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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
Telescope OTAs
58 products
58 products
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Sky-Watcher Evostar ED72 refractors provide the finest images obtainable in their design class. These doublet refractors deliver dramatic, coal-black skies and faithful, contrast-rich views of planetary and deep-space phenomenon that are second to none. Sky-Watcher Evostar refractors are the logical choice for the discriminating amateur astronomer looking for an investment in advanced instrumentation for exceptional viewing and astrophotography, the focus position is designed for use with a camera.
This telescope is designed to be used as an astrograph, it short focal length make it ideal for imaging large star fields without the need for a large astronomical mount. However, we suggest the Skywatcher 0.85x Reducer / Corrector to flatten the wide field for better imaging results
It is also a perfect scope for Autoguiding with the addition of the ZWO ASI 120Mini Guider camera
FEATURES:
- Optical Doublet ED
- Diameter 72 mm
- Focal length 420 mm
- Focal ratio f / 5.8
- Max. Magnification 150x
- Anti-reflective treatment treatment
- 50.8 / 31.8 dual speed focuser
- Weight 1.9 kg
SUPPLIED
- Rings and “Vixen” style dovetail bar with camera mount
- High quality aluminium case for safe storage and travel
Please note: diagonal and eyepiece are not included with this telescope.
See the Universe in HD
The Celestron EdgeHD 8 is an aplanatic, flat field Schmidt-Cassegrain telescope that produces aberration-free images across a wide visual and photographic field of view. The optical system was designed to reduce more than just off-axis star coma; it also provides an astrograph-quality flat focal plane all the way to the edge of the field of view.
True Astrograph Quality
Many optical designs that advertise themselves as "astrographs" actually only produce pinpoint stars across a curved focal plane. While this may be acceptable for some visual observing, stars will appear out of focus at the edge when used with the flat chip sensor of a digital camera. EdgeHD optics produce a focal plane more than three-times flatter than a standard Schmidt-Cassegrain telescope and dramatically flatter than competing coma-free designs. This guarantees you visibly sharp stars across some of the largest CCD chips available today.
Improved Performance
Superior edge performance not only creates rounder, more pleasing stars, but actually improves the resolution and limiting magnitude when compared to telescopes of equal aperture. With StarBright XLT optical coatings on every surface, the Celestron EdgeHD 8 gives you maximum light throughput across the widest visual and photographic spectrum.
Mechanical Features
In addition to EdgeHD’s optimized optical design, the telescope tube has been redesigned to make sure you get the most from your optics each and every night.
- Mirror clutches - Flexible tension clutches hold the mirror in place and reduce image shift when taking long exposure astro-images. Once focused, the flexible rods allow the mirror to be held in place without putting any force or pressure on the mirror assembly, keeping the image centered in the eyepiece (or on the sensor).
- Tube vents - Cooling vents located on the rear cell allow hot air to be released from behind the primary mirror. Each vent has an integrated 60-micron micromesh filter guaranteed to let warm air out without letting dust in.
- Fastar versatility - EdgeHD is the most versatile imaging telescope available today. At its native f/10, you can achieve the image scale necessary to capture the smallest of deep sky objects. Add the optional reducer lens—custom-designed for your size EdgeHD tube—and you can increase your field of view without sacrificing optical performance. A Barlow gives you added power for high-resolution planetary, lunar and solar imaging. All EdgeHD optical tubes are Fastar-compatible, allowing the secondary mirror to be removed and replaced with a third party lens accessory for ultra-fast f/2 wide field imaging.
Individually Tested
Every Celestron EdgeHD 8 that ships has been tested not only for the surface quality of each optical component, but also with a camera and artificial star to ensure the imaging system meets our rigid quality assurance. This “final acceptance test” confirms the Celestron EdgeHD 8 will perform in the field and deliver high-quality astroimages.
Celestron EdgeHD 8 Whitepaper
Want the full story behind EdgeHD optics? Celestron’s Product Development team has released a whitepaper outlining the development of EdgeHD, the manufacturing and QA process, and how to get the most out of your system. It also includes cross-sections of the EdgeHD series, comparative spot diagrams for the EdgeHD and competing “coma-free” Schmidt-Cassegrain designs, a table with specifications for visual and imaging, and graphics showing how to place sensors at the optimum back-focus distance for astroimaging.
Specifications
| Optical Design | EdgeHD |
|---|---|
| Aperture (mm) | 203.2 mm (8 in) |
| Focal Length | 2032 mm |
| Focal Ratio | 10 |
| Focal Length of Eyepiece 1 (mm) | 40 mm |
| Magnification of Eyepiece 1 | 51 x |
| Finderscope | 9x50 |
| Star Diagonal | 1.25" |
| Optical Tube | Aluminium |
| Highest Useful Magnification | 480 x |
| Lowest Useful Magnification | 29 x |
| Limiting Stellar Magnitude | 14 |
| Resolution (Rayleigh) | 0.69 arc seconds |
| Resolution (Dawes) | 0.57 arc seconds |
| Light Gathering Power (Compared to human eye) | 843 x |
| Secondary Mirror Obstruction | 69 mm |
| Secondary Mirror Obstruction by Diameter | 34% |
| Secondary Mirror Obstruction by Area | 11% |
| Optical Coatings | StarBright XLT |
| Optical Tube Length | 432 mm |
| Optical Tube Weight | 6.35 kg |
| Dovetail Compatibility | CGE Mount |
Celestron EdgeHD 9.25 OTA
See the Universe in HD
EdgeHD is an aplanatic, flat field Schmidt-Cassegrain telescope that produces aberration-free images across a wide visual and photographic field of view. The optical system was designed to reduce more than just off-axis star coma; it also provides an astrograph-quality flat focal plane all the way to the edge of the field of view.
True Astrograph Quality
Many optical designs that advertise themselves as "astrographs" actually only produce pinpoint stars across a curved focal plane. While this may be acceptable for some visual observing, stars will appear out of focus at the edge when used with the flat chip sensor of a digital camera. EdgeHD optics produce a focal plane more than three-times flatter than a standard Schmidt-Cassegrain telescope and dramatically flatter than competing coma-free designs. This guarantees you visibly sharp stars across some of the largest CCD chips available today.
Improved Performance
Superior edge performance not only creates rounder, more pleasing stars, but actually improves the resolution and limiting magnitude when compared to telescopes of equal aperture. With Celestron’s StarBright XLT optical coatings on every surface, EdgeHD optics gives you maximum light throughput across the widest visual and photographic spectrum.
Mechanical Features
In addition to EdgeHD’s optimized optical design, the telescope tube has been redesigned to make sure you get the most from your optics each and every night.
- Mirror clutches - Flexible tension clutches hold the mirror in place and reduce image shift when taking long exposure astro-images. Once focused, the flexible rods allow the mirror to be held in place without putting any force or pressure on the mirror assembly, keeping the image centered in the eyepiece (or on the sensor).
- Tube vents - Cooling vents located on the rear cell allow hot air to be released from behind the primary mirror. Each vent has an integrated 95-micron micromesh filter guaranteed to let warm air out without letting dust in.
- Fastar versatility - EdgeHD is the most versatile imaging telescope available today. At its native f/10, you can achieve the image scale necessary to capture the smallest of deep sky objects. Add the optional reducer lens—custom-designed for your size EdgeHD tube—and you can increase your field of view without sacrificing optical performance. A Barlow gives you added power for high-resolution planetary, lunar and solar imaging. All EdgeHD optical tubes are Fastar-compatible, allowing the secondary mirror to be removed and replaced with a third party lens accessory for ultra-fast f/2 wide field imaging.
Individually Tested
Every EdgeHD that ships has been tested not only for the surface quality of each optical component, but also with a camera and artificial star to ensure the imaging system meets our rigid quality assurance. This “final acceptance test” confirms the EdgeHD will perform in the field and deliver high-quality astroimages.
Specifications
| Optical Design | EdgeHD |
|---|---|
| Aperture (mm) | 234.95 mm (9.25 in) |
| Focal Length | 2350 mm |
| Focal Ratio | 10 |
| Focal Length of Eyepiece 1 (mm) | 23 mm |
| Magnification of Eyepiece 1 | 102 x |
| Finderscope | 9x50 |
| Star Diagonal | 2" w/ 1.25" adapter |
| Optical Tube | Aluminium |
| Limiting Stellar Magnitude | 14.4 |
| Resolution (Rayleigh) | 0.59 arc seconds |
| Resolution (Dawes) | 0.49 arc seconds |
| Light Gathering Power (Compared to human eye) | 1127 x |
| Secondary Mirror Obstruction | 3.35 in (85 mm) |
| Secondary Mirror Obstruction by Diameter | 36% |
| Secondary Mirror Obstruction by Area | 13% |
| Optical Coatings | StarBright XLT |
| Optical Tube Length | 559 mm |
| Optical Tube Weight | 9.53 kg |
| Dovetail Compatibility | CGE Mount |
Celestron 8" F/2 RASA - Capture spectacular wide-field deep sky images in seconds with Celestron’s portable astrograph, the 8” Rowe-Ackermann Schmidt Astrograph (RASA). This incredibly fast f/2.0 system is the perfect companion to today’s color astronomical CMOS cameras, smaller CCD cameras, and mirrorless cameras. Thanks to its fast focal ratio and patented optical design, you can produce sharp, detailed images and, in many cases, skip the autoguider completely. Weighing in at just 17 pounds, it’s easy to transport your 8” RASA to the most remote dark sky locations.
RASA Performance Made for Everyone
The 8” RASA is an imaging telescope that delivers a flat field without optical aberrations for razor sharp stars across a wide field of view. It can capture stunning deep-sky astronomical images without the challenges typically presented by longer focal length instruments at a fraction of the cost of those systems.
The latest addition to the RASA family, this 8” version is a much more portable and affordable version of the heralded RASA 11, which was introduced to much acclaim in 2014. With the 8” RASA joining the lineup, a wider range of astroimagers can enjoy the benefits of the RASA design. It has many of the same thoughtfully designed features as its “big brother” RASA 11, including the integrated air-cooling system, internal filter mount, and sturdy CGE dovetail mounting bar.
Purely designed for imaging, the 8” RASA cannot be used visually. The prime focus focal plane is located at the front of the optical system, so it cannot accommodate a traditional eyepiece.
Shorter Exposure Times and Virtual “Real-Time” Observing
Since it is an F/2.0 optical system, imagers can use shorter exposure times to capture detail in faint objects. When combined with sensitive cameras and the proper “live stacking” software, the 8” RASA can provide an almost real-time observing experience. View images on a computer instantly that are brighter and more detailed than can be seen in much bigger telescopes with the naked eye.
Because shorter exposure times are possible, your equatorial mount won’t need to accurately track over extended periods. The 8” RASA’s relatively short 400mm focal length also lessens equatorial tracking demands. In many cases, autoguiding will not be required. Weighing only 17 lb, this optical tube pairs perfectly with a wide variety of mounts.
Ultra-Stable Focus System
With the launch of the 8” RASA, Celestron is unveiling a focuser design that mitigates lateral movement of the primary mirror when focusing, slewing, or tracking with the astrograph. Focusing is easier, more accurate, and more stable than ever. The key to the Ultra-Stable Focus System is two sets of precision bearings that are precisely aligned and tested during assembly to ensure optimal results.
Built for Today’s Latest Cameras
Unlike the larger RASAs that work with DSLR and large CCD cameras, the 8” model was designed with color astronomical CMOS cameras, smaller CCD cameras, and mirrorless cameras in mind. The telescope does not work with standard DSLR cameras. It is optimized for sensors with up to a 22mm diagonal, but performs well with sensors up to 32mm diagonal. The APS-C sized sensors used in many mirrorless cameras are a good choice. 42mm full frame sensors will also work, but performance will be poor at the edges of the sensor and field illumination will be reduced. Additionally, we do not recommend pairing RASA 8 with any camera body more than 4” in diameter. See the chart below to determine if your camera is compatible with RASA 8.
| Camera | Compatible with RASA 8? | Adapter required |
|---|---|---|
| Astronomical CMOS/CCD camera with C-mount | Yes | C-mount adapter (included) |
| Astronomical CMOS/CCD camera with M42-thread mount | Yes | M42 adapter (included) with M42 extension tubes (not included) |
| Astronomical CMOS/CCD camera with other mount | Yes | Custom camera adapter |
| Canon mirrorless with APS-C sensor | Yes |
Canon mirrorless adapter
(sold separately) |
| Sony mirrorless with APS-C sensor | Yes |
Sony mirrorless adapter
(sold separately) |
| Canon mirrorless with full frame (42mm) sensor | Yes, but not optimized across the full sensor |
Canon mirrorless adapter
(sold separately) |
| Sony mirrorless with full frame (42mm) sensor | Yes, but not optimized across the full sensor |
Sony mirrorless adapter
(sold separately) |
| DSLR | No | -- |
Unique Optical Design
RASA’s optical design is patented (US 2016/0299331 A1). The design consists of a Schmidt corrector, primary mirror, lens group, and optical window. The lens group contains 4 elements and utilizes rare-earth elements. Unlike many telescopes that only perform well over the visible spectrum (400-700nm), the 8” RASA’s optics are designed to perform over a wider spectral range, from 390-800nm. This allows more of the light emitted from the astronomical object to be sharply focused in the image.
With many imaging systems, adding an extra piece of flat glass such as a filter does not change optical performance. However, that is not the case with super-fast optical systems like the RASA. Our engineers addressed this by designing the RASA with a removeable optical window, so you can maintain peak optical performance if a filter is added or if a camera has its own optical window. Celestron offers a Light Pollution Imaging Filter designed specifically for the 8” RASA, which mounts in place of the optical window.
All refractive optical surfaces are coated with StarBright XLT coatings, while the primary mirror uses enhanced aluminum coatings. This maintains high light transmission through the entire optical system.
When compared with “Hyperstar SCT” systems, the RASA 8 provides better optical performance and field illumination.
| OPTICAL TUBE INFO: | |
|---|---|
| Optical Design | Rowe-Ackermann Schmidt Astrograph |
| Aperture | 203mm (8") |
| Focal Length | 400mm (15.74") |
| Focal Ratio | f/2.0 |
| Central obstruction diameter | 93mm (3.66") (46% of aperture diameter) |
| Light Gathering Power (Compared to human eye) | 843x |
| Resolution (Rayleigh) | 0.68 arc seconds |
| Resolution (Dawes) | 0.57 arc seconds |
| Image Circle | 22mm (.86") Ø, 3.15° |
| Useable field | 32mm (1.26") Ø, 4.6°, only minimal performance loss at edge of FOV |
| Wavelength range | 390 - 800 nm |
| Spot size | < 4.6 μm RMS across image circle |
| Optical Coatings | StarBright XLT |
| Off-axis Illumination | 93% at 11mm (.43") off-axis |
| Optical Window | 46mm (1.81") Ø |
| Back focus with included camera adapter | 25mm (.98") |
| Back focus from top of threaded collar | 29mm (1.14") |
| Optical Tube | Aluminum |
| Optical Tube Length | 628mm (24.7") length | 235mm (9.3") diameter |
| Focuser | Ultra-Stable Focusing System |
| Finderscope | Not included |
| Optical Tube Weight | 17 lbs (7.7 kg) |
| Other Features | Air-cooling system, integrated filter mount |
| Included items | M42 camera adapter, C-thread camera adapter, fan battery pack |
| Dovetail | CGE Dovetail Bar |
SKY & TELESCOPE’S HOT PRODUCTS 2019 AWARD
"Incredibly fast optical speeds allow deep-sky imaging with short exposures, opening up a new world of scientific- and recreational-astrophotography possibilities."
Q: Why can’t the Rowe-Ackermann Schmidt Astrograph (RASA) 8 be used visually?
A: The optics produce an image at the front end of the telescope, not the back. Therefore, you cannot look through the RASA 8 with your eyes because your head will block the light from entering the telescope. The RASA 8 is an astrograph designed specifically for deep-sky astronomical imaging.Q: Why was the RASA 8 designed to have a camera mount at the front of the telescope?
A: The RASA 8 optical design uses a prime focus focal plane position in order to obtain its super-fast F/2.0 focal ratio. This necessitates the camera having to be mounted at the front of the astrograph.Q: Won’t the camera block the incoming light?
A: The RASA 8 optical design has its own central obstruction which is caused by the sub-aperture lens assembly at the front of the telescope. The lens assembly has an outer diameter of 93mm. If a camera’s body is smaller than this, it will not block any light from reaching the camera sensor. If the camera body is larger than this, then it will block some of the incoming light. As long as the camera body does not greatly exceed about 120mm diameter, the effect on images is negligible.Q: What cameras can be used with the RASA 8?
A: The RASA 8 can be used with many astronomical CMOS and CCD cameras. It also works well with mirrorless digital cameras. Two key considerations are the size of the camera body (should not exceed about 120mm in diameter), and the camera’s backfocus distance (cannot exceed 25mm). Color or monochrome sensors can be used, although color sensors are easiest to use since the RASA 8 cannot accommodate a filter wheel (see question #7).Q: Why can’t a DSLR be used with the RASA 8?
A: The body size of a DSLR is too large compared to the front aperture of the RASA 8, and therefore blocks too much of the incoming light. Also, the DSLR requires too much backfocus (55mm) for the RASA 8, so the camera sensor cannot be placed at the required location relative to the astrograph. For DSLR imaging, we recommend the RASA 11.Q: What about camera cables in front of the optics?
A: Camera cables which cross the front of the RASA 8 do not block much light and, don’t have a significant effect on images. To minimize any potential diffraction spike around the brightest stars, camera cables can be positioned to cross the aperture in a curved pattern, rather than a straight line.Q: Will I need additional camera adapters for my camera?
A: It depends on what camera you are using. For cameras with a C-mount, no additional adapters are required. For cameras which mount with a 42mm thread, a 42mm (or T-thread) spacer ring to place the camera sensor at the proper backfocus distance relative to the optics will be needed. (Note: With the included 42mm camera adapter, the backfocus distance required is 25mm. So, subtract the backfocus distance specification for your camera from 25mm, and that is the length of the M42 spacer ring you will need. If the camera has a backfocus distance of more than 25mm, it cannot be used with the RASA 8.) For Sony and Canon mirrorless cameras, Celestron offers optional camera adapters. For other cameras, a custom camera adapter will be needed.Q: What is the difference between the image circle and the useable field?
A: The image circle is the diameter at the focal plane (i.e. where the camera sensor is positioned) which the astrograph’s performance was optimized for. The useable field is the diameter at the focal plane where the performance of the astrograph is excellent. Most astrographs only mention the useable field in their specifications.Q: What if my camera’s sensor is larger than the useable field?
A: The RASA 8 has a useable field of 32mm. A sensor with a diagonal size larger than that, such as a full-frame mirrorless camera, can be used, but there will be some drop off in optical performance and field illumination in the corners of the image. This may require cropping during image processing.Q: Can filters be used with the RASA 8?
A: The RASA 8 has a removeable optical window which can be replaced with a filter. Currently, Celestron offers a Light Pollution Reduction Filter for the RASA 8. Filter “sliders” offered by some manufacturers may also work with some cameras. A filter wheel cannot be used, since the filter wheel would have to mount in front of the optics and would block too much of the incoming light.Q: Why does the RASA 8 have a removeable optical window?
A: With such a fast optical system, you cannot add a filter into the light path without adversely affecting the optical performance. With a removeable optical window, you can replace the window with a filter with no loss of performance.Q: Why is the fast focal ratio (F/2.0) of the RASA 8 such a big deal?
A: Because it allows much shorter exposures to be used to capture detail in fainter astronomical objects. This makes getting good images much easier and quicker. With a sensitive high-speed camera along with live image stacking software, you can see images in “real-time” on your computer screen.Q: What mounts can be used with the RASA 8?
A: Any mount which can accept a CGE (or Losmandy D) dovetail bar and can handle at least 20 lbs. The RASA 8 weighs 17 lbs, and you’ll also need to account for the weight of your camera and any other accessories.
Q: Will I need to collimate (i.e. align) the optics?
A: The optics are aligned at the factory, and should not normally need adjustment. However, there are screws which adjust the tilt of the lens assembly should collimation adjustment ever be needed.
Q: What is focus shift, and how does the Ultra-Stable Focus System (USFS) help to minimize it?
A: Focus shift is when the image in your camera moves a little bit when focusing. This can make critical focusing more challenging. The RASA 8 focuses by moving the primary mirror inward-and-outward. If the mirror moves at all laterally, then focus shift will result. The USFS works by using pre-loaded precision ball bearings on the focus tube which the primary mirror rides on. This constrains any lateral motion of the primary mirror and minimizes focus shift. This also helps prevent any unwanted lateral motion of the primary mirror (also known as “mirror flop”) as the astrograph is pointed to different positions in the night sky.
Q: What is the extended spectral range (400-800 nm) and what is the benefit?
A: Most telescopes are designed to perform well over the visual spectrum (i.e 400-700nm). The RASA 8 optics were designed to perform over a wider spectral range, from 400-800nm. This means that light from 700nm-800nm will be well focused in the RASA 8, allowing more of the light emitted from the astronomical object to be sharply focused in the image. For cameras which have spectral response in the 700-800nm range, you’ll get brighter and sharper images and won’t necessarily need to use an IR-cut filter.
Q: What else might be needed with the RASA 8?
A: A finderscope can be useful for visually finding objects or for initial alignment of your computerized mount with the night sky. The RASA 8 has mounting holes for a finderscope. If doing longer exposures, you may want to consider using a guide scope and autoguider in order to provide the best tracking performance with your mount. For convenient mounting of a guide scope, Celestron offers a CGE dovetail accessory mounting bar which connects to the top of the RASA 8 and allows easy installation of guide scope rings. Perhaps the most useful accessory is a focus motor, this permits focusing from the computer which is controlling the camera and/or mount. A focus motor which is compatible with the RASA 8 will soon be introduced by Celestron.
Q: What is the purpose of the integrated air-cooling system?
A: The RASA 8 will perform the best when its optics have reached thermal equilibrium with the outside air. The cooling system uses a fan and vents to pull air through the astrograph and around the primary mirror in order to help the RASA 8 reach thermal equilibrium more quickly.
Q: What is the difference between RASA 8 and an 8” SCT or EdgeHD using the Starizona Hyperstar accessory?
A: The RASA 8 provides better optical performance and better field illumination than an 8" SCT or Edge HD with a Hyperstar accessory. The Hyperstar accessory provides great flexibility for an SCT or EdgeHD optical system, as it allows the telescope to be used at two different focal lengths. When imaging at F/2.0 however, it cannot provide the performance of the RASA 8.
Q: What about dew?
A: Just like any telescope design which uses a lens at the front of the telescope, the RASA 8 Schmidt corrector lens can be susceptible to dew under certain environmental conditions. To prevent dew when the outside temperature drops below the dew point, we recommend using a dew shield or dew heater.
$499.00
SkyWatcher Evoguide ED50-V2
Sky-Watcher’s new Evoguide ED50-V2 with ED lenses and low dispersion 50mm diameter.
The 31.8mm ring focuser allows you to use the Evoguide ED50 both as a finder and as a guide telescope, in fact, it is equipped with a T2 thread to allow the attachment to most of the driving and shooting cameras on the market. It is obviously compatible with 31.8mm eyepieces. The Evoguide ED50 is equipped with collimated rings, each with 3 nylon-tipped screws. The Evoguide ED50 has a Vixen mini bar, compatible with the majority of commercially available bases.
Ideal as a high-quality finder and guide telescope.
EVOGUIDE 50ED-V2 Features:
- Designed for use with all Autoguiders
- High-quality ED Glass
- Small compact size
- Vixen Style Dovetail Foot
- 242mm (f/4.8) focal length
- Advanced color correction
- Helical Focuser
| Evoguide ED50-V2 Specifications | |
| Optical Design | Apochromatic Refractor |
| Aperture | 50mm |
| Focal Length | 242mm |
| Focal Ratio | f/4.8 |
| Mounting | Vixen Style Dovetail Bar |
| Dimensions |
Length: 267mm with extender
Length: 226mm without extender Diameter: 56mm |
| Weight | 862g |
| Package weight | 1.1kg |
| Box Dimensions | (L x W x H) 337mm x 203mm x 127mm |
You might also like these accessories ...
The Sky-Watcher family of EvoStar ED telescopes started with the 80ED, a value for money favourite of astronomers all over the world.
The new Sky-Watcher Evolux 82ED refractor is perfect for those looking for a compact and ultra-transportable instrument ideal for Wide Field, Deepsky astrophotography.
An optional custom designed 0.90X reducer/ flattener is available as an option.
It flattens the field for pinpoint stars right out to the edges, whilst reducing the focal length to 480mm
The new EVOLUX 82ED continues this tradition with major enhancements including:
- Unparalleled levels of optic performance for an ED telescope
- Updated 2-lens element design
- New ED glass
- 82mm / f 6.4 (f5.8 with optional reducer)
- New optional re-designed dedicated reducer/field flattener for wider field of view and faster imaging
- Retractable integrated dewshield for improved handling
- Precision 61mm (2.4″) dual-speed focuser
Here's a great mount option:
Specifications:
- Focal length=530mm / f = 6.4
- Focal length = 480mm / f=5.8 with optional dedicated reducer/flattener for wider field of view
- Net Weight: 2.6kg
- Retractable dewshield for compact handling and storage
- High precision new 61mm (2.4″) dual-speed focuser
- Aluminium hard case
- V style Dovetail
The Sky-Watcher family of EvoStar ED telescopes started with the 80ED, a value for money favourite of astronomers all over the world.
The new Sky-Watcher Evolux 62ED refractor is perfect for those looking for a compact and ultra-transportable instrument ideal for Wide Field, Deepsky astrophotography.
An optional custom designed 0.90X reducer/ flattener is available as an option.
It flattens the field for pinpoint stars right out to the edges, whilst reducing the focal length to 360mm
The new EVOLUX 62ED continues this tradition with major enhancements including:
- Unparalleled levels of optic performance for an ED telescope
- Updated 2-lens element design
- New ED glass
- 62mm / f 6.5 (f5.8 with optional reducer)
- New optional re-designed dedicated reducer/field flattener for wider field of view and faster imaging
- Retractable integrated dewshield for improved handling
- Precision 61mm (2.4″) dual-speed focuser
Here's a great mount option:
Specifications:
- Focal length=400mm / f = 6.5
- Focal length = 360mm / f=5.8 with optional dedicated reducer/flattener for wider field of view
- Net Weight: 2.5kg
- Retractable dewshield for compact handling and storage
- High precision new 61mm (2.4″) dual-speed focuser
- Aluminium hard case
- V style Dovetail
$8,499.00
Normally available for pickup or shipping approx. 2-3 business days from your order
Celestron EdgeHD 11 OTA
See the Universe in HD
EdgeHD is an aplanatic, flat field Schmidt-Cassegrain telescope that produces aberration-free images across a wide visual and photographic field of view. The optical system was designed to reduce more than just off-axis star coma; it also provides an astrograph-quality flat focal plane all the way to the edge of the field of view...
True Astrograph Quality
Many optical designs that advertise themselves as "astrographs" actually only produce pinpoint stars across a curved focal plane. While this may be acceptable for some visual observing, stars will appear out of focus at the edge when used with the flat chip sensor of a digital camera. EdgeHD optics produce a focal plane more than three-times flatter than a standard Schmidt-Cassegrain telescope and dramatically flatter than competing coma-free designs. This guarantees you visibly sharp stars across some of the largest CCD chips available today.
Improved Performance
Superior edge performance not only creates rounder, more pleasing stars, but actually improves the resolution and limiting magnitude when compared to telescopes of equal aperture. With Celestron’s StarBright XLT optical coatings on every surface, EdgeHD optics gives you maximum light throughput across the widest visual and photographic spectrum.
Mechanical Features
In addition to Celestron EdgeHD 11 OTA optimized optical design, the telescope tube has been redesigned to make sure you get the most from your optics each and every night.
- Mirror clutches - Flexible tension clutches hold the mirror in place and reduce image shift when taking long exposure astro-images. Once focused, the flexible rods allow the mirror to be held in place without putting any force or pressure on the mirror assembly, keeping the image centered in the eyepiece (or on the sensor).
- Tube vents - Cooling vents located on the rear cell allow hot air to be released from behind the primary mirror. Each vent has an integrated 95-micron micromesh filter guaranteed to let warm air out without letting dust in.
- Fastar versatility - EdgeHD is the most versatile imaging telescope available today. At its native f/10, you can achieve the image scale necessary to capture the smallest of deep sky objects. Add the optional reducer lens—custom-designed for your size EdgeHD tube—and you can increase your field of view without sacrificing optical performance. A Barlow gives you added power for high-resolution planetary, lunar and solar imaging. All EdgeHD optical tubes are Fastar-compatible, allowing the secondary mirror to be removed and replaced with a third party lens accessory for ultra-fast f/2 wide field imaging.
Individually Tested
Every EdgeHD that ships has been tested not only for the surface quality of each optical component, but also with a camera and artificial star to ensure the imaging system meets our rigid quality assurance. This “final acceptance test” confirms the EdgeHD will perform in the field and deliver high-quality astroimages.
Specifications
| Optical Design | EdgeHD |
|---|---|
| Aperture (mm) | 279.4 mm (11 in) |
| Focal Length | 2800 mm |
| Focal Ratio | 10 |
| Focal Length of Eyepiece 1 (mm) | 23 mm |
| Magnification of Eyepiece 1 | 122 x |
| Finderscope | 9x50 |
| Star Diagonal | 2" w/ 1.25" adapter |
| Optical Tube | Aluminium |
| Limiting Stellar Magnitude | 14.7 |
| Resolution (Rayleigh) | 0.5 arc seconds |
| Resolution (Dawes) | 0.42 arc seconds |
| Light Gathering Power (Compared to human eye) | 1593 x |
| Secondary Mirror Obstruction | 3.75 in (95 mm) |
| Secondary Mirror Obstruction by Diameter | 34% |
| Secondary Mirror Obstruction by Area | 12% |
| Optical Coatings | StarBright XLT |
| Optical Tube Length | 610 mm |
| Optical Tube Weight | 13 kg |
| Dovetail Compatibility | CGE Mount |
$1,599.00
Celestron C6
Striking a comfortable balance between power and portability, the Celestron C6 -A XLT OTA 6" f/10 Schmidt-Cassegrain Telescope is an ideal choice for observing objects within or beyond our solar system. It features a Schmidt-Cassegrain optical system consisting of a corrector plate, spherical primary mirror, and secondary mirror that work together to reduce spherical and chromatic aberrations to crisp and clear high-resolution images with accurate color representation with distortion - especially at the edges. Complementing the optical system is the proprietary StarBright XLT optical coating system, which improves light transmission and reflectivity across the entire visual spectrum. Perfect for mounting on a Celestron Advanced VX or alternatively a Skywatcher HEQ5 Pro.
- 6" Schmidt-Cassegrain Optical Tube Assembly
- Aluminum Optical Tube
- Celestron's premium StarBright XLT coatings
- 1500 mm focal length (f/10)
- 25 mm eyepiece included (60x)
- Visual back allows for use with 1.25" accessories
- 6x30 finderscope to help accurately find objects
- Star diagonal provides more comfortable viewing position when observing objects that are high in the sky
- Includes dovetail rail compatible with CG-5 Advanced Series mount
| Aperture (mm) | 150 mm (5.91 in) |
| Apparent Field of View | .83 " |
| Dovetail Compatibility | CG-5 Mount |
| Fastar Compatible | Yes |
| Finderscope | 6x30 |
| Focal Length | 1500 mm (59 in) |
| Focal Length of Eyepiece 1 ... | 25 mm (0.98 in) |
| Focal Ratio | 10 |
| Highest Useful Magnification | 354 x |
| Light Gathering Power (Comp... | 459 x |
| Limiting Stellar Magnitude | 13.4 |
| Linear Field of View (@1000... | 44 ft (13 m) |
| Lowest Useful Magnification | 21 x |
| Magnification of Eyepiece 1 | 60 x |
| Optical Coatings | StarBright XLT |
| Optical Design | Schmidt-Cassegrain |
| Optical Tube | Aluminum - black |
| Optical Tube Length | 16 in (406 mm) |
| Optical Tube Weight | 10 lbs (4.54 kg) |
| Resolution (Dawes) | 0.77 arc seconds |
| Resolution (Rayleigh) | 0.93 arc seconds |
| Secondary Mirror Obstructio... | 14% |
| Secondary Mirror Obstruction | 2.2 in (56 mm) |
| Star Diagonal | 1.25 |
$14,899.00
Celestron EdgeHD 14 OTA
See the Universe in HD
EdgeHD is an aplanatic, flat field Schmidt-Cassegrain telescope that produces aberration-free images across a wide visual and photographic field of view. The optical system was designed to reduce more than just off-axis star coma; it also provides an astrograph-quality flat focal plane all the way to the edge of the field of view.
True Astrograph Quality
Many optical designs that advertise themselves as "astrographs" actually only produce pinpoint stars across a curved focal plane. While this may be acceptable for some visual observing, stars will appear out of focus at the edge when used with the flat chip sensor of a digital camera.
EdgeHD optics produce a focal plane more than three-times flatter than a standard Schmidt-Cassegrain telescope and dramatically flatter than competing coma-free designs. This guarantees you visibly sharp stars across some of the largest CCD chips available today.
Improved Performance
Superior edge performance provides two distinct advantages. You'll enjoy rounder, more pleasing stars. It also improves the resolution and limiting magnitude when compared to telescopes of equal aperture. With Celestron’s StarBright XLT optical coatings on every surface, EdgeHD optics gives you maximum light throughput across the widest visual and photographic spectrum.
Mechanical Features
In addition to EdgeHD’s optimized optical design, the telescope tube has been redesigned to make sure you get the most from your optics each and every night.
- Mirror clutches - Flexible tension clutches hold the mirror in place and reduce image shift when taking long exposure astro-images. Once focused, the flexible rods allow the mirror to be held in place without putting any force or pressure on the mirror assembly, keeping the image centered in the eyepiece (or on the sensor).
- Tube vents - Cooling vents located on the rear cell allow hot air to be released from behind the primary mirror. Each vent has an integrated 95-micron micromesh filter guaranteed to let warm air out without letting dust in.
- Fastar versatility - EdgeHD is the most versatile imaging telescope available today. At its native f/10, you can achieve the image scale necessary to capture the smallest of deep sky objects. Add the optional reducer lens—custom-designed for your size EdgeHD tube—and you can increase your field of view without sacrificing optical performance. A Barlow gives you added power for high-resolution planetary, lunar and solar imaging. All EdgeHD optical tubes are Fastar-compatible, allowing the secondary mirror to be removed and replaced with a third party lens accessory for ultra-fast f/2 wide field imaging.
Individually Tested
Every EdgeHD that ships has been tested not only for the surface quality of each optical component, but also with a camera and artificial star to ensure the imaging system meets our rigid quality assurance. This “final acceptance test” confirms the EdgeHD will perform in the field and deliver high-quality astroimages.
Specifications
23 mm2581 x
| Optical Design | EdgeHD |
|---|---|
| Aperture (mm) | 355.6 mm (14 in) |
| Focal Length | 3910 mm |
| Focal Ratio | 11 |
| Focal Length of Eyepiece 1 (mm) | |
| Magnification of Eyepiece 1 | 170 x |
| Finderscope | 9x50 |
| Star Diagonal | 2" w/1.25" adapter |
| Optical Tube | Aluminium |
| Limiting Stellar Magnitude | 15.3 |
| Resolution (Rayleigh) | 0.39 arc seconds |
| Resolution (Dawes) | 0.33 arc seconds |
| Light Gathering Power (Compared to human eye) | |
| Secondary Mirror Obstruction | 114 mm |
| Secondary Mirror Obstruction by Diameter | 32% |
| Secondary Mirror Obstruction by Area | 10% |
| Optical Coatings | StarBright / XLT |
| Optical Tube Length | 787 mm |
| Optical Tube Weight | 21 kg |
| Dovetail Compatibility | CGE Mount |
$3,599.00
The Celestron C9.25-A is an unusual size with its 9.25” aperture and 2350 mm focal length, but many consider it to be the Goldilocks of optical tubes—not too big, not too small. This rugged aluminum optical tube is only 558mm long and weighs just 9kgs, making it easy to transport and set up. But the views are much more impressive than what you’d expect from such a compact instrument. The tube offers a focal ratio of f/10 with the added versatility of Fastar (see below).
It is equipped with Celestron’s patented StarBright® XLT optical coatings, which visibly increase contrast and light transmission for brighter deep space images and shorter exposure times. With StarBright XLT, you’ll be able to discern subtle details while viewing the Moon and planets as well as faint galaxies and nebulae.
The Celestron C9.25-A
Fastar Technology
In 1997, CCDs were making a name for themselves in the astrophotography world, quickly supplanting traditional film photography thanks to their speed and convenience. This was the year that Celestron joined forces with the Santa Barbara Instruments Group (SBIG) to produce Fastar, a revolutionary add-on to Celestron’s hugely popular Schmidt-Cassegrain (SCT) optical system.
With Fastar, the SCT’s secondary mirror can be removed and replaced with a field-flattening lens assembly (sold separately by third party manufacturers) so that a CCD camera can be used in the front of the telescope at the f/2 focus of the instrument’s primary mirror. The potential of the Fastar system is staggering: exposures are 25 times shorter than if the camera was placed at the instrument’s native f/10 focus. Imagers can capture galaxies and nebulae with exposures of just 30 seconds.
StarBright XLT is Celestron’s revolutionary optical coating system. It consistently outperforms all other coatings in the commercial telescope market. There are three major components that make up our StarBright XLT high-transmission optical system design:
- Unique enhanced multi-layer mirror coatings made from precise layers of aluminum, SiO2 (quartz), TiO2 (titanium dioxide), and SiO2 (silicon dioxide). Reflectivity is fairly flat across the spectrum, optimizing it for both imaging and visual observing.
- Multi-layer anti-reflective coatings made from precise layers of MgF2 (magnesium fluoride) and HfO2 (hafnium dioxide). Hafnium—a rare element that costs nearly $2,000 per kilogram—gives us a wider band pass than the titanium used in competing coatings.
- High-transmission water white glass is used instead of soda lime glass for the corrector lens. Water white glass transmits about 90.5% of light without anti-reflective coatings; that’s 3.5% better than uncoated soda lime glass. When water white glass is used in conjunction with StarBright XLT’s anti-reflective coatings, the average transmission reaches an astonishing 97.4.
$1,920.00
Standard features of Tele Vue 60 OTA include a 2-stage 1.25" focuser with quick-focus drawtube, plus fine-focus helical, exquisitely machined and anodized all-metal construction, and a sliding captive dew shield. Offering wide field, pristine, color free views throughout a wide range of magnification.
- 1.25" focuser accept in-line Porro Prism, 45° erectors or 60° and 90° diagonals
- Maximum True Field: 4.3° (great for terrestrial and astronomical use)
- Maximum Power: 180x (with Nagler™ 2-4mm Zoom - for lunar/planetary viewing)
- Adjustable dovetail balancing bar fits all camera tripods, Tele Vue Mounts and new mounting brackets for SCT's
It’s a super-finder, day/night scope with great telephoto and imaging capability for digital cameras. Optional padded carry bag available.
Specifications
| Type | APO (Doublet) Refractor |
| (Elements/Groups: 2/1) | |
| Objective (mm) | 60 |
| Focal Length (mm) | 360 |
| Focal Ratio (f/#) | 6 |
| Drawtube/Focuser | 1¼-inch, helical |
| Length OTA (inch) | 10 |
| Length with diagonal (inch) | 12 (with 1¼-inch diagonal) |
| Weight OTA/Std. Config (lbs) | 3 / 3.3 |
| Maximum Visual Field (deg.) | 4.3° (with 1¼-inch 32mm Plössl) |
| Maximum Recommended Power (x) | 150 |
QBT-1006 Tele Vue Quik Point Basic
DPC-1250 Tele Vue 1.25" 90° Everbrite Diagonal
TVB-2403 Tele Vue TV60 Carry Bag
EAD-25.0 Tele Vue 25mm Plossl
QBT-1006 Tele Vue Quik Point Basic
DPC-6012 Tele Vue 1.25" 60° Everbrite Diagonal
TVB-2403 Tele Vue TV60 Carry Bag
EAD-25.0 Tele Vue 25mm Plossl
Reviews
Excerpt from Living Bird article by Dr. KenRosenberg, director of conservation science at Cornell University's Lab of Ornithology.
TeleVue has introduced a new 60mm scope for birders, which includes the 45-degree prism, and when fitted with the same 8-24mm zoom provides powers from 15-45x. This scope is comparable in size, weight, and image quality to the best Swarovski or Kowa spotting scopes and may cost considerably less, ...
— Dr. Rosenberg, K. "Scope Quest 2008". Living Bird (2008 Winter). 46 - 47.
Excerpts from Dennis di Cicco review of the TV-60 in Sky & Telescope, December 2004
Even at 120x, brilliant Vega, one of the most challenging stars for a refractor to image cleanly, appears as a blue-white Airy disk surrounded by several white diffraction rings and no perceptible color halo.
— di Cicco, D. "Pint-Size Powerhouse: Tele Vue's TV-60". Sky & Telescope (Dec. 2004).
Read what SmartMoney has to say about the TV-60
SmartMoney magazine, The Wall Street Journal Magazine of Personal Business, is all about recommending the wisest buys for their readers. The 'Smart Spending' section of the November, 2004, issue features the article Stargazing; "Today's telescopes are so high-tech they seek out stars themselves. But we wondered: What would the world's top amateur astronomer think of them?" In this context, the Tele Vue-60 was chosen the winner by David Levy after checking out four other scopes and the Tele Vue-60.The article concludes: "Our winner gave us the best view of Jupiter, and without any gizmos. 'This is a sweet instrument,' Levy says."
— Light, J. "Stargazing". Smart Money (Nov. 2004). 133-135.
Excerpts from Raymond Shubinski's review of the TV-60 in Astronomy magazine
A note of caution: You may find yourself spending more time looking through the Tele Vue-60 than through your larger scope.
— Shubinski, R. "The Tele Vue-60". Astronomy (Nov. 2004).
Excerpts from Randy Roy's comments on Cloudy Nights Telescope Reviews website.
If you want wide field, pristine, color free views throughout a wide range of magnification -- if you want a scope that is a superfinder, a guidescope, a piggyback refractor, or an ultra-light travel scope -- and if you demand the best in fit, finish and build quality -- buy this. I've not seen anything else in its class that does so much.
— Roy, R. "Televue-60 APO". Cloudy Nights Telescope Reviews (Feb. 4, 2004).
Excerpts from TV-60 review by Ed Ting, published on The Telescope Review Web Site
- TeleVue's newest telescope is a cute little 60mm f/6 apo. In a departure from their usual styling, the TV60 has a sleek, tapered black body that resembles a spotting scope. .... The construction is heavy-duty and very serious. There's a sliding bar on the bottom that's very similar to the one on the Ranger. Like the Ranger, it has a helical focuser and drawtube assembly. Unlike the Ranger, the TV60 adds a nice sliding dew shield.
- The scope has impressive optics. .... No false color was noted. At only 15X (with a 24 mm Panoptic) Titan could be seen as a tiny pinpoint dot next to the planet. You can see Cassini's Division on Saturn at 70x (with a 5 mm Type 6 Nagler.) .... The Trapezium was easily resolved, .... Castor is an easy split. Most impressively, the scope split Rigel, again at 70X. On deep sky, you have to make some allowances for the small aperture. M35 is just starting to resolve, but the other nearby clusters (M37, M36, M38) look like similar faint smudges in the eyepiece. Not exciting, but again, we're only talking about a 60 mm telescope here.
- I once heard small scopes like this described as "One-Hour Telescopes." You get to see pretty much everything you want to see in about an hour. As such, the TV60 is a great quick peek or travel scope.
- Update, 2/7/04: TeleVue informs me that they plan to offer an X-Y heavy duty version of their Starbeam mount, so that the TV60 can be mounted on a larger scope.
— Ting, E. "Tele Vue-60". The Telescope Review Web Site (Feb. 1, 2004).
$5,999.00
Celestron C11-A XLT Optical Tube Assembly
Celestron provides their Schmidt Cassegrain optics as a tube assembly only to use with your favourite mount.
- 11" Schmidt-Cassegrain Optical Tube Assembly
- Aluminum Optical Tube
- Celestron's premium StarBright XLT coatings
- 2800 mm focal length (f/10)
- 40 mm eyepiece included (70x)
- Visual back allows for use with 1.25" accessories
- 9x50 finderscope to help accurately find objects
- Star diagonal provides more comfortable viewing position when observing objects that are high in the sky
- Includes dovetail rail compatible with CGE (wide 3") dovetails
Celestron C11-A XLT OTA Specifications
| Optical Design | Schmidt-Cassegrain |
|---|---|
| Aperture (mm) | 279.4 mm (11 in) |
| Focal Length | 2800 mm (110 in) |
| Focal Ratio | 10 |
| Focal Length of Eyepiece | 40 mm |
| Magnification of Eyepiece | 70 x |
| Finderscope | 9x50 |
| Star Diagonal | 1.25" |
| Optical Tube | Aluminum |
| Highest Useful Magnification | 660 x |
| Lowest Useful Magnification | 40 x |
| Limiting Stellar Magnitude | 14.7 |
| Resolution (Rayleigh) | 0.5 arc seconds |
| Resolution (Dawes) | 0.42 arc seconds |
| Light Gathering Power (Compared to human eye) | 1593 x |
| Secondary Mirror Obstruction | 95 mm |
| Secondary Mirror Obstruction by Diameter | 34% |
| Secondary Mirror Obstruction by Area | 12% |
| Optical Coatings | StarBright / XLT |
| Optical Tube Length | 610 mm |
| Optical Tube Weight | 12 kg |
| Dovetail Compatibility | CGE Mount |
$68,999.00
CDK20’s Key Features
Large Aperture and Moderate Focal Ratio
The CDK20 f/6.8 features a significant 508 mm aperture and an f/6.8 focal ratio. This combination provides excellent light-gathering capabilities and a wide field of view, enhancing its ability to capture detailed images of deep-sky objects for astrophotography and research purposes.
Advanced Optical Design
Equipped with a state-of-the-art Corrected Dall-Kirkham optical system, the CDK20 offers unmatched image clarity. It eliminates off-axis coma and astigmatism and provides a perfectly flat field, ensuring images are crisp and detailed across the entire field of view, requiring minimal post-processing.
Robust Mechanical Structure
Built with a carbon fiber optical tube, the CDK20 is both durable and lightweight. Its design minimizes thermal expansion, ensuring minimal focus shift with temperature changes, which is ideal for extended observing sessions under diverse environmental conditions.
High-Performance Mirrors and Coatings
Utilizing fused silica mirrors, the CDK20 maintains precise optical alignment and exceptional surface accuracy, even during temperature fluctuations. The high-quality coatings improve light transmission and reduce stray light, optimizing the telescope's performance for specialized observational tasks.
Thermal Management
The CDK20 has cooling fans and a Delta-T ready system to achieve thermal equilibrium swiftly. These features help reduce air turbulence within the tube, thus minimizing image distortion and maintaining consistent imaging quality.
Integrated Dew Control
The telescope includes advanced dew prevention technology with heater pads controlled by PlaneWave’s software. This ensures optical surfaces remain free from condensation in humid conditions, thus maintaining clear and consistent imaging performance.
Application-Specific Benefits
Astrophotography
With its large image circle and exceptional field flatness, the CDK20 allows astrophotographers to capture expansive and breathtaking views of the cosmos with incredible detail and clarity.
Astronomy Research
The stable and precise imaging capabilities of the CDK20 make it an invaluable asset for academic institutions and observatories engaged in sophisticated astronomical research, including deep-sky surveys and detailed photometric studies.
Visual Observations
The CDK20 excels in visual observation, providing bright and clear views ideal for star parties and serious visual astronomy. Its large aperture and superior optical quality deliver stunning views of planetary, lunar, and deep-sky objects, making every viewing session a memorable experience. Here's the updated article adapted for the CDK17 based on the features and specifications from the provided product page:
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
The CDK20 also lends itself to Space Situational Awareness and Space Domain Awareness applications. Its capability to provide detailed observations can be essential for tracking and monitoring satellites and other space debris, contributing valuable data for space traffic management and safety initiatives.
Optical Systems
| Aperture | 508mm (20") |
| Focal Length | 3454mm (136") |
| Focal Ratio | f/6.8 |
| Central Obstruction | 39% of the Primary Mirror Diameter |
| Back Focus From Mounting Surface | 224 mm (8.81") |
| Weight | 140 lbs (63.5 kg) |
| OTA Length | 1194 mm (47") |
| Optical Design Performance | 1.5-micron RMS on-axis, 3.8-micron RMS at 12 mm off-axis, 6.0-micron at 21 mm off-axis |
| Upper Cage | Carbon fiber truss |
| Lower Cage | Carbon fiber truss and light shroud |
| Image Circle Size | 52mm |
Secondary Mirror
| Diameter | 191 mm (7.5") |
| Material | Fused silica (quartz) |
| Shape | Spherical |
| Coating | Enhanced Aluminum - 96% |
Lens Group
| Diameter | 90mm (3.54") |
| Coating | Broadband AR Coatings (less than .5% reflected from 400 to 700 nm) |
Primary Mirror
| Optical Diameter | 508 mm (20") |
| Outer Diameter | 521 mm (20.5") |
| Shape | Prolate Ellipsoid |
| Material | Fused Silica (quartz) |
| Coating | Enhanced Aluminum - 96% |
| Included Items | Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror |
$3,599.00
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 FOT016 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 - 2.7'' 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.
Focuser Rotator Function
Flexible rotated structure provides a convenience for user to have the best position to adjust focuser when observation and photography. The precision machining parts and assembly technique make a good collimation even rotate the focuser and rotator.
Loosen the rotator knob and focuser knob to rotate the focuser and rotator.
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: 106mm
Focal Length: 636mm
Focal ratio: f/6
Image Circle (with Field Flattener): Ø44mm
Focuser: 2.7’’ Rack & Pinion Patented Focuser (Twist Lock)
Weight: OTA: 3.5kg/ with Tube Ring: 4.6kg
Diameter of Main Tube: 113mm
Tube Length: Fully Retracted: 557mm/ Fully Extended: 650mm
What's in the Box:
1) High Quality Aluminum 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 FOT106 Manual
$1,799.00
Designed in Japan, Made in Taiwan
Sharp Optical System & Performance
- Five-element ED APO lens delivers sharp, flat, colour-free images across the field.
- 0.83× reducer provides a fast f/3.9 system ideal for deep-sky astrophotography.
- 44mm image circle supports full-frame and APS-C sensors with no vignetting
Precision focusing & mechanical design throughout
- Integrated 2" dual-speed focuser with travel indicator, motor-ready design.
- Built-in tilt adjustment for fast and accurate optical axis correction.
- Threaded connections minimize flexure and focuser sag.
- 360° rotator with scale allows precise framing for astrophotography.
Mounting & use
- Comes standard with handlebar, tube rings, dovetail, and mounting rails.
- Quick-lock dew shield ring provides firm, secure attachment.
- Supports both astrophotography and visual observing use.
Tough, for the harshest environments
Nitrogen-filled optical tube is IP67-rated: waterproof, fogproof, and sealed against dust.
Lightweight design: 2.4kg OTA (3.2kg with standard accessories).
ED APO Lens
Five-element Air-space design, using ED APO lens level.
Dedicated 0.83x Reducer-f/3.9
Fast ratio f/3.9 can satisfy most deep sky astrophotography.
Waterproof & Fogproof
Nitrogen injected for waterproof IP67.
Hydrophobic coating on the air surface of the lens. Removes issues about temperature difference between indoors and outdoors found on some telescopes.
Unique Collimation Adjustment
Special design collimation function. Built-in ball bearing and a spring structure, simplifying the 12 screws into two. Makes for adjustment and accurate alignment
Mechanical Stability
Threaded components for stability. Reduces the risk of unwanted focuser movement caused by the focuser sagging during installation.
Compatibility with a wide range of Camera Adapters
Supports ZWO cameras, provides M54, M48 adapters, and can also be used with Founder Optics T2 ring mount for all camera types
Rack & Pinion focuser
One piece design- Rack & Pinion focuser and draw tube. This integrated structure reduces the mechanical clearance and assembly tolerance.
Light Weight
Only weighs 2.4kg. It’s 3.2kg including the tube ring, handle, and dovetail plate.
Ideal range of mounting accessories
Multi-functional handle, combined with the tube ring and dovetail plate. Comes with tactical slide rails to provide multiple connection options
Quick Dew Shield Lock Ring
Provides a quick dew shield locking ring, which can tighten evenly, firmly and quickly.
Visual Observation and Imaging
Support for visual astronomical observations and imaging
Specifications:
Optical System: Quintuple, air spaced ED APO lens
Clear Aperture: 62mm
Focal Length: 300mm
Focal Ratio: f/4.8, f/3.8 with 0.83x reducer
Image Circle: Ø44mm
Focuser: 2’’ Dual-Speed Rack & Pinion Focuser,
Helical Rotation Type
Weight OTA: 2.4kg
Weight with Tube Ring, dovetail plate, handle and mounting rail: 3.2kg
Optical system: 5+2 =7 Elements, Quintuplet refractor+ 0.83x reducer
Main lens: Quintuplet, Air-spaced ED APO lens
Image circle: 44mm
Back focus distance: 55mm
Included in the package:
Draco 62 Quintuplet Astrophotography Refractor
- 0.83x Focal Reducer for Draco 62
- M48 Adapter for Draco 62
- M54 Adapter for Draco 62
- 1.25'' 90 degree Mirror Dielectric Diagonal
- Diagonal Adapter
- Tube Ring
- Dovetail Plate
- Tactical rail
- Product Manual
- Quality certification card
- Large hard-shelled carry backpack
$2,599.00
The Celestron C8-A is the direct (but much improved) descendent of Celestron’s revolutionary C8 that transformed the hobby of astronomy when it was unveiled in 1970. This rugged aluminum optical tube is only 17 inches long and weighs just 13 pounds, making it easy to transport and set up. But the views are much more impressive than what you’d expect from such a compact instrument. The tube offers 2032 mm of focal length and a focal ratio of f/10, with the added versatility of Fastar (see below).
It is equipped with Celestron’s patented StarBright® XLT optical coatings, which visibly increase contrast and light transmission for brighter deep space images and shorter exposure times. With StarBright XLT, you’ll be able to discern subtle details while viewing the Moon and planets as well as faint galaxies and nebulae.
The Celestron C8-A can be mounted on a multitude of computerized telescope mounts thanks to its CGEM style dovetail bar. This iconic optical tube provides the best balance of portability, handling ease, light gathering ability and price ever offered to the amateur astronomer.
Fastar Technology
In 1997, CCDs were making a name for themselves in the astrophotography world, quickly supplanting traditional film photography thanks to their speed and convenience. This was the year that Celestron joined forces with the Santa Barbara Instruments Group (SBIG) to produce Fastar, a revolutionary add-on to Celestron’s hugely popular Schmidt-Cassegrain (SCT) optical system.
With Fastar, the SCT’s secondary mirror can be removed and replaced with a field-flattening lens assembly (sold separately by third party manufacturers) so that a CCD camera can be used in the front of the telescope at the f/2 focus of the instrument’s primary mirror. The potential of the Fastar system is staggering: exposures are 25 times shorter than if the camera was placed at the instrument’s native f/10 focus. Imagers can capture galaxies and nebulae with exposures of just 30 seconds.
StarBright XLT is Celestron’s revolutionary optical coating system. It consistently outperforms all other coatings in the commercial telescope market. There are three major components that make up our StarBright XLT high-transmission optical system design:
- Unique enhanced multi-layer mirror coatings made from precise layers of aluminum, SiO2 (quartz), TiO2 (titanium dioxide), and SiO2 (silicon dioxide). Reflectivity is fairly flat across the spectrum, optimizing it for both imaging and visual observing.
- Multi-layer anti-reflective coatings made from precise layers of MgF2 (magnesium fluoride) and HfO2 (hafnium dioxide). Hafnium—a rare element that costs nearly $2,000 per kilogram—gives us a wider band pass than the titanium used in competing coatings.
- High-transmission water white glass is used instead of soda lime glass for the corrector lens. Water white glass transmits about 90.5% of light without anti-reflective coatings; that’s 3.5% better than uncoated soda lime glass. When water white glass is used in conjunction with StarBright XLT’s anti-reflective coatings, the average transmission reaches an astonishing 97.4.
$1,499.00
150mm/1800mm Skymax 150 Maksutov-Cassegrain OTA
| Optical Design | Maksutov-Newtonian |
| Model Number | SWMAK150-OTA |
| Aperture | 150mm |
| Focal Length | 1800mm |
| Eyepieces | LET28mm |
| Focuser Diameter | 2″ |
| Finder Scope | 9 x 50mm |
| Highest Practical Power | 300x |
| Recommended Usage | Advanced |
| Recommended Usage | High Resolution Astrophotography |
The ZWO FF65 APO is a refractive astrograph with a powerful flatfield optical design which saves you from the expensive cost of a field flattener. It eliminates the trouble of calculating the back focus distance of the flattener and connecting various accessories to achieve that distance. You can just connect any possible accessories you need. As long as the target is focused, the whole optical system is perfect for imaging. This makes the whole setting up process much more convenient, and saves you time, allowing you to pay more attention to the image shooting itself.
The ZWO FF65 APO is also a nice choice for your visual observation. It fits diagonals as well as various eyepieces and can achieve a perfect focus, and can even be used to observe planets with a super-high magnification eyepiece.
The whole design of the telescope is compact and lightweight. The OTA weighs only 2kg, and the full package with tube rings and other accessories weighs 2.8kg. It has an aperture of 65mm. The focal ratio is f/6.4 and the focal length is 416mm. Instead of the quadruplet structure of the other ZWO FF APO Refractors, the FF65 APO is a quintuplet, with two ed Glass elements that offer excellent control of Chromatic and other aberrations.
The ZWO FF65 APO supports the full-frame imaging circle and has a fine spot diagram with tiny distortions of the peripheral stars. The 2.5" rigid focuser comes with a new-type 360°rotator with scales and a finder base. M68, M54, and M48 camera adapters are also attached, and the M48 adapter has a 2” female thread for installing filters.
ZWO FF65 APO Main Features
Quintuplet air-spaced APO design - No need to calculate back focus
Small and round stars - with a central RMS radius of 2.5um
Various adapters - M68/ M54/ M48
Dual speed (1:10) focuser - Support both fine and coarse adjustment
No need for a separate field flattener - Self-flattening design
Supports full-frame cameras - Produces a 44mm image circle
Optional Focal Reducer -
Specifications
| Aperture | 65mm |
| Focal Length | 416mm |
| Focal Ratio | f/6.4 |
| Image Circle | 44mm |
| Net Weight | 2kg |
| Gross Weight | 2.8kg |
| Rear End Thread Type | M68 x 1 -M54 x 0.75, M54 x 0.75 - M54 x 0.75,
M54 x 0.75 - M48 x 0.75 M48 x 0.75 mm Filter Thread Size |
| Total Length | 328mm (including 1.25″ eyepiece holder as dewshield contracted) 360mm. (including the 3-piece adapter as dewshield contracted) 388mm (including 1.25" eyepiece holder as dewshield fully stretched) 420mm (including 3 piece adapter as dewshield fully stretched) |
| Rear End of 3 Piece Photographic Adapters | M48 x 0.75 |
SKU: ZWO-FF65-APO
New from Sky-Watcher - the smallest member of their Esprit range of APO triplet refractors
The Sky-Watcher 70mm Esprit 70EDX Triplet APO Refractor is a professional instrument for the most demanding and exacting astrophotographers. The air spaced apochromatic triplet lenses have 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.
Main Features:
- Air Spaced 70mm Apochromatic Triplet
- 490mm Focal Length
- Fully multi coated lenses
- Optional 0.92x Reducer Available
In The Box:
- 70/490 Apochromatic Refractor
- Retractable Dew Shield
- D Style dovetail Bar and rings w/handle
- Aluminium Foam-Lined Case
Specifications:
| Optical Design | Airspaced Apochromatic Triplet |
| Aperture | 70mm |
| Focal Length | 490mm |
| Focal Ratio | f/7 |
| Image Height | 44mm |
| Length after Lens Hood Retracted | 368mm |
| Total Length | 420mm |
| Optical Tube Weight | 3.2kg |
$7,749.00
Capturing impressive deep-sky astroimages is easier than ever with Celestron’s Rowe-Ackermann Schmidt Astrograph (RASA 11) V2, the perfect companion to today’s top DSLR or astronomical CCD cameras. This fast, wide-field f/2.2 system allows for shorter exposure times compared to traditional f/10 astroimaging, without sacrificing resolution. Because shorter sub-exposure times are possible, your equatorial mount won’t need to accurately track over extended periods. The short focal length also lessens equatorial tracking demands. In many cases, autoguiding will not be required.
RASA 11 V2 builds on the legacy of Celestron’s Schmidt Cameras, which allowed astrophotographers to produce images with much shorter exposure times on film in the 1970s.
Today, with CCD sensor sizes as large as film or larger, the RASA 11 V2 offers a 43.3mm optimized image circle to capture pinpoint stars on the largest imaging chips. Optical performance for huge sensors with diagonals of up to 52mm wide is still excellent.
Combine this large image circle with a focal length of just 620mm and you have an instrument suitable for wide-field imaging, creating huge mosaics of the night sky, surveying, and even comet hunting.
Optical Performance
The RASA 11 V2 features optics with 4-element rare-earth glass for images free of false color and aberrations like coma and field curvature. The optical quality and spot size across the entire image circle are unprecedented for an astrograph in this price range—or even that of a much more expensive instrument. The design also provides minimal vignetting.
Advanced Features
RASA 11 V2 utilizes the Ultra-Stable Focus System (USFS). At the heart of this system is a precision linear ball bearing. The bearing serves to minimize focus shift (unwanted lateral motion of the primary mirror during focusing which causes shifting of the image) and mirror flop (movement of the primary mirror when the telescope is pointing to different positions in the sky). The USFS is also compatible with the optional Celestron Focus Motor (#94155-A). The integrated 12V DC MagLev fan reduces cooldown time and provides optimal airflow through the dust filtered optical tube.
Engineered as a complete astroimaging system, every component of the RASA 11 V2 is optimized for peak performance with DSLR and astronomical CCD cameras. Down to the thickness of the glass used in the included fully-multicoated optical window or optional imaging filter, every component of the system has been taken into careful consideration to work together seamlessly. The Dovetail CGE bars on the top of the optical tube provides a connection for use of optional accessories like a guidescope.
| OPTICAL TUBE INFO: | |
|---|---|
| Optical Design | Rowe-Ackermann Schmidt Astrograph |
| Aperture | 279mm (11") |
| Focal Length | 620mm (24.4") |
| Focal Ratio | f/2.2 |
| Central obstruction diameter | 114mm (4.48") (41% of aperture diameter) |
| Light Gathering Power (Compared to human eye) | 1588x |
| Resolution (Rayleigh) | 0.49 arc seconds |
| Resolution (Dawes) | 0.41 arc seconds |
| Image Circle | 43.3mm (1.7") Ø , 4.0° |
| Useable field | 52mm (2.04") Ø , 4.8° only minimal performance loss at edge of FOV |
| Wavelength range | 400 - 700 nm |
| Spot size | < 4.4 μm RMS across FOV |
| Optical Coatings | StarBright XLT |
| Off-axis Illumination | 83% at 21mm (.82") off-axis |
| Optical Window | 68mm (2.67") Ø |
| Back focus with included camera adapter | 55mm (2.16") |
| Back focus from top of threaded collar | 72.8mm (2.86") |
| Optical Tube | Aluminum |
| Optical Tube Length | 838.2mm (33") |
| Optical Tube Diameter | 330.2mm (13") |
| Focuser | Ultra-Stable Focus System |
| Finderscope | Not included |
| Optical Tube Weight | 43 lbs (19.5 kg) |
| Other Features | Ventilation fan, dual dovetail mounting bars |
| Included items | 42mm (1.65") T-thread camera adapter | 48mm (1.89") camera adapter | Dust cover | Fan battery pack |
| Dovetail | CGE Dovetail Bar |
$2,349.00
180mm/2700mm Skymax 180 Maksutov-Cassegrain OTA – High Performance Optical Tube Assembly
The Sky-Watcher Skymax 180 Maksutov-Cassegrain OTA Telescope is perfect for the seasoned enthusiast moving up to a more powerful scope. The larger aperture enables more detailed views of our close planetary neighbours and sharper images of deep space objects.
Maksutov-Cassegrain Advantage
This telescope design has the inherent advantage of minimizing coma aberrations. It also presents a flatter and a more improved edge to edge clarity. Wide angle views of star fields and clusters have never looked so good!
Bring it to Your Favorite Viewing Spot
These Optical Tube Assemblies have a distinct advantage of being designed for use with different mounts. As long as the standard adaptors are present, you should be able to attach the OTA on it. The quick release mechanism enables you to assemble the tube quickly. It also allows you to make minor adjustments to the tube like a stroll in the park.
| Optical Design | Maksutov-Newtonian |
| Model Number | SWMAK180-OTA |
| Aperture | 180mm |
| Focal Length | 2700mm |
| Focuser Diameter | 1.25″ |
| Finder Scope | 9 x 50mm |
| Highest Practical Power | 360x |
| Recommended Usage | Advanced |
| Recommended Usage | High Resolution Astrophotography |
$2,399.00
The ZWO FF80 APO is a refractive astrograph with a powerful flatfield optical design which saves you from the expensive cost of a field flattener. It eliminates the trouble of calculating the back focus distance of the flattener and connecting various accessories to achieve that distance. You can just connect any possible accessories you need. As long as the target is focused, the whole optical system is perfect for imaging. This makes the whole setting up process much more convenient, and saves you time, allowing you to pay more attention to the image shooting itself.
The ZWO FF80 APO is also a nice choice for your visual observation. It fits diagonals as well as various eyepieces and can achieve a perfect focus, and can even be used to observe planets with a super-high magnification eyepiece.
The whole design of the telescope is compact and lightweight. The OTA weighs only 3.9kg, and the full package with tube rings and other accessories weighs 4.7kg. It has an aperture of 80mm. The focal ratio is f/7.5 and the focal length is 600mm.
The ZWO FF80 APO adopts a 3+1 quadruplet lens structure which contains two pieces of ED glass that can effectively reduce chromatic aberration and enhance clarity and sharpness. It supports the full-frame imaging circle and has a fine spot diagram with tiny distortions of the peripheral stars. The 3" rigid focuser comes with a new-type 360°rotator with scales and a finder base. M76, M68, M54, and M48 camera adapters are also attached, and the M48 adapter has a 2” female thread for installing filters.
ZWO FF80 APO Main Features
Quadruplet air-spaced APO design - No need to calculate back focus
Small and round stars - with a central RMS radius of 3um
Various adapters - M76/ M68/ M54/ M48
Dual speed (1:10) focuser - Support both fine and coarse adjustment
No need for a separate field flattener - Self-flattening design
Supports full-frame cameras - Produces a 44mm image circle
Focal reducer -
Specifications
| Aperture | 80mm |
| Focal Length | 600mm |
| Focal Ratio | f/7.5 |
| Image Circle | 44mm |
| Net Weight | 3.9kg |
| Gross Weight | 4.7kg |
| Objective Lens | Quadruplet (including two ED glass elements |
| Rear -end thread type | M76x1-M 68x1, M 68x1- M54x0.75, M54x0.75-M54x0.75, M54x0.74-M48x0.75, (M48 X0.75 filter thread inside) |
| Total Length | 450mm (including including 1.25" eyepiece holder as dew shield contracted) 480mm (including the 4-piece adapter as dew shield contracted) 540mm (including 1.25" eyepiece holder as dew shield fully stretched) 570mm (including the 4-piece adapter as dew shield fully stretched) |
| Rear end of the 4-piece photographic adapters: | M48x0.75 |
SKU: ZWO-FF80-APO
The ZWO FF130APO is a refractive astrograph with a powerful flatfield optical design which saves you from the expensive cost of a field flattener. It eliminates the trouble of calculating the back focus distance of the flattener and connecting various accessories to achieve that distance. You can just connect any possible accessories you need. As long as the target is focused, the whole optical system is perfect for imaging. This makes the whole setting up process much more convenient, and saves you time, allowing you to pay more attention to the image shooting itself.
Compared to the ZWO FF107 APO, the ZWO FF130 APO has a larger size. The aperture is 23mm larger. The focal length at f7/7 is also longer, this will yield higher details and slightly higher magnifications but with a field of view suitable for all deep-ky objects. The longer focal length will be especially effective on planetary and larger deep-sky objects which, when combined with the larger 130mm aperture, will provide stunning details in a reasonable time.
The ZWO FF130 APO with its quadruplet lens structure which contains two pieces of ED glass will control chromatic and other aberrations. With its self-flattening design, the ZWO FF130 APO offers strong advantages in astronomical shooting. It supports a medium frame 60mm image circle, has a fine spot diagram with tiny distortion on the peripheral stars, and its central RMS radius is less than 2 microns.
The OTA weighs only 10.5 kg, and the full package with tube rings and other accessories weighs 12.5kg. The 3.4″ rigid focuser comes with a new-type 360°rotator with scales and a finder base. M86, M68, M54, and M48 camera adapters are also attached, and the M48 adapter has a 2” female thread for installing filters. When used with the 3" 0.7x flat-field reducer, the telescope can reach a focal ratio of f/5.4 and a focal length of 700mm, effectively reducing exposure time. The Multifunctional handle comes with a central slot for attaching an M6 screw with an M6 screw hole. standard KLOsmandy dovetail plate, together with sturdy double rings. It is perfectly suitable for viewing and shooting.
ZWO FF130 APO Main Features
Quadruplet air-spaced APO design – No need to calculate back focus
Small and round stars – with a central RMS radius of less than 2um
Various adapters – M86/ M68/ M54/ M48
Dual speed (1:10) focuser – Support both fine and coarse adjustment
No need for a separate field flattener – Self-flattening design
Supports medium-frame cameras – Produces a 60mm image circle
Focal Reducer -
Specifications
| Aperture | 130mm |
| Focal Length | 1000m |
| Focal Ratio | f/7.7 |
| Image Circle | 60mm |
| Objective Lens | Quadruplet air-spaced APO (including two ED glass elements |
| Net Weight | 10.5kg |
| Gross Weight | 12.5kg |
| Rear end thread type | M86x1 - M68x1, M68x1 - M54x0.54,
M54x0.75 - M54x0.54, M54x0.75 - M48x0.75 (M48 x0.75 filter thread inside) |
| Total Length | 842.5mm (including 1.25" eyepiece holder with dew shield contracted)
1011.5mm (including the 4-piece adapter with dew shield contracted) 889.5mm (including 1.25" eyepiece holder with dew shield extended) 1061.5mm (including the 4-piece adapter with dew shield extended) |
| Four-piece photographic adapter | M48x0.75 |
The ZWO FF107 APO is a refractive astrograph with a powerful flatfield optical design which saves you from the expensive cost of a field flattener. It eliminates the trouble of calculating the back focus distance of the flattener and connecting various accessories to achieve that distance. You can just connect any possible accessories you need. As long as the target is focused, the whole optical system is perfect for imaging. This makes the whole setting up process much more convenient, and saves you time, allowing you to pay more attention to the image shooting itself.
The ZWO FF107 APO is also a nice choice for your visual observation. It fits diagonals as well as various eyepieces and can achieve a perfect focus, and can even be used to observe planets with a super-high magnification eyepiece.
The whole design of the telescope is compact and lightweight. The OTA weighs only 5.7kg, and the full package with tube rings and other accessories weighs 6.9kg. It has an aperture of 107mm. The focal ratio is f/7 and the focal length is 749mm.
The ZWO FF107 APO adopts a 3+1 quadruplet lens structure which contains two pieces of ED glass that can effectively reduce chromatic aberration and enhance clarity and sharpness. It supports the full-frame imaging circle and has a fine spot diagram with tiny distortions of the peripheral stars. The 3″ rigid focuser comes with a new-type 360°rotator with scales and a finder base. M86, M68, M54, and M48 camera adapters are also attached, and the M48 adapter has a 2” female thread for installing filters.
ZWO FF107 APO Main Features
Quadruplet air-spaced APO design – No need to calculate back focus
Small and round stars – with a central RMS radius of 3um
Various adapters – M86/ M68/ M54/ M48
Dual speed (1:10) focuser – Support both fine and coarse adjustment
No need for a separate field flattener – Self-flattening design
Supports full-frame cameras – Produces a 44mm image circle
Focal Reducer -
Specifications
| Aperture | 107mm |
| Focal Length | 749mm |
| Focal Ratio | f/7 |
| Net Weight | 5.7kg |
| Gross Weight | 6.9kg |
| Image Circle | 44mm |
| Objective Lens | Quadruplet Air Spaced (including two ED Glass elements) |
| Rear end thread type | M86x1 - M68x1, M68x1 - M54 x 54x0.75,
M54x0.75 - M542x0.75, M52x0.75 - M48x0.75 (with M48x0.75 filter thread) |
| Total Length | 602mm (including 2" eyepiece holder with dew shield contracted)
655mm (including the 4-piece adapter with dew shield contracted) 754mm (including 2" eyepiece holder with dew shield extended) 806mm (including the 4-piece adapter with dew shield extended) |
| Four-piece photographic adapter | M48x0.75 |
SKU: ZWO-FF107-APO
$5,925.00
The BORG 107FL Telescope Set CR is the premium model BORG telescope, designed for professional astro-watchers. This telescope features a 600mm focal length objective lens that incorporates high-end apochromat fluorite glass elements from Canon Optron, Inc.
Axial chromatic aberrations are suppressed even further with the 107FL objective lens when matched against the 90FL. The BORG 107FL Telescope Set CR is constructed with a lightweight and compactable carbon fiber barrel. Arca-Swiss Quick Release base plates are included for tripod mounting. The BORG 107FL Telescope Set CR is recommended for starry sky, nebula, star cluster, and planet observation.
You can convert this telescope to tele lens by swapping the prism and eyepiece with a BORG camera mount adapter (sold separately).
Main Features
- Fluorite glass elements from Canon Optron, Inc. are incorporated in the optical design for ultimate resolution and minimal axial chromatic aberrations.
- Objective lens optical construction: 2 elements in 2 groups, fluorite apochromat, fully multicoated.
- Robust and beautiful carbon fiber barrel.
- BORG 80Ø barrel system.
- Rack & pinion focusing system.
- Erect prism (included) allows users to observe both on-ground objects and celestial bodies.
- 20mm and 9mm eyepieces included.
- Super lightweight at 3.7 kilograms (including accessories).
- Arca-Swiss Quick Release System tripod plate.
- Objective lenses and major parts are Made in Japan.
'CR' stands for carbon fiber barrel and rack & pinion focusing system.
Camera mount adapters and other camera components are sold separately.
Specifications
Model Name
BORG 107FL Telescope Set CR
Product Code
6207
Focal Length, mm
600
Focal Ratio
f/5.6
Min. Length, mm
504
Weight, g
3700
Filter Size, mm
82
$1,999.00
Superb optical performance thanks to Canon Optron, Inc. fluorite glass elements in the optical construction. The precise optical design results in an extremely sharp image with practically no chromatic aberrations.
Recommended for starry sky, nebula, star cluster, and planet observation.
Main Features
- Modular BORG Design
- Apochromat fluorite glass elements.
- Objective lens optical design: 2 elements in 2 groups, fluorite element, apochromat, fully multicoated.
- Erect prism (included) allows users to observe both on-ground objects and celestial bodies.
- 20mm and 9mm eyepieces included.
- Arca-Swiss Quick Release System tripod collar.
- Ultra-lightweight of 962 grams.
- Objective lenses and major parts are Made in Japan.
| Product Code | 6155 |
|---|---|
| Focal Length, mm | 250 |
| Focal Ratio | f/4.5 |
| Min. Length, mm | 260 |
| Weight, g | 962 |
| Filter Size, mm | 58 |
$117,999.00
After successfully introducing the DeltaRho 350, the DeltaRho 500 is now available for transcending the challenges of-ultra wide field imaging. With a primary mirror that is fixed in place, collimation is quickly achieved with a simple adjustment to the tip and tilt of the secondary mirror. With more than twice the light-gathering power of the DeltaRho 350, maximizing the performance of your astrograph has never been easier due to PlaneWave’s pursuit of the perfect telescope!
- Corrected Cassegrain focus optical design
- Aperture – 508 mm (20″)
- Focal length – 1537 mm
- Focal Ratio – f/3.03
- 70mm Image Circle > 2.6 degrees
- Fixed Primary Mirror
- Collimation performed via 3 tip/tilt screws at the secondary mirror
- 9.166” (232.8 mm) from mounting surface (without focuser and rotator).
- Backfocus of 5.81″ (147.6mm) with Series-5XL focuser and Series-5 Rotator installed (with focuser at midpoint of travel range).
- Built-in primary and secondary dew heaters with temperature sensors
- Compatible with L-500 or 600 series direct drive mounts.
Our team at PlaneWave is passionate about designing exceptional telescopes so that users around the world are able to capture the most awe-inspiring astro images possible. From design to manufacture, our goal with the DeltaRho 500 was centered around creating a revolutionary wide-field telescope. The DeltaRho 500 is a Cassegrain Optical Design with the imaging train at the back of the telescope to prevent obstruction of the instrument. This offers a real advantage against prime focus designs, which can severely limit users’ ability to operate with filter wheels or large cameras. Witness the incredible breakthrough in telescope technology as the DeltaRho 500 operates at f/3 and 1537 mm focal length, which is sure to revolutionize your astrophotography.
Last, but not least, the DeltaRho 500 provides a flat field, which ensures stunning clarity from corner-to-corner images without field curvature degradation. The DeltaRho 500 offers the simplicity of single-mirror collimation, stray light control of advanced 3D printed baffles, and structural performance created through finite element analysis (FEA). DeltaRho 500 users can experience pinpoint stars edge-to-edge and a 2-degree field of view when using large 16803/4040 (52mm) size camera sensors. This field of view is over twice as large as our CDK 20! This kind of equipment allows users to experience a whole new level of wide-field imaging that can bring them closer than ever to deep space. The DeltaRho 500 allows nothing to stand in between the user and amazing astro images.
Carbon Fiber Tube 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 that excellent imaging data is produced.
Collimation software
Along with the included collimation mask, PlaneWave Collimation software allows for quick and easy collimation necessary to maximize the performance of a fast f-ratio optical system.
3D Printed Baffles
PlaneWave's digital 3D printing technology adds successive layers of material to our baffle systems for lightweight, precision-positioned internal stray light control to minimize vignetting and maximize image contrast.
Cooling Fans
Three fans are strategically placed on the backplate of the optical tube to ventilate through the telescope and by the primary mirror. Four additional fans on the side of the optical tube provide airflow across the primary, bringing thermal equilibrium efficiently to prevent distorted images due to temperature variations.
The fans are controlled via the PWI 4 software with the PlaneWave Series 5 Controller sold separately.
Dew Control Ready
For added dew prevention, the DR500 is internally wired with polyimide film heater pads and a temperature sensor, which is ready to be controlled with the Series 5 Controller via PWI 4 software.
Optical system
| Optical Design | Corrected Cassegrain |
| Aperture | 508 mm (20 inch) |
| Focal Length | 1537 mm (60.5 inch) |
| Focal ratio | f/3 |
| Central Obstruction | 59 % by diameter |
| Back Focus from Mounting Surface (No focuser/rotator installed) | 9.166 in (232.8 mm) from mounting surface; 7.271 inch (184.7 mm) from lens cell |
| Weight | 165 lbs (75 kg) |
| OTA Length | 35.1 inch (892 mm) |
| Optical Design Performance (Spot Diameter) | 3.86 micron RMS on-axis, 4.04 micron RMS at 22 mm off-axis, and 6.04 micron RMS at 35 mm off-axis (Spot Diameters) |
| Telescope Cage | Carbon fiber truss poles with carbon fiber shroud |
| Optimal Field of View | 70mm image circle |
Primary Mirror
| Optical Diameter | 20 inch (508 mm) |
| Outer Diameter | 20.8 inch (528 mm) |
| Shape | Prolate ellipsoid |
| Material | Fused silica (quartz) |
| Coating | Enhanced aluminum – 96% |
Secondary Mirror
| Diameter | 286 mm (11.26 inch) |
| Material | Fused silica (quartz) |
| Shape | Spherical |
| Coating | Enhanced aluminum – 96% |
Lens Group
| Diameter | 160 mm (6.3 inch) Largest Lens |
| Number of lenses | Three |
| Coating | Broadband AR Coatings (on avg. less than .5% reflected from 400 to 700 nm) |
Included items
| Heating elements for dew prevention | The heating pads on the primary and secondary mirror require the Series 5 Controller (sold separately). |
| OTA Cover | Which protects the primary mirror and the inside of the optical tube. |
| Flashdrive | Contains software and instructions for collimation and spacing the primary to the secondary mirror. |
| Wrench Set (5812A35) | Standard hex wrenches (European orders only) |
Configurations
For the DeltaRho 500 and Series-5XL Focuser:
To achieve proper mechanical clearance, a 0.5″ spacer (#6003165) is required.
If the user plans on using our Focuser and Rotator, the 0.5″ spacer is placed in between the Focuser and Rotator, then the Tip-Tilt Adapter.
If the user plans on using only the focuser, the 0.5″ spacer, assembles as follows: OTA, Focuser, Spacer, then Tip-Tilt Adapter.
The Tip Tilt Adapter is compatible with the Series- 5XL Focuser, as both the focuser and the tip-tilt accessory use the 7.125″ flange interface.
Recommended Accessories
Mount Accessories
- L-500 Direct Drive Mount (600550)
Imaging Accessories
- Tip-Tilt Adapter for Series-5 Focuser or Rotator to SecureFit (6061006)
OTA Accessories
- 0.5″ Extension Spacer for 7.125″ Flange Interface (6003165)
- Piggyback Dovetail Bar (201990)
- Series-5XL Focuser (6071001)
- Series-5 Rotator (6021001)
- Series-5 Controller (600199)
$38,000.00
Through years of dreaming of the perfect telescope for wide-field imaging, our pursuit of innovation has finally been honored with PlaneWave’s revolutionary DeltaRho 350 f/3 telescope. The DeltaRho 350 is designed for unsurpassed wide-field imaging and ease of use in the field. Since the primary mirror is fixed in place, collimation is quickly achieved by adjusting the tip and tilt of the secondary mirror. With the Delta Rho 350, your astrophotography experience will be second to none!
- Corrected Cassegrain focus optical design
- Aperture – 350 mm
- Focal length – 1050 mm
- Focal Ratio – f/3
- 60mm Image Circle > 3 degrees
- Fixed Primary Mirror
- Collimation performed via 3 tip/tilt screws at the secondary mirror
- Backfocus of 5.651” (143.535 mm) from mounting surface (without focuser and rotator). This distance includes refraction from filters.
- Backfocus of 2.525″ (64.135 mm) with Series-5 focuser and Series-5 Rotator installed (with focuser at midpoint of travel range).
- Built-in primary and secondary dew heaters with temperature sensors
- *L-350 mount seen in product photo is sold separately
Capturing the most stunning astrophotographs possible is something our team is passionate about. From design to manufacture, our goal with the DeltaRho 350 was centered around creating a game-changing wide-field telescope. The DeltaRho 350 is a Cassegrain optical design which means the imaging train is secured at the back of the telescope and does not block the light path compared to prime focus designs, which severely limit users’ ability to operate with filterwheels or large cameras.
The DeltaRho 350 is an incredible breakthrough in telescope technology and ease of use. Operating at f/3 and 1050 mm focal length, the DeltaRho is a wide-field telescope that is sure to revolutionize your astrophotography!
Additionally, the DeltaRho 350 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 DeltaRho 350 is an exceptional telescope. DeltaRho 350 users can experience pinpoint stars edge-to-edge and a 170 x 170 arcminute field of view when using large 16803/4040 size camera sensors. This field of view is nearly 3 times as large as our CDK14! When equipment fades into the background and simply performs, the astrophotography experience becomes even more fun and rewarding!
Optical System
| Optical Design | Corrected Dall-Kirkham (CDK) |
| Aperture | 350 mm |
| Focal Length | 1050 mm (41.34 in.) |
| Focal ratio | f/3 |
Secondary Mirror
| Diameter | 7.48 in. (190 mm) |
| Material | Fused silica (quartz) |
| Shape | Spherical |
| Coating | Enhanced aluminum – 96% |
Primary Mirror
| Optical Diameter | 13.78 inches (350mm) |
| Outer Diameter | 14.5 inches (468.3mm) |
| Shape | Prolate Ellipsoid |
| Material | Fused Silica (quartz) |
Lens Group
| Diameter | 110 mm (4.33 inch) |
| Number of lenses | Three |
| Coating | Broadband AR Coatings (less than .5% reflected from 400 to 700nm) |
Standard Features
| Corrected Cassegrain | The corrected design yields a flat field free from off-axis astigmatism, coma, and field curvature. |
| 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 blow air inside the back of the telescope. 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. |
| Delta-T Ready | For added dew prevention, the DR350 is internally wired with polyimide film heater pads and temperature sensor, ready to be controlled with the optional Delta-T controller. |
Shipping
| Crated Shipping Weight | 225 lbs | 102 KG |
| Crate Width | 31 inches | 787.4 mm |
| Crate Height | 26 inches | 660.4 mm |
| Crate Length | 53 inches | 1346.2 mm |
Included Items
| Heating elements for dew prevention | The heating pads on the primary and secondary mirror require the 5-Series 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) |
Recommended Accessories
OTA Accessories
- Series-5 Focuser (6011001)
- Series-5 Rotator (6021001)
- Series-5 Controller (600199)
Mount Accessories
- L-350 Direct Drive Mount (600549)
- DeltaRho 350 Piggyback Dovetail (140990)
Imaging Accessories
- Tip-Tilt Adapter for Series-5 Focuser or Rotator to SecureFit (6061006)
$4,790.00
Tele Vue 85 OTA
The Tele Vue-85's mix of aperture and small physical size makes it a wonderful "go anywhere, do anything," crossover instrument—with Tele Vue quality, of course. With APO performance and airline portability, the Tele Vue-85 has been delighting astronomy and birding enthusiasts and reviewers alike. "Eye-popping performance that raises the standard of excellence for highly portable instruments." Evaluation of double-stars, lunar detail, deep sky and photography were reported in Sky and Telescope as: "Truly awesome! ...Incredible!...the view almost blew me off my chair!..." The conclusion, "...an extremely powerful, compact instrument capable of delivering stunning images of the universe."
The Better View Desired website reviewer summed up the Tele Vue "experience" when he said he would choose the Tele Vue-85, "...to really enjoy the incredible beauty of the living birds... And, even now, every time I look at a bird through one of the exceptional conventional spotting scopes, I'll be thinking: 'I wonder what this would look like through the Tele Vue-85? I wonder what this bird really looks like?'" Yes, pure enjoyment of nature's beauty without awareness of a thing in between.
Soft case included
New Accessory Kit from Tele Vue includes the following items
EDE-18.2 18.2mm Tele Vue DeLite eyepiece
RS3-8003 3" Ring Mount
DSF-8002 2" 90° Tele Vue Everbrite - Satin
ASF-8125 2" - 1.25" Adapter - Satin Hi Hat
| Type: | APO (Doublet) Refractor |
| Elements /Groups: | 2 / 1 |
| Objective Diameter: | 85mm |
| Focal Length: | 600mm |
| Focal Ratio (f/): | f/7 |
| Drawtube / Focuser | 2 inch, Focusmate Dual Speed Rack and Pinion |
| Length OTA | 484mm |
| Length with Diagonal | 556mm (with 2" diagonal) |
| Weight OTA / std configuration (kg) | 2.77kg / 3.63kg |
| Maximum Visual Field of View (degrees) | 4.4 degrees (with 2" 55mm Plossl) |
| Maximum recommended magnification | 225 X |
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