Ritchey-Chrétien telescope
(RCT, RC)
(type of two-mirror reflector telescope)
A Ritchey-Chrétien telescope (RCT or RC)
is a type of reflector telescope that has
a specific reflector configuration of two hyperbolic mirrors,
designed to limit telescope-induced
aberrations. The primary mirror is hyperbolic
but very close to parabolic. The secondary
mirror is convex and hyperbolic.
Curvature is chosen to eliminate third-order coma
(the cubed term of a series-expansion that describes the aberration).
The design is common for large telescopes, including:
(telescope type,reflector)
Further reading:
https://en.wikipedia.org/wiki/Ritchey-Chretien_telescope
https://www.telescope-optics.net/classical_and_aplanatic.htm
https://dictionary.obspm.fr/index.php?formSearchTextfield=ritchey&showAll=1
https://physics.stackexchange.com/questions/24979/why-is-the-ritchey-chr%c3%83%c2%a9tien-telescope-preferred-in-professional-astronomy
https://www.astronomy.com/observing/the-history-of-the-ritchey-chretien-telescope/
Referenced by pages:
Cassegrain reflector
CHEOPS
Dall-Kirkham telescope
Large Altazimuth Telescope (BTA-6)
Pan-STARRS
reflector telescope
telescope type
Index