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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
Planewave Vendor
68 products
68 products
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From $1,730.00
- The EFA kit automates focusing on the optional Hedrick Focuser, or IRF90 rotating focuser.
- Monitors temperature (primary-mirror and OTA back-plate).
- Controls the fans built into CDK telescopes.
- Ensure you have the proper EFA kit selected for your telescope below.
- 125901-Kit is for all 12.5″ OTAs (CDK/ IRDK).
- 240901-Kit is for all 14-24″ OTAs (CDK/ IRDK/ RC) and CDK700s.
*If the EFA is not purchased, the ability to automate temperature regulation for the primary mirror will be lost. This is especially significant when using a third-party focuser, as the EFA is required for full automation.
$440.00
From $440.00
Adapter to feather touch focuser for CDK's.
$1,440.00
- Feathertouch 2″ Diameter Dual Speed Focuser with 2.5″ of Travel.
- Great choice for refractors and Ritchey Chretien and CDK telescopes.
- It is precision engineered to deliver smooth operation and no image shift.
From $600.00
Tandem Bar for Planewave A200 Equatorial Mount.
From $450.00
Counterweights for 1.87″ Shaft. Used for Fork Mounted Telescopes with #600540 and #600541.
From $1,040.00
Counterweights for 1.5″ shaft (For Paramount, ORIGINAL/MX/MX+, NOT MEII )
From $1,040.00
Counterweights for1.875″ shaft (For Ascension 200, Paramount ME II and Astrophysics Mounts), including 18lbs, 30lbs and 40lbs. You can find the 1.875" Shafts here.
From $310.00
Counterweight shafts for the 1.875" diameter counterweights, including 3" and 6". You can find the counterweights here.
$810.00
Now, one person can easily balance a CDK on the L-Series mounts using the Ascend accessory! The Ascend can attach to either the front or rear of the #200919 Dovetail Clamp and precisely slide the CDK forward or back for accurate balance. Ascend uses a long pushrod to safely balance in the mount’s declination/altitude axis with the turn of a bolt.
From $400.00
Counterweights compatible for L-350, L-500, and L-600 Direct Drive L-Mounts, including 2lbs, 5lbs and 10lbs.
$1,800.00
- Add to the versatility of your L-500/L-600 mount with this external Right Ascension axis balance accessory.
- Balance of the mount is important for optimal direct drive motor performance and with this accessory users have the ability to fine tune Right Ascension balance.
- The accessory includes one 2, 5, and 10 lb weights.
- Please note this balance accessory requires the Right Ascension sliding weight accessory (L500204) to be already installed inside the mount in order to fit the additional weight system.
- The L500204 is a required product to install with the item(s) L500206/L600206 for L-500, L-550, and L-600 Direct Drive Mounts.
$930.00
- Add to the versatility of your L-500/L-600 mount with this internal Right Ascension sliding weight balance accessory.
- The accessory includes one 5 lb weight and shaft that installs inside the Right Ascension axis.
- Balance of the mount is important for optimal direct drive motor performance and with this accessory, users have the ability to fine-tune Right Ascension balance.
- The L500204 balance accessory is required to install the L500206 Right Ascension balance accessory.
- This item is included with the L-600 Direct Drive Mount.
$124,480.00
The PlaneWave T-600 Direct Drive Gimbal is engineered to meet the rigorous demands of advanced astrophotography, complex astronomical research, SSA/SDA, and FSOC applications. Leveraging cutting-edge technology, this gimbal provides a robust, precise, versatile observational platform suitable for demanding environments.
Core Features of the T-600 Gimbal
High-Torque Direct-Drive Motors
The T-600 Gimbal has high-torque, double-stacked direct-drive motors, ensuring smooth, fast, and virtually silent operation. This feature is critical for tracking celestial objects with minimal vibration and supreme accuracy, accommodating substantial payloads effectively.
High-Resolution Absolute Encoders
With high-resolution absolute encoders on each axis, it offers incredibly precise pointing and tracking capabilities, crucial for capturing sharp, detailed celestial images and conducting rigorous scientific observations.
Zero Backlash and Periodic Error
The design of the T-600 Gimbal eliminates backlash and periodic error, facilitating consistent and reliable tracking that enhances astrophotography and supports precise applications in research and space surveillance.
Advanced Customization Options
The T-600 includes optional contact gasket seals for full weatherization and supports limitless Az rotation, making it adaptable for specific research observational requirements across various environments.
Rugged and Environment-ready
Designed with rugged environments in mind, the gimbal features electronics enclosed within the mount and weatherproof cable pass-throughs, ensuring durability and reliability in light-to-moderate rain and preventing debris entry.
Application-Specific Advantages
Astrophotography
With its robust load capacity and exceptional slew speeds, it allows astrophotographers to reposition heavy equipment quickly and smoothly, capturing breathtaking images of the cosmos with ease and efficiency.
Research
Researchers will find the gimbal’s precise tracking and advanced software ideal for detailed celestial observations and data collection, particularly in demanding environments where equipment adaptability and operational reliability are paramount.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
Professionals in SSA/SDA will benefit from the T-600 Gimbal’s high-precision tracking and configurable features, which are perfect for monitoring space debris and tracking satellites, ensuring accurate surveillance and data collection in space domain awareness initiatives.
System Performance
| Acceleration (Azimuth and Altitude) | Acceleration up to 100°/second² *Depending upon installed payload-induced moment of inertia |
| Velocity | Up to 100 degrees per second *Depending upon acceleration and distance traveled |
| Pointing Accuracy | <5-arcsecond RMS* with PointXP Model *Under stable environmental conditions |
| Pointing Precision | 2 arcseconds at sidereal velocity |
| Open Loop Tracking Accuracy | 0.2 arcseconds RMS over 300 second exposure at siderial rate |
| Open Loop Axis Following Error | <0.15 arcseconds RMS at sidereal rate, <0.3 arcseconds RMS at 1 degree per second* <2 arcseconds RMS at 10 degrees per second* *Dependent on Payload |
| Internal Servo-Loop (Drive to Motor) | 10 kHz cascaded velocity/position controller, PID + Filters |
| Software Command Round-Trip | 5 – 25 msec (depending on application) |
| System Natural Frequency | 20 Hz or greater (for gimbal only) |
Mount system
| Type | Alt-Azimuth / Equatorial Direct-Drive Mount |
| Weight | 605 lbs |
| Max. Load Capacity | 600 lbs (with payload limited to 100 kg-m² moment per port with center of gravity ≤ 15 inches from mounting surface and an lowest eigenmode frequency of 20 Hz. i.e. dual mounted CDK24 telescopes are compatible) |
| Dimensions | 34” x 20” x 23.5” (H/D/W) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Motor Torque (Azimuth and Altitude) | 127 ft-lbs (peak) |
| Azimuth Axis Range of Motion (Optional) | |
| Cable Management | Through-the-mount cabling |
| Coudé Path (Optional) | Limits elevation axis range of motion to 180º |
| Power Requirement | 100 to 240 VAC (50-60 Hz), 20 amp service at 120 VAC, 10 amp service at 240 VAC |
| Operating Temperature Range | -30 C to +50 C |
| Storage Temperature Range | -50 C to +70 C |
Mechanical structure
| Gimbal Assembly | Fully CNC machined construction (Surface finish treated with UV resistant coating on all exposed metal surfaces) |
| Default Weatherization | 2-Layer non-contact labrynth sealing at each motion-surface to prevent water (light-to-moderate rain) and debris entry. *Optional rubber seals may be added for further ruggedization. |
| Azimuth Bearing | 4-way loaded radial ball bearings |
| Altitude Bearing | 4-way loaded radial ball bearings |
| Instrument Mounting | Breadboard plate on both mounting surfaces (see interface document for complete mounting information) |
| Lifting Points | Present for lifting in “any orientation” |
Motion control
| Drive Electronics (Azimuth and Altitude) | Elmo Motion Control Systems industrial grade off-the-shelf brushless motor drives |
| Motors (Azimuth and Altitude) | Each axis includes a double stacked direct-drive 3 phase axial-flux torque motor |
| Encoders (Azimuth and Altitude) | 26-bit absolute encoder ring with readhead |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software by Dave Rowe. Includes ASCOM driver. |
| Advanced Timing Features (Optional) | Timestamped using GPS Reciever, or PTP/NPT Server <100-microseconds accuracy |
Included items
| Included Items | Hardware- Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment |
| One 16' USB cable - Too connect the mount to the observatory control computer | |
| One 120VAC power cable- to provide power to the mount | |
| Flashdrive - Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror | |
| 3/8 Socket - Used for operating the RA balance leadscrew on the mount | |
| Gamepad - Used for control of the mount tracking speeds for visual observing |
$111,570.00
The CDK500 Observatory System from PlaneWave Instruments is a sophisticated solution designed for the serious astrophotographer and dedicated astronomy researcher. This high-end system combines the powerful CDK20 optical tube with the precise L-500 direct-drive mount, creating an exceptional observational platform that excels in a variety of scientific and imaging applications.
Key Features of the CDK500 Observatory System
CDK20 Optical Tube Assembly
- Advanced Optical Design: Employs a Corrected Dall-Kirkham optical design, achieving a field free of off-axis coma and astigmatism and a perfectly flat field across a 52 mm image circle, resulting in critically sharp images over the entire viewing area.
- High-Quality Construction: Constructed with robust carbon fiber, reducing thermal expansion and enabling quick thermal equilibration, which helps maintain precise optical alignment under fluctuating temperatures.
- Superior Mirrors and Coatings: Equipped with high-stability fused silica mirrors known for minimal thermal expansion, paired with high-performance coatings that maximize light throughput while minimizing stray light for optimal imaging quality.
- Thermal Management: Incorporates an advanced cooling system with strategically placed fans that ensure rapid thermal stabilization, essential for maintaining consistent, high-quality imaging and minimizing focus shifts caused by temperature changes.
CDK20 f/6.8 OTA
- Aperture and Focal Length: Features a 20-inch aperture, a shorter 3454 mm focal length at a faster f/6.8 focal ratio, and a shorter back focus of 223 mm.
CDK20 f/7.7 OTA
- Aperture and Focal Length: Features a 20-inch aperture, a longer 3947mm focal length at an f/7.7 focal ratio, and a longer 269.24 mm back focus.
L-500 Direct Drive Mount
- Direct Drive Motors: Features state-of-the-art direct-drive motors on each axis, providing smooth, fast, and virtually silent movement of the telescope with zero backlash and zero periodic error, perfect for precise tracking and rapid repositioning of celestial objects.
- High-Resolution Encoders: Outfitted with high-resolution optical encoders on both axes, offering precise positioning and movement, which is crucial for elite astrophotography and detailed astronomical studies.
- Azimuth Dovetail Balance System: Includes a finely adjustable balance system that enhances the stability and performance of the setup in both alt-azimuth and equatorial configurations, essential for prolonged accurate tracking and reducing stress on the mount during extended observations.
- Rapid Target Acquisition: Capable of impressive slew speeds up to 50 degrees per second, allowing for quick and efficient targeting of celestial bodies and satellites, vital for dynamic observations and responsive astrophotography.
Application-Specific Advantages
Astrophotography
The CDK500 is a formidable system for astrophotographers, offering unmatched tracking accuracy and image stability, which facilitate capturing spectacular celestial images with detailed resolution and vibrant colors.
Astronomy Research
Researchers will find the CDK500 invaluable for its consistent performance and precise data collection capabilities. It serves as a robust platform for sophisticated photometry, spectroscopy, and minor planet tracking, offering a solid foundation for scientific discovery and exploration.
Visual Observations
For enthusiasts of visual astronomy, the CDK500 provides vibrant and detailed views of the universe. Its significant aperture and high-quality optical components ensure exceptional viewing of planetary, lunar, and deep-sky objects, enriching every observational experience.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its swift and precise repositioning capabilities, the L-500 mount in the CDK500 system is capable of tracking satellites and space debris. However, it's important to note that while the L-series mounts are highly effective for astrophotography and research applications, they might not meet the optimal performance standards required for dedicated SSA/SDA operations. For those needs, we recommend exploring our T-600 Direct-Drive Gimbal, specifically engineered to exceed the demanding requirements for SSA/SDA applications, ensuring superior tracking and responsiveness in monitoring and cataloging space objects.
Mount systems
| Mount Weight | 257 lbs (100 kg) |
| Max. Load Capacity | 200 lbs (91 kg) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
Control systems
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 VAC. Supplied with 12VDC 15A Regulated Power Adapter |
Optical systems
| Aperture | 508 mm (20") |
| Focal Length | 3454 mm (135.98") or 3947 mm (155.4") |
| Focal Ratio | f/6.8 or f/7.77 |
| Central Obstruction | 39% of the Primary Mirror Diameter |
| Back Focus | f/6.8 - 223 mm (8.81 in), f/7.77 - 269.24 mm (10.6") |
Mechanical structure
| Fork Assembly | L-500 Mount |
| Fork Base | Welded stainless steel torsion box |
| Optical Tube | Carbon Fiber Truss with Carbon Fiber Light Shroud |
| Instrument Payload | 200 lbs (91 kg) |
Motion control
| Motor – Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder – Azimuth and Altitude | 152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution). |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | PlaneWave Interface (PWI4). Incorporates PointXP mount modeling software by Dave Rowe. Provides HTTP and ASCOM control interfaces. MaxIm DL is required for camera control when building a pointing model within our PWI4 software. |
System Performance
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcseconds at sidereal velocity |
| Tracking Accuracy | 0.3 arcseconds over a 5-minute period at sidereal velocity |
| System Natural Frequency | 11 Hz or greater |
Induced items
| Included Items | Dovetail Saddle (200919) - The PW wide saddle comes standard with the L-500 mount. |
| Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately | |
| OTA Cover - To protect the primary mirror and inside of the optical tube | |
| Flashdrive - Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror | |
| Hardware - Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier, or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment | |
| One 16′ USB cable - To connect the mount to the observatory control computer | |
| One 120VAC power cable - To provide power to the mount | |
| Standard Allen Key set - For tightening bolts used on the mount | |
| Gamepad - Used for control of the mount tracking speeds for visual observing |
$99,310.00
The CDK450 Observatory System from PlaneWave Instruments is a sophisticated solution designed for the serious astrophotographer and dedicated astronomy researcher. This high-end system combines the powerful CDK17 optical tube with the precise L-550 direct-drive mount, creating an exceptional observational platform that excels in a variety of scientific and imaging applications.
Key Features of the CDK450 Observatory System
CDK17 Optical Tube Assembly
- Advanced Optical Design: Employs a Corrected Dall-Kirkham optical design, achieving a field free of off-axis coma and astigmatism and a perfectly flat field across a 52 mm image circle, resulting in critically sharp images over the entire viewing area.
- High-Quality Construction: Constructed with robust carbon fiber, reducing thermal expansion and enabling quick thermal equilibration, which helps maintain precise optical alignment under fluctuating temperatures.
- Superior Mirrors and Coatings: Equipped with high-stability fused silica mirrors known for minimal thermal expansion, paired with high-performance coatings that maximize light throughput while minimizing stray light for optimal imaging quality.
- Thermal Management: Incorporates an advanced cooling system with strategically placed fans that ensure rapid thermal stabilization, essential for maintaining consistent, high-quality imaging and minimizing focus shifts caused by temperature changes.
CDK17 f/6.8 OTA
- Aperture and Focal Length: Features a 17-inch aperture, a shorter 3454 mm focal length at a faster f/6.8 focal ratio, and a shorter back focus of 262 mm.
L-550 Direct Drive Mount
- Direct Drive Motors: Features state-of-the-art direct-drive motors on each axis, providing smooth, fast, and virtually silent movement of the telescope with zero backlash and zero periodic error, perfect for precise tracking and rapid repositioning of celestial objects.
- High-Resolution Encoders: Outfitted with high-resolution optical encoders on both axes, offering precise positioning and movement, which is crucial for elite astrophotography and detailed astronomical studies.
- Azimuth Dovetail Balance System: Includes a finely adjustable balance system that enhances the stability and performance of the setup in both alt-azimuth and equatorial configurations, essential for prolonged accurate tracking and reducing stress on the mount during extended observations.
- Rapid Target Acquisition: Capable of impressive slew speeds up to 50 degrees per second, allowing for quick and efficient targeting of celestial bodies and satellites, vital for dynamic observations and responsive astrophotography.
Application-Specific Advantages
Astrophotography
The CDK450 is a formidable system for astrophotographers, offering unmatched tracking accuracy and image stability, which facilitate capturing spectacular celestial images with detailed resolution and vibrant colors. The L-550 carries a greater payload capacity – perfect for holding a second telescope on the outside hub.
Astronomy Research
Researchers will find the CDK450 invaluable for its consistent performance and precise data collection capabilities. It serves as a robust platform for sophisticated photometry, spectroscopy, and minor planet tracking, offering a solid foundation for scientific discovery and exploration.
Visual Observations
For enthusiasts of visual astronomy, the CDK450 provides vibrant and detailed views of the universe. Its significant aperture and high-quality optical components ensure exceptional viewing of planetary, lunar, and deep-sky objects, enriching every observational experience.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its swift and precise repositioning capabilities, the L-550 mount in the CDK450 system is capable of tracking satellites and space debris. However, it's important to note that while the L-series mounts are highly effective for astrophotography and research applications, they might not meet the optimal performance standards required for dedicated SSA/SDA operations. For those needs, we recommend exploring our T-600 Direct-Drive Gimbal, specifically engineered to exceed the demanding requirements for SSA/SDA applications, ensuring superior tracking and responsiveness in monitoring and cataloging space objects.
Mount system
| Mount Weight | 338 lbs (153 kg) |
| Max. Load Capacity | 300 lbs (136 kg) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
Control system
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter. |
Optical systems
| Aperture | 17 inch (432 mm) |
| Focal Length | 2939 mm (115.71 inch) |
| Focal Ratio | f/6.8 |
| Central Obstruction | 23.7% by surface area; 48.6% of the primary mirror diameter |
| Backfocus from Mounting Surface | 10.32 inch (262.33 mm) |
| Backfocus from Racked in Focuser | 7.24 inch (184 mm) |
| Weight | 106 lbs (48 kg) |
| Optimal Field of View | 70mm image circle |
Motion control
| Motor – Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder – Azimuth and Altitude | 152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution). |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | Uses PWI4. Incorporates PointXP mount modeling software by Dave Rowe. All ASCOM compatible. |
System Performance
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcseconds at sidereal velocity |
| Tracking Accuracy | 0.3 arcseconds over a 5-minute period at sidereal velocity |
| System Natural Frequency | 10 Hz or greater |
Included Items
| Included Items | Heating elements for dew prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube | |
| Flash drive - Contains PWI4 software for mount control , instructions for installation, software, and instructions for collimation and spacing the primary to secondary mirror | |
| Hardware - Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier, or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment | |
| One 16′ USB cable - To connect the mount to the observatory control computer | |
| One 120VAC power cable - To provide power to the mount | |
| Standard Allen Key set - For tightening bolts used on the mount | |
| Gamepad - Used for control of the mount tracking speeds for visual observing | |
| Dovetail Saddle (200919) - The PW wide saddle comes standard with the L-550 mount |
$63,800.00
The DeltaRho 350 Telescope System from PlaneWave Instruments is crafted for elite astronomers and astrophotographers who demand the best. Created with a passion for excellence, the DeltaRho 350 Telescope System brings groundbreaking features to advanced imaging, offering unmatched versatility across a spectrum of scientific and communicative applications. The DeltaRho 350 Telescope System from PlaneWave Instruments features a 350mm wide-field, f/3 aperture. This premium CDK optical tube combines a DeltaRho 350 with a L-350 direct drive mount.
DeltaRho 350 Telescope System’s Key Features
Large Aperture and Fast Focal Ratio
The DeltRho 350 has a 350 mm aperture and an impressively fast f/3 focal ratio. This combination allows significant light-gathering capability and rapid image capture, perfect for detailed SSA/SDA object capture and deep-sky photography.
Advanced Optical Design
Featuring a corrected Cassegrain focus optical system, the DeltaRho 350 ensures top-tier image clarity. Achieve sharp, flat fields across the entire field of view with no curvature, capturing stellar images that require minimal post-processing.
Mechanical Structure
Constructed with a lightweight yet sturdy carbon fiber tube. This Offers enhanced durability and stability while minimizing thermal expansion and maintaining optimal image quality under various environmental conditions.
High-Performance Coatings
Equipped with high-quality mirror coatings that can be customized to meet specific observational requirements. It enhances light transmission and reduces stray light, optimizing the telescope for specialized applications such as SSA/SDA and FSO.
Collimation Software
The DeltaRho 350 is equipped with user-friendly collimation software designed to ensure optimal alignment of optical elements quickly and accurately. This feature is crucial for maintaining the high resolution and sharpness needed for professional-level imaging and research, allowing users to adjust collimation on the fly easily.
Dew Control
Integrated dew control systems in the DeltaRho 350 utilize advanced heater technology to prevent condensation on optical surfaces. This system ensures that dew does not interrupt observations and imaging sessions, providing consistent clarity and performance in various environmental conditions.
Application-Specific Benefits
Astrophotography
The DeltaRho 350’s fast exposures and expansive field view allow astrophotographers to capture breathtaking night sky images with exceptional detail and clarity.
Astronomy Research
With its robust build and advanced optics, the DeltaRho 350 is an excellent tool for universities and research institutions engaged in long-term astronomical studies.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
The Delta Rho's fast focal ratio and large image circle allow you to take shorter exposures and use larger Sensors. Making it perfect for surveying larger areas of the sky for quicker monitoring and cataloging of space debris and satellites.
Mount Systems
| Mount Weight | 110 lbs (50 kg) |
| Max. Load Capacity | 100 lbs (45 kg) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
Control systems
| Control Electronics | PlaneWave Interface dual axis telescope control |
| User Interface | PlaneWave Interface 4 (PWI4) Control Software with integrated PointXP mount modeling software |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter. |
Optical Systems
| Aperture | 350 mm |
| Focal Length | 1050 mm (41.34 in.) |
| Focal Ratio | f/3 |
| Central Obstruction | 56 % by diameter |
| Backfocus from Mounting Surface | 5.6 in. (142.24 mm). This distance includes refraction from filters. |
| Weight | 46 lbs (21 kg) |
Motion control
| Motor – Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder – Azimuth and Altitude | 152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution). |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | Uses PWI4. Incorporates PointXP mount modeling software by Dave Rowe. All ASCOM compatible. |
System Performance
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcseconds at sidereal velocity |
| Tracking Accuracy | 0.3 arcseconds over a 5-minute period at sidereal velocity |
| System Natural Frequency | 10 Hz or greater |
Included items
| Included Items | Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube | |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror |
$114,599.00
RC20’s Key Features
Large Aperture and Ritchey-Chrétien Optics
The RC20 features a purely reflective Ritchey-Chrétien optical system, which includes high-quality mirrors with enhanced coatings. This setup minimizes chromatic aberration and ensures excellent light throughput, providing superb image fidelity and contrast. This optical design shines when making observations, primarily on-axis, and wide-field imaging is not a concern.
Mechanical Structure
Constructed from lightweight yet durable materials, including a dual carbon-fiber truss design, the 20-inch Ritchey-Chrétien ensures structural integrity and reduces the overall weight. This makes it easier to handle and mount on various telescope mounts.
Thermal Management
Equipped with three cooling fans at the back of the telescope, the RC20 achieves thermal equilibrium quickly. This feature helps to reduce air turbulence inside the telescope tube, minimizing thermal distortions and maintaining optimal imaging conditions.
Application-Specific Benefits
Astrophotography
The large aperture and precision optics of the 20-Inch Ritchey-Chrétien enable astrophotographers to capture detailed and crisp images of celestial phenomena, making it an excellent tool for capturing faint galaxies, nebulae, and star clusters.
Astronomy Research
With its reliable performance and detailed imaging capabilities, the 20-inch Ritchey-Chrétien is a valuable asset for universities and research observatories that engage in complex studies such as stellar classification, photometric research, and other scientific investigations.
Optical Systems
| Aperture | 508 mm (20") |
| Focal Length | 3556 mm (140") |
| Focal Ratio | f/7 |
| Central Obstruction | 39% of the Primary Mirror Diameter |
| Back Focus from Racked in Focuser | 147 mm (5.8") |
| Weight | 63.5 kg (140 lbs) |
| OTA Length | 1194 mm (47") |
| Upper Cage | Carbon Fiber Truss |
| Lower Cage | Carbon Fiber Truss with Carbon Fiber Light Shroud |
Secondary Mirro
| Diameter | 191mm (7.5") |
| Material | Fused silica |
| Shape | Hyperbolic |
| Coating | Enhanced Aluminum – 96% |
Primary Mirror
| Optical Diameter | 508 mm (20") |
| Outer Diameter | 521 mm (20.5") |
| Shape | Hyperbolic |
| Material | Enhanced Aluminum – 96% |
| Coating | Fused Silica |
| Included Items | Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube | |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror | |
| Wrench Set (5812A35) - Standard hex wrenches (European orders only) |
$62,999.00
State-of-the-Art Direct-Drive Motors
Equipped with PlaneWave's proprietary direct-drive motors on each axis, the L-550 ensures the telescopes' smooth, fast, and whisper-quiet movement. This capability is crucial for swiftly tracking celestial objects and satellites across the sky with minimal vibration and maximum accuracy.
High-Resolution Encoders
With high-resolution encoders on each axis, the L-550 delivers exact positioning, essential for capturing crisp, detailed night sky images. These encoders are vital for scientific applications demanding precise data collection.
Zero Backlash and Periodic Error
The L-550's design eliminates backlash and periodic error, facilitating steady tracking vital for top-notch astrophotography and dependable, long-term observational research.
Flexible Installation Options
The L-550 is available in both Alt/Az and equatorial configurations to meet a variety of observational needs. This versatility makes it suitable for fixed installations in educational observatories and adaptable setups for amateur astronomers.
Through-the-Mount Cabling
The innovative through-the-mount cabling system enhances setup cleanliness and safety, preventing cable snagging and reducing setup time.
Azimuth Dovetail Balance System
Provides precise center of gravity adjustments, enhancing the stability and performance of the system in both alt-azimuth and equatorial configurations, crucial for maintaining accurate tracking and reducing strain on the mount during extended observations.
Optional Dual Mounting Bracket
Allows for the attachment of additional telescopes or accessories on the mount, enhancing versatility and enabling simultaneous multi-instrument use, ideal for complex observational setups or educational demonstrations.
Rapid Target Acquisition
Equipped with direct-drive motors capable of slew speeds up to 50 degrees per second, enabling quick and efficient targeting of celestial objects and satellites, crucial for dynamic observations and time-sensitive astrophotography.
PointXP Mount Modeling Software
Included with the mount, PointXP software precisely models the mount's tracking behavior, enhancing its accuracy for critical applications. This software is invaluable for projects that require exact positioning and consistent tracking over extended periods.
Application-Specific Advantages
Astrophotography
The L-550's rapid slew speeds and silent operation allow astrophotographers to reposition swiftly and quietly between shots, capturing stunning celestial images without disrupting the observational setting.
Research
Researchers benefit from the L-550's robust construction and precise tracking to conduct detailed celestial observations and night-long monitoring with minimal interruption and consistent data quality.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
With its ability to swiftly and accurately reposition, the L-550 has ben been used for tracking satellites and space debris. However, our L-series mounts work best for astrophotography and research applications. To exceed the ideal performance requirements for SSA/SDA applications, we created the T-600 Direct-Drive Gimbal.
Mount Systems
| Type | Alt-Azimuth / Equatorial Direct Drive Mount |
| Weight | 153kg (338 lbs) |
| Max Load Capacity | 136kg (300 lbs) |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Equipment cables can be wired through mount |
| Swing-Through Length (From Altitude Axis) | 650.748 mm (25.62") |
Control Systems
| Control Electronics | PlaneWave Interface dual axis telescope control |
| Homing Sensors | Home position sensors are included allowing the mount can find its home position on power up. |
| Slew Rate | 20 degrees per second (standard); 50 degrees per second (maximum), both axes |
| Power Requirement | Accepts 120 to 240 VAC. Supplied with 120 VAC 15A IEC Type B Regulated Power Adapter. |
Motion control
| Motor Control | Industrial grade brushless motor control system and built in electronics |
| Motor – Azimuth and Altitude | Direct Drive 3 Phase Axial-Flux Torque Motors |
| Encoder – Azimuth and Altitude | 152mm stainless steel encoder ring with reader built into the azimuth and altitude axes. 18,880,000 counts per revolution (0.069 arcsecond resolution). |
| Motor Torque | Approximately 20 ft-lbs continuous; 50 ft-lbs peak |
| Drive Electronics | Industrial grade, off-the-shelf brushless motor drives for each axis with custom designed interface card |
| Telescope Control Software | Uses PWI4. Incorporates PointXP mount modeling software by Dave Rowe. All ASCOM compatible. |
System Performance
| Pointing Accuracy | <10 arcsecond RMS with PointXP Model |
| Pointing Precision | 2 arcseconds at sidereal velocity |
| Tracking Accuracy | 0.3 arcseconds over a 5-minute period at sidereal velocity |
| System Natural Frequency | 10 Hz or greater |
| Included Items | Dovetail Saddle (200919) - The PW wide saddle comes standard with the L-550 mount |
| Hardware - Six 1/2-13 x 1 1/4″ socket head cap screws to bolt the mount to the pier or wedge; Six 1/2-13 washers; One extended length shoulder bolt for RA axis to EQ wedge alignment | |
| One 16' USB Cable - To connect the mount to the observatory control computer | |
| One 120VAC power cable- To provide power to the mount | |
| Standard Allen Key Set- For tightening bolts used on the mount | |
| Flash drive- Contains PWI4 software for mount control and instructions for installation | |
| 3/8 Socket - Used for operating the RA balance leadscrew on the mount | |
| Gamepad - Used for control of the mount tracking speeds for visual observing | |
| Standard Allen Key Set- For tightening bolts used on the mount |
$9,999.00
- The IRF90 is a large capacity Integrated Focuser and Rotator for use with Alt/Az, or equatorially mounted systems.
- Occupies 3.5″ of backfocus with the focuser fully racked in, and 4.7″ when fully racked out.
- The Focuser is capable of lifting 40 lbs (18 kg) with a range of 30mm (30000 microns/1.2″).
- The Rotator has a 90mm aperture with a range of 365 degrees with hard stops to eliminate any chance of cord wrap.
- IRF90 is controlled via PWI4 software for autofocusing and optional field de-rotation (if using an Alt/Az mounted system).
$2,640.00
- The Hedrick focuser designed by PlaneWave is a heavy duty no-slip focuser capable of handling an imaging payload of up to 20lbs.
- Occupies 3″ of backfocus with the focuser fully racked in, and 4.2″ when fully racked out.
- Focuser travel range of 30mm (30000 microns/1.2″)
- The focus tube runs on 5 bearings and is driven by a leadscrew so there is no chance of slipping.
- Focus may be automated through a computer using PlaneWave’s EFA Kit and PWI3 software.
- The focuser comes with pre-installed motor that can be controlled with the EFA hand controller or PWI3 software.
$139,599.00
Large Aperture and Optimized Focal Ratio
The IRDK24 features a generous 610 mm aperture paired with an f/6.5 focal ratio, enhancing its ability to capture light effectively. This combination is ideal for detailed infrared observations and long-exposure imaging, providing superb light-gathering capabilities.
Specialized Optical Design for Infrared
The Dall-Kirkham optical design of the IRDK24 is optimized for infrared wavelengths. There are no refractive lenses, only reflective fused silica mirrors. Reflective coatings are a protected gold with better than 98% reflectivity from .65 microns (650nm) to 5 microns (5000nm), ideal for infrared astronomy or LIDAR applications. UV-optimized coatings can also be provided, so please contact our technical sales team to discuss UV optimization.
Robust Mechanical Structure
Constructed using carbon fiber, the optical tube of the IRDK24 offers durability and stability with minimal thermal expansion. This design ensures consistent performance under varying environmental conditions, making it suitable for intensive scientific applications.
Advanced Thermal Management
The IRDK24 incorporates cooling fans and a system ready for Delta-T applications, facilitating rapid thermal equilibrium. This setup is crucial for minimizing air turbulence within the tube, thus reducing potential image distortion and enhancing overall imaging quality.
Integrated Dew Control
Infrared observations can be susceptible to condensation, but the IRDK24 addresses this with sophisticated dew prevention technology. Heater pads, controlled via PlaneWave’s software, ensure the optical surfaces remain clear from dew, thereby maintaining consistent and clear imaging performance.
Application-Specific Benefits
Infrared Astronomy: The IRDK24 is especially effective for infrared astronomy, where its large aperture and infrared-optimized optics allow for detailed observation of celestial objects in infrared light. This capability is essential for studying astrophysical phenomena invisible to the naked eye or standard optical wavelengths.
Advanced Research and LIDAR Applications: With its specialized design and infrared optimization, the IRDK24 is a robust platform for advanced scientific research, including LIDAR.
Optical Systems
| Aperture | 610 mm (24") |
| Focal Length | 3974 mm (156") |
| Focal Ratio | f/6.5 |
| Central Obstruction | 47% of the primary mirror diameter |
| Back Focus From Mounting Surface | 364.46 mm (14.349") |
| Weight | 240 lbs (108.9 kg) |
| OTA Length | 1422 mm (56") |
| Optical Design Performance | 2.4-micron RMS on-axis, 4.0-micron RMS at 26 mm off-axis, 4.8-micron at 35 mm off-axis |
| Upper Cage | Carbon fiber truss |
| Lower Cage | Carbon fiber truss with aluminum light shroud |
Primary Mirror
| Optical Diameter | 610 mm (24") |
| Outer Diameter | 622 mm (24.5") |
| Shape | Prolate Ellipsoid |
| Coating | Protected Gold |
Secondary Mirror
| Diameter | 280 mm (11") |
| Material | Fused silica (quartz) |
| Shape | Spherical |
| Coating | Protected Gold |
| Included Items | CDK24 Focus Spacer (240343-1) - This 5.539″ long spacer is installed between the backplate and the focuser to take up some of the CDK24’s extra backfocus and reduce the torque placed on the focuser mechanism. This spacer is sized such that the backfocus distance behind the focuser is 8.8″. |
| Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately | |
| Primary Mirror Cover - To protect the primary mirror | |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror |
$127,499.00
CDK24’s Key Features
Large Aperture and Moderate Focal Ratio
The CDK24 features a substantial 610 mm aperture and a moderate f/6.5 focal ratio. This setup enhances its capability to capture deep-sky objects with remarkable detail, providing excellent light-gathering efficiency and a broad field of view for research and imaging.
Advanced Optical Design
Equipped with a state-of-the-art Corrected Dall-Kirkham optical system, the CDK24 offers exceptional image clarity. Its design eliminates off-axis coma and astigmatism and delivers a perfectly flat field, ensuring images are sharp and detailed across the entire field of view with minimal post-processing adjustments.
Robust Mechanical Structure
Constructed with a carbon fiber optical tube, the CDK24 is lightweight and durable. Its thermal expansion coefficient ensures minimal focus shift as temperatures change, making it ideal for prolonged observing sessions under varying environmental conditions.
High-Performance Mirrors and Coatings
Utilizing fused silica mirrors, the CDK24 maintains precise optical alignment and surface accuracy, even with temperature fluctuations. Its high-quality coatings enhance light transmission and reduce stray light, optimizing performance for specialized observational tasks.
Thermal Management
The CDK24 is equipped with cooling fans and a Delta-T ready system to achieve thermal equilibrium swiftly. These features help to minimize air turbulence within the tube, thus reducing image distortion and maintaining consistent imaging quality.
Integrated Dew Control
The telescope incorporates advanced dew prevention technology with heater pads controlled by PlaneWave’s software. This ensures that optical surfaces remain clear of condensation during humid conditions, thus maintaining clear and consistent imaging performance.
Application-Specific Benefits
Astrophotography
With its large image circle and exquisite field flatness, the CDK24 allows astrophotographers to capture expansive and breathtaking views of the cosmos with incredible detail and clarity.
Astronomy Research
The precise and stable imaging capabilities of the CDK24 make it an invaluable tool for academic institutions and observatories engaged in complex astronomical research, including deep-sky surveys and detailed photometric studies.
Visual Observations
The CDK24 excels in visual observation, offering bright and crisp views ideal for star parties and serious visual astronomy. The telescope's large aperture and superior optical quality provide stunning views of planetary, lunar, and deep-sky objects, making every viewing session a remarkable experience.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
The CDK24 also lend itself to applications in Space Situational Awareness and Space Domain Awareness. 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 | 610 mm (24") |
| Focal Length | 3974 mm (156") |
| Focal Ratio | f/6.5 |
| Central Obstruction | 47% of the primary mirror diameter |
| Back Focus From Mounting Surface | 364.46 mm (14.349") |
| Weight | 240 lbs (108.9 kg) |
| OTA Length | 1422 mm (56") |
| Optical Design Performance | 2.4-micron RMS on-axis, 4.0-micron RMS at 26 mm off-axis, 4.8-micron at 35 mm off-axis |
| Upper Cage | Carbon fiber truss |
| Lower Cage | Carbon fiber truss with aluminum light shroud |
| Image Circle Size | 70mm |
Secondary Mirror
| Diameter | 280 mm (11") |
| Material | Fused silica (quartz) |
| Shape | Spherical |
| Coating | Enhanced Aluminum - 96% |
Lens Group
| Diameter | 135 mm (5.31") |
| Coating | Broadband AR Coatings (less than .5% reflected from 400 to 700 nm) |
Primary Mirror
| Optical Diameter | 610 mm (24") |
| Outer Diameter | 622 mm (24.5") |
| Shape | Prolate Ellipsoid |
| Coating | Enhanced aluminum – 96% |
$78,399.00
IRDK20’s Key Features
Large Aperture and Optimized Focal Ratio
The IRDK20 features a substantial 508 mm aperture and an f/6.8 focal ratio, enhancing its ability to gather infrared light effectively. This setup is ideal for detailed infrared observations and long-exposure imaging, offering excellent light-gathering capabilities.
Specialized Optical Design for Infrared
The Dall-Kirkham optical design of the IRDK20 is optimized for infrared wavelengths. There are no refractive lenses, only reflective fused silica mirrors. The reflective coatings are a protected gold with better than 98% reflectivity from .65 microns (650nm) to 5 microns (5000nm), ideal for infrared astronomy or LIDAR applications. UV-optimized coatings can also be provided, so please contact our technical sales team to discuss UV optimization.
Robust Mechanical Structure
Constructed using carbon fiber, the optical tube of the IRDK20 provides durability and stability with minimal thermal expansion. This design ensures consistent performance across varying environmental conditions, making it suitable for intensive scientific applications.
Advanced Thermal Management
The IRDK20 includes cooling fans and a system prepared for Delta-T applications, promoting rapid thermal equilibrium. This setup is crucial for minimizing air turbulence within the tube, thus reducing potential image distortion and enhancing overall imaging quality.
Integrated Dew Control
Infrared observations can be prone to condensation, but the IRDK20 addresses this with advanced dew prevention technology. Heater pads, controlled via PlaneWave’s software, ensure the optical surfaces remain clear from dew, maintaining consistent and clear imaging performance.
Application-Specific Benefits
Infrared Astronomy
The IRDK20 excels in infrared astronomy, where its large aperture and infrared-optimized optics allow for detailed observation of celestial objects in infrared light. This capability is crucial for studying astrophysical phenomena invisible to the naked eye or standard optical wavelengths.
Advanced Research and LIDAR Applications
With its specialized design and infrared optimization, the IRDK20 is a robust platform for advanced scientific research, including LIDAR applications.
Optical Systems
| Aperture | 508 mm (20") |
| Focal Length | 3454mm (136") |
| Focal Ratio | f/6.8 |
| Central Obstruction | 39% of the Primary Mirror Diameter |
| Back Focus From Mounting Surface | 8.81 in (224 mm) |
| Weight | 63.5kg (140 lbs) |
| OTA Length | 1194mm (47") |
| Upper Cage | Carbon Fiber Truss |
| Lower Cage | Carbon Fiber Truss and light shroud |
Secondary Mirror
| Diameter | 191mm (7.5") |
| Material | Fused Silica (Quartz) |
| Shape | Spherical |
| Coating | Protected Gold |
Primary Mirror
| Optical Diameter | 508mm (20") |
| Outer Diameter | 521mm (20.5") |
| Shape | Prolate Ellipsoid |
| Material | Fused Silica (quartz) |
| Coating | Protected Gold |
| Included Items | Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube | |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror |
$8,599.00
- Add to the versatility of your L500/600 Direct Drive Mount with PlaneWave’s Equatorial Wedge for precise polar alignment and tracking accuracy.
- Each wedge is made for your specific latitude and has an alignment range of +/- 3 degrees.
- Uses oversized fine thread adjustment screws and brass tightening nuts for fine latitude adjustment.
- Weighs 145lbs fully assembled
From $6,499.00
- Create a rock-solid foundation for your PlaneWave Direct-Drive mount by using a PlaneWave heavy-duty steel pier.
- Our piers come in standard 12″ increments ranging from 12″ tall to 48″ tall.
- Each pier has a cutout in the top plate and side for routing cables.
- Custom pier heights are available. Please contact us if you require a custom pier.
From $6,469.00
- Create a rock-solid foundation for your PlaneWave Direct-Drive mount by using a PlaneWave heavy-duty steel pier.
- Our piers come in standard 12″ increments ranging from 12″ tall to 48″ tall.
- Each pier has a cutout in the top plate and side for routing cables.
- Custom pier heights are available. Please contact us if you require a custom pier.
$47,299.00
CDK17’s Key Features
Large Aperture and Moderate Focal Ratio
The CDK17 features a 432 mm aperture and an f/6.8 focal ratio. This combination enhances its capability to capture deep-sky objects with exceptional detail, offering excellent light-gathering efficiency and a broad field of view suitable for advanced research and high-quality imaging.
Advanced Optical Design
Equipped with a state-of-the-art Corrected Dall-Kirkham optical system, the CDK17 delivers outstanding image clarity. Its innovative design eliminates off-axis coma and astigmatism. It provides a perfectly flat field, ensuring images are sharp and detailed across the entire field of view with minimal need for post-processing.
Robust Mechanical Structure
Constructed with a carbon fiber optical tube, the CDK17 is lightweight and durable. Its design minimizes thermal expansion, ensuring minimal focus shift with temperature changes, making it ideal for extended observing sessions under varying environmental conditions.
High-Performance Mirrors and Coatings
Using fused silica mirrors, the CDK17 maintains precise optical alignment and surface accuracy, even amid temperature fluctuations. The high-quality coatings enhance light transmission and reduce stray light, optimizing performance for specialized observational tasks.
Thermal Management
The CDK17 is equipped with cooling fans and a Delta-T ready system to achieve thermal equilibrium swiftly. These features help to minimize air turbulence within the tube, thus reducing image distortion and maintaining consistent imaging quality.
Integrated Dew Control
The telescope incorporates advanced dew prevention technology with heater pads controlled by PlaneWave’s software. This ensures that optical surfaces remain clear of condensation during humid conditions, thus maintaining clear and consistent imaging performance.
Application-Specific Benefits
Astrophotography
With its large image circle and exceptional field flatness, the CDK17 allows astrophotographers to capture expansive and breathtaking views of the cosmos with incredible detail and clarity.
Astronomy Research
The precise and stable imaging capabilities of the CDK17 make it an invaluable tool for academic institutions and observatories engaged in complex astronomical research, including deep-sky surveys and detailed photometric studies.
Visual Observations
The CDK17 excels in visual observation, offering bright and crisp views ideal for star parties and serious visual astronomy. The telescope's superior optical quality provides stunning views of planetary, lunar, and deep-sky objects, making every viewing session a remarkable experience.
Space Situational Awareness (SSA) and Space Domain Awareness (SDA)
The CDK17 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 | 432mm (17 in) |
| Focal Length | 2939 |
| Focal Ratio | f/6,8 |
| Central Obstruction | 23.7% by surface area; 48.6% of the primary mirror diameter |
| Back Focus From Mounting Surface | 262.33mm (10.32 in) |
| Back Focus From Racked In Focuser | 184mm (7.24 in) |
| Weight | 48kg (106 lbs) |
| OTA Length | 1067mm (42 in) |
| Optical Design Performance | 6.5 micron rms at 21mm and 9.6 micron at 26mm off-axis |
| Upper Cage | Carbon Fiber Truss |
| Lower Cage | Carbon Fiber Truss and light shroud |
| Image Circle Size | 70mm |
Secondary Mirror
| Diameter | 165mm (6.5 in) |
| Material | Fused Silica (Quartz) |
| Shape | Spherical |
Lens Group
| Diameter | 105mm (4.13 in) |
| Coating | Broadband AR Coatings (less than .5% reflected from 400 to 700nm) |
Primary Mirror
| Optical Diameter | 432 mm (17 in) |
| Outer Diameter | 445 mm (17.5 in) |
| 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 |
| 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 |
$29,799.00
IRDK12.5’s Key Features
Large Aperture and Optimized Focal Ratio
The IRDK12.5 features a significant 318 mm aperture and an f/8 focal ratio, enhancing its efficiency in capturing infrared light. This setup is perfect for detailed infrared observations and extensive exposure imaging, offering outstanding light-gathering capacity.
Specialized Optical Design for Infrared
The Dall-Kirkham optical design of the IRDK12.5 is tailored for infrared wavelengths. It incorporates only reflective fused silica mirrors and no refractive lenses. The reflective coatings are protected gold, ensuring more than 98% reflectivity from 0.65 microns (650nm) to 5 microns (5000nm), making it ideal for infrared astronomy and environmental LIDAR applications. UV-optimized coatings are also available upon request.
Robust Mechanical Structure
Constructed using carbon fiber, the optical tube of the IRDK12.5 ensures durability and stability with minimal thermal expansion. This design maintains consistent performance under varying environmental conditions, suitable for rigorous scientific applications.
Advanced Thermal Management
Equipped with cooling fans and a system ready for Delta-T applications, the IRDK12.5 promotes rapid thermal equilibrium. This feature is critical for minimizing air turbulence inside the tube, thereby reducing potential image distortion and enhancing the quality of imaging.
Integrated Dew Control
The IRDK12.5 is designed to combat condensation, a common challenge in infrared observations. Advanced dew prevention technology, including heater pads controlled via PlaneWave’s software, keeps the optical surfaces clear of dew, ensuring consistent and clear imaging performance.
Application-Specific Benefits
Infrared Astronomy
The IRDK12.5 excels in infrared astronomy, where its large aperture and infrared-optimized optics allow for detailed observation of celestial objects in infrared light. This capability is essential for studying astrophysical phenomena not visible in standard optical wavelengths.
Advanced Research and LIDAR Applications
With its specialized design and infrared optimization, the IRDK14 is a robust platform for advanced scientific research, including LIDAR and other remote sensing applications.
Optical Systems
| Aperture | 318mm (12.5 in) |
| Focal Length | 2541 (100 in) |
| Focal Ratio | f/8 |
| Central Obstruction | 42% of the primary mirror diameter |
| Back Focus From Mounting Surface | 265mm (10.4 in) |
| Weight | 19kg (42 lbs |
| OTA Length | 787mm (31 in) |
| Upper Cage | Carbon Fiber Truss |
Secondary Mirror
| Diameter | 118mm (4.65 in) |
| Material | Fused Silica (Quartz) |
| Shape | Spherical |
| Coating | Protected Gold |
Primary Mirror
| Optical Diameter | 318mm (12.5 in) |
| Outer Diameter | 330mm (13 in) |
| Shape | Prolated Ellipsoid |
| Material | Fused Silica (Quartz) |
| Coating | Protected Gold |
| Included Items | Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube | |
| Flash drive - Contains software and instructions for collimation and spacing the primary to secondary mirror | |
| Wrench Set (5812A35) - Standard hex wrenches (European orders only) | |
| Cable connector for fan power - Provides a connection method for powering for the fans if the user does not have the 125901 EFA kit. User must provide 12VDC power supply 2.1 barrel jack connector that is center positive. (Not included for European orders) |
$39,000.00
The IRDK14 from PlaneWave Instruments is a precisely engineered optical system designed for high performance in infrared wavelengths. It is an excellent tool for advanced astronomical research and remote sensing applications, offering superior performance for infrared imaging.
IRDK14’s Key Features
Large Aperture and Optimized Focal Ratio
The IRDK14 features a 356 mm aperture and an f/7.2 focal ratio, enhancing its capacity to gather infrared light effectively. This setup is ideal for detailed infrared observations and long-exposure imaging, providing exceptional light-gathering capabilities.
Specialized Optical Design for Infrared
The Dall-Kirkham optical design of the IRDK14 is optimized for infrared wavelengths. There are no refractive lenses, only reflective fused silica mirrors. The reflective coatings are a protected gold with better than 98% reflectivity from .65 microns (650nm) to 5 microns (5000nm), making it well-suited for infrared astronomy or LIDAR applications. UV-optimized coatings can also be provided, and potential customers are encouraged to contact our technical sales team to discuss UV optimization.
Robust Mechanical Structure
Constructed using carbon fiber, the optical tube of the IRDK14 offers durability and stability with minimal thermal expansion. This design ensures consistent performance under various environmental conditions, making it suitable for intensive scientific applications.
Advanced Thermal Management
The IRDK14 includes cooling fans and a system prepared for Delta-T applications, promoting rapid thermal equilibrium. This feature is critical for minimizing air turbulence within the tube, thus reducing potential image distortion and enhancing overall imaging quality.
Integrated Dew Control
Infrared observations are prone to condensation, but the IRDK14 tackles this with advanced dew prevention technology. Heater pads, controlled via PlaneWave’s software, ensure the optical surfaces stay clear from dew, maintaining consistent and clear imaging performance.
Application-Specific Benefits
Infrared Astronomy
The IRDK14 excels in infrared astronomy, where its significant aperture and infrared-optimized optics allow for precise observation of celestial objects in infrared light. This capability is essential for studying astrophysical phenomena invisible to the naked eye or standard optical wavelengths.
Advanced Research and LIDAR Applications
With its specialized design and infrared optimization, the IRDK14 is a robust platform for advanced scientific research, including LIDAR and other remote sensing applications.
Key Features Overview
The IRDK14 comes with impressive specifications tailored for infrared optimization:
- Gold-coated mirrors optimized for high reflectivity in infrared wavelengths (ultraviolet optimization available)
- 14-inch (356 mm) aperture
- 2563 mm focal length
- f/7.2 focal ratio
- 282mm back focus from mounting surface
- 70mm image circle
- Rock-solid fused silica mirrors with low thermal expansion
- Lightweight and rigid carbon fiber optical tube assembly
Optical Systems
| Aperture | 356mm (14 in) |
| Focal Length | 2563mm (101 in) |
| Focal Ratio | F/7.2 |
| Central Obstruction | 23.5% by Surface Area: 48.5% by Diameter |
| Back Focus From Mounting Surface | 282mm (11.09 in) |
| Weight | 22kg (48lbs) |
| OTA Length | 889mm (35 in) |
| Upper Cage | Carbon Fiber Truss |
| Lower Cage | Carbon Fiber Truss And Light Shroud |
Secondary Mirror
| Diameter | 165mm (6.5 in) |
| Material | Fused Silica (Quartz) |
| Shape | Spherical |
| Coating | Protected Gold |
Primary Mirror
| Optical Diameter | 355.6mm (14 in) |
| Outer Diameter | 468.3mm (14.5 in) |
| Shape | Prolated Ellipsoid |
| Material | Fused Silica (Quartz) |
| Included Items | Heating Elements for Dew Prevention - The heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately |
| OTA Cover - To protect the primary mirror and inside of the optical tube | |
| Flashdrive - Contains software and instructions for collimation and spacing the primary to secondary mirror | |
| Wrench Set (5812A35) - Standard hex wrenches (European orders only) |
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