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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
Telescopes Melbourne
Are you looking to buy a telescope in Victoria, Australia? Look no further than Bintel!
For decades, the team here at BINTEL have been supplying telescopes and a myriad range of accessories to our customers in Melbourne and throughout Victoria.
On offer are great shipping rates all over Australia and New Zealand, with telescopes and binoculars sent every week. Typically orders of items will be delivered within 1 or 2 buisness days for metro areas in VIC, or 4 to 5 for regional areas.
We specialise in helping beginners choose high quality first telescopes and binoculars, which will last for years and years - our products have been hand-picked by expert staff, all of whom are professional astronomers or birdwatchers. Bintel has been supporting Australian optics enthusiasts for over 40 years.
172 products
172 products
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$3,349.00
FF131 APO. Flat field, built in.
A 131 mm f/7.5 four-element apochromatic refractor with a native flat field and a 44 mm full-frame image circle. The flagship of the FF series, with 983 mm of focal length and serious light grasp for deep-sky imaging.
Designed as an astrograph first.
Every FF series telescope is built around a native flat field, so the optics, focuser and rear interfaces all serve one goal: clean stars across the whole sensor.
Attach your camera, reach focus, start imaging. No flattener. No spacing maths.
Four elements, fully air-spaced.
The FF131 APO uses a four-element, fully air-spaced apochromatic design in which all four elements work together to form the image. One ED (extra-low dispersion) glass element reduces chromatic aberration for cleaner colour correction and sharper stars.
Flat to the edge. No flattener.
The flat imaging field is generated by the optical design itself, so there is no field flattener to buy and no back focus calculations to get right. Once focus is achieved, you are ready to capture.
44 mm image circle.
A 44 mm corrected image circle fully covers full-frame sensors, with sharp star fields and consistent illumination from centre to corner. Smaller APS-C and dedicated astronomy sensors have generous headroom.
1:10 dual-speed control.
A rigid 3″ rack-and-pinion focuser offers precise control, and the 1:10 coarse and fine adjustment makes critical focus easy to hit. A built-in 360° rotator at the rear sets your framing without disturbing focus.
Retractable dew shield.
The dew shield retracts to shorten the tube for packing and travel. Precision CNC machining, a high-quality painted finish and an internal anti-reflection coating keep stray light down and image contrast up.
Adapters in the box.
A four-section photography extension tube with a 2″ filter thread is included, along with rear adapters in M48×0.75 and M54×0.75 standards. The quick-release mounting rings detach in seconds for fast setup and teardown.
Four elements. One flat field.
All four air-spaced elements work together to form the image, with one ED glass element controlling chromatic aberration for clean colour correction and tight, well-defined stars.
The light path, end to end.
The optical layout delivers a corrected, flat field at the sensor with no additional optics in the imaging train. What leaves the objective arrives at your camera, flat.
44 mm image circle.
Full-frame sensors are covered corner to corner with sharp star fields and consistent illumination, and smaller sensors sit comfortably inside the sweet spot.
Coarse and fine, 1:10.
The rigid 3″ rack-and-pinion focuser moves heavy imaging trains smoothly, and the 1:10 fine knob gives you the resolution to land exact focus on a star.
360° of rotation.
A built-in rotator at the rear lets you set the camera angle for perfect framing without unthreading anything or disturbing focus.
Quick-release rings. Retractable dew shield.
The mounting rings detach in seconds for fast setup and teardown, and the dew shield slides back to shorten the tube for transport. CNC machining and an internal anti-reflection coating keep contrast high.
Photography extension tube.
A four-section photographic extension tube with a 2″ filter thread is included, plus M48×0.75 and M54×0.75 rear adapters, connecting cameras, filters and accessories cleanly out of the box.
131 mm of light grasp, 983 mm of reach.
The flagship of the FF series pulls in the most light and resolves the finest detail of the range, and the 983 mm focal length frames smaller targets tightly. The optical tube weighs 7.9 kg, or 9.4 kg with the handle, mounting rings and dovetail plate fitted.
One telescope. Three configurations.
Pair the FF131 APO with ZWO ASI astronomy cameras, attach a DSLR or mirrorless body, or drop in a diagonal and eyepiece for visual observing. Focus is reached within a back focus range of 42–73 mm, measured from the M54–M48 interface shoulder. Visual accessories are available separately.
Every detail, considered.
Four-element, fully air-spaced apochromatic design with one ED glass element.
Native flat-field design, no separate field flattener or spacing adjustments required.
44 mm image circle with full-frame sensor support and edge-to-edge sharpness.
3″ rack-and-pinion focuser with 1:10 coarse and fine adjustment.
Built-in 360° rotator for precise camera angle adjustment.
Retractable dew shield with internal anti-reflection coating for higher contrast.
Quick-release mounting rings for fast setup and teardown.
Four-section photography extension tube with 2″ filter thread plus M48×0.75 and M54×0.75 rear adapters included.
Specifications.
91 mm (from the M54×0.75 male thread)
142 mm (from the 2″ interface)
60 mm (from M54×0.75 male thread)
111 mm (from 2″ interface)
941 mm (photography extension tube retracted)
963 mm (1.25″ interface, dew shield extended)
1026 mm (photography extension tube, dew shield extended)
M78×1 – M54×0.75
M54×0.75 – M54×0.75
M54×0.75 – M48×0.75 (built-in M48×0.75 filter thread)
Built to last a lifetime.
**Special Price on the BINTEL Display Model! One only available**
Highlights:
- Ideal for visual observation and astrophotography.
- Designed for the amateur astronomer or photographer who wants to view and photograph the moon, planets, and deep sky objects.
- Features FPL53 "super" extra-low dispersion (ED) glass in a fully multicoated apochromatic lens system that corrects for both spherical and chromatic aberrations, astigmatism, and off-axis comas.
- This correction creates a wide flat field of view without distortion and removes the blue-tinted halo effect for true high-contrast color transmission.
- Can accept both 2" and 1.25" eyepieces and accessories for visual use.
- Threads on the drawtube allow direct connection of T-rings and other camera mounts.
A ring spacer placed around the objective lens refines star images beautifully in astrophotography.
In the previous SD81S model, a set of three tiny tin foils are placed around the objective lens as a spacer between the doublet lens. The end of the tin foils protruding over the objective lens obstruct the incoming light. As a result, the protruding tin foils make the light of diffraction of stars chipped radially. Exchanging the tin foils for the spacer ring makes the diffraction of the stars' light equal. It allows you to create more refined and beautiful star images in your astrophotography.
The SD lens suppresses residual chromatic aberration far below the threshold of visibility.
A lens of refracting telescopes has chromatic aberration which is caused by different wavelength of visible light (colors) focusing at different distances. The Vixen SD lenses, made of FPL53 super extra-low dispersion glass, allow for correcting the chromatic aberration over a wide spectrum of light. The SD81SII delivers outstandingly sharp images with high contrast for both visual and photographic applications. Moderately bright F7.7 images will satisfy the most demanding visual astronomer or astrophotographer.
A short optical tube in length is handy for not only visual observation but also astrophotography.
The ED81SII optical tube has a moderate short length to enable you to carry and set it up readily. Also, a lightweight optical tube allows you to balance it with fewer counterweights. The ED81S comes equipped with a metal carry handle and the Vixen standard dovetail slide bar M for quick attaching and detaching. The provided Flip mirror diagonal switches incoming light to allow for using two eyepieces of different magnifications alternately. Also, you can install a camera on the straight side and view an image through an eyepiece on the right-angled side of the flip mirror diagonal.
Full-frame imaging with a DSLR camera.
Using an SD reducer HD kit or an SD Flattener SD kit, which are available optionally, the SD80SII provides an image circle of 44mm, adequate for taking photos with a DSLR camera. (Photo) M8, M20 nebulae taken with Vixen SD81SII with SD reducer HD kit (compound focus 496mm) and Pentax K-1 at ISO1600, 49 minutes exposure.
Optional accessories to expand your pleasure of taking astrophotography.
SD Reducer HD Kit: This kit includes a flattener lens to be combined with a reducer lens for a flat and wide imaging field when you use them with the SD81SII, SD103SII, or SD115SII optical tube. The reducer lens reduces a focal length by 0.7X. Direct Wide Photo Adapter 60DX: It is available for Canon EOS or Nikon DSLR cameras. It is possible to change the orientation of a camera for a framing of the photographic field.
Wide Photo Adapter 60DX
High precision camera adapters for prime focus astrophotography are optionally available for Canon EOS and Nikon. The Wide Photo Adapter 60DX is designed to be an integrated camera mount reducing vignetting to the maximum. They are highly effective with full-frame DSLR cameras, and can be used with SD series refractors (in combination with the SD Reducer HD Kit or SD Flattener HD Kit).
Specifications
| Optical Tube | |
|---|---|
| Objective Lens / Effective Aperture | 81mm SD Apochromat Multi-Coated |
| Focal Length (Focal Ratio) | 625mm (F7.7) |
| Resolution / Limiting Magnitude | 1.43 arc sec., 11.3 mag., 134× unaided eye |
| Dimensions / Weight | Length 585mm, outer diameter 90mm, 3.6kg (main body 2.3kg) |
| Finder Scope | XY Red Dot Finder II (one-power aiming device) |
| Eyepiece / Focuser | |
| Focusing System | Rack and Pinion |
| Threads / Visual Back | Screw-in: 60mm, 42mm T-ring Push-fit: 50.8mm, 31.7mm (with Flip Mirror Diagonal) |
| Eyepiece — SLV20mm | 31×, 97′ actual field of view |
| Eyepiece — SLV5mm | 125×, 24′ actual field of view |
| Tripod | |
| Material / Form | Large hexagonal aluminium two-stage extension legs (one-touch type) |
| Leg Length / Height | 570–1,296mm leg length; 526–1,159mm height (from ground) |
| Overall Length / Setting Radius / Weight | 598.4mm overall; setting radius 350–710mm; 3.0kg |
| General | |
| Main Accessories | Parts case, counterweight 1kg ×1, 1.9kg ×1 |
| Solar Observation | Compatible with Sun Projection Screen Set B (sold separately) — short-term observation only |
| Total Weight | 13.1kg (excluding eyepiece) |
| Set Contents | |
| Included Items | SD81SII OTA, AP Mount, APP-TL130 Tripod, Eyepiece SLV20mm, Eyepiece SLV5mm, Parts Case, Counterweight 1kg ×1, Counterweight 1.9kg ×1 |
$15,049.00
f/2.75.
What used to take a week now takes a night.
The DeltaRho 280 Argus is PlaneWave’s observatory-class wide-field astrograph for serious imagers and sky-survey programmes. Fused silica quartz mirrors, a carbon fibre OTA, and a 55 mm image circle at f/2.75 — 280 mm of aperture that turns nights of integration into a few productive hours.
f/2.75 is not just fast. It is the difference between finishing a target tonight and coming back next month.
13× faster than f/10. Every photon counts more.
At f/2.75, the DeltaRho 280 gathers light 13 times faster than an f/10 instrument of identical aperture. That is not an incremental advantage — it is the difference between a productive one-hour session and a week of cloud-interrupted integration. Research programmes and sky surveys that would otherwise take months become achievable in a single season.
mm image circle — large enough to cover full-frame sensors and beyond, with sharp stars from centre to corner at 4.5 μm RMS or better at 27.5 mm off-axis.
Focus stays locked. All night.
Primary and secondary mirrors are optical-grade fused silica quartz — near-zero thermal expansion, the same material used in premier research observatories. As temperature drops through the night, conventional glass mirrors shift focus. The DR280’s quartz mirrors do not.
Stiff where it matters. Light where it counts.
Carbon fibre delivers exceptional torsional rigidity with minimal mass. At 14.5 kg for a 451 mm OTA, the DR280 is a 280 mm instrument that mounts on observatory-class and high-end portable mounts alike — without needing a counterweight upgrade.
Sensor alignment without shimming or guesswork.
The integrated tip-tilt focal plane adjuster lets you dial in perfect sensor tilt with precision — no shims, no trial-and-error. It is consistent, repeatable, and done in minutes at the start of any session.
The Heart Nebula. In one frame.
The 770.6 mm focal length paired with the 55 mm image circle delivers over 4 degrees of field of view. Large nebula complexes, galaxy groups, and wide-field targets that require mosaics on narrow-field systems fit comfortably into a single frame — or anchor a multi-panel survey.
Dew control built in. Session-ending fog, ruled out.
Integrated dew control heater technology keeps the optical path clear on humid Australian nights. One less cable to run, one less failure point — the DR280 keeps imaging when lesser rigs fog out and call it a night.
Collimation solved. From first session to thousandth.
The DeltaRho 280 ships with PlaneWave’s collimation software that walks you through mirror alignment step by step — no iterative star-testing, no guesswork. Set it once: the rigid carbon fibre structure holds alignment through the night. The low-profile focuser delivers 0.5 inches of travel from a 163 mm back focus distance, giving your imaging train room to breathe.
M51. The Whirlpool Galaxy.
Galaxy arms, tidal bridges, and foreground stars resolved in a single short session. At f/2.75, integration time that would fill a week on a slower system compresses to a few productive hours.
IC 1805. The Heart Nebula.
H-alpha, RGB narrowband composite. The 4-degree–plus field captures the Heart Nebula’s full complex and surrounding star-forming regions in a single pointing — a target that demands a mosaic from slower, narrower systems.
Built for imagers who treat every clear night as a resource. Nothing wasted.
280 mm (11″) aperture with fused silica (quartz) primary and secondary mirrors for temperature-stable performance
f/2.75 focal ratio — 13 times faster than f/10, reducing required integration time dramatically
55 mm image circle at 4.0 μm RMS on-axis and 4.5 μm RMS at the full 27.5 mm off-axis radius
Integrated tip-tilt focal plane adjuster for precise sensor alignment without physical shimming
Carbon fibre optical tube — 451 mm OTA, 14.5 kg total weight for use on observatory-class mounts
Built-in dew control heater and broadband AR coatings (<1% reflection, 400–800 nm) for consistent all-weather performance
4°+ field of view capability with a 55 mm sensor — ideal for large nebula complexes and sky surveys
Compatible with PlaneWave L350 Direct Drive Mount — designed as an integrated professional imaging system
Every number that matters.
Professional imaging. Backed by Australia’s telescope authority.
$9,869.00
The fast SCT, reinvented.
8 inches. f/2.8. Carry-on weight.
The Observable Space FSCT8 is the first native f/2.8 Schmidt-Cassegrain ever built in an 8-inch form factor. A 42 mm image circle, fused silica quartz mirrors, and a 267 mm carbon-fibre OTA under 9 kg — designed from the optical axis out for astrophotographers who demand observatory results without the observatory.
Every clear night is too short. The FSCT8 makes sure you get the most out of every hour of it.
f/2.8 native. The SCT form factor finally fast.
A conventional 8-inch SCT runs at f/10. The FSCT8 runs at f/2.8 natively — no reducer stacks, no optical compromises. That is a 13-fold increase in photon-gathering speed. A four-hour integration target becomes roughly 20 minutes of effective exposure. For imagers working under Australian skies with limited clear nights, this is the most impactful single step up possible.
mm fully illuminated image circle. Sharp stars across the entire field at under 6.2 μm RMS — covering APS-C and most medium-format sensors with no vignetting.
Quartz mirrors. Focus doesn’t move.
Primary (210 mm) and secondary (114 mm) mirrors are both fused silica quartz — the same glass used in research-grade observatories. Near-zero thermal expansion means the focus point does not drift as temperature drops. Your collimation is still correct at 3 am.
267 mm OTA. Fits where full-size SCTs don’t.
The carbon-fibre upper cage is rigid, thermally stable, and keeps total OTA length at just 267 mm. That is shorter than many refractors. It mounts on mid-range equatorial platforms and travels as carry-on — without sacrificing the optical performance of a full 8-inch system.
Flat field. Corner to corner. No caveats.
The 88 mm broadband AR-coated corrector lens flattens the focal plane and holds sub-6.2 μm RMS optical performance across the full 42 mm image circle — from dead-centre to the corner of a full APS-C sensor.
Your full imaging train. No extensions required.
A 100 mm back focus from the mounting surface accommodates camera, filter wheel, electronic focuser, and off-axis guider without extension tubes. The 2.75 μm per arcsecond image scale is matched to modern small-pixel CMOS sensors — making the most of every pixel in the frame.
Purpose-built for imaging. Not retrofitted for it.
Observable Space — the PlaneWave and OurSky collaboration — built the FSCT8 as an imaging instrument from the ground up. Mirror material, corrector geometry, tube construction, back focus distance: every decision serves the astrophotographer. This is not a visual SCT with a reducer bolted on. It is a dedicated astrograph that fits in a carry-on bag.
8-inch aperture. Mid-range mount. Dark-sky remote site. All viable.
At under 9 kg and just 267 mm OTA length, the FSCT8 is mountable on equatorial platforms that a conventional 8-inch SCT with reducer stack would overload. It travels as carry-on, sets up in minutes, and puts professional-grade optical performance within reach of any dark-sky site — no permanent observatory required.
NGC 6992. The Eastern Veil Nebula.
Supernova remnant in Cygnus. Delicate filamentary emission structure that demands long exposures from slower systems resolves here in a fraction of the integration time — f/2.8 working exactly as intended.
M97. The Owl Nebula.
Planetary nebula in Ursa Major, approximately 2,600 light years distant. Extended shell structure and the characteristic owl-eye cavities resolved in a single night — a target that a slow system would need multiple sessions to match.
More signal per hour. Every clear night finally worth the effort.
Native f/2.8 focal ratio — the first fast SCT in an 8-inch system, designed for wide-field deep-sky imaging from the optical axis out
42 mm fully illuminated image circle with optical performance under 6.2 μm RMS across the full field — sharp stars edge to edge
Fused silica (optical-grade quartz) primary (210 mm) and secondary (114 mm) mirrors with enhanced aluminium coatings for temperature stability
Carbon-fibre upper cage construction — 267 mm OTA, under 9 kg total weight for use on mid-range to high-end imaging mounts
88 mm broadband AR-coated corrector lens delivers a flat focal plane and 2.75 μm per arcsecond image scale suited to modern CMOS sensors
100 mm back focus from mounting surface — accommodates cameras, filter wheels, and electronic focusers in a standard imaging train
4°+ field of view with a 42 mm sensor — ideal for large emission nebulae, galaxy groups, and all-sky survey programmes
An Observable Space instrument — the merger of PlaneWave precision optics engineering and OurSky imaging systems expertise, purpose-built for the astrophotographer
Every number that matters.
The fast SCT, reimagined. Backed by Australia’s telescope authority.
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 |
$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 $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 $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.
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Fast one-star alignment, with optional two-star alignment for higher accuracy
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Compatible with SkySafari, Stellarium, Cartes du Ciel, TheSky, and other ASCOM software
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Works on Windows, macOS, Android, and iOS devices
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Extremely low power consumption, up to 100 hours from a 15,000 mAh USB power bank
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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.
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Built-in encoders and real-time clock maintain accurate sidereal, lunar, and solar tracking rates
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Control via WiFi or Bluetooth using SkySafari, Stellarium, or ASCOM/INDI software
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Compatible with Windows, macOS, Linux, iOS, and Android
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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?
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Sharper images with almost 50% less coma than f/3.7
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Smaller central obstruction (3.5" secondary vs 4.0" on f/3.7)
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Easier to achieve perfect collimation
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Better suited for high-magnification lunar and planetary observing
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A coma corrector is helpful but not essential for many users
Why choose f/3.3 or f/3.7?
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No ladder required at all for f/3.3; only a small step may be needed for f/4.2 near zenith
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Extremely wide true field of view, especially with f/3.3
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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 |
$3,499.95
A new modern large Maksutov telescope for superb viewing and imaging
- 200 mm Maksutov Cassegrain flat field optics Edge to edge sharpness and contrast
- 2000 mm focal length at F10 Large 44 mm image height support
- Optional 0.7x focal reducer compatibility
- Compact well balanced OTA design
Overview
Available May 2026!
Discover why "Maks" are renowned for their sharp imaging and visual observation with the new Sky-Watcher Skymax 200DX Maksutov Cassegrain Telescope
The Sky-Watcher Skymax 200DX Maksutov Cassegrain Telescope is a premium 200 mm optical system built for astronomers and astrophotographers who want exceptional sharpness, strong contrast, and consistent field flatness across a large image circle.
Designed around an optimised flat field Maksutov Cassegrain layout, the Skymax 200DX delivers clean, accurate performance for detailed visual observation and high resolution imaging.
With an effective aperture of 200 mm and a focal length of 2000 mm at F10, this telescope excels at revealing fine surface detail on the Moon and planets while also delivering strong results on compact deep sky targets. Its advanced optical design helps suppress off axis coma and other aberrations, producing consistent star images from the centre of the field right through to the edge.
For imaging applications, the Skymax 200DX includes a generous 44 mm image height, making it well suited for modern large sensor cameras and full frame astrophotography workflows. For users wanting wider fields and faster exposure times, an optional 0.7x focal reducer is available, expanding flexibility without taking away from the telescope’s refined optical purpose.
Despite its high performance optical profile, the Skymax 200DX remains compact and well balanced, making it a practical option for permanent observatory setups or portable imaging rigs when paired with a suitably rated equatorial mount.
Specifications
| Sky-Watcher Skymax 200DX Maksutov Cassegrain Telescope | |
|---|---|
| Optical Design | Maksutov Cassegrain |
| Effective Aperture | 200 mm |
| Focal Length | 2000 mm |
| Focal Ratio | F10 |
| Image Height | 44 mm |
| Optional Focal Reducer | 0.7x |
| OTA Length | 665 mm |
| OTA Diameter | 235 mm |
| OTA Net Weight | 12kg |
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?
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Approximately 30% less coma than the f/4.5 version
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No coma corrector required for most observers
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Lower cost, saving around $500
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Smaller central obstruction (2.76" secondary vs 3.1" on f/4.5)
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Optimised for observers seeking the cleanest possible visual performance
Why choose f/4.5?
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Lower eyepiece height, no ladder required for most users
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Wider true field of view, ideal for large nebulae and star fields
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Slightly more compact overall system
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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 |
$14,990.00
Pictured Telescope is a prototype. (binoviewer not included)
- The APO140FL F/9.6 features an air-spaced apochromatic-doublet objective with a Fluorite (CaF2) rear element that results in a lighter objective.
- The objective weighs about 2.5 lbs., compared to 5 lbs. for the APO140FL F/7 version, allowing it to come to temperature more quickly.
- Starting 2025, the objective includes anti-reflective and hydrophobic coatings for easier cleaning and maintenance.
- Housed in an aluminum cell, it provides excellent thermoregulation while remaining lightweight and strong.
- The optical assembly is inside a lightweight aluminum tube with sharp-edged baffles.
- No collimation is needed after the scope leaves TEC.
- Comes equipped with a Starlight Instruments FTF#2545 Feather Touch Focuser with coarse and fine 9:1 planetary reduction.
- The 2" locking metal collet is temperature-insensitive and holds loads with precision and concentricity.
In classic refractor fashion, the TEC APO140FL F/9.6 is a no-compromise, no-frills design that lets the wonders of nature speak for themselves.
Recommended Accessories;
- Precision adjustable Tube Rings
- 9” Dovetail Plate and Carry Handle facilitate easy transportation and fit seamlessly with most mounts.
- Focal Reducer Corrector converts the F/7 Ratio to F/6.2 with a 115mm back focus.
- TEC Transportation Case that eases transport between observation locations.
- TEC Compact Case for easy lifting and transportation.
- 7×50 Vixen Finderscope with a TEC Finder Bracket and Base for Telescope mounting.
Testing and Quality Assurance
TEC Telescopes go through rigorous testing to ensure top quality performance. Newtonian Rings are used throughout the glass production process and TEC then use an interferometer to correct any remaining imperfections. Every telescope is then tested vigorously to reach the most optimum Strehl ratio possible. Rest assured that your telescope has been optimized to be as optically perfect as possible. If the objective does not reach TEC's expectations, the telescope will not be shipped. As a strict policy, TEC will not release telescope test reports.
While the objectives are fine-tuned under interferometrical control to meet the highest optical standards, cosmetic imperfections may exist in the objective and the tube assembly. Please rest assured that any imperfection in the telescope has been determined not to affect the optical performance.
Specifications
| Clear Aperture | 140mm |
| Focal Length | 1345mm |
| Focal Ratio | 9.6 |
| Resolution | 0.86 arc sec |
| Back Focus Distance | 250mm |
| Dew Shield Diameter | 176mm |
| Tube Diameter | 150mm |
| Working Tube Length | 1430mm |
| Transport Tube Length | 1120mm |
| Glass Weight | 1.1kg |
| Airspace Gap | 1.5mm |
| OTA Weight (Estimate) | 7.7kg |
$2,100.00
For observation of faint nebulae and star clusters in a wide and bright field of view
The 130mm aperture newtonian reflector with excellent light gathering power is ideal for observation of faint nebulae and star clutsters, particularly for beginners who wish to start astronomical life with a large aperture excellent in light gathering power.
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AP Equatorial mount
The Advanced Polaris mount is ideally suited for beginners who want to become familiar with an equatorial mount, as well as for experienced observers looking for a simple, grab-and-go solution. The AP mount securely supports your telescope's optical tube, ensuring stable and comfortable observing. Thanks to its friction control system, the mount can be quickly and smoothly moved to your target object without the need for knobs or clamps. A wide range of optional accessories is available to customize the AP mount to meet your specific observing needs.
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Stylish design
The new stylish and modern design breaks away from the traditionally bulky image of astronomical telescopes. Weighing just 3.6 kg (excluding the counterweight), the lightweight body makes it easy to handle even full-scale telescope setups. The power supply runs on four AA batteries, which are integrated inside the mount. Additionally, the use of internal electrical contacts eliminates the need for external wiring, offering a cleaner, more user-friendly setup compared to previous designs.
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Friction control system
Simply aim at your target object by moving the optical tube by hand. The friction control system allows smooth, manual pointing of the telescope without the need for knobs or clamps.
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Simple polar alignment
The optional Polar Meter can be attached to the equatorial mount for easy and quick polar alignment. Even beginners can align the polar axis with minimal effort. While a polar axis scope is typically used for more precise alignment, the Polar Meter can be more effective—especially in locations where Polaris is not visible.
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Polar alignment scope PF-L
The PF-L polar alignment scope features a three-star alignment system and a built-in dark field illuminator, allowing you to perform polar alignment while looking directly through the scope. The illumination automatically turns off to prevent unnecessary power consumption.
To support the PF-L scope, we offer a free app called "PFL Assist" for smartphones and tablets. This app helps users visualize the correct star positions within the constellation, making polar alignment easier and more intuitive.
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R130Sf Newton reflector
The 130mm aperture newton reflector which is excellent in light gathering power is ideal for observation of faint nebulae and star clusters in a wide and bright field of view.
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APP-TL130 tripod
The compact APP-TL130 tripod is adjustable between 60 cm and 130 cm, combining the portability of a photographic tripod with the strength of an astronomical telescope tripod. The tripod feet can be switched between rubber pads and metal spikes, allowing for stable use on various surfaces without damaging indoor flooring.
Optical tube
| Primary mirror | 130mm parabolic mirror, multicoated |
| Focal length | 650mm (f/5) |
| Resolving power / Limiting magnitude | 0.89 arc sec. / 12.3 |
| Light gathering power | 345x unaided eye |
| Dimensions / Weight | L: 575mm x OD 160mm, 5.3kg (Body 4.0kg) |
| Finder scope | 6x30mm, 7°actual field of view |
Drawtube
| Visual back | 43mm, 42mm for T-ring, 31.7mm push-fit |
| Eyepiece (Dia. 31.7mm) | PL20mm (33x), PL6.3mm (103x) |
Tripod
| Material, Type | Aluminum 3-section leg |
| Dimensions / Weight | L:570⇔1,296mm, H:526⇔1,159mm, closed 598.4mm, Radius: 350⇔710mm, 3.0kg |
Others
| Accessories | Counterweight 1kg x 1 pc., 1.9kg x 1 pc. |
| Photography | Eyepiece projection, prime-focus, afocal imaging. |
| Solar observation | Not possible |
| Total weight | 14.8kg without eyepiece |
Configuration
- Optical tube assembly
- AP equatorial mount
- Eyepiece
- APP-TL130 tripod
$17,325.00
Best for serious astrophotographers who demand a perfect imaging platform with user-friendly functions that allow for comfortable operation.
The AXJ-A103S package comes with the quad element AX103S apochromatic system that features SD glass for uncompromising optical performance, the pinnacle of this aperture class. The mount comes with a sturdy but lightweight ASG-CB90 tripod made of carbon fiber.
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AX103S optical tube assembly.
The three-element objective lens, which includes a centre SD glass element, delivers crystal-clear, sharp, and high-contrast images with no noticeable false colour. Additionally, the built-in field corrector lens ensures that star images remain as small as 20 microns at the edge of the imaging field. Premium AS coatings are applied to every lens surface, enhancing visible light transmission to 99.5% (for wavelengths between 400nm and 700nm), ensuring exceptional light transmission across the entire visible spectrum.
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AXJ equatorial mount.
The AXJ mount, equipped with the advanced Ultimate Periodic Error Correction (VPEC) system, provides highly accurate tracking with precision of +/- 4 arc seconds or better. The VPEC operates automatically during use, ensuring seamless performance. The mount's belt drive system significantly reduces backlash and minimizes motor noise, while delivering quick and stable motor response. Additionally, the AXJ mount supports a maximum payload of 22 kg.
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STAR BOOK TEN star chart go-to navigation controller.
The STAR BOOK TEN features an intuitive "Star-Chart Go-To" system with a high-definition colour LCD display. It shows detailed information, including the telescope's position, the target, and other useful data. The night vision mode can be activated to illuminate the entire screen in red, reducing brightness to protect the observer's night vision.
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Durable and lightweight carbon tripod.
The ASG CB90 is a compact and lightweight tripod which is constructed of durable carbon fibre legs. Also, the tripod head, leg extension part and leg brace have been reviewed completely to realize a highly stable tripod for the AXJ mount.
Optical Tube
| Specification | Details |
|---|---|
| Objective Lens / Effective Aperture | 103mm, triplet SD apochromatic, multi-coated |
| Focal Length (Focal Ratio) | 825mm (F8.0) |
| Resolving Power / Limiting Magnitude | 1.13 arc seconds / 11.8 |
| Light Gathering Power | 217x (unaided eye) |
| Size / Weight | 115mm dia x 762mm long (Retractable to 670mm) / 6.4 kg (Net 4.6 kg) |
| Finder Scope | 7x50mm with illuminated reticle, 7° real field of view |
Focuser
| Specification | Details |
|---|---|
| Adapter Threads / Visual Back | 60mm, 42mm for T-ring / 50.8mm and 31.7mm push fit (with Flip mirror) |
| Eyepiece | SLV20mm (41X, 73' field of view), SLV5mm (165X, 18' field of view) |
Tripod
| Specification | Details |
|---|---|
| Leg Type / Material | Two-section carbon fibre legs, extendable and opens easily with a one-touch mechanism |
| Size / Weight | Adjustable from 545mm to 900mm in length, 510mm to 815mm in height, setup space from 340mm to 520mm in radius / 3.4kg |
Others
| Specification | Details |
|---|---|
| Photography | Usable with Prime focus, Eyepiece projection, and Afocal imaging |
| Solar Observation | Available with Sun projection screen set B |
| Total Weight | 55.3kg |
$6,930.00
For both planetary and deep sky observing and photographic applications.
Vixen's original Catadioptric design, consisting of two high reflectivity dielectric mirrors and a unique double menisus lens unit in front of the seconday mirror, virtually eliminates both spherical aberration and field curvature excellently and delivers high quality of images. With the large 260mm aperture, the VMC260L is a true all purpose telescope in your observing sessions.
Optical Tube
| Specification | Details |
|---|---|
| Primary Mirror | 260mm effective aperture, precision spherical mirror, multicoated |
| Focal Length (Focal Ratio) | 3,000mm (F11.5) |
| Resolving Power / Limiting Magnitude | 0.45 arc seconds / 13.8 |
| Light Gathering Power | 1380× unaided eye |
| Dimensions / Weight | 304mm diameter × 680mm length (720mm including protruding focus knob) / 12.1kg (Net 10kg) |
| Finder Scope | 7×50mm with dark-field illuminated reticle, 7° field of view |
Adapter
| Specification | Details |
|---|---|
| Adapter Thread / Visual Back | 60mm and 42mm for T-ring / 50.8mm and 31.7mm push fit with flip mirror diagonal |
Others
| Specification | Details |
|---|---|
| Accessories | Dovetail attachment rail, Metal carry handle, Saddle plate |
| Photography | Usable with Prime focus, Eyepiece projection, and Afocal imaging |
| Solar Observation | Not available |
Configuration
- AXD-VMC260L
- AXD-VMC260L-P
$1,990.00
More light gathering power is great for viewing deep sky objects.
A combination of a 130mm Newtonian reflector and a simple and easy-to-use "Alt-Azimuth" mount that is comprised of parts of the AP equatorial mount.
Vixen Telescope APZ-R130Sf Description
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APZ Mount
With smooth friction control mechanism of the APZ mount, the telescope can be moved quickly by hand to your trget object. Lightweight grab-and-go telescope to take it to anywhere.
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Derived from the transformation of the AP Mount.
The mount is composed of sectional modules and units that can be easily upgraded to an AP equatorial mount with additional components.
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Sealed Ball Bearings
The sealed type ball bearings are used for movable part to eliminate from mixing in of dust particles and offer excellent durability. It ensures smooth rotation of an optical tube loaded.
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Decent 8kg Loading Weight
The rigid body and sealed ball bearings allows for using a VMC telescope with 200mm aperture.
Optical tubes
| Objective mirror, effective aperture | 130mm parabolic, multicoated |
| Focal length (Focal ratio) | 650mm (F5.0) |
| Resolving power / Limiting magnitude | 0.89 arc seconds / 12.3 |
| Light gathering power | 345x unaided eye |
| Dimensions / Weight | 160mm dia. x 575mm long / 5.3kg (Net 4.0kg) |
| Finder scope | 6x30mm Finder, 7 degrees field of view |
Eyepiece section
| Adapter threads / Visual back | 43mm and 42mm for T-ring / 31.7mm push fit |
| Eyepieces | PL20mm (33x, 89' field of view), PL6.3mm (103x, 30' field of view) |
Tripod
| Leg type, material | 3-section aluminum legs with quick-release leg clamps |
| Size / Weight | Adjustable from 570mm to 1296mm in length, from 526mm to 1159mm in height, setup radius from 350mm to 710mm / 3.0 kg |
Others
| Photography | Usable with Prime focus, Eypiece projection and Afocal imaging |
| Solar observation | Not available |
| Total weight | 12.1kg (without eyepieces) |
Configuration
- Optical tube assembly
- APZ Mount
- Eyepieces
- APP-TL130 Tripod
$8,695.00
At a glance
- Vixen's flagship model with outstanding performance and ease of use for visual observation and astrophotography.
- Features a five-group-five-element Astrography with a fast focal ratio.
|
Objective Design |
Five-group five-element SD Apochromat, AS coatings |
|
Effective Aperture |
90mm |
|
Focal Length (Focal Ratio) |
495mm (F5.5) |
|
Resolving Power |
1.29 arc seconds・ |
|
Limiting Magnitude |
11.5 |
|
Light Gathering Power |
165X unaided eye |
|
Image Circle |
60mmφ (Over 90% illumination at the round edge) |
|
Optical Tube Size |
115mm dia. X 600mm long (476mm long for storage) |
|
Weight |
4.3kg |
| Finderscope | Not included, 7X50mm Finder with illuminated reticle, 50mm XY Finder bracket II sold separately |
| Focusing System | Rack-and-pinion |
| Accessory Threads / Size | Threads/ 84mm (pitch 1mm), 60mm (pitch 1.0mm), 42mm for T-ringPush-fit / 60.2mm, 50.8mm, and 31.7mm |
| Eyepiece (31.7mm) | Not included, SLV series of eyepieces sold separately |
| Plates and/or Tube Rings | Not included, VSD Tube Ring 115S, Dual Slide Bar sold separately |
| Provided Accessories | VSD60.2 to 50.8 Adapter, 2mm and 1.5mm Allen wrenches |
$3,150.00
At a glance
- Pinpoint star images with no coma or field curvature for exceptional clarity.
- Vixen’s unique VISAC system: aspherical primary mirror, convex secondary mirror, and triplet corrector lens.
- Perfectly corrected aberrations (coma, spherical, curvature) for sharp, high-definition results.
- Edge-to-edge performance: star images under 15 microns across the full 42mm image circle.
- Versatile use: ideal for both visual observation and astrophotography, with optional F6.4 reducer for deep sky imaging.
Exceptionally Sharp Star Images with No Coma or Field Curvature — Ideal for Astrophotography
The Vixen VC200L offers outstanding performance for astrophotography, delivering pinpoint star images free of coma, spherical aberration, and field curvature — even at the edges of the image.
At the heart of this telescope is Vixen's unique catadioptric optical system, known as VISAC (Vixen Sixth-order Aspheric Cassegrain). It features a high-precision sixth-order aspherical primary mirror, a convex secondary mirror, and a triplet corrector lens. This advanced design ensures sharp, high-definition star images across a wide 42mm image circle, making it ideal for both visual observing and deep-sky imaging.
Thanks to the superior optical correction, stars remain less than 15 microns in size from center to edge — producing images that are crisp and clean across the entire field.
For those looking to capture faint deep-sky objects, an optional focal reducer is available, converting the system to a fast f/6.4 focal ratio for even better imaging performance.
Specifications
| Primary mirror | 200mm effective aperture, sixth-order aspherical mirror, multicoated |
| Focal length (Focal ratio) | 1,800mm (F9.0) |
| Resolving power / Limiting magnitude | 0.58 arc seconds / 13.3 |
| Light gathering power | 816×unaided eye |
|
Dimensions / Weight
|
232mm dia. and 600mm long / 6.9kg (6.0kg) |
| Finder scope | 7×50mm with dark-field illuminated reticle, 7 degrees field of view |
| Adapter thread / Visual back | 60mm and 42mmforT-ring / 50.8mm and 31.7mm push fit with flip mirror diagonal |
| Accessories | Dovetail attachment rail, Metal carry handle |
| Photography | Usable with Prime focus, Eyepiece projection and Afocal imaging |
| Solar observation | Not available |
In The Box
- Vixen Optics VC200L 200mm f/9 Catadioptric Telescope (Optical Tube Assembly Only)
- Vixen Optics 7x50 Finderscope
- Vixen Optics 50mm SX Finder Bracket - Short
- Vixen Optics Finder Bracket Shoe
- SX 60mm to 50.8mm Adapter
- Vixen Optics Flip Mirror System
- Dovetail Rail
- Carrying Handle
- Limited 5-Year Manufacturer Warranty
$1,600.00
Fluorite lens
A fluorite lens with less chromatic aberration is used to create a sharp image with less color bleeding.
Vixen standard Arimizo, equipped with camera tripod screw
Equipped with slide bar M. It can be mounted as it is on a stand with Vixen standard Arimizo such as AP series and SX series. Equipped with 1/4 inch and 3/8 inch screws. It can be mounted on a commercially available camera tripod.
Compatible with finder (sold separately)
Equipped with screws compatible with the Arimizo finder pedestal (sold separately). Compatible with the separately sold finder (finder legs).
Features
Compact photo visual lens barrel
A very compact photo visual lens barrel equipped with a fluorite lens.
In combination with the high-resolution HR series eyepiece, it demonstrates high visual performance despite its small aperture and short focus. Especially when observing the moon and planets, you can get a higher-grade powerful image.
It can also be used as a high-performance astro camera by using a dedicated flattener lens and reducer lens (sold separately) together. It creates a sharp image over the entire field of a full-frame SLR camera.
Specifications
Lens barrel
| Effective diameter of objective lens | 55mm / Fluorite Apochromat / Multi-coating |
| Focal length (aperture ratio F) | 300mm (F5.5) |
| Resolution / limit grade | 2.11 seconds, 10.5, etc. |
| Condensing power | 62 times the naked eye |
| Size / weight | Length 282mm (without extension tube) Outer diameter 80mm 1.5kg |
| Finder | Arimizo type pedestal (sold separately) can be installed |
Eyepiece
| Parts mounting size | Screwed in / 60mm, 43mm, 36.4mm inserted / 31.7mm |
| Eyepiece (31.7mm diameter) | 31.7mm diameter eyepiece (sold separately) can be used |
Other
| Plates, bands, etc. | Slide bar M |
| photography | Enlargement, direct focus, compact digital camera (colimate) shooting possible * A separate camera adapter etc. is required |
| Sun observation | Can be used in combination with the solar projection plate A set (sold separately) (fits, but the weight balance cannot be perfectly adjusted.) |
| Gross weight | 1.5kg (by eyepiece) |
$5,250.00
Highly advanced "photo andvisual" optical design, the flagship of Vixen SD apochromatic refractors.
Vixen AX103 features a three element objective lens, incorporating an SD lens in its center, and the fourth lens inside of the focuser drawtube. This advanced optical design produces crystal-clear, sharp and high contrast images with no trace of falese color. In spot diagrams of the AX103S, the star images are extremely concentrated and are seen as small as 20 microns at the edge of ther file of view. The precision multicoatings applied to each surface to the lenses enhances visible light transmission to 99.5% on any single surface. An optional AX103 reducer which produces fast F5.6 forcal ratio is best for imaging of deep sky objects.
| Specification | Details |
|---|---|
| Objective lens / Aperture | 103mm, triplet SD apochromatic, multicoated |
| Focal length (Focal ratio) | 825mm (F8.0) |
| Resolving power / Limiting magnitude | 1.13 arc seconds / 11.8 |
| Light gathering power | 217× unaided eye |
| Dimensions / Weight | 115mm diameter × 762mm length (retractable to 670mm), 6.4kg (Net: 4.6kg) |
| Finder scope | 7×50mm with dark-field illuminated reticle, 7° field of view |
Focuser
-
Adapter threads / Visual back60mm, 42mm for T-ring / 50.8mm and 31.7mm push fitwith flip mirror diagonal
Others
-
AccessoriesTube rings, Dovetail tube plate, Metal carry handle
-
PhotographyUsable with Frime focus, Eyepiece projection and Afocal imaging
-
Solar observationAvailable with Sun projection screen set B
Configuration
- SXD2-AX103S
- SXP-AX103S
- AXD2-AX103S
- AXD2-AX103S-P
$514.00
The 130mm aperture Newtonian reflector with excellent light gathering power is ideal for observation of faint nebulae and star clusters, particularly for beginners who wish to start their astronomical journey with a large aperture for light gathering power.
Specifications
|
Optical Design |
Newtonian Reflector |
|
Aperture |
130 mm |
|
Focal Length |
650 mm |
|
Focal Ratio |
f/5 |
|
Focuser |
Single-Speed Rack-and-Pinion |
|
Eyepiece Barrel Diameter |
1.25" |
|
Diagonal |
None |
|
Finderscope |
Yes |
|
Mounting System |
Vixen Style |
|
Optical Tube Dimensions |
57.1 x 16 cm |
In The Box
- Vixen Optics R130SF 130mm f/5 Reflector Telescope (OTA Only)
- 20mm Eyepiece
- 6.3mm Eyepiece
- 6x30 Finderscope
- Mounting Rings with Dovetail Plate
$7,560.00
For both planetary and deep sky observing and photographic applications.
Vixen's original Catadioptric design, consisting of two high reflectivity dielectric mirrors and a unique double meniscus lens unit in front of the secondary mirror, virtually eliminates both spherical aberration and field curvature excellently and delivers high quality of images. With the large 260mm aperture, the VMC260L is a true all purpose telescope in your observing sessions.
The VMC features a combination of a miniscus lens unit in front of the secondary mirror and high-precision spherical mirrors that are shaped with extreme accuracy. Spherical aberration and curvature of field are corrected to a high level of optical performance for clear and sharp images. With its 260mm aperture dielectric coated mirror, the VMC260L collects enough light for serious visual and photographic applications and for both planetary and seep sky observing.
Specifications
Optical Tube
| Specification | Details |
|---|---|
| Primary mirror | 260mm effective aperture, precision spherical mirror, multicoated |
| Focal length (Focal ratio) | 3,000mm (F11.5) |
| Resolving power / Limiting magnitude | 0.45 arc seconds / 13.8 |
| Light gathering power | 1380× unaided eye |
| Dimensions / Weight | 304mm dia. and 680mm long (720mm incl. protruded focus knob) / 12.1kg (Net 10kg) |
| Finder scope | 7×50mm with dark-field illuminated reticle, 7 degrees field of view |
Focuser
| Specification | Details |
|---|---|
| Adapter thread / Visual back | 60mm and 42mm for T-ring / 50.8mm and 31.7mm push fit with flip mirror diagonal |
Other
| Specification | Details |
|---|---|
| Accessories | Dovetail attachment rail, Metal carry handle, Saddle plate |
| Photography | Usable with Prime focus, Eyepiece projection and Afocal imaging |
| Solar observation | Not available |
$1,360.00
Equatorial mount for beginners through to experienced observers
The Advanced Polaris (AP) equatorial mount is ideally suited for beginners who want to become familiar with equatorial mount or experienced observers who want a simple grab and go mount. The AP mount securely supports your telescope optical tube for comfortable observing. With its friction control system, the mount can be quickly moved to your target object. A wide selection of optional accessories are available for the AP mount to meet your observation needs.
Clever Design
With just a 3.6kg lightweight body (without counterweight), it will be easy to handle the mount and telescope of your choice. The four AA batteries for power supply is integrated inside the body.
The motor module operates with 4 pieces of the AA batteries which are commercially available anywhere easily, not only corresponding to the alkaline battery but also economical rechargeable batteries (Ni-MH, Ni-Cd). For long term use, a commercially available USB external power supply such as USB mobile battery or USB AC adapter can be used connecting to the provided USB Micro-B terminal.
Friction Control System
Simply point the target objects by moving the optical tube by hands. The friction control system allows you to manually point the telescope at the object without using knobs and clamps.
Specifications
AP Mount
| Specification | Details |
|---|---|
| R.A. slow motion | Worm and wheel gears with 144-tooth dia. 73.5mm whole-circle movement |
| DEC slow motion | Worm and wheel gears with 144-tooth dia. 58.4mm whole-circle movement |
| Worm axis | R.A.: Dia. 11mm, DEC: Dia. 9.8mm, both made of brass |
| RA, DEC axis (Material) | Dia.59mm, friction-control (aluminium alloy) |
| Bearings | Ball-bearing, 7 pcs. |
| Counterweight bar | Dia. 20mm, Steel |
| Polar axis scope | Polar alignment scope PF-L (Optional) |
| Azimuth adjustment | Twin screw type with knob, range: 6.5°(1.4°/rotation) |
| Altitude adjustment | Tangent screw type with bolt, range* 0-65°(1.9°/rotation) |
| Drive | Electric drive by pulse motor |
| Maximum loading capacity | Approx. 6kg (Max. torque load 150kg-cm) |
| Controller terminal | D-SUB9PIN Male |
| Power supply | AA Battery x 4pcs (Alkaline, Ni-MH, Ni-Cd), or USB compatible external power supply |
| Power consumption | DC5V 0.2-0.5A (1.0-2.5W) |
| Power duration time (Battery drive) | Approx. 4 hours (Alkaline battery, 6kg, 20℃) |
| Dimensions | 274x310x96mm |
| Weight | 3.9kg without battery and counterweight |
$2,199.00
Designed in Japan, Made in Taiwan
Sharp Optical System & Performance
- Superb ED class for remarkable image clarity. Crystal clear, superb sharp, almost zero aberration and distortion.
- 2 ED Glasses S-FPL 53 & S-FPL 51 & Lanthanum - Fully Separated Triplet (FST)
Fully Multi-coated optics ensures maximum light transmission - Impressive user experience, designed for both visual observation and astrophotography
Precision focusing & mechanical design throughout
- Finely CNC machining aluminium body and patented rack and pinion focuser for heavy loading 360 degree rotatable for photography
- Deluxe high-glossy anodizing finish
- Retractable sunshade
- PATENTED:US 8,693,092 B2 / Taiwan 1417570
Design
At the heart of the Founder Optics FOT86 is premium performance 3-element ED APO triplet refractor, designed by a famous optical designer in based in Japan. The optical performance is impressive as a two ED glass elements are employed.
Unlike most ED triplet telescopes which use only 1 ED glass element, Founder Optics adopted 2 ED glass of S-FPL 53 and S-FPL 51 to bring a remarkable image that you'll immediately spot with even a casual viewing. With two fluoro-crown ED glass elements and fully multi-coated optics, these Founder Optics refractors provide a crystal clear, superb sharp, zero aberration and distortion image to your eyes or camera sensor.
In addition, each element is fully separated or air spaced which is not common even among APO triplet telescopes. This offers further improvements to the already impressive optical quality.
Quality
In order to complete this unique design, it requires a very high level machining and assembly capability. Founder Optics partner with an experienced factory located in Taiwan with over 50 years experience in precision manufacturing, especially for Japanese companies.
Besides manufacturing know-how, the high standard of quality control is also crucial to producing FOT86 and FOT106 telescopes. This is recorded in a Quality Certification Card.
Every unit is thoroughly tested, and these unique records help customers understand the quality of their telescope. Founder Optics take their quality checking very seriously as they aim to offer the best triplet APO telescopes to BINTEL customers.
Focuser - 2'' Rack & Pinion
Perfect Hybrid Drive system with 8 Ball bearings- More Smoothly!
2sets of 4pcs ball bearing at 2 sides between the drawtube and the focuser handle linear travel of the focuser. Once the locked the knob, there is no gap among the drawtube, 8pcs ball bearings, and the focuser cover. It does not only keep the focuser always paralleled the optic axis, but also keep it moved very smoothly.
Dual Speed Focuser- 1:11 – Extremely Accurate!
Smooth focus motion and fine focus wheel allow precision adjustment from critical focusing of eyepiece or camera.
Unique Lock Function– Heavy Loading Capability!
Special lock grabs the rack& pinion & drawtube in two directions. The design makes the focuser always paralleled the optics axis. Instead of pushing against the drawtube to eliminate focus shift while it’s focused. And it can handle up to 8kg as well for complex imaging trains.
Longer Traveling Distance– Suitable for a range of Photographing Accessories!
Unlike other focusers, the long travel 95mm provides more room for adjust for fine and accurate focus.
It is compatibly for a wide range of photographic accessories, along with easy to use controls.
Solid, lockable Dew Shield
Built in sliding dew shield. Three screws hold dew shield stable while imaging or observing while keeping it place during transport.
Specifications:
Optical System: 2 ED APO Triplet (Fully Separated Elements)
Clear Aperture: 86mm
Focal Length: 560mm
Image Circle (with Field Flattener): Ø44mm
Focuser: 2’’ Rack & Pinion Patented Focuser (Twist Lock)
Weight: OTA: 3.5kg/ with Tube Ring: 4.6kg
Diameter of Main Tube: 90mm
Tube Length: Fully Retracted: 456mm/ Fully Extended: 545mm
What's in the Box:
1) High Quality Aluminium Case with Key
2) FOT106/ FOT86 with Patent Rack & Pinion Focuser
3) 1.25’’/ 2’’ Twist Lock Adapter
4) Crank Handle with 1pc 1/4"-20 Hexagon Screw
5) Tube Rings with 4pcs Dovetail Screws
6) Star Finder Shoe
7) Field Flattener (M42) with Exchangeable M48 Adapter
8) 7’’ Vixen Type Mount Dovetail
9) Quality Certification Card with Serial Number
10) Cleaning Cloth
11) Dust Caps (for Objective Lens)
Instruction FOT86 Manual
EX-Display Model, 6 Month Warranty
Bintel Ganymede 80mm Semi - APO
- 2021 Whole New Design
- Quality fluorite lens design
- Advanced 2-element objective lens system minimizes colour aberration
- Fully multi-coated optics ensures utmost light transmission
- Finely CNC machining aluminium body and focuser
- Deluxe high-glossy anodizing finish
- Retractable sunshade
- Accept all 1.25” universal telescope eyepieces
- Optical design: Refractor
- Aperture: 80mm
- Focal Length: 500mm
- Focal Ratio : f/6.25
- Lens: ED APO S-FPL53 Doublet, Fully Multi-Coated
$24,990.00
An extension of the highly popular APO140FL, the APO160FL F/7 allows the observer to delve deeper into the beauty of space.
- The TEC APO160FL F/7 features an oil-spaced apochromatic-triplet objective with a Fluorite (CaF2) middle element, resulting in color correction that is optimized for visual use and imaging. This oil-spaced triplet design in combination with multi-layer coatings on all surfaces of the objective ensure maximal light transmission.
- The objective is housed in an aluminum cell, providing for excellent thermoregulation properties while remaining lightweight and strong.
- The optical assembly sits in a lightweight aluminum tube that utilizes anti-reflective coating and sharp-edged baffles throughout the interior and forget about collimation – after the scope leaves TEC, no adjustment is required.
- Further, the crisp all white assembly projects the elegant, handcrafted quality that TEC is known for. Expect deep contrast and rich, natural color out of this compact and timeless design.
-
Each APO160FL F/7 comes equipped with a Starlight Instruments FTF#3545 Feather Touch Focuser that was designed in collaboration with TEC. This is Starlight Instruments’ largest rotating focuser with coarse and fine focusing 9:1 Planetary Reduction Assembly.
- The APO160FL F/7 can be fitted with to other focuser models by request. Please contact TEC to confirm whether the desired focuser will fit with the desired TEC model.
- The 2” locking metal collet is insensitive to temperature fluctuations and holds loads with high precision and concentricity.
- It also comes equipped with a Focuser wheel for easy mount installation and direction.
- Available for purchase as a Binocular Telescope. This requires the purchase of 2 APO160FL F/7.
- Able to accommodate a wide variety of eyepieces and mounts.
In classic refractor fashion, the TEC APO160FL F/7 is a no compromise, no frills design that lets the wonders of nature speak for themselves.
Please know that ALL PRICES AND AVAILABILITY ARE SUBJECT TO CHANGE WITHOUT NOTICE
Recommended Accessories;
- Precision adjustable Tube Rings
- 12” Dovetail Plate and Carry Handle facilitate easy transportation and fit seamlessly with most mounts. The larger size fits effortlessly with our larger models.
- Focal Reducer Corrector converts the F/7 Ratio to F/6.2 with a 115mm back focus.
- 160mm Field Flattener with an 85mm back focus.
- 7×50 Vixen Finderscope with a TEC Finder Bracket and Base for Telescope mounting.
Testing and Quality Assurance
TEC Telescopes go through rigorous testing to ensure top quality performance. Newtonian Rings are used throughout the glass production process and TEC then use an interferometer to correct any remaining imperfections. Every telescope is then tested vigorously to reach the most optimum Strehl ratio possible. Rest assured that your telescope has been optimized to be as optically perfect as possible. If the objective does not reach TEC's expectations, the telescope will not be shipped. As a strict policy, TEC will not release telescope test reports.
While the objectives are fine-tuned under interferometrical control to meet the highest optical standards, cosmetic imperfections may exist in the objective and the tube assembly. Please rest assured that any imperfection in the telescope has been determined not to affect the optical performance.
| Clear Aperture | 160 mm |
| Focal Length | 1120 mm |
| Focal Ratio | 7.0 |
| Resolution (Theoretical) | 0.75 arc sec |
| Dew Shield Diameter | 7.91″ / 201 mm |
| Tube Diameter | 6.38″ / 162 mm |
| Tube Length (Retracted) | 39″ / 991 mm |
| Tube Length (Dew Shield Extended) | 47″ 1194 mm |
| Length Incl. Focuser Fully Extended | +3.5″ / 114 mm |
| Length in Working Position with the Focuser in Middle of Focusing Range | 50.7″ / 1288 mm |
| Dist. From Focuser End to Focal Plane (Back Focus) | 7.48″ / 190 mm +-1 |
| Center of Gravity from the Middle of the Wheel and 2.5 lbs / 1 kg load | 15.6″ / 396 mm |
| Center of Gravity from the Middle of the Wheel (Telescope Retracted) | 16.4″ / 417 mm |
| Telescope Weight | 27 lb / 12.3 kg |
| Weight Incl. Rings, Plate, Handle | 31 lbs / 14 kg |
$31,599.00
Our largest portable refractor, the APO180FL F/7 allows the observer to delve deep into the beauty of space.
- The APO180FL F/7 features an oil-spaced apochromatic-triplet objective with a Fluorite (CaF2) middle element, resulting in color correction that is optimized for visual use and imaging. This oil-spaced triplet design in combination with multi-layer coatings on all surfaces of the objective ensure maximal light transmission.
- The objective is housed in an aluminum cell, providing for excellent thermoregulation properties while remaining lightweight and strong.
- The optical assembly sits in a lightweight aluminum tube that utilizes anti-reflective coating and sharp-edged baffles throughout the interior and forget about collimation – after the scope leaves TEC, no adjustment is required.
- Further, the crisp all white assembly projects the elegant, handcrafted quality that TEC is known for. Expect deep contrast and rich, natural color out of this compact and timeless design.
-
Each APO180FL F/7 comes equipped with a Starlight Instruments FTF#3545 Feather Touch Focuser that was designed in collaboration with TEC. This is Starlight Instruments’ largest rotating focuser with coarse and fine focusing 9:1 Planetary Reduction Assembly.
- The APO180FL F/7 can be fitted with to other focuser models by request. Please contact TEC to confirm whether the desired focuser will fit with the desired TEC model
- The 2” locking metal collet is insensitive to temperature fluctuations and holds loads with high precision and concentricity.
- It also comes equipped with a Focuser wheel for easy mount installation and direction.
- Available for purchase as a Binocular Telescope. This requires the purchase of 2 APO180FL F/7.
- Able to accommodate a wide variety of eyepieces and mounts.
In classic refractor fashion, the TEC APO180FL F/7 is a no compromise, no frills design that lets the wonders of nature speak for themselves. Please know that ALL PRICES AND AVAILABILITY ARE SUBJECT TO CHANGE.
Recommended Accessories;
- 12” Dovetail Plate and Carry Handle facilitate easy transportation and fit seamlessly with most mounts. The larger size fits effortlessly with our larger models.
- Precision adjustable Tube Rings.
- Focal Reducer Corrector converts the F/7 Ratio to F/6.2 with a 115mm back focus.
- 180mm Field Flattener prevents vignetting and ensures high quality imaging.
- 10×60 Baader Vario Finderscope with a TEC Finder Bracket and Base for Telescope mounting.
- 7×50 Vixen Finderscope with a TEC Finder Bracket and Base for Telescope mounting.
- Gutekunst Compact Atmospheric Dispersion Corrector (ADC).
Testing and Quality Assurance
TEC Telescopes go through rigorous testing to ensure top quality performance. Newtonian Rings are used throughout the glass production process and we then use an interferometer to correct any remaining imperfections. Every telescope is then tested vigorously to reach the most optimum Strehl ratio possible. Rest assured that your telescope has been optimized to be as optically perfect as possible. If the objective does not reach Yuri’s expectations, the telescope will not be shipped. As a strict policy, TEC will not release telescope test reports.
While the objectives are fine-tuned under interferometrical control to meet the highest optical standards, cosmetic imperfections may exist in the objective and the tube assembly. Please rest assured that any imperfection in the telescope has been determined not to affect the optical performance.
| Clear Aperture | 180 mm |
| Focal Length | 1260 mm |
| Focal Ratio | 7.0 |
| Resolution (Theoretical) | 0.66 arcsec |
| Dew Shield Diameter | 9.11″ / 231.5 mm |
| Tube Diameter | 7.56″ / 192 mm |
| Tube Length (Retracted) | 44.5″ / 1130 mm |
| Tube Length (Extended) | 53″ / 1346 mm |
| Focuser Tube Fully Extended | +3.5″ / 114 mm |
| Length in Working Position with the Focuser in Middle of Focusing Range | 56.1″ / 1425 mm |
| Dist. From Focuser End to Focal Plane (Back Focus) | 8.27″ / 210 mm +-1 |
| Center of Gravity from the Middle of the Wheel and 2.5 lbs / 1 kg load | 19.7″ / 500 mm |
| Center of Gravity from the Middle of the Wheel (Telescope Retracted) | 21.3″ / 540 mm |
| Tube weight | 36.5 lb / 16.5 kg |
| OTA Weight with Rings, Plate, Handle | 40 lbs / 18.2 kg |
$14,990.00
Owing homage to one of TEC’s earliest designs, the APO140ED, the APO140FL F/7debuted in 2017 and has quickly become TEC’s most popular model.
- The APO140FL F/7 features an oil-spaced apochromatic-triplet objective with a Fluorite (CaF2) middle element, resulting in color correction that is optimized for visual use and imaging. This oil-spaced triplet design in combination with multi-layer coatings on all surfaces of the objective ensure maximal light transmission.
- The objective is housed in an aluminum cell, providing for excellent thermoregulation properties while remaining lightweight and strong.
- The optical assembly sits in a lightweight aluminum tube that utilizes anti-reflective coating and sharp-edged baffles throughout the interior and forget about collimation – after the scope leaves TEC, no adjustment is required.
- Further, the crisp all white assembly projects the elegant, handcrafted quality that TEC is known for. Expect deep contrast and rich, natural color out of this compact and timeless design.
-
Each APO140FL F/7 comes equipped with a Starlight Instruments FTF#3545 Feather Touch Focuser that was designed in collaboration with TEC. This is Starlight Instruments’ largest rotating focuser with coarse and fine focusing 9:1 Planetary Reduction Assembly.
- The APO140FL F/7 can be fitted with to other focuser models by request. Please contact TEC to confirm whether the desired focuser will fit with the desired TEC model.
- The 2” locking metal collet is insensitive to temperature fluctuations and holds loads with high precision and concentricity.
- Able to accommodate a wide variety of eyepieces and mounts.
In classic refractor fashion, the TEC APO140FL F/7 is a no compromise, no frills design that lets the wonders of nature speak for themselves. ALL PRICES AND AVAILABILITY ARE SUBJECT TO CHANGE WITHOUT NOTICE
Recommended Accessories;
- Precision adjustable Tube Rings
- 9” Dovetail Plate and Carry Handle facilitate easy transportation and fit seamlessly with most mounts.
- Focal Reducer Corrector converts the F/7 Ratio to F/6.2 with a 115mm back focus.
- TEC Transportation Case that eases transport between observation locations.
- TEC Compact Case for easy lifting and transportation.
- 7×50 Vixen Finderscope with a TEC Finder Bracket and Base for Telescope mounting.
Testing and Quality Assurance
TEC Telescopes go through rigorous testing to ensure top quality performance. Newtonian Rings are used throughout the glass production process and TEC then use an interferometer to correct any remaining imperfections. Every telescope is then tested vigorously to reach the most optimum Strehl ratio possible. Rest assured that your telescope has been optimized to be as optically perfect as possible. If the objective does not reach TEC's expectations, the telescope will not be shipped. As a strict policy, TEC will not release telescope test reports.
While the objectives are fine-tuned under interferometrical control to meet the highest optical standards, cosmetic imperfections may exist in the objective and the tube assembly. Please rest assured that any imperfection in the telescope has been determined not to affect the optical performance.
| Clear aperture | 140mm |
| Focal Length | 980mm |
| Focal Ratio | 7.0 |
| Resolution (Theoretical) | 0.8 arc sec |
| Dew Shield Diameter | 5.9″ / 176mm |
| Tube Diameter | 5.9″ / 150mm |
| Tube Length (Retracted) | 33″ / 840mm |
| Tube Length (Dew Shield Extended) | 40″ / 1050mm |
| Length Incl. Focuser Fully Extended | +3.5″ / 114mm |
| Length in Working Position with the Focuser in Middle of Focusing Range | 43″ / 1090mm |
| Dist. From Focuser End to Focal Plane (Back Focus) | 7.9″ / 200mm |
| Center of Gravity from the Middle of the Focusing Knob 2.5 lbs / 1 kg load | 14″ / 352mm |
| Center of Gravity from the Middle of the Focuser (Telescope Retracted) | 16″ / 406mm |
| Telescope weight | 18 lbs / 8.2kg |
| Weight Incl. Rings, Plate, Handle, Finder | 21 lbs / 9.5kg |
$67,999.00
Capturing the most stunning astrophotographs possible is something our team is passionate about. From design to manufacture, our goal with the Corrected Dall-Kirkham (CDK) 20″ telescope was centered around performance and ease of use. The Planewave CDK20 f/7.7 OTA is an incredible breakthrough in telescope technology and produces no off-axis coma and no off-axis astigmatism. Additionally, the CDK20 provides a perfectly flat field so your astrophotographs will have stunning clarity from corner to corner of the image without field curvature degrading the photos. Offering the simplicity of single-mirror collimation, the stray light control of advanced baffles, structural performance created through finite element analysis (FEA), and decades of telescope design experience, the CDK20 is an exceptional diffraction-limited telescope. CDK20 users can experience pinpoint stars edge-to-edge and a 45 x 45 arcminute field of view when using large 16803 size camera sensors. When equipment fades into the background and simply performs, the astrophotography experience becomes even more fun and rewarding!
Carbon Fiber Truss Design
Minimizes thermal expansion which causes focus shift as temperature changes during an imaging session. Carbon fiber also reaches ambient temperatures quickly and is extremely lightweight and rigid to help ensure excellent imaging data is produced.
3D Printed Baffles
PlaneWave uses digital 3D printing technology to produce lightweight baffle tubes. 3D printers add successive layers of material to construct a baffle system with precision positioned internal stray light baffles to minimize vignetting and maximize image contrast. Quality baffling makes an incredible difference in overall image quality, so we ensured an optimal design was created for our telescopes.
Dovetail Expansion Joint
Allows for the difference in thermal expansion between carbon fiber and aluminum. The expansion joint allows the aluminum dovetail to expand and contract without stressing the carbon fiber lower truss. This results in images that are not distorted due to expansion, or contraction of the optical tube materials.
Delta-T Ready
For added dew prevention, the Planewave CDK20 f/7.7 OTA is internally wired with polyimide film heater pads and temperature sensor, which is ready to be controlled with the Delta-T via PlaneWave Interface 3 software.
Cooling Fans
Three fans on the backplate of the optical tube pull air through the telescope and by the primary mirror. Three fans on the side of the optical tube also blow air across the primary to ensure a boundary layer of air does not distort images. These fans help the telescope reach thermal equilibrium quickly, further reducing any distortion in images due to temperature variations. The fans are controlled by a switch on the optical tube, or can be controlled by via PWI3 software if a PlaneWave Electronic Focus Accessory (EFA Kit) is purchased.
Planewave CDK20 f/7.7 OTA Specifications
Optical System
| Aperture | 20 inch (508 mm) |
| Focal Length | 3951 mm (155.55 inch) |
| Focal ratio | f/7.77 |
| Central Obstruction | 39% of the Primary Mirror Diameter |
| Back Focus from mounting surface | 10.61 inch (269.49 mm) |
| Weight | 140 lbs (63.5 kg) |
| OTA Length | 47 inch (1,194 mm) |
| Upper Cage | Carbon fiber truss |
| Lower Cage | Carbon fiber truss with carbon fiber light shroud |
| Optimal Field of View | 52mm image circle |
Secondary Mirror
| Diameter | 7.5 inch (191mm) |
| Material | Fused silica (quartz) |
| Shape | Spherical |
| Coating | Enhanced Aluminum – 96% |
Primary Mirror
| Optical Diameter | 20 inch (508 mm) |
| Outer Diameter | 20.5 inch (521 mm) |
| Shape | Prolate ellipsoid |
| Material | Fused silica (quartz) |
Lens Group
| Diameter | 90 mm (3.54 inch) |
| Number of lenses | 2 |
| Coating | Broadband AR Coatings (less than .5% reflected from 400 to 700nm) |
| Optical Diameter | 20 inch (508 mm) |
Standard Features
| Carbon Fiber Truss Design | Minimizes thermal expansion which causes focus shift with changes in temperature |
| Dovetail Expansion Joint | Allows for the difference in thermal expansion between carbon fiber and aluminum. The expansion joint allows the aluminum dovetail expand and contract without stressing the carbon fiber lower truss |
| Cooling Fans | Three cooling fans ejecting air from the back of the telescope and four fans blowing across the boundary layer of the mirror surface. This helps the telescope to reach thermal equilibrium quickly. The fans are controlled by a computer if the optional Electronic Focus Accessory (EFA Kit) is purchased. |
Shipping
| Crated Shipping Weight | 291 lbs (132.0 kg) |
| Crate Width | 33 inch (838 mm) |
| Crate Height | 33 inch (838 mm) |
| Crate Length | 65 inch (1,651 mm) |
Included Items
| Heating elements for dew prevention | The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover | To protect the primary mirror and inside of the optical tube |
| Flashdrive | Contains software and instructions for collimation and spacing the primary to secondary mirror |
| Wrench Set (5812A35) | Standard hex wrenches (European orders only) |
Included Accessories
| Primary Mirror Cover | To protect the primary mirror |
| PlaneWave Thumb Drive | Contains software and instructions for collimation and spacing the primary to secondary mirror |
| 12VDC Power Supply | Provides power for the fans (Not included for European Orders) |
| Wrench Set | Standard hex wrenches (European orders only) |
| (5812A35) |
Recommend Accessories
OTA Accessories
- Reducer .66x CDK20 (200166)
- Delta T Heater Part (600195)
- Hendrick Focuser (200340)
- IRF90 – Integrated Rotating Focuser (600180)
- EFA kit Electronic Focuser (EFA)
- Light Shroud CDK20 (200970)
- Dovetail Clamp CDK20 (200919)
Visual Accessories
- Mounting Bracket for Finderscopes (125360)
- Finderscope and Mounting Bracket (6009003)
- Visual Adapter – CDK20 (200399)
- 2 Inch Mirror Diagonal (D1029ED)
Mount Accessories
- Piggyback Dovetail Bars (200990)
- L-500 Direct Drive Mount (600550)
$126,999.00
Our largest refractor, the APO250VT F/8.8 allows the observer to immerse themselves in the beauty of space. This observatory class instrument provides the best visual experience that TEC has to offer.
- The APO250VT F/8.8 features an air-spaced apochromatic-triplet objective with a Fluorite (CaF2) middle element, resulting in color correction that is optimized for visual use and imaging. This air-spaced triplet design in combination with multi-layer coatings on all surfaces of the objective ensure maximal light transmission.
- The objective is housed in an titanium cell, providing for excellent thermoregulation properties while remaining lightweight and strong.
- The optical assembly sits in a lightweight aluminum tube that utilizes anti-reflective coating and sharp-edged baffles throughout the interior and forget about collimation – after the scope leaves TEC, no adjustment is required.
- Further, the crisp all white assembly projects the elegant, handcrafted quality that TEC is known for. Expect deep contrast and rich, natural color out of this compact and timeless design.
- Each APO250VT F/8.8 comes equipped with a Starlight Instruments FTF#3545 Feather Touch Focuser that was designed in collaboration with TEC. This is Starlight Instruments’ largest rotating focuser with coarse and fine focusing 9:1 Planetary Reduction Assembly.
- The 2” locking metal collet is insensitive to temperature fluctuations and holds loads with high precision and concentricity.
- Includes precision adjustable Tube Rings.
- Able to accommodate a wide variety of eyepieces.
- Recommended to be paired with a high capacity load mount and a stationary observation station.
In classic refractor fashion, the TEC APO250VT F/8.8 is a no compromise, no frills design that lets the wonders of nature speak for themselves. Please know that ALL PRICES AND AVAILABILITY ARE SUBJECT TO CHANGE WITHOUT NOTICE
Recommended Accessories
- Adjustable Dovetail Plate and Semirings.
- 10×60 Baader Vario Finderscope with a TEC Finder Bracket and Base for Telescope mounting.
- 7×50 Vixen Finderscope with a TEC Finder Bracket and Base for Telescope mounting.
- Gutekunst Compact Atmospheric Dispersion Corrector (ADC)
Testing and Quality Assurance
TEC Telescopes go through rigorous testing to ensure top quality performance. Newtonian Rings are used throughout the glass production process and we then use an interferometer to correct any remaining imperfections. Every telescope is then tested vigorously to reach the most optimum Strehl ratio possible. Rest assured that your telescope has been optimized to be as optically perfect as possible. If the objective does not reach Yuri’s expectations, the telescope will not be shipped. As a strict policy, TEC will not release telescope test reports.
While the objectives are fine-tuned under interferomerical control to meet the highest optical standards, cosmetic imperfections may exist in the objective and the tube assembly. Please rest assured that any imperfection in the telescope has been determined not to affect the optical performance.
| Clear aperture | 250mm (10″) |
| Focal length | 2200mm |
| Focal ratio | 8.8 |
| Resolution (theoretical) | 0.5″ |
| Tube diam. | 254mm |
| Tube length (retracted) | 2000mm |
| Tube length (extended) | 2500mm |
| Tube weight | 50 kg |
$2,499.00
New Sky-Watcher 80EDX APO Telescope - redesigned body with famous Esprit optics
**Have a chat with us about availability**
Highlights:
- Air Spaced 80mm Apochromatic Triplet (APO)
- FPL-53 extra low dispersion glass
- Zero detectable colour fringing even on bright objects
- Diffraction limited optics
- Fully multi coated lenses
- 3″ CNC machined 11:1 dual speed linear power focuser – rotatable
- Indexed focuser tube
- Knife-edge baffled system to enhance contrast
The Sky-Watcher 80mm Esprit 80EDX Triplet APO Refractor is a highly portable instrument, while still having the imaging capabilities to deliver deep-sky astro photos of stunning quality. It's especially suited for those seeking wide field images and visual observations.
The air spaced apochromatic triplet lenses use the remarkable Ohara FPL-53 ED (extra low dispersion) glass, with exceptional colour correction over the entire visible spectrum there is no chromatic aberration even on bright objects! Knife edge baffles reduce internal reflections and increase contrast, helping to bring out faint structure in deep sky objects.
A 2-element field flattener is available separately to iron out the natural off-axis astigmatism and field curvature of the objective lens, leaving a fully corrected 42mm field of view.
In The Box:
- 80/400 Apochromatic Refractor
- Rotatable focuser adapter
- Collapsible Dew Shield
- 2″ Dielectric Star Diagonal
- 9×50 Right Angled Erect Image Diagonal
- D Style dovetail Bar
- 2″ to 1.25″ Eyepiece Adaptor
- Aluminium Foam-Lined Case
SPECIFICATIONS
| Model | SWESPRIT80 |
| Optical Design | Air spaced Apochromatic Triplet |
| Aperture | 800mm |
| Focal Length | 400mm |
| Focal Ratio | f/5 |
| Diameter of the corrected field | 33mm |
| Visual Back Focus | 160mm |
| Resolving Power | 1.50″ |
| Stellar Limit Magnitude | 11.8 |
| Highest Practical Magnification | 160X |
| Light gathering power (compared to the unaided eye) | 131 |
| Focuser | 3″ Crayford dual speed with 2″ and 1.25″ adaptor |
| Optical Tube Length | 380mm |
| Optical Tube Weight | 3.97g |
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