Miscellanea Curiosa, Vol. 1: Containing a collection of some of the principal phaenomena in nature, accounted for by the greatest philosophers of this age
History
Miscellanea Curiosa, Vol. 1: Containing a collection of some of the principal phaenomena in nature, accounted for by the greatest philosophers of this age
Natural history; Science -- Early works to 1800; Voyages and travels -- Early works to 1800
8. Nor afterwards from the adjacent quiet _Medium_: These two
Propositions are manifest _de Facto_ in Homogeneal Light, whose Colour
and Refrangibility is not at all changeable, either by Refraction, or by
the Contermination of a quiet _Medium_. And as for Heterogeneal Light,
it is but an Aggregate of several sorts of Homogeneal Light, no one sort
of which suffers any more alteration than if it were alone; because the
Rays act not on one another, by _Prop._ 6. and therefore the Aggregate
can suffer none. These two Propositions also might be further proved
apart, by Experiments too long to be here described.
9. There can no Homogeneal Colours be reduced out of Light by
Refraction, which were not commixt in it before. Because by _Prop._ 7.
and 8. Refraction changeth not the Qualities of the Rays, but only
separates those which have divers Qualities, by means of their different
Refrangibility.
10. The Sun's Light is an Aggregate of an indefinite variety of
Homogeneal Colours, by _Prop._ 1, 3, and 9. And hence it is, that I call
Homogeneal Colours also Primitive or Original. And thus much concerning
Colours.
_For a further Illustration of this Doctrine, Mr. _Newton_, in his Book
of Opticks lately published, has by undeniable Experiments explained
most of the Principal Phænomena of Light and Colours: To which we
refer the Reader._
_A Demonstration concerning the Motion of Light, communicated from
_Paris_._
Philosophers have been labouring for many Years to decide by some
Experiment, whether the Action of Light be conveyed in an instant to
distant Places, or whether it requireth time. M. _Romer_, of the _Royal
Academy_ of Sciences, hath devised a way taken from the Observations of
the first Satellit of _Jupiter_, by which he demonstrates, that for the
distance of about 3000 Leagues, such as is very near the bigness of the
Diameter of the Earth, Light needs not one Second of Time.
Let (in _Fig. 3. Plate 3._) _A_ be the _Sun_, _B_ _Jupiter_, _C_ the
first Satellit of _Jupiter_, which enters into the shadow of _Jupiter_,
to come out at _D_, and let _EFGHKL_ be the _Earth_, placed at divers
distances from _Jupiter_.
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