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I- ?a I<br />
fha’t hole to th@ P&l. For i‘o the Circles AG,<br />
B 13 i~llC$ the Seti, ~~rOUld 1lOt aIly lOll$Jer Zlflf\\‘er<br />
to the whok Difque of the sun, but only to<br />
that part of it which could be fee11 from the<br />
~rifm through that hole, that is to the :qyarent<br />
magnitude of that hole viewed from the<br />
Prifh, 4jut that thefe Circles may anfker more<br />
diitin&ly to thar hol.e, a Lens is to be placed by<br />
the Priiin to cait: the Image of the hole, (that<br />
is, every and of the Circles A G, BH, &.) difiin&ly<br />
upon the Paper at I? T, after Such a<br />
mai~ner as by a Lens placed at a Window the<br />
Species of Objckts abroad are cait diilin&ly.up;<br />
on .a Paper within the Room, and the reC‘tilinear<br />
Sides of the oblong folar Image in the fifth<br />
Experiment became dif1inCt without ally Penumbra,<br />
If this,be done it will not be neceiG~ry<br />
to place that hole very far OB; 110 not beyone<br />
the Window. And therefore initead of that<br />
hole, I ufed the hole in the Window-fhut as<br />
follows.<br />
Exper. II. In the Sun’s Light let into my<br />
darkned Chamber through ;I ir~xA round hole<br />
in my \\‘indon~-ikut , ilt >IbOUt tel1 01’ tWClVe<br />
Fixt from the Window, % placed a Ecns , by<br />
which the Image of the hole m@ht be dil’Ein&-<br />
ly caf? upon a Sheet of white Paper, placed qt<br />
the difkwx of fix, eight, ten or twelve Feet<br />
from the Lens. For according to the differexxe<br />
of the Lenlks I ufed various dii.tancesg,<br />
which I think not worth the \vhilc to dei‘cribcA<br />
The11 immediately after thk LOIIS I phced a<br />
Frih, by which the trajekd I..,iglJt: might bc<br />
refraCted either upwwds or fidelways, and therebY