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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

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