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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
Optical Tube Assemblies (OTAs)
22 products
22 products
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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 |
$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 |
$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.
$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 |
$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.
$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 |
$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 |
$1,575.00
The easy-to-maintain refractor is an excellent choice for beginners though to experts.
Vixen achromatic objective lens delivers clear images with less colour fringe.
Specifications
| Objective lens, effective aperture | 105mm achromatic, multicoated |
| Focal length | 1000mm |
| Focal ratio | F9.5 |
| Resolving power | 1.1arc seconds |
| Limiting magnitude | 11.9 |
| Light gathering power | 225×unaided eye |
| Focusing mechanism | Rack-and-pinion |
| Finder scope | XY Red dot finder (1×aiming device) |
| Adapter thread / Visual back | 60mm and 42mm for T-ring / 50.8mm and 31.7mm push fit with flip mirror diagonal |
| Accessories | Tube rings, Dovetail slide bar |
| Photography | Usable with Prime focus, Eyepiece projection and Afocal imaging |
| Solar observation | Available with Sun projection screen set B |
| Dimensions / weight | 1010mm dia. and 115mm long / 4.8kg (Net 3.8kg) |
$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 |
$8,695.00
At a glance
- Vixen's flagship model with outstanding performance and ease of use for visual observation and astrophotography.
- Features a five-group-five-element Astrography with a fast focal ratio.
|
Objective Design |
Five-group five-element SD Apochromat, AS coatings |
|
Effective Aperture |
90mm |
|
Focal Length (Focal Ratio) |
495mm (F5.5) |
|
Resolving Power |
1.29 arc seconds・ |
|
Limiting Magnitude |
11.5 |
|
Light Gathering Power |
165X unaided eye |
|
Image Circle |
60mmφ (Over 90% illumination at the round edge) |
|
Optical Tube Size |
115mm dia. X 600mm long (476mm long for storage) |
|
Weight |
4.3kg |
| Finderscope | Not included, 7X50mm Finder with illuminated reticle, 50mm XY Finder bracket II sold separately |
| Focusing System | Rack-and-pinion |
| Accessory Threads / Size | Threads/ 84mm (pitch 1mm), 60mm (pitch 1.0mm), 42mm for T-ringPush-fit / 60.2mm, 50.8mm, and 31.7mm |
| Eyepiece (31.7mm) | Not included, SLV series of eyepieces sold separately |
| Plates and/or Tube Rings | Not included, VSD Tube Ring 115S, Dual Slide Bar sold separately |
| Provided Accessories | VSD60.2 to 50.8 Adapter, 2mm and 1.5mm Allen wrenches |
$1,600.00
Fluorite lens
A fluorite lens with less chromatic aberration is used to create a sharp image with less color bleeding.
Vixen standard Arimizo, equipped with camera tripod screw
Equipped with slide bar M. It can be mounted as it is on a stand with Vixen standard Arimizo such as AP series and SX series. Equipped with 1/4 inch and 3/8 inch screws. It can be mounted on a commercially available camera tripod.
Compatible with finder (sold separately)
Equipped with screws compatible with the Arimizo finder pedestal (sold separately). Compatible with the separately sold finder (finder legs).
Features
Compact photo visual lens barrel
A very compact photo visual lens barrel equipped with a fluorite lens.
In combination with the high-resolution HR series eyepiece, it demonstrates high visual performance despite its small aperture and short focus. Especially when observing the moon and planets, you can get a higher-grade powerful image.
It can also be used as a high-performance astro camera by using a dedicated flattener lens and reducer lens (sold separately) together. It creates a sharp image over the entire field of a full-frame SLR camera.
Specifications
Lens barrel
| Effective diameter of objective lens | 55mm / Fluorite Apochromat / Multi-coating |
| Focal length (aperture ratio F) | 300mm (F5.5) |
| Resolution / limit grade | 2.11 seconds, 10.5, etc. |
| Condensing power | 62 times the naked eye |
| Size / weight | Length 282mm (without extension tube) Outer diameter 80mm 1.5kg |
| Finder | Arimizo type pedestal (sold separately) can be installed |
Eyepiece
| Parts mounting size | Screwed in / 60mm, 43mm, 36.4mm inserted / 31.7mm |
| Eyepiece (31.7mm diameter) | 31.7mm diameter eyepiece (sold separately) can be used |
Other
| Plates, bands, etc. | Slide bar M |
| photography | Enlargement, direct focus, compact digital camera (colimate) shooting possible * A separate camera adapter etc. is required |
| Sun observation | Can be used in combination with the solar projection plate A set (sold separately) (fits, but the weight balance cannot be perfectly adjusted.) |
| Gross weight | 1.5kg (by eyepiece) |
$5,250.00
Highly advanced "photo andvisual" optical design, the flagship of Vixen SD apochromatic refractors.
Vixen AX103 features a three element objective lens, incorporating an SD lens in its center, and the fourth lens inside of the focuser drawtube. This advanced optical design produces crystal-clear, sharp and high contrast images with no trace of falese color. In spot diagrams of the AX103S, the star images are extremely concentrated and are seen as small as 20 microns at the edge of ther file of view. The precision multicoatings applied to each surface to the lenses enhances visible light transmission to 99.5% on any single surface. An optional AX103 reducer which produces fast F5.6 forcal ratio is best for imaging of deep sky objects.
| Specification | Details |
|---|---|
| Objective lens / Aperture | 103mm, triplet SD apochromatic, multicoated |
| Focal length (Focal ratio) | 825mm (F8.0) |
| Resolving power / Limiting magnitude | 1.13 arc seconds / 11.8 |
| Light gathering power | 217× unaided eye |
| Dimensions / Weight | 115mm diameter × 762mm length (retractable to 670mm), 6.4kg (Net: 4.6kg) |
| Finder scope | 7×50mm with dark-field illuminated reticle, 7° field of view |
Focuser
-
Adapter threads / Visual back60mm, 42mm for T-ring / 50.8mm and 31.7mm push fitwith flip mirror diagonal
Others
-
AccessoriesTube rings, Dovetail tube plate, Metal carry handle
-
PhotographyUsable with Frime focus, Eyepiece projection and Afocal imaging
-
Solar observationAvailable with Sun projection screen set B
Configuration
- SXD2-AX103S
- SXP-AX103S
- AXD2-AX103S
- AXD2-AX103S-P
$514.00
The 130mm aperture Newtonian reflector with excellent light gathering power is ideal for observation of faint nebulae and star clusters, particularly for beginners who wish to start their astronomical journey with a large aperture for light gathering power.
Specifications
|
Optical Design |
Newtonian Reflector |
|
Aperture |
130 mm |
|
Focal Length |
650 mm |
|
Focal Ratio |
f/5 |
|
Focuser |
Single-Speed Rack-and-Pinion |
|
Eyepiece Barrel Diameter |
1.25" |
|
Diagonal |
None |
|
Finderscope |
Yes |
|
Mounting System |
Vixen Style |
|
Optical Tube Dimensions |
57.1 x 16 cm |
In The Box
- Vixen Optics R130SF 130mm f/5 Reflector Telescope (OTA Only)
- 20mm Eyepiece
- 6.3mm Eyepiece
- 6x30 Finderscope
- Mounting Rings with Dovetail Plate
$378.00
Achromatic Refractor Optical Tube Assemblies.
Vixen achromatic refractors allow sharp views of the Moon and planets. The easy-to-maintain refractor is an excellent choice for beginners though to experts.
Specifications
| Achromatic objective | D=70mm F=900mm(f12.9),multicoated optics |
| Resolving power | 1.66 arc seconds |
| Limiting magnitude | 11 |
| Light gathering power | 100x unaided eye |
| Finder scope | 6x24mm finder,5 degrees filed of view |
| Adapter thread | 42mm for T-ring |
| Visual back | 31.7mm push fit |
| Accessories | PL20mm,PL6.3mm,Erect-image diagonal 31.7mm,Tube rings, Dovetail tube plate |
| Size | 76mm dia. X 860mm long |
| Weight | 2.5kg/5.5 lb |
$7,560.00
For both planetary and deep sky observing and photographic applications.
Vixen's original Catadioptric design, consisting of two high reflectivity dielectric mirrors and a unique double meniscus lens unit in front of the secondary mirror, virtually eliminates both spherical aberration and field curvature excellently and delivers high quality of images. With the large 260mm aperture, the VMC260L is a true all purpose telescope in your observing sessions.
The VMC features a combination of a miniscus lens unit in front of the secondary mirror and high-precision spherical mirrors that are shaped with extreme accuracy. Spherical aberration and curvature of field are corrected to a high level of optical performance for clear and sharp images. With its 260mm aperture dielectric coated mirror, the VMC260L collects enough light for serious visual and photographic applications and for both planetary and seep sky observing.
Specifications
Optical Tube
| Specification | Details |
|---|---|
| Primary mirror | 260mm effective aperture, precision spherical mirror, multicoated |
| Focal length (Focal ratio) | 3,000mm (F11.5) |
| Resolving power / Limiting magnitude | 0.45 arc seconds / 13.8 |
| Light gathering power | 1380× unaided eye |
| Dimensions / Weight | 304mm dia. and 680mm long (720mm incl. protruded focus knob) / 12.1kg (Net 10kg) |
| Finder scope | 7×50mm with dark-field illuminated reticle, 7 degrees field of view |
Focuser
| Specification | Details |
|---|---|
| Adapter thread / Visual back | 60mm and 42mm for T-ring / 50.8mm and 31.7mm push fit with flip mirror diagonal |
Other
| Specification | Details |
|---|---|
| Accessories | Dovetail attachment rail, Metal carry handle, Saddle plate |
| Photography | Usable with Prime focus, Eyepiece projection and Afocal imaging |
| Solar observation | Not available |
$749.00
Sky-Watcher 127mm/1500mm Skymax 127 Maksutov-Cassegrain OTA
- Compact dimensions, ideal for transportation
- Practical main mirror focusing mechanism
- Universal accessory adaptation
- High contrast image without distracting false colour
- Quick release system for the tube
- Impressive viewing capabilities for its price range
- 5 years Sky-Watcher limited warranty
| Model Number | SWMAK127-OTA |
| Optical Design | Maksutov-Cassegrain |
| Aperture | 127mm |
| Focal Length | 1500mm |
| Eyepieces | LET28mm |
| Focuser Diameter | 2″ |
| Finder Scope | 6 x 30mm |
| Highest Practical Power | 254x |
| Recommended Usage | Advanced |
| Weight | 5.6kg |
| Recommended Usage | High Resolution Astrophotography |
$4,599.00
The BORG 90FL CR has exceptional optical resolution, accomplished by apochromat fluorite glass elements from Canon Optron, Inc. built in the optical design of the objective lens, and a super tele 500mm focal length and aperture of f/5.6.
A great piece of gear for observing celestial bodies and bird life in the Australian bush and city environments.
The 90mm front element diameter does not hamper the 90FL's extreme compact and lightweight capabilities thanks to the detachable carbon fiber made barrel. Recommended for starry sky, nebula, star cluster, and planet observation. You can convert this telescope to a tele lens by swapping the prism and eyepiece with a BORG camera mount adapter (sold separately).
- Objective lens equipped with apochromat fluorite glass elements from Canon Optron, Inc.
- Objective lens optical design: 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.
- Lightweight construction of 3 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.
Main Features
Model Name
BORG 90FL Telescope Set
Product Code
6390
Focal Length, mm
500
Focal Ratio
f/5.6
Min. Length, mm
420
Weight, g
2900
Filter Size, mm
82
$33,599.00
PlaneWave CDK 14" Fused Silica
The CDK (Corrected Dall-Kirkham) Optical Design is an innovative solution for unsurpassed astroimaging quality at an affordable price. The CDK telescope design provides excellent imaging with large format CCD cameras while remaining superb for visual use. The CDK design far exceeds the off-axis performance of most commercial telescope designs including the Ritchey-Chrétien design.
FUSED SILICA
Fused Silica is a synthetic amorphous silica glass of the highest purity and one of the most transparent glasses made.
The optical and thermal properties of fused silica are superior to other types of glass due to its purity. Its transmission and homogeneity exceed those of crystalline quartz without the problems of temperature instability inherent in the crystalline form.
Fused Silica has a coefficient of thermal six times lower than Borosilicate glass, which means that as fused silica cools down, it preserves its shape to a high degree of accuracy. This translates into consistent optical performance and unchanging focus over temperature changes.
With high melting temperature (~1,600 degrees Celsius), a very low coefficient of thermal expansion and resistance to thermal shock, fused silica is the material of choice for professional observatories as well as various scientific applications.
This no-compromise design is unique in making the optical alignment forgiving and collimation very easy. This guarantees the user the best possible performance from the telescope. The end result at the image plane of the CDK design is no off-axis coma, no off-axis astigmatism, perfectly flat field (no off-axis defocus). The CDK design will give you pinpoint stars from the center to the corner of the field of view.
Features:
|
Carbon Fiber Truss Design |
Open truss tube design with carbon fiber frame minimizes thermal expansion which causes focus shift with changes in temperature. Carbon fiber truss design also promotes quick thermal cooling and provides a rigid, lightweight structure. | |
| 3D Printed Baffles | Planewave uses digital 3D printing technology to produce lightweight baffle tubes. 3D printers add successive layers of material to construct a baffle system with precision positioned internal stray light baffles to minimize vignetting and maximize image contrast. | |
| Dovetail Expansion Joint | Allows for the difference in thermal expansion between carbon fiber and aluminum. The expansion joint allows the aluminium dovetail expand and contract without stressing the carbon fiber lower truss. | |
| Cooling Fans | Three cooling fans blow air inside the back of the telescope. Internal diverting fins circulate air flow behind the mirror for even cooling to help the telescope reach thermal equilibrium quickly. The fans are controlled with PWI PC software with the optional Electronic Focus Accessory (EFA Kit). | |
| Delta-T Ready | For added dew prevention, the CDK14 is internally wired with polyimide film heater pads and temperature sensor, ready to be controlled with the optional Delta-T controller. |
PlaneWave CDK 14" Fused Silica Specifications
OPTICAL SYSTEM
| Optical Design | Corrected Dall-Kirkham (CDK) |
| Aperture | 14 inch (356mm) |
| Focal Length | 2563mm (101 inch) |
| Focal ratio | F/7.2 |
| Central Obstruction | 23.5% by surface area; 48.5% by diameter |
| Back Focus from Mounting Surface | 11.09 inch (282 mm) |
| Weight | 48 lbs (22 kg) |
| OTA Length | 35 inch (889 mm) |
| Optical Performance | 3.1 micron RMS at 13mm off-axis; 6.0 micron RMS at 35mm off-axis - Spot Diagram |
| Upper Cage | Carbon Fiber Truss |
| Lower Cage | Carbon Fiber Truss and Light Shroud |
| Optimal Field of View | 70mm Image Circle |
SECONDARY MIRROR
| Diameter | 165 mm (6.5 inch) |
| Material | Precision Annealed Borosilicate |
| Shape | Spherical |
| Coating | Enhanced Aluminum - 96% |
PRIMARY MIRROR
| Optical Diameter | 14 inches (355.6) |
| Outer Diameter | 14.5 inches (468.3mm) |
| Shape | Prolate Ellipsoid |
| Material | Fused Silica |
| Coating | Enhanced Aluminum - 96% |
LENS GROUP
| Diameter | 95mm (3.7 inch) |
| Number of lenses | Two |
| Coating | broadband AR Coatings (less than .5% reflected from 400 to 700nm) |
STANDARD FEATURES
| CDK Optics | The Corrected Dall-Kirkham design yields a perfectly flat field free from off-axis astigmatism, coma and defocus. |
| 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 CDK14 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 |
| Crate Width | 31 inches |
| Crate Height | 26 inches |
| Crate Length | 53 inches |
NOTE: This product has a lengthy lead time. Please contact education@bintel.com.au for further information.
$31,499.00
The Rowe-Ackermann Schmidt Astrograph (Celestron RASA 36), is a cost-effective optical system for space surveillance, Space Situational Awareness (SSA), other scientific applications, and advanced wide field astroimaging. It offers unprecedented value in aperture, speed, field of view, and optical performance. The RASA design has a convenient external prime-focus image capture location with a flat focal plane, providing small spot sizes to the edge of a wide field. The result is images free of optical defects like field curvature, off-axis coma, and astigmatism.
The 36 cm aperture version is the largest RASA Celestron manufactures; it is the biggest and fastest (f/2.2) optical instrument of its kind available off-the-shelf. Unlike most telescopes, which only focus visible light (400-700 nm), the RASA 36 cm focuses an extended spectral range (400-900 nm), allowing a brighter signal to be detected by a camera sensor. The RASA 36 cm also features a redesigned focus system, which ensures easy and stable focusing.
RASA 36 c sample back-focus distance (77.5 mm) accommodates a wide variety of imaging sensors. A custom camera adapter can be added for a field of view up to 4.4 degrees.
Important freight requirement RASA 36 is a professional-caliber, high-precision instrument. It is manufactured and aligned to an exacting standard to provide exceptional optical performance. The telescope has been packaged to ensure it retains alignment and resulting performance during transport. However, due to the weight, size, and known stresses of shipping via parcel service, Celestron has determined that the ideal transport is a palletized delivery via LTL truck freight. For all Australian deliveries, Celestron will ship via this method. Please contact us for further freight costs
| OPTICAL TUBE INFO: | |
|---|---|
| Optical Design | Rowe-Ackermann Schmidt Astrograph |
| Aperture | 355.6mm (14") |
| Focal Length | 790mm (31.1") |
| Focal Ratio | f/2.2 |
| Central obstruction diameter | 158mm (6.22")(44% of aperture diameter) |
| Light Gathering Power (Compared to human eye) | 2581X |
| Resolution (Rayleigh) | 0.39 arc seconds |
| Resolution (Dawes) | 0.36 arc seconds |
| Image circle | 60.1mm (2.36") Ø, 4.4° |
| Useable field | 70mm (2.75") Ø, 5.1°, only minimal performance loss at edge of FOV |
| Wavelength range | 400 – 900 nm |
| Spot size | < 6.3 μm RMS across FOV |
| Optical coatings | Enhanced aluminum, XLT multi-coatings used throughout |
| Off-axis Illumination | 83% at 30mm (1.18") off-axis |
| Optical window | 104mm (4.09") Ø |
| Back focus with included camera adapter | 55mm (2.16") |
| Back focus from top of threaded collar | 77.5mm (3.05") |
| Optical Tube | Aluminum |
| Optical Tube Length | 1079.5mm (42.5") |
| Optical Tube Diameter | 406.4mm (16") |
| Focuser | New focuser design, minimizes focus shift |
| Finderscope | Not included |
| Optical Tube Weight | 75 lbs (34.02 kg) |
| Other features | Ventilation fan, dual dovetail mounting bars |
| Included items | 48mm (1.89") camera adapter, fan battery pack |
$12,499.00
Celestron C14-AF XLT Optical Tube Assembly
- 14" Schmidt-Cassegrain Optical Tube Assembly
- Aluminum Optical Tube
- Fastar Compatible
- Celestron's premium StarBright XLT coatings
- 3910 mm focal length (f/11)
- 40 mm 1.25" eyepiece included (98x)
- Visual back allows for use with 2" accessories
- 9x50 finderscope to help accurately find objects
- 2" mirror diagonal provides more comfortable viewing position when observing objects that are high in the sky
- Includes dovetail rail compatible with CGE mount
SPECIFICATIONS
| Optical Design | Schmidt-Cassegrain |
|---|---|
| Aperture (mm) | 355.6 mm (14 in) |
| Focal Length | 3910 mm |
| Focal Ratio | 11 |
| Focal Length of Eyepiece | 40 mm |
| Magnification of Eyepiece | 98 x |
| Finderscope | 9x50 |
| Star Diagonal | 1.25 |
| Optical Tube | Aluminum |
| Fastar Compatible | Yes |
| Highest Useful Magnification | 840 x |
| Lowest Useful Magnification | 51 x |
| Limiting Stellar Magnitude | 15.3 |
| Resolution (Rayleigh) | 0.39 arc sec |
| Resolution (Dawes) | 0.33 arc sec |
| Light Gathering Power (Compared to human eye) | 2581 x |
| 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 |
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