Catoptrics (from Ancient Greek: κατοπτρικός katoptrikós, "specular",[1] from Ancient Greek: κάτοπτρον katoptron "mirror")[2] deals with the phenomena of reflected light and image-forming optical systems using mirrors. A catoptric system is also called a catopter (catoptre).
Catoptrics is the title of two texts from ancient Greece:
The Latin translation of Alhazen's (Ibn al-Haytham) main work, Book of Optics (Kitab al-Manazir),[6] exerted a great influence on Western science: for example, on the work of Roger Bacon, who cites him by name.[7] His research in catoptrics (the study of optical systems using mirrors) centred on spherical and parabolic mirrors and spherical aberration. He made the observation that the ratio between the angle of incidence and refraction does not remain constant, and investigated the magnifying power of a lens. His work on catoptrics also contains the problem known as "Alhazen's problem".[8] Alhazen's work influenced Averroes' writings on optics,[citation needed] and his legacy was further advanced through the 'reforming' of his Optics by Persian scientist Kamal al-Din al-Farisi (d. ca. 1320) in the latter's Kitab Tanqih al-Manazir (The Revision of [Ibn al-Haytham's] Optics).[9][10]
16th-century Jewish-Ferraresi physicist Rafael Mirami wrote a treatise on the subject, Compendiosa introduttione alla prima parte della specularia, which became influential in a revival of the field, and contributed towards Pope Gregory XIII's astronomical calculations that led to the creation of the Gregorian Calendar.[11][12]
The first practical catoptric telescope (the "Newtonian reflector") was built by Isaac Newton as a solution to the problem of chromatic aberration exhibited in telescopes using lenses as objectives (dioptric telescopes).