next up previous contents
Next: Finder telescope Up: The Jacobus Kapteyn Telescope Previous: Mechanical performance

Optics

Details of the individual optical elements are collected in Table 1. Table 2 gives the most important parameters of the available optical configuration, illustrated in Figure 3. The parabolic primary has a clear diameter of 1.000m and a focal length of 4.596m.

The hyperbolic secondary constitutes with the primary a conventional f/15 Cassegrain system. The curved focal surface is located 760 mm behind the pole of the primary mirror, giving a 34.4 arcmin diameter field with a scale of 13.8 arcsec/mm.

The maximum movement of the secondary mirror is 20mm about the nominal focus position. For the f/15 system this produces a shift of 241mm about the optimum focal position; the on-axis image size is calculated to grow approximately linearly with focus shift up to a maximum diameter of 0.3 arcsec.

As of 1998 the Harmer-Wynne f/8.06 focus has been decommissioned.


 
Figure 3: Optical layout of the JKT, showing the f/15 Cassegrain configuration
\begin{figure}\centerline{\psfig{figure=jagccdfig3.eps,width=15cm}}\end{figure}


 
Table 1: Summary of mirror characteristics for the JKT
Element Shape Asphericity Working Focal Separation from Material
      Diameter length primary  
             
Primary Paraboloid -1 1000mm 4596mm   Cervit
f/15 Secondary Hyperboloid -3.545 307mm 1811mm 3342mm Zerodur
Finder (doublet) Sph. surfaces   200mm 3250mm    


 
Table 2: Optical characteristics of JKT foci
Focal station Cassegrain Finder
Focal length (mm) 15000 3250
Focal ratio f/15 f/16.25
Field diameter (arcmin)    
    no vignetting 34 10,30,90( 2)
    50% vignetting 50  
Scale (arcsec/mm) 13.8 63.5
Diameter of central obstruction (mm) 406  
Focus/mirror shift( 1) 11.7  
1) Movement of focal position for unit movement of secondary mirror
2) Depends on eyepiece used


next up previous contents
Next: Finder telescope Up: The Jacobus Kapteyn Telescope Previous: Mechanical performance

1999-11-12