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An ancient theory which extended all the way
back to Aristotle and his followers, suggested a certain class of colour phenomena, such as
the rainbow colours will arise from the modification of light. Light which appears white in its
pristine form. Descartes generalized the theory for all colours, then translated
it into mechanical imagery. Through a series of experiments performed in 1665 and
1666, in which the spectrum of a narrow beam was projected onto the wall of a
darkened room, Isaac Newton denied the concept of modification and replaced it
with that of analysis. Basically, he denied the suggestion that light is simple and
homogeneous. He concluded, instead that it is complex and heterogeneous and that the
phenomena of colours manifest from the examination of the heterogeneous mixture into
its simple components. The ultimate source of Newton's belief that light is
corpuscular was his recognition that individual beams of light have immutable
criteria; in Newton's view, such properties imply immutable particles of matter. He
held that individual rays that is, particles of given size excite sensations of
individual colours as they impact against the retina of the eye. He also concluded that
rays refract at distinct angles--hence, the prismatic spectrum, a beam of
heterogeneous rays, i.e., alike incident on one face of a prism, separated or
analyzed by the refraction into its component parts--and that phenomena such as
the rainbow are produced by refractive analysis. Because Neton believed that
chromatic aberration could never be eliminated from lenses, Newton turned to
reflecting telescopes; he constructed the first ever built. The heterogeneity of
light has been the foundation of physical optics since his time.
There is no evidence that the theory of colours, fully described by Newton in his
inaugural lectures at Cambridge, made any impression, just as there is no evidence
that aspects of his mathematics and the content of the Principia, also pronounced
from the podium, made any impression. Rather, the theory of colours, like his later
work, was transmitted to the world through the Royal Society of London, which
had been organized in 1660. When Newton was appointed Lucasian professor, his
name was probably unknown in the Royal Society; in 1671, however, they heard of
his reflecting telescope and asked to see it. Pleased by their enthusiastic
reception of the telescope and by his election to the society, Newton volunteered
a paper on light and colours early in 1672. On the whole, his dissitation was also well
received, although a few questions and some dissent were muttered.
Primary among the dissenters to Newton's paper was Robert Hooke,
a forceful figure within the Royal Society. Hooke considered himself the custodian of optics
and hence he wrote a scathing critique of the young upstart. One can
understand how the critique would have annoyed a normal man. The bitter rage it
provoked, with the desire publicly to humiliate Hooke, however, bespoke the
abnormal. Newton was unable rationally to confront criticism. Within a year
of submitting the paper, he was so unsettled by the give and take of honest
discussion that he began to cut his ties, and he withdrew into virtual isolation.
In 1675, during a visit to London, Newton thought he heard Hooke accept his
theory of colours. He was emboldened to bring forth a second paper, an
examination of the colour phenomena in thin films, which was identical to most of
Book Two as it later appeared in the Optics. The purpose of the paper was to
explain the colours of solid bodies by showing how light can be analyzed into its
components by reflection as well as refraction. His explanation of the colours of
bodies has not survived, but the paper was significant in demonstrating for the
first time the existence of periodic optical phenomena. He discovered the
concentric coloured rings in the thin film of air between a lens and a flat sheet of
glass; the distance between these concentric rings (Newton's rings) depends on
the increasing thickness of the film of air. In 1704 Newton combined a revision of
his optical lectures with the paper of 1675 and a small amount
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