— Ch. 1 · Newton's Optical Theory —
Newton's reflector.
~4 min read · Ch. 1 of 6
Isaac Newton built his reflecting telescope as a proof for his theory that white light is composed of a spectrum of colours. He had concluded that the lens of any refracting telescope would suffer from the dispersion of light into colours known as chromatic aberration. The telescope he constructed used mirrors as the objective which bypassed that problem entirely. This approach allowed him to create an instrument free from the colour fringing that plagued glass lenses of the era. Newton chose a spherical shape for his mirror instead of a parabola to simplify construction. He had satisfied himself that the chromatic, and not the spherical aberration, formed the chief faults of refracting telescopes.
Mirror Construction Methods
To create the primary mirror Newton used a custom composition of metal consisting of six parts copper to two parts tin. This early composition of speculum metal required precise handling during the grinding process. He devised means for shaping and grinding the mirror and may have been the first to use a pitch lap to polish the optical surface. Newton described the object-metal as two inches broad and about one-third part of an inch thick to keep it from bending. He made two of these metals and when he had polished them both he tried which was best. He then ground the other again to see if he could make it better than that which he kept.The 1668 Prototype Design