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2.7<br />
great& Refra&ion, mufi be more refrangible<br />
than thofe which go to the lower end T, unlefs<br />
the inequality of RefraCtion be cafual.<br />
This Image or Sp&rum I? T was coloured,<br />
being red at its leait refra&ed end T, and violet<br />
at its mofi refra&ed end P, and yellow<br />
green and blue in the intermediate Spaces..<br />
.Which agrees with the firfi Propofitioy ,,** that<br />
Lights which differ in Colour do allb dukr in<br />
Kefrai$bility, The length of the Image in the<br />
, foregomg Experiments I meafured from, the<br />
faintefi and outmofi red at one end, to the<br />
fainteit and outmoit blue at the other end, excepting<br />
only a little Penumbra, whole breadth<br />
fcarce exceeded a quarter. of an Inch, as was<br />
a:;lid above.<br />
Ex~P~. 4. In the Sun’s beam which was propagated<br />
into the Room through the hole in the<br />
Window-fhut, at the di,rtance of ibme Feet<br />
from the hole, I held the Prifrn in fuch a poiflure<br />
that its Axis might be perpendicular to<br />
that beam. Then I looked through the Prifm<br />
zlpon the hole, and turning the Prifm to and<br />
fro about its Axis to make the Image of the<br />
hole afcend and d&end, when bctwecn its<br />
two contrar Motions it feemed fiationary, I<br />
itopp’d the P %fm that the RefraCtions of both<br />
iides of the refraAing Angle might be equal to<br />
each other ) as in the former Experiment. In<br />
this Situation of the Prifm viewing through it<br />
the faid hole, I obferved the length of its refra8ed<br />
Image to be many times greater than<br />
its breadth, and that the nlofi ref%aAed part<br />
thereof agpeared . violet, the leafi refraAed red,<br />
the