C262A3 在设计时也充分考虑了便携性,重量仅为 4.5 公斤,可支撑高达 12 公斤的有效载荷,安装重量与有效载荷之比高达 2.6。实现这种比率的关键是 CEM 设计将安装和有效载荷的重量直接集中在三脚架的中心,从而实现“自然稳定性”。
在早期 CEM 型号的基础上,我们增加了一些功能,以提高便利性和实用性。正向锁定齿轮啮合系统(即使戴着手套也易于使用)、内置 Wi-Fi,实现无与伦比的连接性,以及可记录的永久周期性误差校正 (PPEC),以重复最佳的 PEC 训练课程。在功能方面,C262A3 提供精确的指向和准确的跟踪。CEM26 为紧凑型赤道仪树立了新标准。
中心平衡设计的支架将有效载荷的重量置于重心,从而实现更大的自然稳定性。其他功能包括可调节的配重杆,以防止三脚架受阻。由于极轴镜不受偏角轴阻挡,因此极轴校准快速且随时可用。
C262A3 配备了最新的先进 GOTONOVA® GOTO 技术,使其成为目前最强大、最准确的 GOTO 支架之一。其数据库包含超过 212,000 个物体。Go2Nova® 手动控制器使用直观,其大型 4 行 LCD 屏幕简化了设置望远镜和定位物体的过程。
CEM26A 支架配有集成电子极地寻星镜(称为 iPolar)。此工具可确保望远镜准确对准,即使北极星被遮挡。它配有 1.5 英寸重型不锈钢三脚架和铝制手提箱。
特征
- 独特的设计,中心平衡赤道仪 (CEM),可实现最大有效载荷和最小安装重量
- 非常适合视觉观察和天文摄影
- 低周期误差(< ± 10 角秒)
- 有效载荷为 12 公斤(26 磅),仅安装重量为 4.5 公斤(10 磅)
- CNC 加工和铸造的金属机身
- 弹簧加载齿轮系统
- 大型、易于使用的快速锁齿轮离合器
- 0º 纬度操作,配备可选适配器
- 低功耗步进电机
- 集成 iOptron iPolar TM电子极轴镜
- 为无法看见北极星的人提供极地校准程序
- 采用先进 GOTONOVA® GOTO 技术的 Go2Nova® 8409 控制器
- 集成 ST-4 自动导航端口
- 内置 Wi-Fi
- USB 端口用于固件升级和计算机控制
- LiteRoc 重型不锈钢三脚架,带减震垫(7.5 千克)
- 带附件托盘的压铸金属三脚架扩展器
- 硬质便携包
- 可选 32 通道全球定位系统 (GPS)
- 可选 iGuider TM自动导航系统 #3360
工厂提供美国电源
$2,559.00
与其前代产品一样,C261A3 在设计时也充分考虑了便携性,重量仅为 4.5 公斤,可支撑高达 12 公斤的有效载荷,安装重量与有效载荷之比高达 2.6。实现这种比率的关键是 CEM 设计将安装和有效载荷的重量直接集中在三脚架的中心,从而实现“自然稳定性”。
在早期 CEM 型号的基础上,我们增加了一些功能,以提高便利性和实用性。正向锁定齿轮啮合系统(即使戴着手套也易于使用)、内置 Wi-Fi,实现无与伦比的连接性,以及可记录的永久周期性误差校正 (PPEC),以重复最佳的 PEC 训练课程。在功能方面,C261A3 提供精确的指向和准确的跟踪。CEM26 为紧凑型赤道仪树立了新标准。
中心平衡设计的支架将有效载荷的重量置于重心,从而实现更大的自然稳定性。其他功能包括可调节的配重杆,以防止三脚架受阻。由于极轴镜不受偏角轴阻挡,因此极轴校准快速且随时可用。
C261A3 配备了最新的先进 GOTONOVA® GOTO 技术,使其成为目前最强大、最准确的 GOTO 支架之一。其数据库包含超过 212,000 个物体。Go2Nova® 手动控制器使用直观,其大型 4 行 LCD 屏幕简化了设置望远镜和定位物体的过程。
CEM26A 支架配有集成电子极地寻星镜(称为 iPolar)。此工具可确保望远镜准确对准,即使北极星被遮挡。它配有 1.5 英寸重型不锈钢三脚架和铝制手提箱。
装运箱 #1:C261A-CEM26 头部,带 iPolar/托盘 (C261A)
装运箱#2:8283-CEM26/GEM28 LiteRoc 三脚架(无托盘)(C26/G28 LiteRoc)
特征
- 独特的设计,中心平衡赤道仪 (CEM),可实现最大有效载荷和最小安装重量
- 非常适合视觉观察和天文摄影
- 低周期误差(< ± 10 角秒)
- 有效载荷为 12 公斤(26 磅),仅安装重量为 4.5 公斤(10 磅)
- CNC 加工和铸造的金属机身
- 弹簧加载齿轮系统
- 大型、易于使用的快速锁齿轮离合器
- 0º 纬度操作,配备可选适配器
- 低功耗步进电机
- 集成 iOptron iPolar TM电子极轴镜
- 对于那些看不到北极星的人来说,极星校准程序
- 采用先进 GOTONOVA® GOTO 技术的 Go2Nova® 8409 控制器
- 集成 ST-4 自动导航端口
- 内置 Wi-Fi
- USB 端口用于固件升级和计算机控制
- LiteRoc 重型不锈钢三脚架,带减震垫(7.5 千克)
- 带附件托盘的压铸金属三脚架扩展器
- 可选 32 通道全球定位系统 (GPS)
- 可选硬质便携包
- 可选 iGuider TM自动导航系统 #3360
工厂提供美国电源
$2,349.00
和前代产品一样,CEM26 在设计时也充分考虑了便携性,重量仅为 4.5 公斤,可支撑高达 12 公斤的有效载荷,安装重量与有效载荷之比高达 2.6。实现这种比率的关键在于 CEM 设计将安装和有效载荷的重量直接集中在三脚架的中心,从而实现“自然稳定性”。
在早期 CEM 型号的基础上,我们增加了一些功能,以提高便利性和实用性。正向锁定齿轮啮合系统(即使戴着手套也易于使用)、内置 Wi-Fi,实现无与伦比的连接性,以及可记录的永久周期性误差校正 (PPEC),以重复最佳的 PEC 训练课程。在功能方面,CEM26 提供精确的指向和准确的跟踪。CEM26 为紧凑型赤道仪设定了新标准。中心平衡设计的支架将有效载荷的重量置于重心,从而实现更大的自然稳定性。其他功能包括可调节的配重杆,以防止三脚架受阻。由于极轴镜不会被偏角轴阻挡,因此极轴对准始终快速且方便。CEM26 配备了最新的先进 GOTONOVA® GOTO 技术,使其成为目前最强大、最准确的 GOTO 支架之一。其数据库包含超过 212,000 个对象。 Go2Nova® 手动控制器使用直观,其大型 4 行 LCD 屏幕简化了设置望远镜和定位物体的过程。
CEM26A 支架配有集成电子极地寻星镜(称为 iPolar)。此工具可确保望远镜准确对准,即使北极星被遮挡。它配有 1.5 英寸重型不锈钢三脚架。
装运箱 #1:C261A-CEM26 头部,带 iPolar/托盘 (C26A1)
装运箱#2:8281-CEM26/GEM28 1.5英寸三脚架(无托盘)(C26/G28 1.5T)
特征
- 独特的设计,中心平衡赤道仪 (CEM),可实现最大有效载荷和最小安装重量
- 非常适合视觉观察和天文摄影
- 低周期误差(< ± 10 角秒)
- 有效载荷为 12 公斤(26 磅),仅安装重量为 4.5 公斤(10 磅)
- CNC 加工和铸造的金属机身
- 弹簧加载齿轮系统
- 大型、易于使用的快速锁齿轮离合器
- 0º 纬度操作,配备可选适配器
- 低功耗步进电机
- 集成 iOptron iPolar TM电子极轴镜
- 为无法看见北极星的人提供极地校准程序
- 采用先进 GOTONOVA® GOTO 技术的 Go2Nova® 8409 控制器
- 集成 ST-4 自动导航端口
- 内置 Wi-Fi
- USB 端口用于固件升级和计算机控制
- 标准1.5英寸重型不锈钢三脚架(5kg)
- 带附件托盘的压铸金属三脚架扩展器
- 可选 32 通道全球定位系统 (GPS)
- 可选硬质便携包
- 可选 iGuider TM自动导航系统 #3360
工厂提供美国电源
| 山 | 中心平衡赤道仪 |
| 有效载荷 * | 26 磅(12 千克),不含配重 |
| 安装重量 | 10 磅(4.5 公斤) |
| 有效载荷/安装重量 | 2.60 |
| 结构材料 | 全金属,铸造+数控加工 |
| 外墙装饰 | 粉末涂料 |
| 周期性误差 (PE) ** | <±10 角秒 |
| 聚乙烯醇 | 是的,永久 PEC |
| 蠕虫期 | 600 秒 |
| 赤经蜗轮 | φ88mm、144齿铝 |
| 偏角蜗轮 | φ88mm、144齿铝 |
| 赤经轴 | φ35mm钢材 |
| 赤纬轴轴 | φ35mm钢材 |
| 赤经方位 | φ55mm滚珠轴承 |
| 偏角方位 | φ55mm滚珠轴承 |
| 蜗轮 | φ15.2mm, 黄铜 |
| 电机驱动 | 1.8º步进电机,128X细分 |
| 解决 | 0.17 角秒 |
| 传播 | 同步带 |
| 纬度调整范围 | 0º ~ 60º(若<10°,则采用特殊的顺时针轴安装) |
| 方位调整范围 | ± 6° |
| 极地望远镜 | iPolar TM电子极轴镜 |
| 液位指示器 | 水准气泡 |
| 手持控制器 | Go2Nova® 8409 拥有约 212,000 个对象的数据库 |
| 追踪 | 自动的 |
| 回转速度 | 1×,2×,8×,16×,64×,128×,256×,512×,MAX(6度/秒) |
| 功耗 | 0.5A(跟踪),0.8A(GOTO) |
| 电源要求 | 12V 直流,5A |
| 交流适配器 | 100V~240V(含) |
| 掉电记忆 | 是的 |
| 无线上网 | 内置 |
| 通信端口 | 是(Wi-Fi 和 USB) |
| 自动导航端口 | 是(兼容 ST-4) |
| 固件升级 | 是的 |
| PC电脑控制 | 是 (ASCOM) |
| 配重轴 | φ20X200mm,带120mm延长杆(M16,SS) |
| 配重 | 10 磅(4.5 公斤) |
| 三脚架 | 1.5英寸不锈钢(5千克) |
| 燕尾鞍座 | 3.8 英寸 Vixen 风格,中心可调 |
| 全球定位系统 | 可选外置32通道GPS |
| 自动导航 | 可选外置 iGuider 1 |
| 操作温度 | -10℃~40℃ |
| 保修单 | 两年有限 |
$169.00
Die-cast and machined metal. Perfect for adding distance between scope and tripod on iOptron CEM26/HEM27/GEM28/HAE29 mounts.
Height: 5.5"
Diameter: 4" (100 mm)
Weight: 1lb 9oz
Gross weight and dimension: 2.5 lbs, 9 x 6 x 6 in
Option:
To convert the top center stud to 3/8" threaded bolt for uses with
- Sky-Tracker-Pro (3322s),
- Sky-Guider-Pro (3550s), and
- Sky-Hunter (3700xx),
- HAZ31, HAZ46
$3,999.00
iOptron® CEM40 赤道仪是新一代中心平衡赤道仪。这款赤道仪非常赏心悦目,其美感不仅仅体现在外观上。这款赤道仪的功能非常出色。这款赤道仪重量仅为 17.4 磅,可承载高达 40 磅的有效载荷!这真是太不可思议了!
创新的 iOptron 技术
为创新的支架让路!该支架有一个集成的电子极地寻星镜,称为 iPolar。此工具可确保望远镜准确对准,即使北极星被遮挡。快速锁定驱动啮合系统上有大型杠杆;这些大型杠杆可轻松将齿轮卡入到位。
这款 iOptron CEM40G 支架具有双鞍座,可容纳 Losmandy 和 Vixen 式燕尾板。CEM40 还使用 iOptron 的超静音、低功耗步进电机驱动系统,帮助支架提供精确的跟踪。
电脑化安装功能
iOptron CEM40 支架使用 Go2Nova® 8407 手动控制器来导航夜空。这项令人难以置信的技术可帮助观察者借助支架的 212,000 多个天体数据库找到天体!对于那些正在寻找能够跟踪和找到美丽夜空天体的望远镜的人来说,这款支架是必备工具。
借助附带的三脚架、11 磅的配重以及支架的计算机化技术,观察者只需轻轻一按,即可享受壮观的观看体验!
(此支架使用#8027 配重)
特征
- 独特的设计,中心平衡赤道仪 (CEM),可实现最大有效载荷和最小安装重量
- 适合视觉观察和天文摄影
- 最大有效载荷为 40 磅(18 千克),安装重量仅为 17.4 磅(7.9 千克)
- 全金属,CNC加工,红色/黑色阳极氧化
- 易于使用的快锁齿轮离合器
- 集成 iPolar TM电子极轴仪
- 低周期误差(< ± 7 角秒)
- 永久周期误差校正(PPEC)
- 精密步进电机,实现精确 GOTO 和准确跟踪
- Go2Nova® 8407+ 控制器采用先进的 GOTONOVA® GOTO 技术,内置加热器
- 集成 ST-4 自动导航端口
- 32 通道全球定位系统 (GPS)
- USB 通信端口
- 电缆管理系统
- 6 英寸 Losmandy D & Vixen 双燕尾鞍座
- 标准1.5英寸重型不锈钢三脚架(5kg)
- 可选 WiFi,可通过智能手机/平板电脑/电脑控制安装
工厂提供美国电源
| 山 | 中心平衡赤道仪 |
| 最大有效载荷* | 40 磅(18 千克),不包括配重 |
| 安装重量 | 17.4 磅(7.9 千克) |
| 有效载荷/安装重量 | 2.28 |
| 结构材料 | 全金属,CNC加工 |
| 外墙装饰 | 阳极氧化红/黑 |
| 纬度调整范围 | 0º ~ 60º(若<10°,则采用特殊的顺时针轴安装) |
| 方位调整范围 | ± 6° |
| 跟踪精度(PE)** | <±7 角秒 |
| 聚乙烯醇 | 太平洋石油公司 |
| 时期 | 400 秒 |
| 蜗杆直径 | φ17mm,黄铜 |
| 赤经蜗轮 | φ110mm、216齿、零背隙 |
| 偏角蜗轮 | φ110mm、216齿、零背隙 |
| 赤经轴 | φ45mm钢材 |
| 赤纬轴轴 | φ45mm钢材 |
| 赤经方位 | φ68毫米 |
| 偏角轴承 | φ68毫米 |
| 配重轴 | φ28x280毫米 不锈钢 1.2公斤 |
| 配重 | 5公斤(11磅) |
| 发动机 | 精密步进电机,1.8º/128X微步 |
| 电机分辨率 | 0.08 角秒(200 PPS) |
| 传播 | 同步带 |
| 手持控制器 | Go2Nova® 8407+,8 行 21 个字符 LCD |
| 星型数据库 | 212,000+,明星识别 |
| 力量 | DC 12V,5A(5.5mm/2.5mm插头) |
| 交流适配器 | 100V ~ 240V (含,仅限室内使用) |
| 功耗 | 0.6A(跟踪),0.9A(GOTO) |
| 掉电记忆 | 是的 |
| 极地观测镜 | 内置 iPolar TM电子极轴镜 |
| 经络治疗 | 停止(0-10°通过),翻转 |
| 零位 | 自动零点搜索 |
| 燕尾鞍座 | 6" 洛斯曼迪 D & Vixen |
| 最大回转速度 | 4.5°/秒 (1080x) |
| 导向口 | ST-4 |
| 通信端口 | USB |
| 全球定位系统 | 是的 |
| 无线上网 | 外部(可选) |
| 电缆管理 | DC12V(3A)、ST4、USB |
| 三脚架 | 1.5英寸不锈钢(5千克),可选2英寸或三柱 |
| 硬盒 | 选修的 |
| 操作温度 | -10℃~40℃ |
| 保修单 | 两年有限 |
$4,099.00
配备 LiteRoc 的 iOptron® CEM40 是新一代中心平衡赤道仪。这款赤道仪令人赏心悦目,其美感不仅仅体现在外观上。赤道仪的功能性也非常出色。重量仅为 17.4 磅。,该支架可支撑高达 40 磅的有效载荷!太不可思议了!
创新的 iOptron 技术
为创新的支架让路!这款支架有一个集成的电子极地寻星镜,称为 iPolar。此工具可确保望远镜准确对准,即使北极星被遮挡。快速锁定驱动接合处有大型杠杆系统;这些大杠杆使得齿轮很容易卡入到位。
这款配备 LiteRoc 的 iOptron CEM40 具有双鞍座,可容纳 Losmandy 和 Vixen 式燕尾板。它还使用 iOptron 的超静音、低功耗步进电机驱动系统,帮助支架提供精确的跟踪。
电脑化安装功能
iOptron CEM40 支架使用 Go2Nova® 8407 手动控制器来导航夜空。这项令人难以置信的技术可帮助观察者借助支架的 212,000 多个天体数据库找到天体!对于那些正在寻找能够跟踪和找到美丽夜空天体的望远镜的人来说,这款支架是必备工具。
借助附带的三脚架、11 磅的配重以及支架的计算机化技术,观察者只需轻轻一按,即可享受壮观的观看体验!
(配备 Literoc 的 CEM40 使用 #8027 配重)
特征
- 独特的设计,中心平衡赤道仪 (CEM),可实现最大有效载荷和最小安装重量
- 适合视觉观察和天文摄影
- 最大有效载荷为 40 磅(18 千克),安装重量仅为 17.4 磅(7.9 千克)
- 全金属,CNC加工,红色/黑色阳极氧化
- 易于使用的快锁齿轮离合器
- 集成 iPolar TM电子极轴仪
- 低周期误差(< ± 7 角秒)
- 永久周期误差校正(PPEC)
- 精密步进电机,实现精确 GOTO 和准确跟踪
- Go2Nova® 8407+ 控制器采用先进的 GOTONOVA® GOTO 技术,内置加热器
- 集成 ST-4 自动导航端口
- 32 通道全球定位系统 (GPS)
- USB 通信端口
- 电缆管理系统
- 6 英寸 Losmandy D & Vixen 双燕尾鞍座
- LiteRoc 1.75 英寸重型不锈钢三脚架(7 千克)
- 可选 WiFi,可通过智能手机/平板电脑/电脑控制安装
工厂提供美国电源
| 山 | 中心平衡赤道仪 |
| 最大有效载荷* | 40 磅(18 千克),不包括配重 |
| 安装重量 | 17.4 磅(7.9 千克) |
| 有效载荷/安装重量 | 2.28 |
| 结构材料 | 全金属,CNC加工 |
| 外墙装饰 | 阳极氧化红/黑 |
| 纬度调整范围 | 0º ~ 60º(若<10°,则采用特殊的顺时针轴安装) |
| 方位调整范围 | ± 6° |
| 跟踪精度(PE)** | <±7 角秒 |
| 聚乙烯醇 | 太平洋石油公司 |
| 时期 | 400 秒 |
| 蜗杆直径 | φ17mm,黄铜 |
| 赤经蜗轮 | φ110mm、216齿、零背隙 |
| 偏角蜗轮 | φ110mm、216齿、零背隙 |
| 赤经轴 | φ45mm钢材 |
| 赤纬轴轴 | φ45mm钢材 |
| 赤经方位 | φ68毫米 |
| 偏角轴承 | φ68毫米 |
| 配重轴 | φ28X280MM不锈钢1.2KG |
| 配重 | 5公斤(11磅)X1 |
| 发动机 | 精密步进电机,1.8º/128X微步 |
| 电机分辨率 | 0.08 角秒(200 PPS) |
| 传播 | 同步带 |
| 手持控制器 | Go2Nova® 8407+,8 行 21 个字符 LCD |
| 星型数据库 | 212,000+,明星识别 |
| 力量 | DC 12V,5A(5.5mm/2.5mm插头) |
| 交流适配器 | 100V ~ 240V (含,仅限室内使用) |
| 功耗 | 0.6A(跟踪),0.9A(GOTO) |
| 掉电记忆 | 是的 |
| 极地观测镜 | 内置 iPolar TM电子极轴镜 |
| 经络治疗 | 停止(0-10°通过),翻转 |
| 零位 | 自动零点搜索 |
| 燕尾鞍座 | 6" 洛斯曼迪 D & Vixen |
| 最大回转速度 | 4.5°/秒 (1080x) |
| 导向口 | ST-4 |
| 通信端口 | USB |
| 全球定位系统 | 是的 |
| 无线上网 | 外部(可选) |
| 电缆管理 | DC12V(3A)、ST4、USB |
| 三脚架 | LiteRoc 1.75" 不锈钢(7千克) 可选三墩 |
| 硬盒 | 选修的 |
| 操作温度 | -10℃~40℃ |
| 保修单 | 两年有限 |
$5,349.00
iOptron CEM70AW Center-Balanced Equatorial Mount
Following the success of the acclaimed iOptron CEM60, we’re excited to introduce the next generation of center-balanced equatorial mounts — the CEM70 and CEM70AW.
The CEM70AW sets a new standard in the 70 lb payload class, offering advanced features such as USB 3.0 connectivity and built-in Wi-Fi.
Precision. Balance. Performance.
Retaining the inherent advantages of the center-balance design, these medium-payload mounts deliver the efficiency, accuracy, and portability that astronomers demand.
With precise GoTo pointing and tracking accuracy better than ±5 arcseconds, the CEM70 is a solid performer for both visual observers and astrophotographers.
Innovative features such as the integrated iPolar™ electronic polar scope, large easy-lock gear levers (usable with gloves), and an advanced cable-management system demonstrate iOptron’s commitment to real-world usability.
The CEM70AW includes both the iPolar™ electronic polar scope and a hard case for convenient transport and protection.
Key Features
- New center-balanced design (CEM) for maximum payload and natural stability
- Ideal for both visual observing and astrophotography
- 70 lb (31.8 kg) payload capacity with a mount weight of only 30 lb (13.6 kg)
- Reliable, easy-to-use gear clutches
- Precision altitude and azimuth adjustments
- High-precision stepper motors (0.07 arcsec resolution) for accurate GoTo and tracking
- Integrated iPolar™ electronic polar scope
- Go2Nova® 8410 controller with Advanced GoToNova® technology and built-in heater
- High-precision tracking with periodic error < ±5 arcsec
- Permanent Periodic Error Correction (PPEC)
- Built-in 32-channel GPS
- Integrated Wi-Fi for remote operation
- USB 3.0 connection for modern data-transfer speeds
- ST-4 autoguiding port
- Advanced cable-management system with multiple output options
- Spring-loaded 8″ dual Vixen/Losmandy saddle
- Includes iOptron-subsidized TheSky Imaging Edition software
Technical Specifications
| Mount type | Center-balanced Equatorial Mount (CEM) |
| Payload capacity* | 31.8 kg (70 lb) – excluding counterweight |
| Mount weight | 13.6 kg (30 lb) |
| Payload : Mount weight ratio | 2.33 |
| Construction | All metal |
| Latitude adjustment | 0° – 65° |
| Azimuth adjustment | ± 4° |
| Periodic error (encoder) | < ± 5 arcsec |
| Worm period | 348 sec |
| Periodic Error Correction | PPEC |
| RA worm wheel | Ø 151 mm, 248 teeth |
| DEC worm wheel | Ø 151 mm, 248 teeth |
| Worm diameter | Ø 21.2 mm |
| RA axle | Ø 55 mm (steel) |
| DEC axle | Ø 55 mm (steel) |
| RA bearings | Ø 80 mm |
| DEC bearings | Ø 80 mm |
| Counterweight shaft | Ø 28 × 415 mm (SS, 1.9 kg) |
| Counterweight | 9.5 kg (20 lb) × 1 |
| Mount base diameter | Ø 152 mm |
| Motor drive | Precision stepper motor with 128 micro-steps |
| Resolution | 0.07 arcseconds |
| Max slew speed | 3.75°/sec (900×) |
| Hand controller | Go2Nova® 8410 (8-line × 21-character LCD) |
| Power requirement* | DC 12 V 5 A (5.5 mm / 2.5 mm plug) |
| Power consumption | 0.6 A (tracking) / 0.8 A (GoTo) |
| Polar scope | Internal iPolar™ electronic polar scope |
| Meridian treatment | Stop (0–10° pass) or auto flip |
| Zero position | Automatic zero search |
| Park positions | Horizontal, vertical, current, alt/az input |
| Level indicator | Yes |
| Dovetail saddle | 8″ Losmandy D & Vixen |
| GPS | Yes (32-channel built-in) |
| Guiding port | ST-4 |
| Communication ports | USB 3.0, Wi-Fi |
| Cable management | 1 × DC 12 V (3 A), 3 × USB 3.0, 1 × DC in / 2 × DC out, iPort |
| USB input support | Mount, iGuider, iPolar, and more |
| Operating temperature | −10 °C to +40 °C |
Manuals & Resources
$5,039.00
继 iOptron CEM60 中心平衡赤道仪大获成功之后,我们 iOptron 很高兴推出两款新型中等有效载荷中心平衡赤道仪。CEM70 和 CEM70G 是 31.8KG 有效载荷段赤道仪的新标准。两种型号都配备了先进的功能,但 CEM70G 是同类产品中第一款配备机载光学引导系统的赤道仪,该系统可提高跟踪精度,同时简化组件,从而实现更便携的成像设置。
这些相对紧凑的中型有效载荷支架保留了中心平衡设计的固有特性,满足了天文学家对高效、精确的便携式支架的期望。凭借精确的 GOTO 指向和精确的跟踪(PE <±3.5 弧秒),CEM70 对观察者和成像者来说都是一款可靠的产品。
创新的操作功能,如内部 iPolar 电子极轴镜、易锁驱动齿轮啮合(杠杆足够大,可以戴着手套使用)、用于支架、iPolar、导向器和相机的先进电缆管理系统,共同确保 CEM70 和 70G 的设计充分考虑了用户的需求。
|
规格
| 山 | 中心平衡赤道仪 (CEM) |
| 有效载荷* | 31.8 千克(70 磅),不含配重 |
| 安装重量 | 13.6千克(30磅) |
| 有效载荷/安装重量比 | 2.33 |
| 材料 | 全金属 |
| 纬度调整范围 | 0°~ 65° |
| 方位调整范围 | ± 4° |
| PE (通过编码器)** | < ±3.5 角秒 |
| 蠕虫期 | 348 秒 |
| 聚乙烯醇 | 太平洋石油公司 |
| 赤经蜗轮 | φ151mm、248齿 |
| 偏角蜗轮 | φ151mm、248齿 |
| 蠕虫 | φ21.2毫米 |
| 赤经轴 | φ55mm,钢 |
| 偏角轴 | φ55mm,钢 |
| 赤经方位 | φ80毫米 |
| 偏角轴承 | φ80毫米 |
| 配重轴 | φ28×415毫米(不锈钢,1.9千克) |
| 配重 | 9.5 公斤(20 磅)x1 |
| 安装底座尺寸 | φ152毫米 |
| 电机驱动 | 精密步进电机,128 微步 |
| 解决 | 0.07 角秒 |
| 回转速度 | 最大 3.75°/秒(900x) |
| 手持控制器 | Go2Nova® 8407+,8 行 21 个字符 LCD |
| 电源要求 | DC 12V,5A(5.5mm/2.5mm 插头) |
| 功耗 | 0.6A(跟踪),0.8A(GOTO) |
| 极地望远镜 | 内置电子极轴镜,iPolar |
| 经络治疗 | 停止(0-10°通过),自动翻转 |
| 零位 | 自动零点搜索 |
| 驻车位置 | 水平、垂直、电流、高度/方位角输入 |
| 液位指示器 | 是的 |
| 燕尾鞍座 | 8" 洛斯曼迪 D & Vixen |
| 全球定位系统 | 是的 |
| 导向口 | ST-4 |
| 通信端口 | USB2.0 |
| 电缆管理 | 2xDC12V(3A)、3xUSB2.0、1xDC 输入/1xDC 输出、iPort。 1X USB 输入用于安装和 USB 集线器 |
| 工作温度范围 | -10℃~+40℃ |
| 硬盒 | 是的 |
| 墩座/三脚架 | 可选的 LiteRoc 三脚架 (8023ACC) 或码头 |
| 保修单 | 两年有限 |
|
$7,199.00
|
|
规格
| 山 | 中心平衡赤道仪 (C704A0) |
| 有效载荷* | 31.8 千克(70 磅),不含配重 |
| 安装重量 | 13.6千克(30磅) |
| 有效载荷/安装重量比 | 2.33 |
| 材料 | 全金属 |
| 纬度调整范围 | 0°~ 65° |
| 方位调整范围 | ± 4° |
| PE (通过编码器)** | < 0.3 角秒均方根** |
| 蠕虫期 | 348 秒 |
| 聚乙烯醇 | 实时肺动脉收缩末期 (RPEC) |
| 赤经蜗轮 | φ151mm、248齿 |
| 偏角蜗轮 | φ151mm、248齿 |
| 蠕虫 | φ21.2毫米 |
| 赤经轴 | φ55mm,钢 |
| 偏角轴 | φ55mm,钢 |
| 赤经方位 | φ80毫米 |
| 偏角轴承 | φ80毫米 |
| 配重轴 | φ28×415毫米(不锈钢,1.9千克) |
| 配重 | 9.5 公斤(20 磅)x1 |
| 安装底座尺寸 | φ152毫米 |
| 电机驱动 | 精密步进电机,128 微步 |
| 解决 | 0.07 角秒 |
| 回转速度 | 最大 3.75°/秒(900x) |
| 手持控制器 | Go2Nova® 8407+,8 行 21 个字符 LCD |
| 电源要求 | DC 12V,5A(5.5mm/2.5mm 插头) |
| 功耗 | 0.6A(跟踪),0.8A(GOTO) |
| 极地望远镜 | 内置电子极轴镜,iPolar |
| 经络治疗 | 停止(0-10°通过),自动翻转 |
| 零位 | 自动零点搜索 |
| 驻车位置 | 水平、垂直、电流、高度/方位角输入 |
| 液位指示器 | 是的 |
| 燕尾鞍座 | 8" 洛斯曼迪 D & Vixen |
| 全球定位系统 | 是的 |
| 导向口 | ST-4 |
| 通信端口 | USB2.0 |
| 电缆管理 | 2xDC12V(3A)、3xUSB2.0、1xDC 输入/1xDC 输出、iPort。 1X USB 输入用于安装和 USB 集线器 |
| 工作温度范围 | -10℃~+40℃ |
| 硬盒 | 是的 |
| 墩座/三脚架 | 可选的 LiteRoc 三脚架 (8023ACC) 或码头 |
| 保修单 | 两年有限 |
|
$7,349.00
|
|
规格
| 山 | 中心平衡赤道仪 (CEM) |
| 有效载荷* | 31.8 千克(70 磅),不含配重 |
| 安装重量 | 13.6千克(30磅) |
| 有效载荷/安装重量比 | 2.33 |
| 材料 | 全金属 |
| 纬度调整范围 | 0°~ 65° |
| 方位调整范围 | ± 4° |
| PE (通过编码器)** | < 0.3 角秒均方根 |
| 蠕虫期 | 348 秒 |
| 聚乙烯醇 | 实时 PEC (RPEC) |
| 赤经蜗轮 | φ151mm、248齿 |
| 偏角蜗轮 | φ151mm、248齿 |
| 蠕虫 | φ21.2毫米 |
| 赤经轴 | φ55mm,钢 |
| 偏角轴 | φ55mm,钢 |
| 赤经方位 | φ80毫米 |
| 偏角轴承 | φ80毫米 |
| 配重轴 | φ28×415毫米(不锈钢,1.9千克) |
| 配重 | 9.5 公斤(20 磅)x1 |
| 安装底座尺寸 | φ152毫米 |
| 电机驱动 | 精密步进电机,128 微步 |
| 解决 | 0.07 角秒 |
| 回转速度 | 最大 3.75°/秒(900x) |
| 手持控制器 | Go2Nova® 8407+,8 行 21 个字符 LCD |
| 电源要求 | DC 12V,5A(5.5mm/2.5mm 插头) |
| 功耗 | 0.6A(跟踪),0.8A(GOTO) |
| 极地望远镜 | 内置电子极轴镜,iPolar |
| 经络治疗 | 停止(0-10°通过),自动翻转 |
| 零位 | 自动零点搜索 |
| 驻车位置 | 水平、垂直、电流、高度/方位角输入 |
| 液位指示器 | 是的 |
| 燕尾鞍座 | 8" 洛斯曼迪 D & Vixen |
| 全球定位系统 | 是的 |
| 导向口 | ST-4 |
| 通信端口 | USB2.0 |
| 电缆管理 | DC12V(3A)、DC(5A)、指南、USB 对于 NUC:DC 19V、LAN 和 USB |
| 工作温度范围 | -10℃~+40℃ |
| 硬盒 | 是的 |
| 墩座/三脚架 | 可选的 LiteRoc 三脚架 (8023ACC) 或码头 |
| 保修单 | 两年有限 |
|
$249.00
CEM120 支架需额外配备 10 公斤配重。
$299.00
iOptron CW 10kg
低纬度 (<10°) 的 CEM120 支架配备 10 公斤配重
$45.00
iOptron CW 1kg
此配重套件专为 iOptron SkyTracker Pro 相机支架设计,用于平衡重载荷/长相机镜头。它也适用于 SkyTracker 支架。
iOptron CW 1kg 包装包括:
- 燕尾板
- 配重杆和安全帽
- 1.35kg配重
- 锁定手柄
$150.00
This 4.5 kg (~10 lbs) counterweight can be used for the following iOptron mount:
- CEM26/CEM26EC
- HEM27/HEM27EC
- GEM28/GEM28EC
- HAE29/HAE29EC
- HAE43/HAE43EC
- HAE69/HAE69EC
- HEM44/HEM44EC
- AZ Mount Pro
- iEQ30/iEQ30 Pro
- CEM25/CEM25P/CEM25EC
- ZEQ25
- MiniTower Pro
- MiniTower II
- MiniTower
- CEM40/CEM40EC* (early version with 20mm CW shaft)
* Check your CEM40/CEM40EC mount CW shaft diameter before ordering.
It can be used for other mount with a 20mm diameter counterweight shaft.
$220.00
iOptron CW 9.5kg
该平衡重物可安装在以下支架上:
- CEM70/CEM70G
- GEM45/GEM45G/GEM45EC*
- iEQ45/iEQ45 Pro
- CEM60/CEM60EC
- CEM40、CEM40G、CEM40EC*
* 请检查配重轴直径。
iOptron CW 9.5kg 规格
重量:9.5公斤
外径:147毫米
内径:28.28 毫米
高度:75mm
颜色:黑色
库存单位:7226
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