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j&cd to the Chart or reflefied back to the<br />
Quick-UVer ) accordingly as, they are in their<br />
Iits of eafy Reflexion or Tranfkilion n$c~~<br />
t]~y arrive at that Surf&et. For the Intervals<br />
of the Fits of the Rays which Ml perpendicu-<br />
~;xrIy on the Speculum, and are retlctted bacl;<br />
in the ike perpendicular Lines, bV r&on of<br />
the equality of thefe Angles and Likes, are of<br />
the fame length and number within the ~lafs<br />
drcr Reflexion as before bv rhc Tgth Prop&.<br />
ticn of the third Part of this Eool;. end tlrer’+<br />
fore fince all the Rays that enter through the<br />
firit Surface are in their Fits of eajy Tranfmi&<br />
iion at their entrance, and as n-~any of thefe as<br />
arc reflerSted by the fecond are in their Fits of<br />
eafy Reflexion there, all thefe muik be again’in<br />
their Fits ‘of eafy TranfmifIion at their return<br />
to the firit-, and by confequence there go out<br />
of the Glafs to the Chart, and form upon it the<br />
nfhite Spot of Light in the center of the Rings,<br />
For the reafon holds good in all forts of Rays,<br />
and therefore all forts muit go out promifcu-i<br />
oufly to that Spot, and by their ,mixturc cauk<br />
it to be white. But the Intervals of the Fits of<br />
thofe Rays which are refle&d more obliquely<br />
than the enter, muit be greater after Retlexion<br />
than be E! ore by the rjth and 20th Propofitions.<br />
And thence it may happen that the Rays at their<br />
return to the fir-it Surface, may in certain Qbfiquities<br />
be in Fits of eafy ReAexion, and return<br />
back to the Quick-filver, and in other intcrmedihte<br />
Obliquities be again in Fits of eafy Tranfmillion,<br />
and fo go out to rhe Chart, and aint<br />
on it the Rings of Colours about the tihite sp poti<br />
T% And