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PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics

PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
Ask About Stock
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
PlaneWave CDK 17" f/6.8 Astrograph OTA with Fused Silica Optics
£27,290.00
Ex Tax: £22,741.67
  • Stock: Ask About Stock
  • Model: 1323217Q
  • Shipping Weight: 75.00kg
  • SKU: 1323217Q
  • MPN: 1323217Q
  • Location: E180

PlaneWave CDK 17" f/6.8 OTA (Optical Tube Assembly) with Fused Silica Optics

Please call us for availability info!

  • CDK17 Astrograph, 17 inch with Fused Silica Optics
  • modified to Dall-Kirkham, with fully corrected image field
  • 8" Dovetail bar, focal length 2,940 mm (f/6.8) and 70 mm field of view (instead of the normal CDK 17" - 52mm) without any field curavature, off-axis coma, or astigmatism
  • Delta T Ready, (3.5" Hedrick Focuser and EFA Kit available separately)

The PlaneWave Instruments CDK17 is a 17 inch (0.43 m) f/6.8 Corrected Dall-Kirkham Astrograph telescope. 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 back plate retaining ring ready to accept the focuser of your choice.

The abbreviation CDK stands for the optical system of the PlaneWave astrographs - a Dall Kirkham Cassegrain with a optical correction unit. More about the Optical Design (CDK).

The PlaneWave CDK17 is available in various types of mirror material. Standard mirror material is borosilicate. The telescope is also available in fused silica optics.

Fused Silicia 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 expansion six times lower than Borosilicate (Pyrex) 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 its high melting temperature ()~ 1.600 degree 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.

Due to the relatively low weight of just under 43kg (telescope tube), the CDK17 can be used on one of our medium-to-large mounts - e.g. a Fornax 52, Fornax 100 or Paramount

  • Aperture: 17" = 430 mm
  • Focal length: 2.940 mm
  • Focal ratio: f/6.8
  • Obstruction: 49% of the Primary Mirror Diameter
  • Field of View = 70 mm (instead of the normal CDK 17" - 52mm)
  • Figure = diffraction plates of 6.5 mu / 21mm off axis and 9.6 mu / 26mm off axis at 430, - 585 and 730 nanometer wavelength
 
Spot diagramm for CDK 17 Widefield Astrograph
 
 

The graphic above shows the vignetting and spot diagrams for the CDK 17 Widefield Astrographer depending on the large CCD chips KAF 6303, KAF 11000 and KAF 09000 for the three wavelengths 730, 585 and 430 Nanometer.

The diameter of a star at the edge of the flat field corresponds to the pixel size of current large-format CCD chips and the imaging quality of the optics is limited only by the seeing conditions and the quality of the tracking. The large field of view of 70mm diameter offers enough tolerance for CCD cameras with ever larger chips - also for amateur astronomy.

 

Pictures taken by CDK17":

NGC 6960, Veil Nebula
NGC 6960, Veil Nebula
M 31, The Andormeda Galaxy
M 31, The Andormeda Galaxy
M 81
M 81
NGC 6888, Crescent Nebula
NGC 6888, Crescent Nebula

Specifications:

OPTICAL SYSTEM

Aperture17 inch (432 mm)
Focal Length2939 mm (115.71 inch)
Focal ratiof/6.8
Central Obstruction23.7% by surface area; 48.6% of the Primary Mirror Diameter
Back Focus from Mounting Surface10.24 inch (260 mm)
Back Focus from Racked in Focuser7.24 inch (184 mm)
Weight106 lbs (48 kg)
OTA Length42 inch (1067 mm)
Optical Performance6.5 micron rms at 21mm and 9.6 micron at 26mm off-axis
UpperCageCarbon Fiber Truss
Lower CageCarbon Fiber Truss and Light Shroud
Optimal Field of View70mm Image Circle

 

SECONDARY MIRROR

Diameter190 mm (7.48 inch)
MaterialPrecision Annealed Pyrex
ShapeSpherical
CoatingEnhanced Aluminum - 96%
 

PRIMARY MIRROR

Optical Diameter17 inch (432 mm)
Outer Diameter17.5 inch (445 mm)
ShapeProlate Ellipsoid
MaterialPrecision Annealed Borosilicate or Fused Silica
CoatingEnhanced Aluminum - 96%

LENS GROUP

Diameter105 mm (4.13 inch)
Number of lenses2
CoatingBroadband AR Coatings (less than .5% reflected from 400 to 700nm)

STANDARD FEATURES

Carbon Fiber Tube DesignMinimizes thermal expansion which causes focus shift with changes in temperature
Dovetail expansion jointAllows 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 FansThree 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.
General Information
Weight in Kg43

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