Planewave - CDK400 Observatory System - CDK17 with L500 Mount
The Planewave CDK400 includes a Planewave CDK17 telescope and the L500 Direct Drive mount. Designed for affordability and high demand applications, this is a high precision observatory system.
The CDK17 features a truss tube design, 3 built in cooling fans and fused silica optical glass for maximized temperature stability.
Prewired to accept Delta-T.
The L500 direct drive mount can be configured in either AZ or EQ, and with no gears the L500 exhibits zero backlash and no periodic error.
High resolution encoders provide feedback to counteract gusts of wind and further enhance mount precision.
If you choose to place an order for this item, you will be contacted for crating and shipping fee information and options. To receive a quote contact us at [email protected].
Planewave - CDK400 Observatory System
Built for exceptional optical and tracking performance, and, designed for astrophotography or research, the CDK400 observatory package includes a Planewave CDK17 and an L500 mount. Building on a legacy of high performance 1 meter telescopes, Planewave has drawn from that same advanced optical system and precision direct drive mount to meet the demands of research and educational observatories. The CDK400 observatory system was also designed to be an affordable observatory solution.
The PlaneWave Instruments CDK17 is a 17 inch (0.43 m) f/6.8 Corrected Dall-Kirkham Astrograph telescope. The CDK17 has a dual carbon-fiber truss design, with 3 cooling fans ejecting air from the back of the telescope, and 4 fans blowing across the boundary layer of the mirror’s surface. The CDK17 covers a 70 mm field of view without any field curvature, off-axis coma, or astigmatism. The instrument weight is 94 lbs (43 kg) and comes standard with a backplate retaining ring ready to accept the focuser of your choice.
CDK400 Features
CDK17 Optical Tube:
- f/6.8 and 2939mm focal length
- No coma, no off-axis astigmatism, and no field curvature.
- Pinpoint stars across a 70mm image circle.
- Rock solid fused silica mirrors with low thermal expansion.
- Carbon fiber optical tube assembly for rigidity and fast cooling.
- Simple secondary mirror collimation thanks to the fixed primary mirror.
- Pre-wired for Delta-T, and equipment with a polyimide film heater pads and temperature sensor. DeltaT sold separately.
- 3 cooling fans at the rear of the primary and 3 cooling fans at the side of the telescope body, allow the system to reach thermal equilibrium quickly.
- Dovetail expansion joint provides a buffer between the expansion rate of the carbon fiber trusses and the aluminum dovetail for additional thermal stability.
- 3D printed baffles minimize stray light and vignetting, while maximizing contrast.
Planewave Fused Silica Mirrors
With a coefficient of thermal expansion 6 times lower than Borosilicate Pyrex glass, fused silica optical glass is exponentially more stable as temperatures change. For long observing or imaging sessions, this added stability reduces the need to adjust focus.
3D Printed Baffles
Using 3D printing technology, Planewave is able to produce a lightweight successive layers with highly precise positioning to minimize stray light and vignetting while maximizing contrast.
Dovetail Expansion Joint
To provide additional thermal expansion stability, the CDK24 is equipped with an expansion joint to account for the different expansion rates of the carbon fiber trusses and the aluminum dovetail.
Cooling Fans
Three rear cooling fans pull air through the optical tube near the primary mirror, and three additional fans blow air across the primary from the side of the telescope body. This combination of fans and open truss design allow the CDK24 to reach thermal equilibrium quickly. The fans are controlled by a manual switch on the optical tube or can be controlled with PWI3 software when the Planewave EFA kit is added.
CDK vs. RC Optical Design
Ritchey Chretien optical design, though highly successful in eliminating many typical optical problems naturally found in preceding designs, does not correct off-axis astigmatism and field curvature. While these issues can be corrected with the addition of correctors and flatteners as accessories to the telescope, David Rowe developed a new Corrected Dall Kirkham design that effectively incorporates these correctors into the optics. By utilizing an ellipsoid primary mirror, a spherical secondary mirror and a lens specifically configured doublet lens group, coma, off-axis astigmatism and field curvature are eliminated.
L500 Mount
The Planewave L500 combines versatility, simplicity and affordability by combining all the technology of our Observatory class telescopes into a compact stand-alone mount. In its Alt/Az configuration, it is considerably more compact than its equatorial counterpart, allowing a larger telescope to fit in a smaller enclosure. The mass it takes to make a rigid alt/az mount is substantially less, leading to cost savings. Unlike German Equatorial mounts, there are no meridian flips to deal with, and no large protruding counterweights to create a dangerous hazard in a public observatory. Alt/Az is more intuitive to use and no polar alignment is needed.
L-Series Mount Features:
- Direct-drive motors on each axis for smooth, fast, and virtually silent movement of the telescope.
- Load capacity of up to 200 pounds.
- Slew speeds up to 50 degrees per second
- High-resolution encoders on each axis for precise positioning with feedback to counteract gusts of wind.
- Sidereal tracking accuracy of <0.30 arcseconds RMS over 5 minutes.
- Zero backlash
- Zero periodic error
- PointXP mount modelling software
- Enclosed electronics and through mount cabling for neat cable management with easy to access panels.
- PWI4 telescope control with PointXP mount modeling software.
- Can be configured either AZ or EQ.
- Optional dual mounting with additional dovetail bracket.
Additional Included Items:
- Heating elements for dew prevention, heating pads on the primary and secondary mirror require the 600195 Delta-T controller sold separately.
- OTA cover to protect the primary and interior of the optical tube.
- Flashdrive containing all software and instructions for collimation and spacing the primary to the secondary. A second flashdrive contains PWI4 software and installation instructions.
- Hardware: 6 1/2-13x1 1/4" socket head cap screws to bolt the mount to th e pier or wedge. 6 1/2-13 washers. 1 extended length shoulder bolt for RA axis to EQ wedge alignment.
- 1 16' USB cable for computer connection.
- 1 120VAC power cable to power the mount.
- Standard Allen key set
- Game pad for mount control while visually obvserving.
CDK400 System Specifications:
CDK17Specifications:
| Optical Design | Corrected Dall Kirkham |
| Aperture | 17 inch 432mm |
| Focal Length | 2939mm |
| Focal Ratio | f/6.8 |
| Central Obstruction | 23.7% by surface area: 48.6% of the primary mirror diameter |
| Back Focus from Mounting Surface | 10.32 inch (262.33mm) |
| Back Focus from Racked in Focuser | 7.24 inch (184mm) |
| Weight | 106 pounds |
| OTA Length | 42 inches (1067mm) |
| Optical Performance | 6.5 microns RMS at 21mm and 9.6 micron at 26mm off axis |
| Optical Tube Material and Construction | Carbon fiber trusses with an aluminum shroud on the lower cage |
| Optical Field of View | 70m image circle |
| Secondary Mirror Diameter | 190mm (7.48 inch) |
| Secondary Mirror Material | Fused silica quartz |
| Secondary Mirror Shape | Spherical |
| Secondary Mirror Coating | Enhanced Aluminum - 96% |
| Primary Mirror Diameter | 17 inch (432mm) |
| Primary Mirror Outer Diameter | 17.5 inch (445mm) |
| Primary Mirror Shape | Prolate ellipsoid |
| Primary Mirror Material | Fused silica quartz |
| Primary Mirror Coataing | Enhanced Aluminum 96% |
| Lens Group Diameter | 105mm (4.13 inch) |
| Number of Lenses | 2 |
| Coating | Broadband AR Coatings (less than 0.5% reflected from 400 - 700nm) |
L500 Mount Specifications:
| Type | Alt-Azimuth/ Equatorial Direct Drive mount |
| Weight | 257 pounds |
| Component Weights | Azimuth base = 121 pounds, fork arm = 136 pounds |
| Max. Load Capacity | 200 pounds |
| Latitude Range | 0 to 90 degrees, Northern and Southern hemispheres |
| Cable Management | Through mount cabling with easy to access panels |
| Swing Through Length (from Altitude Axis) | 25.62" |
| Control Electronics | PWI dual axis control |
| User Interface | PWI4 with PointXP |
| Homing Sensors | Included for finding home postition at start up. |
| Slew Rate | 20 degres 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 supply. |
| 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. 18,800,000 counts per revolution. (0.069 arcsecond resolution). |
| Motor Torque | Approx 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 |
| Telescope Control Software |
PWI4 with PointXP mount odeling software. HTTP and ASCOM control interfaces. Maxim DL is required for camera control with using PWI4 modeling. |
| 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 |
Shipping Informatione
The crated weight of this system is 225 pounds, 30x37x58 inches. The CDK400 is an oversize and heavy crated shipment that does require air, ship or truck freight delivery. At this time our website is not able to calculate shipping rates for freight You will be contacted to discuss shipping options and crating fees for your order. If you require a quote at any time prior to placing an order, please reach out to us at [email protected].
Warranty
1 year warranty on optics and 2 years on mechanical
| Brand | PlaneWave Instruments |
|---|---|
| Free Shipping | Does Not Qualify for Free Shipping |
| Aperture | 17" (432mm) |
| Case Included | No |
| Focal Length | 2939mm |
| Focal Ratio | F/6.8 |
| Focus Type | None, ready to accept user choice of focuser. |
| Finderscope Included | No |
| Diagonal Included | No |
| Optical Tube Material | Carbon Fiber |
| Highest Useful Magnification | 864x |
| Resolution - Dawes | 0.04 arcseconds |
| LIght Gathering Power (Compared to the Human Eye) | 3809x |
| Secondary Mirror Obstruction By Diameter | 23.7% |
| Secondary Mirror Obstruction By Area | 48.6% |
| Optical Coatings | Aluminum |
| Optical Tube Length | 1067mm |
| Optical Tube Weight | 106 pounds |
| Included Dovetail | D series with expansion joint |
| Mount Load Capacity | 200 pounds |
| Accessory Tray Included? | No |
| Counterweights Included | No |
| Adjustable Legs? | No |
| Slew Speeds | 20 degrees per second standards, up to 50 degrees per second max on both axes |
| Mount Motor Drive | Direct Drive |
| GPS | No |
| Includes Autoguide Port | Yes |
| USB Port | Yes |
| Power Requirements | Accepts 120 to 240 VAC, supplied with 120 VAC 15 IEC Type B regulated power adapter |
| Computerized Hand Controller | Yes, for manual control during visual use |
| Included Software | PWI4 with PointXP mount modeling |
| Periodic Error Correction | No |
| Total System Weight | 363 pounds |
| Warranty | 1 year on optics and 2 years on mechanical |
| In The Box |












