A few years later, Italian optical designer Massimo Riccardi worked Honders's system into the
Cassegrain configuration found in today's astrographs.
The
cassegrain configuration for the X-band portion of the antenna is an adaptation of a 17th century optical telescope design.
For our night of observing it was set up in its "bent"
Cassegrain configuration. Because the primary mirror isn't perforated, the only way to achieve a Cassegrain focus is to direct the light path out the side of the tube with a flat tertiary mirror.
We have been unable to find any written records that address the condition of the reflecting surfaces of the three mirrors used in the
Cassegrain configuration. (The 100-inch primary is not perforated.) If all three mirrors were not silvered, the resulting light loss would be about 3 1/2 magnitudes per unsilvered surface.
This has led to a need for shorter feeds for use in
Cassegrain configurations.
Maksutovs in f/10 to f/16
Cassegrain configurations have been popular in the astronomy marketplace since Questar introduced its 311/42-inch model in the 1950s.